Which quantum theory must be reconciled with gravity? (And what does it mean for black holes?)

We consider the nature of quantum properties in non-relativistic quantum mechanics (QM) and relativistic QFTs, and examine the connection between formal quantization schemes and intuitive notions of wave-particle duality. Based on the map between classical Poisson brackets and their associated commutators, such schemes give rise to quantum states obeying canonical dispersion relations, obtained by substituting the de Broglie relations into the relevant (classical) energy-momentum relation. In canonical QM, this yields a dispersion relation involving $\hbar$ but not $c$, whereas the canonical relativistic dispersion relation involves both. Extending this logic to the canonical quantization of the gravitational field gives rise to loop quantum gravity, and a map between classical variables containing $G$ and $c$, and associated commutators involving $\hbar$. This naturally defines a"wave-gravity duality", suggesting that a quantum wave packet describing {\it self-gravitating matter} obeys a dispersion relation involving $G$, $c$ and $\hbar$. We propose an ansatz for this relation, which is valid in the semi-Newtonian regime of both QM and general relativity. In this limit, space and time are absolute, but imposing $v_{\rm max} = c$ allows us to recover the standard expressions for the Compton wavelength $\lambda_C$ and the Schwarzschild radius $r_S$ within the same ontological framework. The new dispersion relation is based on"extended"de Broglie relations, which remain valid for slow-moving bodies of {\it any} mass $m$. These reduce to canonical form for $m \ll m_P$, yielding $\lambda_C$ from the standard uncertainty principle, whereas, for $m \gg m_P$, we obtain $r_S$ as the natural radius of a self-gravitating quantum object. Thus, the extended de Broglie theory naturally gives rise to a unified description of black holes and fundamental particles in the semi-Newtonian regime.


Introduction
The Compton wavelength λ C gives the minimum radius within which the mass of a particle may be localized due to relativistic quantum effects, neglecting the particle's self-gravity, while the Schwarzschild radius r S gives the maximum radius within which the mass of a black hole may be localized due to classical relativistic gravity, neglecting quantum effects. In a mass-radius diagram, the two lines intersect near the Planck point (m P , l P ), where m P denotes the Planck mass and l P the Planck length, so that relativistic-quantum-gravitational effects become significant in this region. In addition, the equivalence of the Compton and Schwarzschild radii close to the Planck scales suggests that a final theory of quantum gravity (QG) should yield a unified description of fundamental particles and black holes. Nonetheless, how such a unification could be achieved may be considered an outstanding problem for both elementary particle physics, and the physics of black holes, even in the absence of a final theory.
Since canonical non-gravitational QM and quantum field theories (QFTs) are based on the concept of wave-particle duality, encapsulated in the de Broglie relations, these may break down close to (m P , l P ). However, it is unclear what (if any) physical interpretation can be given to quantum particles with energies E m P c 2 , since these correspond to "matter waves" with sub-Planckian wavelengths λ l P and time periods τ t P (t P = l P /c), according to canonical quantum dispersion relations. On the other hand, "particles" with rest masses m > m P have sub-Planckian Compton wavelengths, λ C < l P , but super-Planckian Schwarzschild radii, r S > l P , and may be interpreted as black holes. We therefore propose corrections to the standard de Broglie relations, which are valid in the semi-Newtonian limit, allowing them to be extended into the region m m P . Here, the semi-Newtonian theory is defined as the Newtonian limit of general relativity, in which space and time are absolute but there exists a cosmic speed limit v max = c, which must be imposed "by hand" on the quantum sector. Though, from the viewpoint of a final theory, this is clearly inadequate, it has the advantage of allowing us to describe key phenomenological features of spherically symmetric systems on both halves on the mass-radius diagram, m ≤ m P and m ≥ m P , within a unified ontological framework. In other words, using the same set of assumptions about the nature of space and time, the finite speed of light, and the form of the quantum dispersion relations, we recover well-known features of both canonical QM and classical gravity. These assumptions gives rise to both a modified Schrödinger equation and a modified expression for the Compton wavelength. Both reduce to the standard forms for m m P , as required for consistency, but, crucially, also allow us to recover the standard expression for the Schwarzschild radius for m m P , using standard "quantum" arguments. Thus, we interpret the additional terms in the modified de Broglie relations, which involve all three fundamental constants, G, c and , as representing the self-gravitation of the wave packet in the semi-Newtonian background.
The structure of this paper is as follows. In Sec. 2, we review the basic arguments for the "quantum" nature of non-relativistic point-particles and relativistic fields, focussing on the equivalence of wave-particle duality, as expressed via the canonical dispersion relations, and formal quantization schemes. In Sec. 3.1, we briefly review Newtonian gravity and general relativity, with special emphasis on their application to spherically symmetric bodies (i.e., particles and black holes). The gravitational implications of the the semi-Newtonian approximation are discussed in 3.2. Sec. 3.3 considers two previous attempts to incorporate quantum effects into gravitational theories, the Schrödinger-Newton equation and Loop Quantum Gravity (LQG). Their relations to the extended de Broglie theory, and to the problem of obtaining a unified description of fundamental particles and black holes, are also discussed. In Sec. 3.4, the quantum mechanical implications of the semi-Newtonian approximation are considered and the conceptual framework for the extended de Broglie theory is defined. The ansatz for the extended relations is motivated by considering the asymptotic black hole regime in Sec. 4.1 and the full relations are presented in Sec. 4.2. In Sec. 5, we determine the equations of motion (EOM) for the quantum state and the associated Hamiltonian and momentum operators, in both the particle and black hole regimes. The implications of the extended theory for the Hawking temperature are discussed in Sec. 6, and alternative unification schemes for black holes and fundamental particles, based on Generalized Uncertainty Principle (GUP) phenomenology, are considered in Sec. 7, with special emphasis on how these relate to the ideas discussed in Secs. 2-6. A brief summary our our main results is given in Sec. 8. For reference, the four postulates of canonical QM are listed in the Appendix.
Thus, the results presented in Secs. 2-3 are mostly pedagogical, while those presented in Secs. 4-6 are based primarily on results obtained in [1], in which the extended de Broglie theory was first introduced. However, the purpose of the present work is not simply to review the results of previous studies, but to propose a provisional answer to the questions posed in the title, "Which quantum theory must be reconciled with gravity? (And what does it mean for black holes?)", which may be considered important open questions in black hole physics. For this reason, the material presented in Secs. 2-3 is chosen to highlight the steps required to obtain a unified ontology for the description of black holes and fundamental particles. Since this necessarily entails important modifications to our existing notions of what makes a theory "quantum", it leads naturally to the extended de Broglie theory as a provisional scheme for unification in the semi-Newtonian limit. Throughout, we explore the relation between this theory and existing models of modified quantum theory − relativistic, non-relativistic and semirelativistic − motivated by gravitational considerations. In each case, we attempt to clarify the theoretical assumptions underpinning different approaches and to identify which (if any) of the physical assumptions on which different models are based may be in contradiction with one another. In particular, special emphasis is given to particle-black hole unification schemes arising in the context of GUP phenomenology, which are considered in detail in Sec. 7.
2 What makes a theory "quantum"?
The essence of quantum theory is wave-particle duality. Though, philosophically, a somewhat slippery concept [2], it is encapsulated mathematically in a very precise form via the de Broglie relations [3] E = ω , p = k . (2.1) In 1924, de Broglie's great insight was to relate the constants of motion of a classical point particle, energy E and momentum p, with properties hitherto associated only with waves; frequency f and wavelength λ, or, equivalently, angular frequency ω = 2πf and wave number k = 2π/λ. This was made possible by Planck's earlier discovery of new fundamental constant with dimensions of action, = h/(2π) = 1.055 × 10 −34 Js, which proved necessary to explain the observed spectrum of black body radiation. The quantization of absorbed and emitted radiation, according to Eq. (2.1), was able to account for the suppression of high-energy modes that otherwise result in an "ultraviolet catastrophe" [4]. The breakthrough leading, ultimately, to the development of modern quantum mechanics (QM) and quantum field theory (QFT) came when de Broglie proposed that the relations (2.1) were applicable to all forms of matter and radiation. Thus, the foundation of any quantum theory is the quantum dispersion relation, which is obtained by substituting (2.1) into the classical relation between E and p. In general, this may be relativistic or non-relativistic and may apply to objects with zero or nonzero rest mass. Typically, the latter are considered "particles" in the classical theory and acquire wave-like characteristics via quantization, whereas the former are considered classically as "waves", which acquire particle-like properties via (2.1). The equation of motion (EOM) for the quantum state must satisfy the dispersion relation obtained by combining the classical energy-momentum relation with the de Broglie relations and be invariant under the symmetries of the corresponding classical theory.
For massive particles, the quantum dispersion relation involves and will also include c, the speed of light, if the theory is relativistic. Roughly speaking, we may say that a theory describing massive particles is quantum (meaning it incorporates wave-particle duality) and non-relativistic if its dispersion relation contains, but not c, and if the resulting EOM are invariant under rotations, translations in time and space, and local Gallilean boosts. Likewise, a theory of massive particles is quantum and relativistic if its dispersion relation contains both and c, and if the resulting EOM are invariant under the action of the Poincáre group, comprising rotations, translations and local Lorentz boosts.

