1. Introduction
Modern cosmology started with Hubble’s discovery of the linear redshift–apparent magnitude relation for nearby galaxies. Soon after the discovery, it was interpreted as direct observational evidence for an expanding universe, meaning that it agrees with the expanding solution of Einstein’s equations (more specifically the Friedman equation). Although, at that stage, the general relativity (GR) was engaged to interpret the discovery. In fact, the symmetry, expressed by the Robertson–Walker (RW) metric (see, for example, [
1,
2]) and based on the assumptions of homogeneity and isotropy of the universe, is sufficient. It provides the interpretation of Hubble’s Law as a consequence of the RW symmetry for small redshifts illustrated by the linear region in the luminosity distance versus the redshift curve. The dynamics based on the GR equations, which are reduced to the Friedman equations under the assumption of a constant density, are needed for defining the expansion parameters, particularly cosmological acceleration.
The issue of acceleration emerged much more recently, being announced by Perlmutter, Riess and their colleagues [
3,
4] as the result of work using supernovae of Type Ia as standard candles. The Hubble law played a significant role in that work. The point is that SNe Ia are not really standard candles. If they all were of the same maximum luminosity, then they would be ideal for standard candles owing to their high luminosity, which allows them to be detected even at large distances. However, the SNe Ia maximum luminosity varies from object to object, as was revealed by the Hubble diagram for relatively nearby SNe Ia. Belief in validity of the Hubble law for nearby objects was a crucial point for the analysis, as it was presumed that, in the case of all SNe Ia having the same maximum luminosity, the data points in the diagram should be aligned along a straight line, as follows from the Hubble law. However, a scatter around the Hubble relation was significantly larger than the photometric measurement errors.
Two advancements allowed overcoming this challenge. First, Phillips [
5] found convincing evidence for a correlation between the light curve shape and the luminosity at maximum brightness. Namely, the slower the decline, the higher the absolute luminosity. Next, it was understood that the observed flux is possibly affected by extinction in the host galaxy, in addition to extinction in the Milky Way. The colors of SNe Ia provide a way to correct for extinction with dust in both our galaxy and the host. The combined analysis of these effects gives a possibility for deducing an empirical correction to the maximum luminosity, accounting for both the relation of the decline and width of the light curve to the observed luminosity and for the extinction. The Hubble diagram for nearby SNe Ia, plotted with the corrected data, was commonly used as a consistency test for a method of parametrization of the effects (e.g., [
6,
7,
8,
9,
10]). It was found that with a proper ‘standardization’ of the luminosity, the deviations from the Hubble law became dramatically smaller. As a result, SNe Ia indeed became standard candles, providing quite accurate relative distances.
All of the above shows that in the cosmic acceleration discovery, the validity of the Hubble law for cosmologically nearby objects played a significant role, providing both a crucial test and strong support for using the corrected SNe Ia observational data as relative distance indicators. The belief in the validity of the Hubble law for the objects at small redshifts z is usually justified by the luminosity distance versus the redshift z’s curve, obtained either as a kinematical consequence of the RW metric or as a solution to the Friedman equation of GR, being approximately linear in the small z part. However, it is important to remember that the assumptions of homogeneity and a uniform density underlying the Robertson–Walker–Friedman (RWF) cosmological model are supported by the observational evidence only after averaging the observed universe over scales that are many orders of magnitude larger than those on which the calibration of the SNe Ia data were implemented. The objects of our local universe are filtered out as a result of such averaging, and only then does the distant universe look approximately uniform or homogeneous. Observations of the distribution of galaxies in our local universe clearly show that the assumptions of homogeneity and a constant density become meaningless at those scales. Therefore, claiming the Hubble law to be the small z limit of the luminosity distance versus the redshift curve, obtained within the framework of the Robertson–Walker–Friedman (RWF) cosmology, is an inconsistent application of the model on scales where the assumptions, and thus the results, of the model are invalid. In a sense, this is similar to applying the continuum equations (Euler or Navier-–Stokes) to rarefied gas, where the molecular mean free path is not negligible.
