Abstract:In linearized gravity, two linearized metrics are considered gauge-equivalent, hµν ∼ hµν + Kµν [v], when they differ by the image of the Killing operator, Kµν [v] = ∇µvν + ∇ν vµ. A universal (or complete) compatibility operator for K is a differential operator K1 such that K1 • K = 0 and any other operator annihilating K must factor through K1. The components of K1 can be interpreted as a complete (or generating) set of local gauge-invariant observables in linearized gravity. By appealing to known results in t… Show more
“…Next, we find a way to express the projector r 2 Ω µν onto the warped factor in terms of the curvature. Here we find a slight dimension dependence (as already noted in [15,Sec.3.3]). In dimension n ≥ 5, one can find a formula that involves only products and contractionsḡ ofT :…”
“…In the recent work [15], we have explicitly exhibited (by a different method) complete sets of linear invariants for each geometry in the gST family. Relating these invariants to the linearization of the IDEAL characterization tensors, as well as vice versa, can accomplish two goals: give a geometric interpretation to the invariants of [15] and to prove the completeness of the linearized invariants that can be obtained from the present work.…”
Section: Discussionmentioning
confidence: 99%
“…For future reference, we also compute some algebraic combinations among these tensors (see [15,Sec.3.3] for more intermediate steps of the calculations):…”
In general relativity, an IDEAL (Intrinsic, Deductive, Explicit, ALgorithmic) characterization of a reference spacetime metric g0 consists of a set of tensorial equations T [g] = 0, constructed covariantly out of the metric g, its Riemann curvature and their derivatives, that are satisfied if and only if g is locally isometric to the reference spacetime metric g0. We give the first IDEAL characterization of generalized Schwarzschild-Tangherlini spacetimes, which consist of Λ-vacuum extensions of higher dimensional spherically symmetric black holes, as well as their versions where spheres are replaced by flat or hyperbolic spaces. The standard Schwarzschild black hole has been previously characterized in the work of Ferrando and Sáez, but using methods highly specific to 4 dimensions. Specialized to 4 dimensions, our result provides an independent, alternative characterization. We also give a proof of a version of Birkhoff's theorem that is applicable also on neighborhoods of horizon and horizon bifurcation points, which is necessary for our arguments.
“…Next, we find a way to express the projector r 2 Ω µν onto the warped factor in terms of the curvature. Here we find a slight dimension dependence (as already noted in [15,Sec.3.3]). In dimension n ≥ 5, one can find a formula that involves only products and contractionsḡ ofT :…”
“…In the recent work [15], we have explicitly exhibited (by a different method) complete sets of linear invariants for each geometry in the gST family. Relating these invariants to the linearization of the IDEAL characterization tensors, as well as vice versa, can accomplish two goals: give a geometric interpretation to the invariants of [15] and to prove the completeness of the linearized invariants that can be obtained from the present work.…”
Section: Discussionmentioning
confidence: 99%
“…For future reference, we also compute some algebraic combinations among these tensors (see [15,Sec.3.3] for more intermediate steps of the calculations):…”
In general relativity, an IDEAL (Intrinsic, Deductive, Explicit, ALgorithmic) characterization of a reference spacetime metric g0 consists of a set of tensorial equations T [g] = 0, constructed covariantly out of the metric g, its Riemann curvature and their derivatives, that are satisfied if and only if g is locally isometric to the reference spacetime metric g0. We give the first IDEAL characterization of generalized Schwarzschild-Tangherlini spacetimes, which consist of Λ-vacuum extensions of higher dimensional spherically symmetric black holes, as well as their versions where spheres are replaced by flat or hyperbolic spaces. The standard Schwarzschild black hole has been previously characterized in the work of Ferrando and Sáez, but using methods highly specific to 4 dimensions. Specialized to 4 dimensions, our result provides an independent, alternative characterization. We also give a proof of a version of Birkhoff's theorem that is applicable also on neighborhoods of horizon and horizon bifurcation points, which is necessary for our arguments.
“…It is important to notice that the Einstein operator Ω → E ij = R ij − 1 2 ω ij ω rs R rs is self-adjoint with 6 terms though the Ricci operator is not with only 4 terms. Recently, many physicists (See [1], [2], [8], [9], [24]) have tried to construct the compatibility conditions (CC) of the Killing operator for various types of background metrics, in particular the three ones already quoted, namely an operator D 1 : S 2 T * → F 1 such that D 1 Ω = 0 generates the CC of Dξ = Ω. We have proved in the above references the following crucial results:…”
The search for generating compatibility conditions (CC) for a given operator is a very recent problem met in General Relativity in order to study the Killing operator for various standard useful metrics (Minkowski, Schwarschild and Kerr). In this paper, we prove that the link existing between the lack of formal exactness of an operator sequence on the jet level, the lack of formal exactness of its corresponding symbol sequence and the lack of formal integrability (FI) of the initial operator is of a purely homological nature as it is based on the long exact connecting sequence provided by the so-called snake lemma. It is therefore quite difficult to grasp it in general and even more difficult to use it on explicit examples. It does not seem that any one of the results presented in this paper is known as most of the other authors who studied the above problem of computing the total number of generating CC are confusing this number with a kind of differential transcendence degree, also called degree of generality by A. Einstein in his 1930 letters to E. Cartan.The motivating examples that we provide are among the rare ones known in the literature and could be used as testing examples for future applications of computer algebra.
“…[SDH14, BDS14, BDHS14, FL16, Ben16, BSS16], but there also exist similar developments for e.g. linearized gravity [FH13,BDM14,Kha16,Kha18] and linearized supergravity [HS13]. In addition to such non-interacting models, examples of perturbatively interacting quantum gauge theories were constructed in [Hol08, FR12, FR13, TZ18] by means of an appropriate adaption of the BRST/BV formalism to AQFT.…”
It is observed that the shifted Poisson structure (antibracket) on the solution complex of Klein-Gordon and linear Yang-Mills theory on globally hyperbolic Lorentzian manifolds admits retarded/advanced trivializations (analogs of retarded/advanced Green's operators). Quantization of the associated unshifted Poisson structure determines a unique (up to equivalence) homotopy algebraic quantum field theory (AQFT), i.e. a functor that assigns differential graded * -algebras of observables and fulfills homotopical analogs of the AQFT axioms. For Klein-Gordon theory the construction is equivalent to the standard one, while for linear Yang-Mills it is richer and reproduces the BRST/BV field content (gauge fields, ghosts and antifields).
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