Quasi-Noether systems and quasi-Lagrangians

We study differential systems for which it is possible to establish a correspondence between symmetries and conservation laws based on Noether identity: quasi-Noether systems. We analyze Noether identity and show that it leads to the same conservation laws as Lagrange (Green-Lagrange) identity. We discuss quasi-Noether systems, and some of their properties, and generate classes of quasi-Noether differential equations of the second order. We next introduce a more general version of quasi-Lagrangians which allows us to extend Noether theorem. Here, variational symmetries are only sub-symmetries, not true symmetries. We finally introduce the critical point condition for evolution equations with a conserved integral, demonstrate examples of its compatibility, and compare the invariant submanifolds of quasi-Lagrangian systems with those of Hamiltonian systems.


Introduction
For variational systems the relation between symmetries of the Lagrangian function and conservation laws was known from the classical Noether result [10]. It was shown that there is one-to-one correspondence between variational symmetries (symmetries of variational functional) and local conservation laws of a differential system, [11].
In this paper, we study differential systems that allow a Noether-type association between its conservation laws and symmetries (quasi-Noether systems). Our approach is based on the Noether operator identity [12] that relates the infinitesimal transformation operator to the Euler and divergence operators. The Noether operator identity has been shown to provide a Noether-type relation between symmetries and conservation laws not only for Lagrangian systems, but also for a large class of differential systems that may not have a well-defined variational functional, see [13], [14]. Noether operator identity was also demonstrated to allow derivation of extension of Second Noether Theorem for non-Largangian systems possessing infinite symmetry algebras parametrized by arbitrary functions of all independent variables, [16]. These infinite symmetry algebras were shown to lead to differetial identities between the equations of the original differential system and their derivatives. Recently Noether identity was used to generate relations between sub-symmetries [17] and corresponding local conservation laws [18] for quasi-Noether systems.
In this paper, we analyze quasi-Noether systems and some of their properties. In Section 2, we review known correspondence between symmetries and conservation laws for variational systems from the standpoint of the Noether identity. In Section 3, we discuss this correspondence for a more general class of differential systems (quasi-Noether systems) that includes non-variational problems. We review conservation laws obtained with the use of approach based on the Noether identity and compare them with the results obtained from the Lagrange (Green-Lagrange) identity. We also find the class of quasi-Noether evolution equations of the second order, and quasi-linear equations of the second order. In Section 4, we generalize the concept of quasi-Lagrangian, and use it to prove a new extension of the Noether theorem to non-Lagrangian systems. In this approach, variational symmetries of quasi-Lagrangians are only sub-symmetries, and need not be symmetries. We give an example where all lower conservation laws are generated in this way, but where the previous correspondence fails. As a geometric application, we compare the invariant submanifolds of quasi-Noether systems to those of Hamiltonian systems and show that they behave in an "opposite" way. To address this fact we introduce the notion of a critical point of a conserved quantity, and demonstrate examples of the compatibility of the critical point condition with the time evolution of the PDE system.

Symmetries and conservation laws of variational systems
Let us briefly outline the approach we follow.
We consider smooth functions u a = u a (x) defined on an open subset D ⊂ R p . Let be the action functional, where L is the Lagrangian density. The equations of motion are is the a-th Euler (Euler-Lagrange) operator (variational derivative). We call the tuple E = (E 1 , . . . , E n ) the Euler operator. In the notation of [11], we could give it the following form: The operator E a annihilates total divergences. Consider an infinitesimal (one-parameter) transformation with the canonical infinitesimal operator where α a = α a (x, u, u (1) , . . . ), and the sum is taken over all (unordered) multi-indices J. The variation of the functional S under the transformation with operator X α is where M i = M i (x, u, u (1) , . . . ) are smooth functions of their arguments. The Noether (operator) identity [12] (see also, e.g. [6] or [13]) relates the operator X α to E a , (2.9) The expression for R i can be presented in a more general form [12,8]: where J and K sum over multi-indices. Applying the identity (2.8) with (2.9) to L and using (2.7), we obtain which on the solution manifold (∆ = 0, D i ∆ = 0, . . . ) leads to the statement of the First Noether Theorem: any one-parameter variational symmetry transformation with infinitesimal operator X α (2.5) gives rise to the conservation law (2.12).
Note that Noether [10] used the identity (2.11) and not the operator identity (2.8). The first mention of the Noether operator identity (2.8), to our knowledge, was made in [12]. We next consider differential systems that may not have well-defined Lagrangian functions.