Another widespread interpretation of the Hubble law, as an effect of expanding space, is somewhat related to the above discussion. This interpretation emerged soon after the Hubble 1929 discovery, when the Hubble observations were set within the framework of general relativity or, more precisely, the GR-based Robertson–Walker–Friedman cosmology. It is clear from the FRW form of the spacetime metric that for a fixed coordinate of time
t, the physical separation of objects depends on the size of the scale factor
, and the increase in
with
t results in the increasing separation of objects. This is typically taken to be the expansion of space. Usually, in textbooks, when the expanded space concept is introduced, space is represented as being defined by a network of comoving coordinates and analogies of stretching rubber sheets or a river, carrying matter along with it in its motion. As was formulated in [
11], ‘
According to the expanding space paradigm … the galaxies do not move through space, but instead float stationary in space. Their separating distances increase because the space between the galaxies expands’.
The concept of expanding space has been the subject of considerable debate, and explaining the increasing separation of galaxies with the expansion of space has recently been criticized from different points of view (e.g., [
11,
12,
13,
14,
15,
16]) as an idea which leads to confusion and misconceptions. J.A. Peacock [
13] stated that ‘
… the very idea that the motion of distant galaxies could affect local dynamics is profoundly anti-relativistic …’ A.B. Whiting [
12] claimed the following: ‘
The fact that space in GR has an active role in dynamics, however, does not mean it has the attributes of a physical object. It does not act like a viscous fluid, drawing all bodies into the Hubble flow, even asymptotically; it does not affect things by ‘expanding’, nor by accelerating this expansion’. S. Weinberg, in the course of discussing the Big Bang issue in [
17], answered the question:
Popular accounts, and even astronomers, talk about expanding space. But how is it possible for space, which is utterly empty, to expand? How can ‘nothing’ expand?
’Good question’, says Weinberg. ‘The answer is: space does not expand. Cosmologists sometimes talk about expanding space—but they should know better’.
It was found in [
18] that the concept of the expansion of space could acquire meaning only in the context of mathematics of general relativity from which it arose. In the FRW cosmological model, the dynamics of the expansion is defined by solving the GR field equations under the assumptions that a homogeneous universe is filled with a fluid of uniform density and that the test observers can measure their velocity with respect to that fluid. The privileged observers, whose watches are synchronized with cosmic time, are at rest with regard to the cosmic fluid, and the change in the metric with time via the scale factor implies that (in an expanding universe) the physical distance between any two privileged observers increases with time. Thus, only under the assumption of a homogeneous universe filled with a fluid of a uniform density does ‘the expansion of space’ acquire the meaning of an increase in the distances between privileged observers that are at rest with respect to that fluid. The same is stated in [
12]: ‘
In fact, if one looks at space itself apart from the associated fluid of cosmological matter, it is not at all certain what ‘the expansion of space’ means’. The concept of cosmic homogeneous fluid filling all the space, which is inherent in the RWF cosmological model, is evidently not valid on the scales of galaxies. This was concluded in [
18]: ‘
The expansion of space is global but not universal, since we know the FRW metric is only a large scale approximation’, and ‘
… we should not expect the global behaviour of a perfectly homogeneous and isotropic model to be applicable when these conditions are not even approximately met. The expansion of space fails to have a ‘meaningful local counterpart’.
Thus, validity of the linear Hubble law at cosmologically small scales cannot be proven within the framework of the standard model based on the global RWF spacetime. Nevertheless, the low-redshift SNe Ia data, corrected according their pick luminosity (e.g., [
7,
8,
9,
10]), provide the best evidence that the relation between the distance modulus and redshift of an object is linear. Thus, validity of the Hubble Law at cosmologically small scales should be admitted despite the fact that, at those scales, it cannot be explained with reference to the RWF-type models or by the expansion of space. This suggests that we have to accept the Hubble linear relation between the redshift of an extragalactic object and its distance as a physical reality which may be considered a law of nature and, as such, used as the basis for the theory.