Wave-particle duality in Newtonian space -without Newtonian gravity
The non-relativistic energy-momentum relation is where V ( x, t) represents an external classical potential, not generated by the particle itself. The quantum dispersion relation is, therefore, By assuming that a single "matter wave" mode, corresponding to a single value of the classical momentum p, is given by exp[i( k. x − ωt)], and that a general quantum state ψ( x, t) is given by a superposition of modes, the next fundamental breakthrough was made by Schrödinger, who obtained the EOM for a non-relativistic quantum system: For a given V , this equation is unique and, hence, is the only EOM consistent with Eqs. (2.1)-(2.2). The operatorĤ is called the Hamiltonian and its eigenvalues represent the possible results of measurements of the system's energy.
In the position space representation, the results of position measurements are given by the classical position vector, so that the operators corresponding to classical canonical coordinates are given byˆ The equivalents of Eqs. (2.5)-(2.6) in the momentum space representation are obtained by applying the transformation x ↔ p, so that the position and momentum operators obey the canonical commutation relations, in either representation. In general, consistency requires that these hold in any representation, so that (2.7) may be taken as a definition: any pair of operators satisfying the canonical commutation relations are valid representations ofx i andp j . It is a fundamental postulate of canonical QM that operators representing other dynamical variables bear the same functional relation to these as do the corresponding classical quantities to the classical position and momentum [3].
In the Schrödinger picture, operators representing physical observables are time-independent, whereas the quantum state ψ is time-dependent, according tô Equivalently, in the Heisenberg picture, operators are time-dependent and states time-independent, so thatÔ is the classical Poisson bracket for the functions f (q i , p i ), g(q i , p i ). (The Schrödinger equation may also be related to Hamilton's equation via the transformation ψ = ψ 0 e iS/ , where S(q i , p i , t) is the action.) In classical mechanics, the Poisson bracket for the canonical coordinates is so that applying the transformation yields (2.7). These results suggest a general quantization scheme, defined by the following association between classical quantities and the Hermitian operators representing the corresponding QM observables [6]: Such an abstract scheme seems far removed from our initial considerations regarding the dual wave/particle nature of quantum states, but follows logically from the definition of waveparticle duality encapsulated in the de Broglie relations (2.1). The principle of superposition, applied to de Broglie waves, also implies the equivalence of the wave function ψ, in real space, and the wave vector |ψ , in a vector space that forms the state space of the theory. Thus, a general quantum state |ψ may be expressed as a superposition of eigenfunctions of an arbitrary operatorÔ, which form an arbitrary set of basis vectors in the corresponding Hilbert space [3,6,7]. This, in turn, is key to the interpretation of QM as a probabilistic theory, and the entire formalism of canonical QM can be defined in terms of four basic Postulates that relate its mathematical structure to the outcomes of physical measurements [7]. (For reference, these are listed in the Appendix.) An immediate consequence is the existence of the General Uncertainty Principle, for a pair of arbitrary operators, Furthermore, it may be shown that operators representing classically conserved quantities may be identified (up to factors of ) with the generators of the associated symmetry group. In classical physics, the state space is a manifold and the invariance of an arbitrary state under a given isometry leads to existence of a conserved charge Q via Noether's theorem [8]. In quantum mechanics, the state space is a vector space and the invariance of an arbitrary state under the same isometry gives rise to the canonical commutation relation involvingQ [7].
The discussion above gives a brief account of the logical development of the formalism of canonical non-relativistic QM. For our current purposes, the key point is that, no matter how abstract this formalism appears, its fundamental physical root is the association of particle and wave properties according to (2.1). The precise form of the dispersion relation (2.3), EOM (2.4), commutation relations (2.16), and state space (Hilbert space) structure, follow from the way in which the de Broglie relations are combined with the energy-momentum relation for a point-particle in Newtonian mechanics (2.2). Crucially, this approach ignores the effect of the particle's self-gravity, even in the Newtonian limit.

Wave-particle duality in Minkowski space -without general relativity
In the relativistic case, the classical energy-momentum relation for a free particle is Combining this with (2.1), the quantum dispersion relation is and λ C is the Compton wavelength. This is the length-scale that can be naturally associated with the particle's rest mass using the constants h and c and may be interpreted as the minimum possible radius of a quantum "particle" of mass m. (The quantity k −1 C = /(mc) is known as the reduced Compton wavelength.) In this case, the corresonding EOM is not unique, and depends on several factors, including: • The explicit form in which the quantum dispersion relation is written, i.e. as on the left-hand or right-hand side of Eq. (2.20).
• The gauge symmetries -in addition to the Poincáre symmetry of the Minkowski space background -under which the action of the corresponding classical theory is invariant.
A fundamental difference between this and the non-relativistic case is the existence of two solution branches, which seem to give rise to particles with both positive and negative energy. Furthermore, although the two forms of the energy-momentum relation given in (2.19) are classically equivalent, this equivalence does not extend to the corresponding quantum EOM, obtained via the substitutions E →Ĥ, p →p. In other words, the two forms of the dispersion relation given on the left-hand and right-hand sides of Eq. (2.20) are quantum mechanically inequivalent.
An example of an EOM satisfying the left-hand ("squared") form of the dispersion relation is the Klein-Gordon equation [9], which may be generalized to describe a wave function moving in a potential V (ψ) by adding the term ∂V /∂ψ. Equation (2.22) obeys both Poincáre symmetry and the local U (1) gauge symmetry of the complex scalar ψ, which gives rise to a conserved electric current. It describes spinless, electrically charged, relativistic quantum particles, but is not the EOM for a fully self-consistent theory of a quantum one-particle state. Though the mathematical subtleties are complex, the physical reason for this is simple: no such theory exists. In fully self-consistent theories (QFTs), negative energy states given by the right-hand side of (2.19) may be reinterpreted as positive energy particles under charge inversion (+ ↔ −), so that relativistic quantum theories predict the existence of anti-matter. States with E mc 2 then lead to the the production of particleanti-particle pairs, giving rise to multi-particle states that conserve electric charge [9]. It is straightforward to show that the classical inequality E mc 2 corresponds to λ λ C in the quantum picture, so that pair-production occurs when the size of a local field oscillation becomes smaller than the Compton wavelength. This gives rise to an effective cut-off for the spread of the wave packet in the non-relativistic theory, ∆ ψ x λ C , so that the HUP (2.18) implies Hence, while the de Broglie wavelength of an object marks the length-scale at which nonrelativistic quantum effects become important for its description, and the classical concept of a particle gives way to the wave packet, the Compton wavelength marks the point at which relativistic quantum effects become significant and the concept of a single wave packet corresponding to a state in which particle number remains fixed breaks down. This acts as an effective minimum width because, for de Broglie modes with λ λ C , we must switch to a field description in which particle creation occurs in place of further spatial localization. By contrast with Eq. (2.22), the right-hand ("square root") form of the quantum dispersion relation gives rise, uniquely, to the Dirac equation, from which the original prediction of antimatter was derived [3,6,9]. This may be written in a manifestly Lorentz invariant form as where µ ∈ {0, 1, 2, 3} are space-time indices and γ µ denotes a set of 4 × 4 matrices where I 2 is the 2 × 2 identity matrix and σ i are the Pauli matrices [3,9]. The Dirac equation describes spin-1/2, electrically charged, relativistic quantum particles. Crucially, it also enables us to explain the (otherwise mysterious) property of quantum mechanical spin as a necessary consequence of the union of quantum mechanics and special relativity.
It is straightforward to show that "squaring" the Dirac equation (2.24) gives the Klein-Gordon equation (2.22) and that Taylor expanding this -using an appropriate definition of the "square root" of a differential operator -yields the Schrödinger equation (2.4). In fully consistent QFTs, the Klein-Gordon equation also reemerges as the EOM governing the components of all free (i.e. non-interacting) quantum fields. The solutions of the free field EOM are used to build the state space -in this case, a Fock space [9] -of the theory, since these form a basis that spans the space. Hence, while integer spin particles may obey any EOM that is consistent with the "squared" form of the quantum dispersion relation, together with the other requirements of the theory, such as gauge invariance, etc., particles with half-integer spin always obey the Dirac equation, or its generalization to include interactions with electromagnetic field [3,9]. However, since only two quantum mechanically inequivalent forms of the dispersion relation exist, there are only two types of quantum relativistic particle: bosons and fermions.
In the field theory approach, the classical field variables become quantum operators, so that, for example, a scalar field φ(x) and its canonical momentum π(x) satisfy the relation [9] [φ(x),π( This is equivalent to the map is the classical Poisson bracket. Thus, equations like (2.25) represent the field theory analogue of the canonical quantization of point particles, (2.15). The discussion in this subsection gives a brief account of the logical development of relativistic QM and a very brief introduction to some of the basic concepts of QFT. We have seen that antimatter, bosons and fermions, the existence of the Compton wavelength and pair-production arise as necessary consequences of any theory that successfully incorporates both wave-particle duality -encapsulated in the de Broglie relations (2.1) -and local Lorentz invariance. Though the field replaces the particle as the fundamental object to be "quantized", and multiple excitations are interpreted as multi-particle states [9], the time-evolution of each excitation remains consistent with the point-particle dispersion relation (2.20).
For our current purposes the key point is that, no matter how complex or abstract the mathematical formulation of realistic QFTs -including the SU (3) × SU (2) × U (1) gauge theories of the Standard Model of particle physics -become, their basic architecture must be compatible with the dispersion relation (2.20), which follows directly from combining the de Broglie relations with the energy-momentum relation for a point-particle in special relativity. Again, this approach ignores the effect of the particle's self-gravity, which, in the relativistic regime, must be described by Einstein's theory of general relativity.
3 What makes a theory gravitational? By our previous logic, a crude definition of a gravitational theory is any set of EOM involving Newton's constant G that reduce to Einstein's field equations (EFEs) in an appropriate limit. These, in turn, reduce to the Newtonian theory of gravity in the weak field approximation [10]. The EFEs include both G and c, and incorporate both relativistic and gravitational effects. More specifically, we may say that they describe the regime in which relativistic-gravitational effects become important.