Symmetries and conservation laws of quasi-Noether systems
For a general differential system, a relationship between symmetries and conservation laws is unknown. In [13] and [14], an approach based on the Noether operator identity (2.8) was suggested to relate symmetries to conservation laws for a large class of differential systems that may not have well-defined Lagrangian functions. In the current paper, we will follow this approach.
(3.2) If our system (3.1) allows the existence of coefficients β a (cosymmetries) such that on the solution manifold (∆ = 0, D i ∆ = 0, . . . ), then according to (3.2), each symmetry of the system X α will lead to a local conservation law (see [14], see also [13]) for any differential systems of class (3.3). In [13], the quantity β a ∆ a was referred to as an alternative Lagrangian. Let us note that the correspondence between symmetries and local conservation laws defined above for differential systems without well-defined Lagrangian functions may not be one-to-one or onto, as in the case of variational symmetries and local conservation laws [11], and non-trivial symmetries may lead to trivial conservation laws. If β generates a conservation law, i.e. E(β · ∆) ≡ 0, then it was shown in [1] that translation symmetries α = a i u i , a = const. lead to trivial conservation laws if β x = 0.
In general, the nontriviality of a conservation law is determined by the characteristic. To compute it explicitly, let X α (β · ∆) = A · ∆ and E(β · ∆) = B · ∆ for A, B differential operators. Then the Noether identity and integration by parts yield where (B * ) va = (−D) I • B avI is the adjoint operator. Integrating by parts the LHS and rearranging yields overall where the divergence is equivalent to (3.4) on solutions, and Thus, the conservation law obtained from Noether identity and corresponding to symmetry X α is nontrivial if on solutions of the original system (3.1). The condition (3.3) can be written in a somewhat more general form [14] E v (β ac ∆ a ) . = 0, a, c = 1, . . . n, v = 1, . . . , q. (3.8) In terms of the Fréchet derivative operator D ∆ and its adjoint D * ∆ [11] ( the condition (3.3) was shown in [15] to be related to the condition of self-adjointness of the operator D ∆ (generalized Helmholtz condition) (3.11) this relationship being: Expression (3.12) provides a relationship between the condition (3.3) for a system to be quasi-Noether and the existence of a variational functional for a transformed differential system.
The condition (3.3) can be considered as defining quasi-Noether systems, see also [16]. A system (3.1) is quasi-Noether if there exist functions (differential operators) β a such that the condition (3.3) is satisfied. In [13], the quantity β v ∆ v was referred to as an alternative Lagrangian. If coefficients β a generate a conservation law, they are related to adjoint symmetries [19], and referred to as characteristics of a corresponding conservation law [11], generating functions [20] or multipliers [2]. In general, we call them cosymmetries [20] if they satisfy (3.3).
It should be noted that the condition (3.3) (for a system to be quasi-Noether and possess a correspondence between symmetries and conservation laws) was obtained earlier within an alternative approach based on the Lagrange identity. In [21], the classical Lagrange identity (Green's formula) was used for generating conservation laws for a linear differential system. A condition for the existence of a certain conservation law written in terms of an adjoint differential operator was presented in [20] within a general framework of algebraic geometry. In [22], a correspondence between symmetries and conservation laws based on Green's formula and a condition similar to (3.3) was obtained for evolution systems. For the case of point transformations, this correspondence was discussed in [5]. In [19], the geometric meaning of this condition was discussed for mechanical systems. In [8], a condition that can be reduced to (3.3) was presented for a general differential system.
Note that the condition (3.3) played a key role in later developed direct method [2] and the nonlinear self-adjointness approach [7].