The theory, based on the above statement, could be questioned on the grounds that gravity, which is a ubiquitous phenomenon, is not involved in the framework. We note in this respect that, in fact, the modern cosmology is built of two parts such that the primary part,
cosmography, does not involve any issues related to gravity but serves as a basis for the second part, which applies GR to the analysis of the observational data. Cosmography analyzes the observations based on the cosmological principle (Copernican principle), which implies validity of the assumptions of spatial homogeneity and isotropy and leads to the Robertson–Walker metric in that way. Then, astronomical observations can be interpreted as measurements of the scale factor
and the curvature constant
k. In particular, the RW metric can be used to derive the luminosity distance
versus the redshift
z relation as a power series:
where
is endowed with the meaning of the Hubble constant, and with the interpretation of the redshift as a recession velocity,
acquires the meaning of the ‘deceleration parameter’ of the cosmological expansion. The dynamics of the cosmological expansion is treated by applying the gravitational field equations of Einstein which, upon making some tentative assumptions about the constituents of the universe and their properties, allows one to relate the parameters of the expansion contained in Equation (
1) to the values of the cosmic energy density and pressure.
The above outlined framework of the large-scale cosmology was seriously challenged by the SNe Ia data which correspond to the deceleration parameter . (The expansion of the universe is accelerating.) This result contradicts the results of applying the matter-dominated cosmological model of the universe which yields the luminosity distance–redshift relation with the deceleration parameter , which is positive for all three possible values of the curvature parameter k. This stimulated an avalanche of explanations, with many involving speculative new physics. In the modern cosmology, represented by the standard CDM model, that challenge is resolved by introducing dark energy, a new component of the energy density with strongly negative pressure that makes the universe accelerate. The challenge caused by the SNe Ia data did not touch the cosmography part of the description of the large-scale universe since that part is not influenced by changes in the view on the constituents of the universe, modifications to the field equations or the introduction of alternative theories of gravity.
The approach adopted in the present study may be identified as the
small-scale cosmography since, like the large-scale cosmography, it does not refer to any physics in justifying the basic assumptions of the theory but nevertheless provides a theoretical framework for interpretation of observations. The meanings for the terms ‘large-scale’ and ‘small-scale’ are provided by the scales of validness of the basic assumptions of the theories. In the large-scale cosmology, it is the homogeneity scale, and in the small-scale cosmology, it is the scale in which the linear Hubble law is valid. Both scales cannot be precisely determined. In particular, the homogeneity scale ‘depends on the averaging procedure (see, for example, the discussons in [
19,
20,
21,
22]). A.A. Coley and G.F.R. Ellis in their review of theoretical cosmology [
23] remarked that ‘
… it would thus be better if the cosmological principle could be deduced rather than assumed a priori (i.e., could late time spatial homogeneity and isotropy be derived as a dynamical consequence of the Einstein field equations (EFE) under suitable physical conditions and for appropriate initial data)’. This statement of Colley and Ellis regarding the potential role of gravity in the large-scale cosmography is completely applicable to the discussion of the (potential) role of gravity in the present framework. If the Hubble law could be deduced from the GR equations as the solution of the many-body problem of interacting galaxies, then this would provide a physical background for the theory, but this is an intractable task.
When presenting a cosmological model, it is unavoidable to discuss the (potential) role in the theory of the two issues inherent to the modern cosmology: dark matter and dark energy. Starting with dark matter, we remark that, in fact, dark matter arises in two conceptually different contexts. The first one is related to cosmologicaly small scales, where dark matter is introduced to explain some gravitational effects that cannot be explained within the framework of general relativity unless more matter is present than can be seen. Such effects occur in the galaxy rotation curves, the motion of galaxies within galaxy clusters, gravitational lensing, mass position in galactic collisions and some other instances (see, for example, [
24,
25,
26]). Dark matter, as a substance whose presence is discerned from its gravitational attraction rather than its luminosity, is not known to interact with ordinary baryonic matter and radiation except through gravity, making it difficult to detect in a laboratory. The most prevalent explanations of its nature range from some (not-yet-discovered) particles, like weakly interacting massive particles (WIMPs) or axions, to primordial black holes (see, for example, [
27,
28,
29]).