Newtonian and Einstein gravity -without wave-particle duality
We now briefly review Newtonian gravity and the the general theory of relativity, with special emphasis on their application to spherically symmetric systems. Specifically, we show how the Newtonian gravitational potential arises as the weak field limit of the unique, static, spherically symmetric vacuum solution of the EFEs, the Schwarzschild solution [10].

Newtonian gravity for spherically symmetric objects
In spherical polar coordinates, Newton's law of gravity gives the gravitational potential energy (per unit mass) of a body of mass M , or, equivalently, the force between two spherically symmetric bodies with masses M and M : This is consistent with Newton's second law of motion, F = M a, since a = − ∇Φ. The potential is the Green's function [11] solution of Poisson's equation, where ρ is the mass density of a gravitating body. This is invariant under rotations, translations and Gallilean boosts, as required by the background of absolute space and time. Though it is straightforward to set V (r) = Φ(r) in Schrödinger's equation, this models a quantum wave packet moving in an external (classical) gravitational field, and cannot account for the self-gravity of the quantum "particle". At present it is unclear whether such an effect can be successfully incorporated into canonical QM, though one semi-classical attempt -the Schrödinger-Newton equation -is described in Sec. 3.3.

General relativity and the Schwarzschild solution
The general theory of relativity is based on the action [10] The first integral is the Einstein-Hilbert term, which describes the vacuum theory, and L M is the matter Lagrangian. Variation with respect to the metric g µν gives the EFEs where the energy-momentum tensor for the matter sector is defined implicitly via G µν is called the Einstein tensor, R µν = R α µαν is the Ricci tensor, R = R µ µ is the scalar curvature, and R µναβ is the Riemann curvature tensor [10]. This determines the deviation of geodesics due to the curvature of space-time, induced by the presence of matter [12].
In the static, weak field limit, the vacuum EFEs reduce to [10,12] 1 where i, j denote spatial coordinates, which is simply the covariant version of Laplace's equation (Poisson's equation with ρ = 0). As g 00 /c 2 must be close to unity, we may set where Φ/c 2 1, giving g 1/2 00 /c = 1 + Φ/c 2 . The function Φ/c 2 also obeys Laplace's equation, but, as it does not correspond to the flat space solution, must be identified with the Green's function solution of Poisson's equation and hence with the Newtonian potential −GM/r (3.1). In this way, c explicitly "drops out" of the EFEs in the Newtonian approximation, as expected. Nonetheless, the derivation of the Newtonian potential from the weak field limit of Einstein's theory shows that it is compatible with a cosmic speed limit c, which may be re-introduced "by hand", giving rise to a more accurate semi-Newtonian description.
Since all quantities in Eq. (3.4) are expressed in terms of tensors, the EFEs are invariant under general coordinate transformations (GCTs), a property also known as general covariance. This is the mathematical expression of the fact that coordinates do not exist a priori in nature -being, instead, only artifices used to describe physical systems -and hence play no role in the formulation of fundamental physical laws. Thus, any fundamental "quantum" theory of gravity (whatever this may mean) must also be generally covariant. That the gravitational field equations take the form of tensor equations may also be seen as the mathematical expression of the principle of general relativity. This states that the laws of physics take the same form in all reference systems and is a generalization of the principle of special relativity, which states that the laws of physics take the same form in all inertial frames. That the gravitational field is equivalent to the curvature of the space-time background follows from applying the principle of general relativity to accelerating frames, combined with local Lorentz invariance [12].
The unique, static, spherically symmetric vacuum solution of the EFEs -which corresponds to the external gravitational field of a point-like particle of mass M -is the Schwarzschild metric. In canonical polar coordinates this gives the line-element [10,12] where t is the time measured by a static observer at r → ∞. Two key physical properties of the Schwarzschild metric are: • The "event horizon" at r = 2GM/c 2 . This is a spherical surface on which the escape velocity is equal to the speed of light c. Thus, objects located within the sphere are causally disconnected from those outside it.
• The singularity at r = 0. This is a point at which the space-time curvature becomes formally infinite, which marks the break down of the classical theory of general relativity.
The radius of the event horizon in the Schwarzschild solution is called the Schwarzschild radius and is denoted

The semi-Newtonian approach
Equation (3.1) represents Newton's law of gravity for spherically symmetric bodies and results directly from the weak field approximation (3.6)-(3.7) of the Schwarzschild solution (3.8). As expected, c "drops out" of the field equations in this limit, yielding a formula which is valid in the non-relativistic gravitational regime. Remarkably, we may also "derive" a crucial relativistic-gravitational result, namely, the existence of the Schwarzschild radius (3.9), without imposing the full structure of general relativity. Specifically, we may consider the gravitational field in a Newtonian background of absolute space and time, in which a cosmic speed limit v max = c is imposed "by hand", without imposing any of its logical consequences, i.e. local Lorentz invariance and the unification of space and time (in the zero gravity limit), or general covariance and space-time curvature (required in the strong gravity regime).
Combining Newton's laws of motion with Eq. (3.1), we obtain the expression for the total energy of a particle of mass m, moving in the gravitational field of a body of mass M , as The escape velocity, at a given radius r, is obtained by setting E total = 0, giving Setting v esc ≤ c then implies that the particle must be situated at a radius in order to escape from the gravitational field of the massive body. Conversely, test particles initially within r S remain trapped in the region r ≤ r S for all time. We call this the semi-Newtonian approach, and its advantages for constructing a naïve theory of quantum gravity, which permits a unified description of black holes and fundamental particles, are discussed in Sec. 3.4.

Newtonian and Einstein gravitywith wave-particle duality?
In this sub-section, we review two attempts to incorporate quantum effects into gravitational theories -one in the Newtonian picture, leading to the Schrödinger-Newton equation [13] -and the other in background-independent form, via the canonical quantization of general relativity, leading to loop quantum gravity (LQG) [14,15,16,17].

Newtonian gravity -the Schrödinger-Newton equation
One attempt to combine wave-particle duality with the existence of the Newtonian gravitational field is based on the observation that the quantity m|ψ| 2 behaves like a "quantum" mass density for the wave function. Formally identifying this with the source term in Poisson's equation (3.2), we obtain The next step is to replace the external classical potential V in Schrödinger's equation (2.4) with mΦ, which is supposed to represent the self-gravity field generated by the particle itself. This gives which is known as the Schrödinger-Newton equation [13]. The main problem with this approach is that the explicit solution of Eq. (3.13), is semi-classical, in the sense that it is an explicit function of the classical coordinates x − which, here, cannot be interpreted as quantum operators − as well as the wave function ψ. Therefore, though useful in models of wave function collapse [13] and potentially testable in the near future [18,19], Eq. (3.14) cannot be interpreted as the EOM for the wave function of a "free" quantum particle, interacting only with its own (self-generated) gravitational field. In short, it fails to adequately "quantize" the particle's self-gravity potential, which remains a function of external classical coordinates.
In fact, it may be explicitly shown that the Schrödinger-Newton equation arises as the weak field limit of semi-classical general relativity, in which only matter fields are quantized, while the gravitational field remains classical even at the fundamental level. This is given by the semi-classical Einstein equations [13] whereT µν denotes the set of quantum mechanical operators associated with the components of the classical energy-momentum tensor. In the linearized theory, g µν = η µν + h µν , where η µν is the Minkowski metric and h µν represents a small perturbation, Eq. (3.16) reduces to where Φ = −h 00 c 2 /2. IdentifyingT 00 /c 2 =ρ = m|ψ| 2 in the non-relativistic limit, we recover Eq. (3.14) [13].