Approach using Lagrange identity
Let us briefly describe the alternative approach based on the Lagrange identity and compare the results with those of the Noether identity approach.
The well-known Lagrange identity is as follows: where D ∆ is the Fréchet derivative of ∆, and D * ∆ is its adjoint. An explicit expression for the trilinear fluxes Q[α, β, ∆] was given in [8]: (see (2.5), and (3.9)) we can express (3.13) as follows: If, for a given system ∆, there exist functions β a and operators Υ va = υ vaJ D J such that the following relationships hold: then (D * ∆ ) av β a= 0. Thus, for each symmetry X α of the system ∆ = 0, (X α ∆ a = Λ ab ∆ b for some operators Λ ab = λ abJ D J ), equation (3.15) provides a corresponding conservation law: We now show that the correspondence between symmetries and conservation laws in terms of Lagrange identity is equivalent to the one using the Noether identity and leads to the same conservation laws. Indeed, using the product rule [11]: in (3.15) gives: The last term in (3.19) is a total divergence by (3.13): Thus, (3.19) provides the same result as the Noether identity: Let us show that the condition used in direct method [2] (D * ∆ ) av β a= 0 (3.21) is equivalent to the quasi-Noether condition (3.3). Indeed, using the identity [11] E 22) and the fact that An alternative key expression of the direct method is a special case of (3.3). Note also that the direct method aims at the generation of conservation laws for a differential system without regard to its symmetries while the goal of both approaches above taken earlier was to establish a correspondence between symmetries and conservation laws.
It can be shown that the general case of differential systems (3.1) satisfying the condition (3.3), with β a being differential operators can be reduced to the case of the condition (3.3) with the β aJ being differential functions. Indeed, (see [11]) Since the contribution of the first term in the RHS, being a total divergence, is zero after applying the Euler operator, we find that where eachβ a = (−D) J β aJ is a differential function.
In the following theorem, we prove that local conservation laws exist only for quasi-Noether systems.
Theorem 1 (Quasi-Noether systems and conservation laws). Any differential system (3.1) that possesses local conservation laws is quasi-Noether. A quasi-Noether system that admits continuous symmetries in general, possesses local conservation laws.
Proof. Assume that the system (3.1) has some local conservation law where P i and γ a are differential functions. Then which shows that the system is quasi-Noether.
Suppose now that the quasi-Noether system (3.3) possesses a continuous symmetry with the infinitesimal operator X α (2.5). Rewriting condition (3.3) in the form where the sum is taken over 1 ≤ a ≤ n, β a are differential functions, and Γ va = Γ vaJ D J are differential operators. Multiplying the equation (3.31) by α v and taking a sum over v, we obtain Applying the Noether identity (2.8) in the LHS, we obtain Since X α is a symmetry operator for the system ∆ a , we obtain and therefore, a quasi-Noether system with continuous symmetries in general, possesses local conservation law (3.34).
Note that in some cases the conservation law (3.34) may be trivial. Note also that condition (3.3) allows one to find and classify quasi-Noether equations of a certain type. For example, it can be shown that equations of the following class:

Classes of Quasi-Noether equations
The quasi-Noether class of equations for which it is possible to establish a Noether type correspondence between symmetries and conservation laws is quite large, and covers practically all interesting differential systems of mathematical physics, and all systems possessing conservation laws. Many examples of equations of the class were given in [13], [14], and [15]. Quasi-Noether systems include all differential systems in the form of conservation laws, e.g. KdV, mKdV, Boussinesq, Kadomtsev-Petviashvili equations, nonlinear wave and heat equations, Euler equations, and Navier-Stokes equations; as well as the homogeneous Monge-Ampere equation, and its multi-dimensional analogue, see [13]. In [16], the approach based on the Noether identity was applied to quasi-Noether systems possessing infinite symmetries involving arbitrary functions of all independent variables, in order to generate an extension of the Second Noether theorem for systems that may not have well-defined Lagrangian functions.

Evolution equations
Consider evolution equations of the form Assuming β = β(t, x, u, u x , u xx , . . . , u nx ), and requiring our equation to be quasi-Noether (3.3) we obtain the following condition It can be shown that β = β(t, x, u). Moreover, it can be shown that for this system, the above equality holds for all u (=) rather than strictly solutions (= ). We obtain the following classes of equations: 1.
where H(u, u x ) and S(u) are arbitrary functions, and α is a constant. In this case the equation ∆ = u t − Au xx − B is obviously, quasi-Noether since the left hand side turns into total divergence upon multiplication by β:
We do not pursue the remaining cases, since these necessarily involve dependence on 1/u x . However, the above analysis gives insight into, for instance, equations of the following class: u t = u xx + u n x , n = 0, 1, 2, 3, ...

Quasi-linear equations
Consider now quasi-linear equations of the form We require our equation to be quasi-Noether (3.3) For equations (3.48) condition (3.51) takes a form Solving (3.52) for β = β(x, t, u), we obtain and L = L(u, u x ), K = K(u, u x ), f = f (u, u t ), β = β(x, t, u) are functions to be determined. We get the following solutions: 1. where l, m, q are abrbitrary constants, function M(u, u x ) is arbitrary, β = e lx+mt+qu , and Examples: a. If M(u, u x ) = c, we obtain

Quasi-Lagrangians
For β a cosymmetry, the quantity L = β · ∆ serves an analogous role to a Lagrangian. In this section, we examine the applications of such a quasi-Lagrangian L in more detail. We show that equations with a quasi-Lagrangian have a Noether correspondence on a subspace. We then demonstrate the incompleteness of the symmetry/cosymmetry correspondence with an example. We conclude with a comparison of the invariant submanifolds of quasi-Noether systems with those of Hamiltonian systems.