While the hypothesis of dark matter in the above discussed context has an elaborate history, rising to ‘missing mass’ in galaxy clusters, as inferred by Fritz Zwicky in 1933, the concept of dark matter in the second context, related to large-scale cosmological models, arose only in the early 1990s after discovering the accelerated expansion of the universe. In that context, dark matter is one of the energy components in the stress tensor of the general relativity equation. In the standard model of cosmology, the dynamics of the expansion is governed by the general relativity equations that reduce to the fundamental Friedman equation, defining the time dependence of the scale factor
as follows (see, for example, [
2]):
where
G is Newton’s gravitational constant and
K is the curvature parameter. Applying this equation requires making assumptions about the constituents of the cosmic energy density
. It is assumed to be a mixture of non-relativistic matter, which means any constituent of the universe whose energy density scales with the inverse cube of the scale factor (i.e.,
), the relativistic matter (radiation), which scales as the inverse fourth power of the scale factor
, and dark energy (usually named the vacuum energy), which does not change with
a (i.e.,
), which is equivalent to introducing into Einstein’s equation a cosmological constant
. Thus,
is expressed as
where
The parameters
,
and
are defined by
where
,
and
are the present values of the densities and
is the critical energy density. The components of the energy density satisfy the following equation (a consequence of Equation (
2) evaluated at
):
It is found that the radiation density parameter is negligible compared with other values. The values of the parameters , and are defined by fitting the (luminocity distance – redshift) dependence retrieved from the SNIa observational data into that derived from the solutions to the Friedman equation. First of all, it is found that for (i.e., without introducing dark energy), fitting is impossible. In this case, the solutions of the Friedman equation correspond to decelerating expansion for any value of the curvature parameter. In the case of , the best fitting is achieved with , (The universe is flat, which is supported by other observations.) and . In this fitting, corresponds to any substance evolving with time as , particularly the ordinary, visible matter. The amount of visible matter in the universe can be estimated, and the estimation is that it constitutes only five percent of the mass–energy content, and the rest is ‘dark matter’. Thus, in this context, dark matter makes an appearance as a component of a cosmic fluid which, together with dark energy, uniformly fills the space in the large-scale averaged RWF model. It is evident that this component of the cosmic fluid of the large-scale CDM model should not be identified with the invisible gravitating substance introduced to make the small-scale astrophysical models consistent with general relativity. The density of dark matter as a component of cosmic fluid is tied to the density of dark energy by the requirement of fitting the SNIa data, and therefore it is not clear at all that the artificially introduced substance is of the same nature as the invisible matter in galaxies and clusters.
When discussing the relevance of dark matter to the ‘small-scale cosmology’ developed in the present paper, one should distinguish between the two contexts in which the concept is involved. Regarding the potential role of dark matter, as an invisible matter in galaxies and galaxy clusters, we can state again the following: if the Hubble law could be deduced from the GR equations as the solution of the many-body problem of interacting galaxies, then of course the input of invisible but gravitating matter should be accounted for. However, since this is impossible, dark matter in this context plays no role in the framework of the present cosmographycal model of a small-scale cosmology. Regarding the second large-scale context of dark matter’s emergence, we can repeat what was said above in the discussions of applicability of the results of the RWF model to small scales: the FR metric is only a large-scale approximation, and the basic assumptions of the RWF model, homogeneous and isotropic space and the uniform-density cosmic fluid filling it are not expected to be applicable when these conditions are not even approximately met.