General relativity -loop quantum gravity
Loop quantum gravity (LQG) represents a canonical quantization of the general theory of relativity; that is, it is based on a map from field variables obeying classical Poisson brackets to commutators involving the corresponding quantum operators. The starting point is, therefore, to rewrite the Einstein-Hilbert action (3.3) in terms of variables satisfying the canonical Poisson bracket structure. These are known as Ashtekar variables [20]. The canonical quantization of the gravitational field then proceeds by analogy with Eqs. (2.15) and (2.26). Though, for the sake of brevity, we are unable to give a detailed account of the mathematical formalism of LQG here, we note that, just as the union of wave-particle duality with special relativity gave rise to many unexpected physical phenomena -including the existence of antimatter, pair production and quantum mechanical spin -the canonical quantization of the spacetime background (whether or not this leads to final theory of quantum gravity [21,22]), also yields profound insights and new predictions. Among the most significant are: • That background-independent theories, including general relativity and all related supergravity theories, can be reformulated as gauge theories. In this case, the required gauge symmetry is diffeomorphism invariance, a key property of space-time in general relativity [23].
• The physical picture that emerges is of dynamical space-time as a network of interwoven finite "loops", known as a spin foam [14,15,16,17].
(The interested reader is referred to [14,15,16,17] and references therein for a full summary of the present state of LQG research.) Strictly, in this picture, the "quantum" nature of gravity arises from the fact that space-time can exist as a superposition of spin foams. These represent generalized Feynman diagrams [9] which, instead of graphs, use higher-dimensional complexes. A spin foam represents the time evolution of spin network -a specific type of 2-complex whose faces represent possible configurations of the field -that must be summed to obtain an amplitude via the path integral approach [14,15,16,17].

The semi-Newtonian approach revisited
In Sec. 3.2, we saw that the imposition of a cosmic speed limit, v max = c, in a Newtonian background of absolute space and time, allowed us to recover the expression for the Schwarzschild radius (3.9) from the formula for the escape velocity. This may be considered a fundamental result of "semi-Newtonian" gravity, that, happily, recovers the correct general-relativistic formula. In Sec. 2.2, a limit on the momentum uncertainty of single quantum particle, in the non-relativistic theory, (∆ ψ p) max ≈ mc, was obtained by noting that, for (∆ ψ x) min ≈ λ C , relativistic field effects imply pair-production instead of further localization of the wave packet. We now note that the identifications in Eq. (2.23) may be obtained in an alternative way, via the imposition of the semi-Newtonian condition in canonical QM. Beginning with the non-relativistic formula for the momentum of a point-particle, and imposing the cosmic speed limit, gives p ≤ mc. Using ∆ ψ p p, we then have (∆ ψ p) max ≈ mc, so that the HUP (2.18) implies (∆ ψ x) min ≈ λ C . The logic used here is the reverse of our previous argument in Sec. 3.2, in which a relativistic result (the existence of λ C ) was used to impose a limit on the spatial extent of a non-relativistic wave packet. This, combined with the HUP (2.18), then gave rise to a limit on the spread in momentum space. In the semi-Newtonian approach, we use a result from the non-relativistic theory (3.18), together with v max = c, to obtain a limit on the momentum uncertainty, which then implies the existence of λ C . This should come as no surprise; since the Compton wavelength marks the boundary between relativistic and non-relativistic quantum theory, approaching the line λ = λ C from either side should give the same results.
However, the realization that the Compton wavelength (2.21) may be obtained by applying the semi-Newtonian condition to the general structure of canonical QM (which "lives" in a Newtonian background) and that the same condition, applied to Newtonian gravity, gives rise to the Schwarzschild radius (3.9), is important. In principle, it allows us to construct a "semi-Newtonian" theory of quantum gravity, in which essential phenomenological features of both relativistic QM and relativistic gravity are recovered in the appropriate asymptotic regimes. Such a theory would be naïve, failing even to account correctly for the local Lorentz invariance of special relativity, let alone general covariance. Nonetheless, it could be interesting, giving rise to a quantum mechanical description of massive objects which is consistent with key general-relativistic results, at least for spherically symmetric systems, as well as key results from relativistic QFT. It would, necessarily, imply a unified description of fundamental particles and black holes, as quantum objects, in an absolute background with a cosmic speed limit.
With this in mind, we note that λ C and r S define radii with fundamentally different physical natures; λ C defines a minimum radius, beyond which further compression is impossible, whereas r S defines a maximum radius, beyond which further compression is inevitable. Since any unified picture of fundamental particles and black holes must reflect this, the question arises, what form of wave-particle duality defines their (unified) "quantum" nature? Does it take the same form in each asymptotic limit? The different physical natures of λ C and r S would suggest "no". It is likely, therefore, that a unified theory could be based on a extension of the notion of waveparticle duality, which reduces to the canonical de Broglie relations (2.1) for small mass objects (particles), but takes a different asymptotic form for large mass objects (black holes).
Hence, for our present purposes, in which we seek only a naïve, semi-Newtonian, theory of quantum gravity, the most relevant insight of LQG, discussed in Sec. 3.3.2, is the following: Since the Ashtekar variables necessarily involve both G and c, and the canonical map relates these to Planck's constant , it is reasonable to assume that, in the semi-Newtonian regime, this gives rise to an effective dispersion relation for the gravitational field involving G, c and . More specifically, we expect a modification of the standard dispersion relation for a (non-gravitating) Newtonian particle, containing all three constants, which reduces to Eq. (2.3) in the appropriate limit. In principle, this may be achieved in two ways: • By substitution of the canonical de Broglie relations (2.1) into a modified, semi-classical, formula for the total energy of a self-gravitating particle (Eq. (2.2) with V ≡ V (ψ) = 0).
• By substituting modified de Broglie relations into the existing Newtonian formula for a free particle (Eq. (2.2) with V = 0).
The first approach results, most naturally, in the Schrödinger-Newton equation (3.14), and does not allow us to accomplish our desired aim, as discussed in Sec. 3.3.1. We therefore adopt the second. However, since, mathematically, we may consider arbitrary modifications of Eq. (2.1), we adopt the following criteria as guidelines for a physical theory: • We require the modified dispersion relation to be consistent with essential phenomenological features of both relativistic QM and relativistic gravity -specifically, the existence of the Compton wavelength for fundamental particles and the Schwarzschild radius for black holes -in appropriate limits.
• Within the constraints imposed by the asymptotic regimes, the new expression should be as simple as possible, containing the minimum number of new fundamental parameters.
• All physically observable quantities must be continuous, including at the transition point between quantum particles and quantum black holes (i.e., close to the Planck point).
• The basic mathematical structure of canonical QM, and its relation to measurements of physical observables, must be preserved. This implies that, of the four postulates [7] of the canonical theory, only Postulate 4, which states that the time-evolution of the quantum state |ψ is given by the Schrödinger equation (2.4), must be revised.
• In particular, the time-evolution given by the new EOM, corresponding to the modified dispersion relation, must be unitary.
The first criteria implies that dependence on G and c should drop out of the modified dispersion relation when m is small, whereas should drop out when m is large, relative to the Planck mass. As we shall see in Sec. 4, this requires "extending" the notion of wave-particle duality into the mass range in which the canonical relations (2.1) break down, namely, the black hole region of the mass-radius diagram. We also note that, though modified dispersion relations necessarily imply modified EOM, this is simply equivalent to modified expressions for the Hamiltonian and momentum operators. Specifically, the Hilbert space structure of the theory and, hence, its probabilistic interpretation, are unaffected by this change, as long as the time-evolution of the state vector |ψ remains unitary.