A Noether correspondence
Let us introduce the operator T depending on β such that E(β · ∆) = T · ∆. If D ∆ is an endomorphism (same number of equations as dependent variables), then T = D * β − D β by (3.12).
We say an operator T is nondegenerate if its restriction to ∆ = 0 is not the zero operator. If β is a characteristic for a conservation law (generator), then E(β · ∆) = 0, so T = 0 (degenerate). Thus β, in this section, will be a cosymmetry which is not a characteristic.
Recall that a functional L[u] = L[u]dx is an equivalence class modulo total divergences. We say a smooth functional L[u] = L[u]dx is nondegenerate if it is nonzero and some representative L[u] (hence all of them) does not vanish quadratically with ∆. We identify nondegenerate functionals with their affine terms: L ∼ L| ∆=0 + β I · D I ∆. Mod a divergence, we then have L ∼ L 0 + β · ∆, where β = (−D) I β I comes from integration by parts. We will abuse notation in the below and identify L with L. As a non-example, consider, for example, a second order scalar nonlinear PDE ∆ = ∆ 1 (u ij ). Then for L = ∆ 2 , we have The concept of sub-symmetry was introduced in [17]. We say X α generates a subsymmetry of ∆ if X α (T · ∆)| ∆=0 = 0 for some nondegenerate T . In the special case that X α (T · ∆)| T ·∆=0 = 0, clearly X α is an "ordinary" symmetry of a sub-system T · ∆; the more general definition will not be needed here. We note that in [18], sub-symmetries of sub-systems generated by co-symmetries yield conservation laws through the mechanism in the previous section. In the present work, we find a new appearance of sub-symmetries.
We now present an extension of Noether theorem. Every variational symmetry X α of a quasi-Lagrangian L corresponds to a conservation law characteristic T * α in the image of T * . The variational symmetry is only a sub-symmetry of the PDE ∆. If L = L 0 + β · ∆ and cosymmetry β is also in the image of T * , then a family of equations ∆ + ker[T ] shares variational symmetries, hence conservation laws generated by the quasi-Lagrangian.
Theorem 2. Let ∆ be a normal, totally nondegenerate PDE system, and suppose there exist smooth and nondegenerate operator T and functional L such that E(L) = T · ∆. Remark 1. Part 3 illustrates that a variational symmetry α of L need not correspond to a symmetry of ∆, since if X α ∆ f = A∆ f , then X α f = Af need not be true for all f ∈ ker[T ]. We will demonstrate this failure in Section 4.2.
Therefore, the Green-Lagrange-Noether approach is incomplete: it requires vector field X α to be a symmetry of ∆, while Part 2 indicates we must instead consider sub-symmetries. The incompleteness was partially demonstrated in [1] in the case β is a characteristic of a conservation law, but the case where cosymmetry β is not a characteristic was not indicated.
Note that Ibragimov's approach [7] is distinct; it uses variational symmetries an extended, Lagrangian system obtained by, essentially, treating the β's as dependent variables.
Such variational symmetries must be symmetries of ∆, which is one reason why our result is different. Another follows from a direct computation of the characteristic; there is an additional term due to the symmetric action of X α on L, which in our approach is simply a divergence not contributing to the characteristic.
Remark 2. The main difference of our extension is that the vector field X α is only a sub-symmetry of the PDE ∆, not a true symmetry, since we are considering variational symmetries of L. This highlights the incompleteness of the previous approach, which requires using ordinary symmetries. We presented an example where all lower conservation laws arise in this way, many only from sub-symmetries.
Remark 3. Upon restricting said symmetries of ∆ to variational symmetries of L, the results are equivalent, of course. Let A∆ = X α ∆. The Green-Lagrange-Noether approach yields the following conservation law: But in fact, (X α β + A * β) = X α L + div = div since α is a variational symmetry. Thus, for some generating function µ. This implies T * α is also a generating function.
Remark 4. We note that L 0 = L| ∆=0 is nonzero (mod divergence) in general. For example, if E(L) = ∆ for L = uv t − λ[u, v] and the two-component evolution system then unless λ is of a special form, L need not vanish on ∆ = 0.