Dark energy, distinct from dark matter, came to light only at the beginning of the 1990s as the dominant contribution to the energy content needed to provide fitting of the distance–redshift relation obtained from the RWF model to one retrieved from the SNIa observations. Later dark energy, as a (main) part of the conceptual framework of the standard CDM model of cosmology, had been used for interpretation of some other observational facts, particularly the flatness of the universe and large-scale wave patterns of mass density in the universe. The nature of dark energy remains a mystery, and explanations abound. The most popular explanation, vacuum energy, (The term ‘vacuum energy’ is commonly used as an equivalent of ‘dark energy’.) should be considered inappropriate because of the substantial disagreement between the observed values of the vacuum energy density and the much larger theoretical value of the zero-point energy suggested by quantum field theory. The ‘cosmological constant’, as a source term that can be added to Einstein field equations of general relativity, is commonly viewed as equivalent to ‘vacuum energy’. The cosmological constant interpretation does not resolve a huge disagreement between the values observed and deduced from quantum field theory for the vacuum energy density, and the problem appears in the literature under two names: the ‘cosmological constant problem’ or ’vacuum catastrophe’. It should also be mentioned that sometimes, dark energy is identified with a negative pressure field which could drive cosmic inflation in the extremely early universe. However, inflation must have occurred at a much higher (negative) energy density than in the dark energy we observe today, and thus it is doubtful that there exists any relation between dark energy and inflation.
It is evident from the above that dark energy is a concept inherent only to the large-scale RWF cosmological model in which, upon large-scale averaging, a homogeneous universe is filled with a fluid of a uniform density, with dark energy being one of the components. Nevertheless, there is a tendency to extend the concept to small scales, treating dark energy as a smooth, persistent component of invisible energy filling (otherwise empty) space and not accumulating preferentially in galaxies and clusters, and applying the
CDM model to explaining the processes on the scales of galaxies and clusters. Note that many observations on galaxy scales now seem to be in conflict with the
CDM paradigm, such as the overabundance of the predicted number of halo substructures, compared with the observed number of satellite galaxies and the discrepancy between the measured densities at the halflight radii of the brightest local dwarf galaxies and the (higher) densities of the most massive subhalos in
CDM simulations (see, for example, [
30,
31,
32,
33]). Curious discrepancies also appear to exist between the predicted clustering properties of CDM on small scales and observations (see, for example, [
34] and the references therein). However, independent of those issues, it should be stated that extending the notion of dark energy, related to the global large-scale dynamics of the universe, to small scales is conceptually inconsistent. Thus, dark energy is irrelevant to the small-scale cosmological model developed in the present paper.
In general, the CDM model has been proven to be explanatory and even predictive, providing us with substantial understanding of observations on large scales. Nevertheless, it is a heuristic theory, which explains the observational data without being able to provide a theoretical foundation for its basic assumptions. The nature of dark energy (treated either as vacuum energy or the cosmological constant) as well as the particle nature of dark matter are entirely mysterious. This and other unresolved serious theoretical issues motivate developing alternative theories, such as the modified gravity theories and the varying fundamental constant theories. Thus far, none of the proposed theories can successfully describe every piece of observational data, which are usually considered as supporting the CDM model, at the same time.
In this context, it is worthwhile to draw attention to ‘relativity with a preferred frame’ [
35], which provides the possibility of explaining the main body of the observational data, commonly mentioned in support of the
CDM model, within the framework of the RWF cosmology but without introducing dark energy and dark matter. Distinct from other theories extending cosmology beyond the standard model, in ‘relativity with a preferred frame’, no ad hoc assumptions are made, the fundamental laws of physics do not change, and relativistic invariance is not violated. It is also important that the theory is designed without any relations to possible applications. Modifications, ingrained into the theory at the fundamental level of special relativity, are introduced to reconcile the existence of the cosmological preferred frame (usually identified with the CMB frame) with the relativity principle. The postulates of special relativity, namely the relativity principle and universality of the speed of light, are retained. Only the freedom in the value of the
one-way speed of light is used such that there is an anisotropy of the one-way speed of light in all the frames except for the preferred frame, while the
two-way speed of light is equal to