Extended de Broglie relations
The Planck mass and length scales are obtained via dimensional analysis using the fundamental constants G, c and : (Strictly, these are the reduced Planck scales, but we will refer to them simply as the Planck scales from here on.) l P is believed to be the shortest resolvable distance due to quantum gravity effects, corresponding to irremovable quantum fluctuations in the metric [24]. It is therefore unclear what (if any) meaning can be attributed to de Broglie waves with λ l P . In fact, the non-relativistic energy-momentum relation (2.2) implies that the angular frequency and wave number of the de Broglie waves reach the Planck values where t P = l P /c is the Planck time, for free particles with energy, momentum and mass given by E = pc = 2πm P c 2 and m = πm P , respectively. Since a further increase in energy would imply a de Broglie wavelength smaller than the Planck length, it is unclear how quantum particles behave for E m P c 2 . However, ignoring numerical factors of order unity, both m P and l P also admit intuitive physical interpretations as the mass and radius, respectively, of an object that is simultaneously a particle and a black hole. In other words, for a "particle" of mass m ≈ m P , the standard formulae for λ C and r S give λ C ≈ r S ≈ l P . We note that this involves extrapolating the standard results of relativistic (non-gravitational) quantum theory and relativistic (non-quantum) gravity to their extreme limit. In the standard scenario, a log-log plot of mass vs radius -hereafter referred to simply as the (M, R) diagram -is separated into two disjoint halves, with the Compton radius of quantum-relativistic (non-gravitational) particles on the left (m m P ) and the Schwarzschild radius of relativistic-gravitational (non-quantum) black holes on the right (m m P ). In this plot, the two lines are symmetric under reflection in the line m = m P (where m P ≈ m P ), which corresponds to the transformation m ↔ m 2 P /m. (This symmetry is discussed further in Sec. 4.2.) But, since both the standard formulae for λ C and r S may be recovered in the semi-Newtonian approximation, this raises the intriguing possibility that a modified form of canonical QM, based on a dispersion relation involving G, c and , could yield a unified description of particles and black holes that unites λ C and r S into a single line. In this scenario, "particles" with E m P c 2 become black holes, and the modified dispersion relation is required to prevent λ l P in this region of the (M, R) diagram.
Though it may be argued that the Newtonian formula is not valid close to the Planck scales, due to both relativistic and gravitational effects, this is not necessarily the case. In nongravitational theories, relativistic effects are important for particles whose kinetic energy higher is than their rest mass energy, E kinetic mc 2 . However, a particle (i.e. a small, spherically symmetric body) can have Planck scale energy if it has Planck scale rest mass, even if it is moving non-relativistically. In the following analysis, we consider the rest frame of quantum particles with rest masses extending into the regime m m P , for which the the standard non-relativistic analysis is expected to hold, except for modifications induced by gravity (rather than relativistic velocities). This is equivalent to applying the semi-Newtonian approximation on both the left-hand and right-hand sides of the (M, R) diagram. Figure 1 shows the Compton and Schwarzschild lines -here denoted λ C and λ S for notational consistency -as asymptotes in the m m P and m m P regimes, respectively. The line λ C/S represents a possible interpolation between the two regions, in which λ C and λ S are unified into a single curve. Since the Compton wavelength may also be "derived" from the HUP in canonical QM by applying the semi-Newtonian approximation, as discussed in Sec. 3.4, a unification of this form is known as the black hole uncertainty principle (BHUP) correspondence [29,30], as well as the Comtpon-Schwarzschild correspondence [1]. Crucially, we again note that any wouldbe unified description of particles and black holes must account for the change in the physical nature of the radius λ C/S at m ≈ m P , from minimum to maximum spatial extent of the wave packet. This is depicted visually in Fig. 2. In the language of semi-Newtonian QM, the shaded region on the left-hand side of Fig. 2 is associated with the "≥" inequality from the HUP. It is therefore reasonable to expect that the shaded region on the right should be associated with the inequality "≤" in a modified uncertainty relation, giving rise to a different kind of positional uncertainty for black holes. The minimum of the curve λ C/S is then associated with equality "=" in which the modified Compton and Schwarzschild radii are equal. This state is unique, with (∆ ψ x) min = (∆ ψ x) max ≈ l P . (Both Fig. 1 and Fig. 2 are taken from [1].) Finally, we note that, in the semi-Newtonian picture, the existence of a minimum radius for the wave packet (∆ ψ x) min for m m P implies a UV cut-off for k in the usual Fourier expansion of |ψ . Likewise, the existence of a maximum radius (∆ ψ x) max for m m P implies an IR cut-off in k for the wave functions black holes. (That these cut-offs are not fundamental, but instead mark the point at which the semi-Newtonian approximation breaks down, and relativistic effects must be more fully accounted for, need not concern us.) Therefore, if a unified description can be based on a modified quantum dispersion relation, we expect such limits to arise naturally from the relations themselves.

de Broglie relations for black holes -the limit E m P c 2
An arbitrary generalization of the usual (one-dimensional) de Broglie relations may be written as where Ω(ω) and κ(k) are arbitrary functions of the angular frequency and wave number, respectively. (For the sake of simplicity, we restrict ourselves to one-dimension, which may also be interpreted as an analysis of spherically symmetric systems.) Let us now suppose that, in the limit E m P c 2 , the generalized de Broglie relations (4.3) take the form Assuming that the momentum operator eigenfunctions take the usual form (2.6), the EOM for the quantum state is of Schrödinger type: which corresponds to modified Hamilton and momentum operators,Ĥ andp . The differential part ofp takes the standard form, but the multiplying factor differs from the canonical one; the first corresponds to the functional form of the dispersion relation, while the second sets the phenomenologically important length scale for the m m P regime. We note that this is proportional to m and is of the same order of magnitude as λ S , whereas the canonical de Broglie relations yield a natural length scale proportional to 1/m, of the order of λ C . Assuming that the position operator may be defined as usual, we havê so that the commutator is The proposed asymptotic form of the extended de Broglie relations (4.4) disturbs the mathematical structure of canonical QM only so far as the momentum operator is multiplied by a The physical nature of the radius λ C/S changes dramatically at the minimum close to m = m P . Particles are defined by the existence of a minimum radius; attempts to compress the width of the wave packet beyond this result in pair-production, rather than further spatial localization. Black holes are defined by the existence of a maximum radius; within this, the wave packet associated with the central black hole mass is "contained", indicating the causal disconnect between the black hole's interior and its exterior surroundings [1]. (Nonetheless, in principle, this picture remains consistent with the existence of Hawking radiation, which may be interpreted as the result of QM tunneling through an effective potential boundary, located in the region of the classical black hole horizon.) constant factor. This modifies the Hamiltonian and momentum operators (and functions of these), together with the commutation relations, but does not affect the underlying Hilbert space structure of the theory. Postulate 4 is changed, but only trivially [7]. The underlying mathematical formalism is the same as in canonical QM, so that the new theory is well defined in the limit E m P c 2 . The physical motivation for suggesting the asymptotic form (4.4) is the natural emergence of the Schwarzschild radius as a phenomenologically significant length scale. The modified uncertainty relation gives For m m P , we use (2.18), together with the semi-Newtonian approximation, to make the identifications (2.23). By contrast, using (4.9), together with the semi-Newtonian approximation for m m P , gives