An example
It is well known that the second order Burgers equation has exactly one conservation law and no cosymmetries other than β = 1. It thus has no quasi-Lagrangians, and its conservation law does not arise from such. We next consider the opposite situation.
Consider a third order evolution equation u t = F [u] of the form Even if f (t) = 0, this cannot be written as a Hamiltonian equation, since although u t = D · E(H) for H = − 1 2 u 2 x and the skew-adjoint operator it can be shown that D does not verify the Jacobi identity. We do, however, see a quasi-Lagrangian structure: We present the cosymmetries of order β(t, x, u, . . . , u 5 ): The even-order cosymmetries in (4.7) are conservation law generators which arise from variational symmetries of the quasi-Lagrangian Indeed, if we rewrite them using (4.5), then we see they generate a translation x → x+ε, a scaling (x, t) → e ε (x, t), and a translation t → t + ε, respectively. These (three) cosymmetries comprise the (order 4) conservation law generators for equation (4.5).
There are two differences from the classical Noether theorem: 1. The variational symmetry u → u + ε does not lead to a conservation law since for α = 1, we have T * (α) = −D x (1) = 0.
2. Time translation is not a symmetry of ∆ = 0 unless f ′ (t) = 0. Nevertheless, since is a divergence expression, we see α = u t generates a variational symmetry of L, and then a conservation law of ∆.

Remark 5.
We present a comparison with the quasi-Noether/nonlinear self-adjointness/Green-Lagrange approach. Suppose the symmetry condition X α ∆ = A∆, and integrate by parts: Also recall the Noether identity and quasi-Lagrangian structure (4.6) Combining these two formulas gives the characteristic for the conservation law generated using this approach: The only symmetry in (4.8) is α = u x . In this case, it can be verified that . Recall the characteristic generated by a variational symmetry is also −D x α. Thus, the two approaches agree when α is a symmetry of (4.5).
Remark 6. Observe that α = u t and α = tu t + xu x do not generate symmetries of (4.5) if f ′ (t) = 0. However, a simple modification yields the desired conservation law. Combining (4.9) with (4.10) without the symmetry condition X∆=0 yields For α = u t , it can be shown that Therefore, after an integration by parts, we recover the conservation law plus an error term: (4.14) In fact, the error is a divergence: f ′ (t)β = D x (− 1 2 uf ′ (t)), so we derive an analogous conservation law. Again, the characteristic is −D x α.
Let us apply the same analysis to α = tu t + xu x . We have As before, we obtain The second expression on the left hand side is a divergence, so we obtain a conservation law. Using −A * β = − 1 2 D x α, we conclude the characteristic is again −D x α.