c in all of the frames. This does not spoil relativistic invariance and does not change the form of physical laws. The preferred fame effects reveal themselves only in that the time and space intervals figuring into equations expressing physical laws should be transformed into ’physical’ (measurable) intervals using some relations in which only one parameter, the anisotropy parameter
b, figures in. This results in particular in the expression for the redshift containing some coefficient dependent on
b such that applying the arguments which led to the
relation in Equation (
1) in the standard RW model yields a modified relation of the form
The luminosity distance–redshift relation in Equation (
7), in principle, makes it possible to fit the SNIa observations to the matter-dominated RWF model. According to Equation (
7), the observed deceleration parameter is
, with
being the deceleration parameter of the RWF matter-dominated model. Since the parameter
b is expected to be negative, the observed negative values of
do not exclude the Friedman dynamics with
, which implies that the universe can be both accelerating and decelerating. Although it is an indication of the SNIa data being explainable within the framework of the RWF model without introducing dark energy, in order to prove this, the Friedman equation (Equation (
2)) is to be solved, and the
dependence derived from the solution is to be compared with that retrieved from the SNIa observations. Assuming, in contrast to the standard model, that in Equations (
4) and (
6),
, one can find the solution to the Friedman equation containing only
and
b. (
can be eliminated using Equation (
6).) By applying this solution, there is no need to specify the nature of the matter density characterized by
. It could either be only the ordinary matter or the mixture of ordinary and dark matter. In the latter case, however, there is a conceptual difference from the
CDM standard model. While, in the standard model, dark matter is a component of the cosmic fluid whose density is tied to the dark energy and thus has no connection to the small-scale dark matter density, in the model, based on ‘relativity with a preferred frame’, it could be an average of the estimated density of dark matter (presumably) accumulated in galaxies and clusters. It was shown in [
35] that for any value of
, the value of the model parameter
b can be found such that the
dependence, derived using the solution, fits the SNIa data with high accuracy. (In fact,
of the
CDM ‘concordance’ model was used as a fitting formula for the SNIa data.) The result is represented by a curve in the plane (
,
b) on which fitting is achieved.
The framework of ’relativity with a preferred frame’, designed from the level of the special relativity foundations, is not specified for any applications and thus can be applied for interpreting other observations within the same framework. The baryon acoustic oscillation (BAO) data are commonly considered as confirming the accelerated expansion and imposing constraints on the dark energy parameters. The BAO observations provide two different sets of data: BAO scales in the transverse and line-of-sight directions. Measurements of the angular distribution of galaxies yield the quantity
, which is the comoving angular diameter distance. Measurements of the redshift distribution of galaxies yield the value of the Hubble parameter
. In the results, obtained within the framework of ’relativity with a preferred frame’ and represented by the regions in the plane (
,
b), within which the predictions of the present theory fit the
and
data, the two regions are overlapped. This both provides a support for the theory and places quite tight constraints on the values of the parameters
and
b, which are confined within a quite narrow overlapping region. An additional (and quite strong) argument in favor of both consistency of the theory and the estimates for the parameter
b is that the line in the plane (
,
b), on which the results of the model fit the SNIa data, lies within that narrow region. It deserves attention that the value of
, which in light of Equation (
6) corresponds to the value
(flat universe), is within the overlapping interval. Thus, the results fit three different sets of observational data well, with the values of the theory parameter
b confined within a quite narrow interval.
Next, the observations of temperature anisotropies in the CMB are commonly considered as providing another independent test for the existence of dark energy. In the standard model, the presence of dark energy affects the CMB anisotropies, leading to a shift in the positions of the acoustic peaks. In the model, based on ’relativity with a preferred frame’, that change can be attributed to the presence of the correction factor in the relation for the redshift. What is more, ‘relativity with a preferred frame’ allows explaining the pussling Auger data on the mass composition of cosmic rays without introducing new physics [
36], and it also explains some abnormal features in the gamma ray spectrum [
37]. It is remarkable that only one universal parameter
b figures into the theory and that the values of the parameter are within the same range in all cases. All of the above are the hallmarks of a good and valuable physical theory. Thus, ‘relativity with a preferred frame’, designed to reconcile the relativity principle with the existence of the cosmological preferred frame, may provide an alternative to the standard model of cosmology (at least in some aspects).