de Broglie relations for all energies
We now propose a physically viable ansatz for the theory of extended de Broglie relations, which is able to provide a unified description of particles and back holes in the semi-Newtonian approximation. This is intended as a toy model, since deviations from canonical QM behaviour due to gravitational effects have yet to be detected experimentally [18,19], and current observations offer no clue regarding the precise mathematical form of the quantum dispersion relation close to the Planck point. In principle, any curve λ C/S that asymptotes to both λ C and λ S in the appropriate regimes remains phenomenologically viable at the present time.
In this section, we show that, for de Broglie relations that hold for all energies, and take appropriate asymptotic forms for E m P c 2 and E m P c 2 , the quantum EOM is not, in general, of Schrödinger type. Deviations from Schrödinger-type evolution are most pronounced for m ≈ m P , though the EOM simplify to (2.4) and (4.6) in the small and large mass limits, respectively. Nonetheless, both unitarity and the Hilbert space structure of the canonical theory are preserved throughout the entire mass range. Once again, only Postulate 4 of [7] must be amended, this time less trivially, while the mathematical structure embodied in Postulates 1, 2 and 3 is unchanged.
The "simplest" form of the functions Ω(ω) and κ(k) in Eq. (4.3), able to satisfy the physical requirements outlined in Sec. 3.4, are: Though "simplicity" remains a subjective judgement, here we take it to mean that the new functions contain only terms in ω and ω −1 or k and k −1 , in the m m P limit, reflecting the m ↔ 1/m symmetry of the (M, R) diagram, with only the minimum number of additional free parameters -in this case, the single numerical constant β > 0. We note that the continuity of E, p, dE/dω and dp/dk, at ω = ω P , k = k P , implies β = 1/4. However, since we require continuity of all physical observables at m ≈ m P , and β must be fixed to ensure this, we leave it as a free parameter for now.
For m m P , combining Eqs. (4.11)-(4.12) with (2.3), gives which reduces to ω ≈ ( /2m)k 2 for ω ω P and k k P , as required. In general, however, (4.13) may be solved to give two solution branches, (4.14) The reality of both branches requires 15) and the inequality is saturated for The reality of these limits then implies m ≤ m P ≡ (π/2)m P . (4.17) The inequality (4.15) is satisfied for two disjoint ranges: Defining k ± (m) = 2π/λ ∓ (m), the lower limit on the value of the wavenumber k − (m) corresponds to an upper limit on the wavelength λ + (m) while the upper limit k + (m) corresponds to a lower limit λ − (m), so that (4.18) is equivalent to For m m P , Eq. (4.16) can be expanded to first order, giving where k S ≡ 2π/λ S , which is equivalent to We note that the first range of wavelengths given by Eqs. (4.18)-(4.19) is compatible with the existence of an "outer" radius, which acts as a minimum obervable width for the particle, whereas the second range is compatible with the existence of an "inner" radius, within which sub-Planckian de Broglie modes become trapped, but which remains unobservable. Though it is unclear whether this range is physically meaningful, we note that, formally extending the (M, R) diagram to R < l P implies λ C > l P and λ S < l P for m m P . In this region, λ S acts like an (inner) unobservable radius, which is disjoint from the (outer) observable radius, λ C . Interestingly, since ∆ ψ x λ C ≥ λ + (m), Eq. (4.21) gives rise to a minimum length uncertainty relation (MLUR) closely resembling the one originally derived, using heuristic arguments, by Salecker and Wigner [25] (see also [26] for recent developments) and later considered by Ng and Vam Dam [27]: (∆x) min ≈ √ λ C d, where d is the distance "probed" using a QM measuring device [28]. For d ≥ l P , the predictions of the extended de Broglie theory coincide with this relation. However, note that, here, we use the notation ∆x, rather than ∆ ψ x, to indicate that the "uncertainty" obtained in [25] differs from the canonical definition given in Eq. (2.16). In summary, for m m P , the extended de Broglie theory implies (∆ ψ x) min ≈ λ C and (∆x) min ≈ λ + (m) ≈ √ λ C l P , where (∆ ψ x) min and (∆x) min differ as described in [25,26,27,28]. Again, two discontinuous wavelength ranges are permitted, according to Eq. (4.19), but the new limits are given by These are equivalent to those given in Eq. (4.21) under the interchange λ C ↔ λ S , up to numerical factors of order unity. This is compatible with the existence of an observable outer radius λ S > l P and an unobservable inner radius λ C < l P . From Eqs. (4.17) and (4.23), we see that β = 1/4 is required to ensure the continuity of physical quantities at close to the Planck point. We then have where m P is defined in Eq. (4.23), giving ω = ω P , k = k P and E = pc = 2m P c 2 for m = m P . The continuity of k 2 ± (m) at k P and ω ± (k, m) at ω P is ensured and the reality conditions justify our initial assumptions about the division between m m P and m m P . Note that the original, approximate, conditions given in Eq. (4.11) have now been replaced by the more precise expressions m ≤ m P and m ≥ m P in Eq. (4.25).
The solutions obtained above exhibit various dualities: Each branch of the quantum dispersion relation for particles (now defined as spherically symmetric objects with rest masses m ≤ m P ) maps to its equivalent for black holes (with rest masses m ≥ m P ), under This is equivalent to a reflection about the line m = m P in the log-log plot of the (ω(k : m), m) plane, at fixed k. For fixed m, the self-duality maps the upper and lower branches of the solution ω ± (k : m) into one another in the (ω(k : m), k) plane, and transforms the upper and lower limits on the wave number into one another.
Using the standard definitions of λ C and λ S , Eq. (4.27) also induces the transformation k C ↔ (π/8)(k 2 P /k C ) = (π/4)k S , which is equivalent to λ S ↔ (π/4)λ C . However, since λ C gives the order of magnitude length scale at which pair production rates become significant, the exact numerical factor used to define it is to some degree arbitrary, whereas the definition of λ S comes from an exact solution of the EFEs. We are therefore free to redefine λ C , such that The new definition gives so that the duality transformation (4.27) induces The new definition (4.30) also ensures λ C = λ S = l P at m = m P , so that we may directly associate the divide between m ≤ m P and m ≥ m P in Eqs.
where we choose k S for m ≤ m P and k C for m ≥ m P . For weakly gravitating particles, m m P and |k| ≤ √ k C k P k P √ k S k P , whereas, for black holes, m m P and |k| ≤ √ To summarize: Formally, there exist two inequivalent dispersion relations, in each mass range m ≤ m P and m ≥ m P , corresponding to the separate branches ω ± (k : m), though the physical interpretation of the ω + (k : m) branch is unclear, as this corresponds to de Broglie waves with sub-Planckian wavelengths. The super-Planckian branch ω − (k : m) depends on both k and m, as in canonical QM, but, in the modified theory, there exist limiting values of k, which are also functions of the rest mass. This may be contrasted with the canonical non-relativistic theory, in which all modes k ∈ (−∞, ∞) may contribute, with some nonzero amplitude, to a given wave packet expansion.
All four solution branches, ω ± (k : m) for both m ≤ m P and m ≥ m P , are plotted in Fig.  3. However, due to the duality (4.27), we have that ω particle ± (k : m) = ω BH ± (k : m 2 P /m), and the curves corresponding to particles with m < m P are overlaid by the curves corresponding to black holes with masses m 2 P /m > m P . Each curve in the first set, labelled by the mass m, is overlaid by a curve in the second set, labelled by m 2 P /m, and each quadrant contains both "particle" and "black hole" solutions. The lower-left, lower-right, upper-left and upper-right quadrants corresponds to the four independent regimes, ω − ≤ ω P , k ≤ k P ; ω − ≤ ω P , k ≥ k P ; ω + ≥ ω P , k ≤ k P and ω + ≥ ω P , k ≥ k P , respectively. Therefore, only the lower left-hand quadrant is definitely physical. It describes both quantum particles and quantum black holes with super-Planckian radii. The canonical QM dispersion relation, ω = ( /2m)k 2 , corresponds to the asymptotic regime in the bottom left-hand corner of the diagram.
If the upper half-plane of Fig 3. is regarded as physical, the upper right-hand quadrant gives the dispersion relation for "sub-Planckian" black holes -that is, black holes with λ S < l P , m < m P , conjectured to exist in LQG [31] -or, equivalently, the dispersion relation for "sub-Planckian" particles -that is, particles with λ C < l P , m > m P . If the latter exist, they may correspond to the point-like matter distributions at the centre of normal (super-Planckian) black holes, thereby preventing the formation of classical singularities. The upper left-hand and lower right-hand quadrants correspond to mixed regimes, where objects are associated with either sub-Planckian time periods and super-Planckian wavelengths, or vice-versa. We note that all four solution branches "touch" in the critical case, m = m P , ω = ω P , k = k P , which corresponds to a unique quantum state in the semi-Newtonian picture. The limits k ± (m) are shown in

Operators and EOM for the modified theory
In this section, we determine the EOM for the quantum system, implied by the extended de Broglie relations proposed in Sec. 4, and the corresponding Hamiltonian and momentum operators of the modified theory.

Basic definitions
For m ≤ m P , Eqs. (4.25)-(4.26) suggest the following definitions for the Hamiltonian and momentum operators, and the quantum EOM: Equation (5.1) is obtained by substituting the standard definitions of the "wave number operator" and "angular frequency operator" which yieldωφ = ωφ,kφ = kφ, where φ(x, t) = e i(kx−ωt) , into the modified de Broglie relations. Though the meaning of the operators inside the square brackets is unclear, we note that they may be defined as Taylor series by analogy with standard algebraic quantities, giving Strictly, Eqs. (5.3)-(5.4) are valid only when applied to wave packets composed of plane-wave modes with ω < ω P and k < k P , since and these series converge for k/k P < 1, ω/ω P < 1, respectively. In the ω ω P and k k P regime, the higher order terms are subdominant and we obtain the standard Schrödinger equation. However, for ω ≈ ω P and k ≈ k P , which necessarily applies for any particle with rest mass m ≈ m P , higher order corrections become significant. This is an important point. Even in the canonical QM, we are not free to consider a quantum state with ω ≈ ω P and k ≈ k P for arbitrary m, since these values necessarily imply E ≈ 2πm P c 2 , m ≈ πm P , according to the standard dispersion relation (2.3). Similarly, in the extended theory, the limit m → m P implies ω → ω P , k → k P and vice-versa. The point (ω P , k P ) is inaccessible for particles with m = m P , due to the existence of the limiting values k ± (m). As stated in Sec. 4.2, systems with mass m P , be they interpreted as particles or black holes, are unique in this prescription. Alternatively, they may be interpreted as black hole relics [32] formed at the end of Hawking evaporation [33,34]. If they exist, such relics represent unique quantum and gravitational states, in which the Schwarzschild and Compton radii coincide.
For m ≥ m P , the quantum EOM may be written aŝ whereĤ andp denote redefined Hamiltonian and momentum operators, that do not reduce to canonical form for ω ω P , k k P . Instead, in this limit, Eq. (5.7) reduces tô This is equivalent to (4.6), with β = 1/4, as expected.