Critical points and symmetries
We will show that quasi-Lagrangians are "opposite" in a sense to Hamiltonians. Let ∆ = u t − P [u] be an evolution system with evolutionary operator Each of these objects satisfies special determining equations: α symmetry, β cosymmetry. Symmetry α satisfies the equation D t α = D P α. These equations imply that symmetry invariance α = 0 and cosymmetry invariance β = 0 are compatible with ∆ = 0. By compatible, we mean if u 0 (x) solves γ(t 0 , x, u 0 , . . . ) = 0, then for time evolution u(t) = U(t; t 0 )u 0 , we have γ(t, x, u(t), . . . ) = 0. This follows for P, u 0 analytic by a (local) power series expansion, since the invariance conditions imply D k t γ| γ=0 = 0 for all k ≥ 0. The same holds for systems in Cauchy-Kovalevskaya form, which can be rewritten as evolution systems.
Remark 7. It was observed in [1] that a co-symmetry β induces an invariant one-form β[u] · du with respect to time evolution, in an analogous way that a symmetry α induces an invariant vector field α[u] · ∂/ ∂u. The determining equations are simply vanishing Lie derivatives of these tensors. The critical sets of these tensors are therefore time invariant, which is a more geometric way to describe the compatibility of these invariance conditions.
Let us note an interesting phenomenon. If E(L) = T ∆ is quasi-Lagrangian and X α is a variational symmetry, then X α is a symmetry of T · ∆, but T * α generates a conservation law of ∆. We thus find a "duality" relation between the existence of compatible systems. Next, if cosymmetry β also generates a conservation law, we call the equation β = 0 the critical point condition for the conserved integral generated by β. To justify this terminology, we recall the well known fact that cosymmetry β is a characteristic if and only if D * β − D β = 0 (self-adjointness), i.e. β = E(T ) for the conserved density T of the conservation law D t T + D i X i = β · ∆ = 0. It follows that β = 0 is the Euler-Lagrange equation for the (possibly time-dependent) functional T [u]dx, i.e. the equation for critical points of this conserved integral.
By the discussion for cosymmetries, the critical point condition is compatible with time evolution u t = P . This is sensible for two reasons: 1. if u(0) is a minimizer of T [u]dx for suitable boundary conditions, then the conservation of T implies u(t) is also a minimizer at later times. 2. If ∂ t T = 0, then so P actually generates a variational symmetry of the functional T dx. It follows that X P is a symmetry of E(T ) = 0, hence preserves the solution space.
Remark 8. Although many current papers are devoted to the construction of Lie-type invariant solutions and conservation laws for non-Hamiltonian systems, we are not aware of any which constructed the critical points of these conservation laws. The possibility for such was raised in [9].
Example 2 (Time-dependent evolution). The generalized KdV equation [3] u t + f (t, u)u x + u xxx = 0, (4.22) where f (t, u) = at −1/3 u + bu + cu 2 for a, b, c constant, has explicit time dependence if a = 0. It has a conservation law D t T + D x X= 0 with conserved density and characteristic (note that [3] has a typo in the u xx term) which solves (4.22) for c = 0. Suppose now that c = 0. If we solve E u T = 0 for u xx , then it is easy to show that (u xx ) t = (u t ) xx , or that (4.22) is consistent with E u T = 0. Alternatively, substituting E t T = 0 into (4.22) gives a first order PDE, which has solution where g is an arbitrary function. Substitution into E u T = 0 gives an ODE for g.
Example 3 (A non-Hamiltonian example). The nonlinear telegraph system [4] v t + ke u u x − e u = 0, where k = 0 is a constant, has a conservation law with density (note the typo in [4]) and characteristic A critical point (u * , v * ) satisfies the system E u T = E v T = 0, whose solution is where W is the Lambert W function. It is straightforward to show that (u * , v * ) solves (4.27).
Before turning to our next result, we recall Hamiltonian systems, see Chapter 7 in [11]. Suppose P = D · E(H) .] ∈ kerD for each t 0 , such that β − C generates a conservation law.
We now compare this situation to the "opposite" quasi-Lagrangian case in the following.
Theorem 3. Let E(L) = T · ∆. If γ = T * α generates a conservation law, then vector field invariance implies the critical point condition. If T is a smoothly invertible (skew-symmetric) matrix function, then the conditions are equivalent. Let u t = D · E(H). If α = D · β for β = E(G), then the critical point condition implies symmetry invariance. If D is an invertible (skew-symmetric) matrix function, then the conditions are equivalent.
If T, D commute with ∂ t , then their invertibility implies that T −1 ∆, D −1 ∆ is Lagrangian, respectively.
Remark 9. In the first case, α need not be a symmetry, but if it is, then symmetry invariance implies the critical point condition. Moreover, in Section 4.2, we see that symmetry invariance occurs after dividing by the kernel f (t) of T , analogous to conservation of β holding after dividing by the kernel of D.

Conclusions
In this paper, we discussed the problem of correspondence between symmetries and conservation laws for a general class of differential systems (quasi-Noether systems). Our approach is based on the Noether operator identity. We discussed some properties of Noether identity, and showed that it leads to the same conservation laws as Green-Lagrange identity. We generated classes of quasi-Noether equations of the second order of evolutionary and quasilinear form.
We introduced the notion of a quasi-Lagrangian, which generalizes the quantity L := β ·∆ used in previous works to the case where L| ∆=0 may not be zero. This generalization recovers the case where ∆ = E(L) is actually a Lagrangian system, thus allowing us to extend Noether theorem (Theorem 2). The previous work was not able to achieve both of the following: 1. achieve an extension of Noether while still involving symmetry vector fields (see [1] for an extension using only cosymmetries), and 2. recover the case of a Lagrangian system ∆ = E(L).
Based on the notion of invariant submanifolds we introduced critical points of conservation laws, and gave examples of the compatibility of cosymmetry invariance and the critical point condition, including for a non-Hamiltonian system.
We concluded with a comparison of the invariant submanifolds of quasi-Noether and Hamiltonian evolution equations, and showed these systems are "opposite" in some sense. For Lagrangian systems, the cosymmetry and symmetry invariant submanifolds coincide, while in general there is a containment in one direction or the other.