Returning to the theory developed in the present paper, it is worth emphasizing that although a cosmological model relying on the universality of the Hubble law may be challenged (as with any model), the conclusion that the local Hubble law cannot be explained in the framework of the currently accepted standard model of the large-scale cosmology and thus should be considered as an independent law of nature (within its area of validness) cannot be challenged. In this respect, it is appropriate to comment on the so-named ’Hubble tension’ which is currently a widely discussed issue. Hubble tension refers to a growing discrepancy between the Hubble constant value, inferred from early universe probes (observations of CMB anisotropies by Planck) assuming the standard flat
CDM cosmological model [
38], and the measurement of that value from late-universe probes by the SHOES project [
39,
40]. It is frequently suggested that the difference might be an indicator of new physics. However, in light of the above discussion, the Hubble tension does not exist. There are no grounds to identify the value of the Hubble constant in the Hubble law, inferred from the measurements in the local universe, with the constant
in the
relation in Equation (
1) obtained from the highly smoothed and symmetrized RW cosmological model. Although in the discussions of the Hubble tension in the literature, both values are referred to as the ‘current expansion rate of the universe’, they are related to different conceptual frameworks. The term ‘expansion’ implies the RWF model which, like as the term itself, is not applicable to the interpretation of local observations. Therefore, no coincidence should be expected.
The theory, based on the concept in which the linear Hubble relation has the status of a fundamental law of small-scale cosmology, can be developed in different ways. In the present paper, the ‘small-scale cosmology’ is formulated as the theory operating in the (redshift–object coordinates) space. This allows developing a conceptual and computational basis of the theory along the lines of that of special relativity such that a complete one-to-one correspondence between the variables and relations of the two theories can be achieved. In pursuing the approach, the effectiveness of group theoretical methods is exploited. Applying the Lie group method yields transformations of the variables (the redshift and space coordinates of a cosmological object) between the reference frames of the accelerated observers. In this paper, the transformations are applied to studying the effects of the solar system observer acceleration on the observed shape, distribution and rotation curves of galaxy clusters.
This paper is organized as follows. In
Section 2, following the introductory section, the framework of the small-scale cosmological model, patterned after special relativity, is developed, and the transformations relating the redshifts and space coordinates of an object measured by two accelerated observers are derived. (Some details of the derivation are placed in
Appendix A). The particular case of the transformations, which relates the measurements made by inertial and accelerated observers, is specified. In
Section 3, the transformations for that particular case are used to make conclusions about the influence of the observer acceleration on the observed shape, distribution and rotation curves of galaxy clusters. In
Section 4, some comments on the conceptual framework of the theory and results are furnished.
4. Discussion
In the present paper, the ‘small-scale cosmology’ was developed as an independent theory, having no relation to the standard cosmology based on the RWF-type models. In the theory, the linear Hubble law status changes from the common interpretation of a small z limit of the RWF model or an effect of expanding space to the basis of the theory. The reasoning behind this is that, contrary to what is commonly accepted, validity of the linear Hubble law at cosmologically small scales cannot be proven using the global RWF cosmological models that are based on the assumptions of homogeneity and isotropy. Those assumptions are supported by observations only upon averaging the observational data over the scales, which are much larger than those with which the ‘small-scale cosmology’ deals such that small-scale structures like galaxies and clusters of galaxies are filtered out. For the same reason, extending the notions of dark matter and dark energy, which are introduced as the cosmic fluid density components in global large-scale dynamics of the universe, to small scales is conceptually inconsistent.
Development of the theory is based on the requirement that the Hubble law should be invariant with respect to a change in the observer acceleration. In pursuing this approach, the effectiveness of group theoretical methods, particularly the Lie group method, is exploited. The variables taking part in the transformations are the redshift and the distance (more precisely, the space coordinates) characterizing a cosmological object. This implies that the distance to the cosmological object is not something ‘absolute’ but relative and depending on the observer reference system. This leads to a profound change in the way we perceive space, similar to the conceptual change introduced by the theory of relativity. In both cases, it is in disagreement with the ‘common sense’ that we use regarding space and time measurements. In particular, regarding the distance to an object as something self-evident is apparently a result of transferring the picture of the physical space, obtained from experiments in our closed surroundings, to cosmological scales. Thinking about the distance to an object, we (unconsciously) represent to ourselves either repeated application of the measuring rod along the line of sight or the movements that must take place to reach the object (see the discussion in [
66]). However, when comparing the scales of our even cosmic experience (e.g., distances to the closest planets) with those for cosmologically nearby objects, one can see by how many orders of magnitude the quantities differ. It is possible that applying the notions deduced from the accessible physical space experience to cosmology is similar to applying the concepts of the macroworld to the microworld of quantum theory and vice versa, and thus it could be expected that, like in the latter case, quantitative differences may result in qualitative changes.