Unitary evolution of self-gravitating states
As both (5.1) and (5.7) contain higher order time derivatives, the issue of unitarity arises. We now demonstrate, explicitly, that the time evolution implied by the extended de Broglie relations The time evolution of a single momentum eigenstate, φ(x, 0) = e ikx , is therefore given by the unitary operatorÛ whereĤ(x)e ikx = E k e ikx and E k ≡ E ω(k) = ω(k). This ensures that the first de Broglie relation, E = ω, holds for each individual eigenfunction φ(x, t) = e i(kx−ω(k)t) , corresponding to the momentum eigenvalue k, but the form of ω(k) cannot be determined without specifying the Hamiltonian. For general wave packets, and it follows from the definition of a function of an operator [7] that the time evolution of a general wave packet, ψ(x, 0) = ∞ −∞ a(k)e ikx dk, is given bŷ The canonical Hamiltonian for a free particle isĤ(x) = − 2 /(2m)(∂ 2 /∂x 2 ). This ensures that the second de Broglie relation, p = k, holds in conjunction with the non-relativistic energymomentum relation (2.2), giving the canonical dispersion relation (2.3). We now consider the time evolution operator implied by Eq. (5.1), which we first rewrite as whereĤ This implies the following time evolution operator, for the single momentum eigenstate φ(x, 0) = e ikx , corresponding to the ω − (k : m) solution branch: Note that Eq. (5.16) holds for any Hamiltonian yieldingĤ(x)e ikx = E ω(k) e ikx , not just the one given in (5.15). If, in addition, we invoke the definition of the Hamiltonian given by Eq. (5.15), we obtain the modified dispersion relation (4.14).
However, in the modified theory, a subtlety arises when dealing with wave packets, since the integral over dk in Eq. (5.11) is not well defined everywhere in the range k ∈ (−∞, ∞), due to the existence of the limits k ± (m). We therefore replace (5.11) with ψ(x, t) = Σ a(k)e i(kx−ω(k)t) dk , (5.17) where Σ ⊂ R is the appropriate range for the quadrant considered. For example, for wave packets governed by Eq. (5.14), the integration must be performed over Σ where k − (m) is given by Eq. (4.16). Substituting (5.17) into (5.14) gives Again using the definition of a function of an operator [7], the time evolution of a general wave packet, ψ(x, 0) = Σ a(k)e ikx dk, iŝ For clarity, we have relabelled the Hamiltonian (5.15), which is valid for the negative solution branch, ω − (k : m), for m ≤ m P , asĤ − (x). Thus, the evolution is non-canonical but unitary.
The operator (5.19) gives the time evolution of a fundamental, self-gravitating, quantum mechanical particle. Using Eqs. (5.15) and (5.3), we see that, if E k (1/2) ω P , which is equivalent to taking the limit m m P , we have ω − (k : m) ≈ E k / ≈ k 2 /(2m). Thus, Eq. (5.16) reduces to the standard time evolution for a single eigenstate (5.10). When this conditions holds for all k ∈ [−k − (m), k − (m)], Eq. (5.19) gives the standard time evolution for a wave packet (5.13). In this case, the wave packet expansion (5.17) also reduces to the standard form (5.11), since |k − (m)| → ∞ for m/m P → 0. In other words, for m m P , corrections due to gravitational effects become negligible and the extended de Broglie theory obeys the time evolution and expansion theorems of canonical QM. For m ≥ m P , an analogous argument implies that the time-evolution operator iŝ whereĤ − (x) denotes the (redefined) Hamiltonian which is valid for the negative solution branch, ω − (k : m), for m ≥ m P . This is defined in Eq. (5.7) and is simply the dual of (5.15) under the transformation (4.27).
The following symmetry exists between the time evolution operators particles (5.19) and black holes (5.20): In the limit we have k + (m P ) = k − (m P ) = k P , so that This is the unique (initial) momentum eigenstate for a particle with mass m = m P in the extended de Broglie theory. In this limit, the Hamiltonians and time evolution operators for the m ≤ m P and m ≥ m P sectors converge, yieldinĝ 6 Implications for the Hawking temperature The Hawking temperature [33,34] for black holes may also be obtained heuristically in the semi-Newtonian approximation of canonical QM. Assuming an upper limit for ∆ ψ x, associated with the Schwarzschild radius, we obtain a corresponding lower limit on ∆ ψ p via the HUP (2.18), giving (∆ ψ p) min may be identified with the momentum uncertainty of a particle emitted during Hawking radiation [29,30], and the associated temperature T H is defined via where T P = m P c 2 /k B is the Planck temperature and χ is a constant. Agreement with the Hawking temperature requires χ = 2π, so that In this scenario, we note that, since T H is associated with a lower limit on the momentum uncertainty, it represents the minimum temperature that can be associated with the mass m of the black hole. In other words, were an observer to localise m on some scale ∆ ψ x < λ S , for example, by crossing the event horizon, we would expect the temperature associated with m, in their frame, to be greater than T H . As shown in Sec. 2.2, we may also obtain the standard expression for the Compton wavelength (up to numerical factors of order unity) by associating this with the lower limit on the size of the wave packet (∆ ψ x) min . The corresponding upper limit on the momentum uncertainty (∆ ψ p) max is associated with the particle's rest mass (2.23). This defines the Compton line on the (M, R) diagram, and the numerical factor may be chosen to ensure that the intersect with the Schwarzschild line occurs at m = m P (4.30). This allows us to associate the two halves of the diagram with the extended de Broglie relations for particles and black holes, respectively, given in Eqs. (4.25)-(4.26).
We then define the "Compton temperature" as where setting χ = 2π ensures that T C = T H = (2π) −1 T P at m = m P . This may also be regarded as the natural temperature associated with the rest mass of the particle. By our previous logic, since T C ∝ (∆ ψ p) max ≈ mc is associated with the upper limit on the momentum uncertainty, it represents the maximum temperature that can be associated with the particle mass m. This matches our intuition, since particles with real temperatures T T C , corresponding to wave packets with ∆ ψ x λ C , have sufficient kinetic energy to pair produce. Additional increases in the total energy of the system then result in pair production rather than increased temperature. Conversely, wave packets with ∆ ψ x λ C are naturally associated with temperatures T T C , which correspond to kinetic energy uncertainties ∆E mc 2 .
T C and T H are plotted as red and blue lines, respectively, in Fig. 5, which is also taken from [1]. The green curve T C/H represents a smooth interpolation between the two, which is associated with a unified Compton-Schwarzschild line, λ C/S , via T C/H ∝ (∆ ψ p) max/min ∝ /λ C/S , by analogy with the semi-Newtonian "derivations" of T C and T H in the asymptotic regions, given above. Just as the physical nature of the radius changes at the critical mass, m = m P , as illustrated explicitly in Fig. 2 Although ∆ ψ x and ∆ ψ p x do not refer to any unavoidable "noise" , "error" or "disturbance" introduced to the system by the act of measurement, it is well known that one can understand this result heuristically as reflecting the momentum transferred to the particle by a probing photon [3]. Hence, in order to distinguish between quantities representing genuine noise, induced by the measurement process, and the standard deviations of repeated perfect, projective, Von Neumanntype measurements, which do not disturb the state |ψ prior to wave function collapse [7], we use the notation ∆O for the former and ∆ ψ O for the latter. (Strictly speaking, any disturbance to the state of the system caused by an act of measurement may also be |ψ -dependent, but we adopt Heisenberg's original notation, in which the state-dependent nature of the disturbance is not explicit.) In this notation, the formulation of the standard uncertainty principle based on the "Heisenberg microscope" thought experiment may be written as ∆x∆p . (7.1) We note that such a statement must be viewed as a postulate with no rigorous foundation in the underlying mathematical structure of quantum theory. Indeed, as a postulate, it has recently shown to be manifestly false, both theoretically [35,36] and experimentally [37,38,39,40]. However, the heuristic "derivation" of Eq. (7.1) may be found in many older texts, alongside the more rigorous derivation of Eq. (2.16) from basic mathematical principles. Unfortunately, it is not always made clear that the quantities involved in each expression are different, as clarified by the recent pioneering work of Ozawa [35,36]. An excellent discussion regarding the various possible meanings and (often confused) interpretations of symbols like "∆x" is given in [41]. The clarifications given above are of key importance when discussing quantum phenomenology based on the Generalised Uncertainty Principle (GUP). This term refers, generically, to any extension of the the standard HUP (7.1), whether based on fundamental modifications of the mathematical formalism of canonical QM, or simply on heuristic results. It must not be confused with the term "general uncertainty principle" used to describe Eq. (2.16), though the terminology adopted in different parts of the literature is confusing [7].
Many GUP proposals are motivated by attempts to incorporate gravitational effects into existing interpretations of quantum uncertainty. Many also give rise to a minimum length, interpreted as a quantum gravitational effect, and are known as minimum length uncertainty relations (MLURs). (For recent reviews of GUP phenomenology, see [42,43]; for reviews of minimum length scenarios in quantum gravity, see [28,44].) One of the earliest and most interesting examples of a quantum gravity inspired GUP was proposed by Adler and Santiago [45], where α is a constant of order l 2 P / ∼ G/c 3 . This is based on an extension of the Heisenberg microscope thought experiment, incorporating the effect of the gravitational interaction between the particle and the photon probe, which gives rise to the additional term on the right-hand side. A GUP of this form was originally proposed in the context of string theory [46], as it implies the existence of a minimum length, (∆x) min ≈ l P + α /l P ≈ l P , which may be identified with the fundamental string scale. From (7.2), it is clear that using the standard identification for the momentum uncertainty ∆p → mc implies ∆x → λ C , where λ C represents a modified Compton wavelength of the form Thus, for m m P , the first (Compton) term dominates, whereas, for m m P , the second (Schwarzschild) term gives the leading order contribution to the total uncertainty. In the this way, a GUP of the form (7.2) may enable a unified description of fundamental particles and black holes based on a modified quantum theory. A GUP-based unification of this this kind, suggested in [29], is termed the black hole uncertainty principle (BHUP) correspondence. However, several theoretical and conceptual issues arise in the context of such a proposal, which we now address.
First, if we wish to give rigorous mathematical definitions of the terms ∆x and ∆p appearing in Eq. (7.2) (i.e., to "promote" them to quantities analogous to ∆ ψ x and ∆ ψ p, which follow directly from the mathematical formalism of the underlying quantum theory (2.16)), it is clear that we must modify either the Hilbert space structure of canonical QM and/or the commutator [x,p] = i . The former is highly non-trivial, while the latter is equivalent to leaving the state space structure unchanged but modifying the dispersion relations and the EOM for the state vector. This, in turn, may be achieved in several different ways: (i) by maintaining the standard de Broglie relations but modifying the classical energy-momentum relation, (ii) by maintaining the classical energy-momentum relation but modifying the de Broglie relations, and (iii) by modifying both. One approach, based on (ii), gives rise to the modified commutator [47] [x,p] ≈ i 1 + αp 2 , (7.4) which corresponds to the individual operatorŝ (7.5) Substituting (7.4) into (2.16) and setting p ≈ 0, so that ∆ ψ p ≈ p 2 , yields a GUP of the form which is obviously equivalently to (7.2), up to numerical factors of order unity, but which may be derived from first principles. Crucially, the approximation p ≈ 0 is valid for spherically symmetric systems, in which it is also reasonable to make the identification ∆ ψ p ≈ mc. (In fact, it may be argued that identifying the momentum uncertainty with the rest mass is valid only in the rest frame of the system, under conditions of spherical symmetry.) Hence, the modified commutator (7.4) is potentially capable of yielding a unified Compton-Schwarzschild line of the form (7.3) under the identification ∆ ψ p ≈ mc, but, for reasons we now address, such an identification is not possible for arbitrary m.
In [47], the modified dispersion relations giving rise to Eqs. (7.4)-(7.6) are where the approximations on the right-hand sides of Eqs. (7.7) are valid for p m P c and E m P c 2 , respectively. If these hold for every de Broglie mode in a single spherically symmetric wave packet, then ∆ ψ p ≈ mc m P c. Hence, this identification is incapable of providing a unified description of particles and black holes, as it does not allow for the extension of the modified Compton wavelength λ C (7.3) into the right-hand side of the (M, R) diagram.
However, other considerations suggest an alternative identification between ∆ ψ p and the rest mass of a spherically symmetric system for m m P . Consider a black hole decaying via Hawking radiation: The average magnitude of the momentum of a particle emitted from a black hole of mass m BH is p 2 particle ≈ (m 2 P /m BH )c ≡ m particle c, where m particle is the effective particle mass (even if the particle is a photon). Therefore, (∆ ψ p) particle ≈ (m 2 P /m BH )c is the total momentum uncertainty; this may also be seen by associating the positional uncertainty of the emitted particle with the black hole radius, (∆ ψ x) particle ≈ Gm BH /c 2 , in the standard HUP, or in the leading order term of the GUP (7.2) for particles with m particle m P . Since momentum conservation implies that the recoil of the black hole, due to a single emission, must be equal in magnitude (but opposite in sign) to the momentum of the outgoing particle, it follows that (∆ ψ p) particle = (∆ ψ p) BH ≈ (m 2 P /m BH )c. Thus, for general spherically symmetric systems of mass m -subject to the HUP or a GUP of the form (7.2) -we may associate ∆ ψ p ≈ mc , (m m P ) (m 2 P /m)c , (m m P ) .

(7.8)
An interesting feature of the GUP proposed by Adler and Santiago (7.2) is that it is invariant under the transformation ∆ ψ p → m P c 2 /∆ ψ p, so that the change in how ∆ ψ p is associated with the rest mass of the system, occurring at m ≈ m P , still enables the construction of a unified Compton-Schwarzschild line of the form (7.3). We also note that the modified commutator and dispersion relations proposed in [47] do not alter the fundamental Newtonian nature of space and time (subject to the cosmic speed limit v max = c), since they leave the fundamental commutator between thex andk operators unchanged, What has changed is, instead, is the the intrinsic relation between p and k, i.e. the functional form of p(k). Thus, in this case, the generators of infitesimal translations in the Gallilean symmetry group may still be identified with thek i operators; translation invariance gives rise to conserved Noether charges for classical systems, the components of the classical momentum p i , and to a set of nontrivial commutators (7.9) for quantum systems. However, the hermitian operatorsp i are no longer directly proportional to the de Broglie wave number operatorsk i , due to the more complex form of the modified de Broglie relations (7.9). As with the extended de Broglie relations presented in Secs. 4-6, these remain the essence of the non-trivial modifications to the quantum sector. (Similar arguments apply regarding time translational symmetry, the frequency operatorω = i(∂/∂t), and the classical energy E, though subject to the caveat that time t is parameter, not an operator, in both canonical QM and the modified theories presented here.) Hence, considering the GUP, together with momentum conservation arguments that give rise to the approximate identifications (7.8) in the two mass regimes, is phenomenologically equivalent to using the HUP together with the associations ∆ ψ x ≈ l P m P m + m 2 P /m , ∆ ψ p ≈ m 2 P c m + m 2 P /m , (7.11) which are assumed to be valid for all m. This makes sense, intuitively, since it relates the positional and momentum uncertainty of quantum-gravitational system to the ADM mass [31,48]. We also note that Eq. (7.11) gives rise to a unified Compton-Schwarzschild line that is (at least) qualitatively similar to the effective mass-dependence of λ C/S , introduced via the extended de Broglie theory given in Secs. 4-6. In the latter, however, the rest mass is directly associated with the minimum uncertainty of a modified momentum operator (∆ ψ p ) min ≈ mc (4.10). The arguments presented here suggest that this cannot be identified with the physical recoil of the black hole during the Hawking emission of a fundamental particle. Another crucial difference between the two approaches is that the modified de Broglie relations proposed in [47], Eqs. (7.7), predict an almost unique quantum state for all black holes, since k(p) → 1/l P for p m P c and ω(E) → c/l P for E m P c 2 . This is a direct result of the fundamental asymmetry between the form of the relations (7.7) for m m P and m m P . By contrast, the extended de Broglie theory presented in Secs. 4-6 explicitly incorporates the symmetry between fundamental particles and black holes present in the (M, R) diagram, via the extensions of the relations themselves. In this scenario, the unique quantum state φ(x : t) = exp[i(k P x − ω P t)] corresponds to the unique physical state for which Schwarzschild radius is equal to the Compton wavelength.
A related point concerns the fact that all forms of modified quantum mechanics proposed thus far in the literature -be they based directly on GUP phenomenology or on modified de Broglie relations -give rise to uncertainty relations of the form ∆ ψ x . . . , even when these are extended to systems with super-Planckian rest mass. This is the mathematical expression of the assumption that the radius of a black hole is, in some sense, physically equivalent to the radius of fundamental particle, i.e. that it may be considered as a minimum, rather than as a maximum limit on rest mass localisation. Were ψ to represent (in some limit) the wave function associated with the mass in the interior of a black hole, it may be argued that a modified quantum theory giving rise to a positional uncertainty of the form ∆ ψ x . . . is required. It would be interesting to consider how such a theory could be reconciled with the "horizon wave function" model, proposed by Casadio et al (see, for example [49,50,51,52]), as even an effective wave function model of a black hole may require both components.

Conclusions
We have shown that, by taking the semi-Newtonian approximation, in which space and time remain absolute but a cosmic speed limit v max = c is imposed "by hand", we can recover essential phenomenological features of both relativistic quantum theory and relativistic gravity from their non-relativistic counterparts. Applying this approximation to the basic mathematical structure of canonical QM yields the formula for the Compton wavelength, via the uncertainty principle, while applying it to Newtonian gravity yields the Schwarzschild radius, via the formula for the escape velocity. On a plot of mass versus radius, these lines meet at the Planck point, suggesting that the final theory of quantum gravity should yield a unified description of fundamental particles and black holes. In the absence of such a theory, we propose a naïve unification, based on recognition of the fact that both sets of objects may be adequately described in the semi-Newtonian regime.
Since the canonical QM dispersion relations break down for Planck mass objects, our new theory is based on modified de Broglie relations, which, when substituted into the classical energy-momentum relation, yield quantum dispersion relations that hold for systems of arbitrary mass. These, in turn, give rise to modified EOM, Hamiltonian, momentum and time-evolution operators, in both the particle and black hole sectors. In each sector, the time-evolution is noncanonical, but unitary, and the particle evolution reduces to canonical form in the asymptotic limit. The new dispersion relations depend on all three fundamental constants, G, c and , and their chosen form gives rise to a new mass-dependence in the phenomenologically significant length scale of the theory. This reduces to the Compton radius for extreme low-mass objects, but corresponds to the Schwarzschild radius in the opposite extreme. We therefore interpret the additional terms in the modified dispersion relations as representing the self-gravity of the quantum wave packet in the semi-Newtonian picture.
In addition, our work suggests a natural definition for the "Compton temperature" of a fundamental particle. This bears the same relation to the Compton wavelength as does the Hawking temperature of a black hole to its Schwarzschild radius, and may be interpreted as the temperature associated with the particle's rest mass. In the extended de Broglie theory, the two lines, plotted as functions of mass on a log-log plot, define asymptotes to a unified temperature curve, which interpolates between the particle and black hole regions. In this formulation, a Planck mass object is represented by a unique quantum state, whose de Broglie wavelength, Compton wavelength and Schwarzschild radius are equal to the Planck length, and whose temperature is equal to the Planck temperature.
To summarize: The pedagogical discussions in Secs. 2-3 aim to clarify the physical assumptions and mathematical foundations on which the extended de Broglie theory is based, while Secs. 4-6 consider its detailed predictions. The discussion in Sec. 7 sets the theory proposed in Secs. 4-6 in the context of the existing literature on modified quantum theories, which attempt to incorporate gravitational effects. Though we make no claims for the quantitative validity of this theory, originally proposed in [1], it is hoped that the considerations raised therein, and in the (expanded) discussion presented here, will help stimulate debate on the important open questions in black hole physics: "Which quantum theory must be reconciled with gravity? (And what does it mean for black holes?)".