Claiming the Hubble law to be the basic equation of the theory, which is formulated in the space, allows developing the theory along the lines of special relativity, where universality of the law of propagation of light is one of basic principles. The similarity reveals itself first in the possibility to establish the one-to-one correspondence between the variables taking part in the Hubble law and in the law of propagation of light, as well as how in both laws, one of the variables requires definition, and those variables in the two laws are in correspondence with each other. Therefore, there are grounds to develop the ‘small-scale cosmology’ maintaining that analogy. Of course, using the similarity of the basic law of the present theory with that of special relativity for development of the theory is a heuristic argument. Note, however, that it is not a rare situation in science where the approach and methods of one theory appear to be fruitful in another one. Thus, it is natural to expect that applying the concepts and methods which led to the well-established results in special relativity should result in meaningful consequences in its counterpart.
It is worth clarifying that the change in the redshifts in the spectra of galaxies due to the observer acceleration is not an effect similar to the Doppler redshift. The redshift in the spectra of galaxies, both before the observer acceleration and after it, is not attributed to the galaxies’ motion with respect to the observer frame; it is the cosmological redshift. Commonly, the cosmological redshift is attributed to space dilatation, but as discussed in the Introduction, applying the concept of space expansion on small scales is inconsistent and physically meaningful. In the ‘small-scale cosmology’, the change in the redshift induced by a change in the observer acceleration is a consequence of the invariance of the universal Hubble law, like how the dependence of the distances on the relative speed of the observers in special relativity is a consequence of the universality and invariance of the law of propagation of light.
In the present paper, the ‘small-scale cosmology’ was designed as a theory operating in the
space. It would also be of interest to develop the theory, based on the concept of universality of the Hubble law, in the
space, which should allow one to define the spacetime metric of the ‘small-scale cosmology’. The requirement of linearity of the relation between the redshift and a distance could be used to (partially) specify the components of the spacetime metric tensor. To further specify the metric, the ‘cosmological principle’ can be applied. The cosmological principle, in its general formulation, states that for any observer in the universe, the observations should yield the same results. In the context of large-scale cosmological models, the cosmological principle evolves to the statement that the universe, on average, should look isotropic and homogeneous for sets of ‘privileged’ observers, but it is irrelevant to the small scales. On the small scales, the cosmological principle implies that observations made by an observer in any galaxy should yield the same Hubble law, with the same Hubble constant as that determined by the observations made from our vantage point. (In some textbooks (e.g., [
67]), one can find a ‘proof’ of this assertion, but the proof is invalid in the present context since it relies on the interpretation of the redshift as a recession velocity.) To apply the cosmological principle to development of the theory, the principle should be formulated as the condition of invariance of the spacetime metric with respect to a change in the observer’s location. This condition should impose restrictions on the components of the spacetime metric tensor, in addition to those imposed by the requirement of validity of the linear Hubble law. As a result, the spacetime (and space) metric would be (at least partially) defined, which in particular would allow revealing whether the statement that the space is Euclidean at small scales is compatible with the linearity of the redshift–distance relation.
To conclude, in this paper, the new conceptual view of cosmology at small scales, as a theory independent of the standard model of cosmology, is presented. The ‘small-scale cosmology’, based on that view, does not suggest any kinematical or dynamical interpretation neither for the redshift, considered a characteristic of an object, nor for the Hubble law, considered a physical reality. Nevertheless, it (like the large-scale cosmography) provides a theoretical framework for interpreting the observations and allows making some predictions, particularly regarding the influence of the observer acceleration on the observed shapes, distributions and rotation curves of the galaxy clusters.