# Positive energy theorem

Positive energy theorem General relativity {estilo de exibição G_{vamos ver }+Lambda g_{vamos ver }={capa }T_{vamos ver }} IntroductionHistory Mathematical formulation Tests show Fundamental concepts show Phenomena show EquationsFormalisms show Solutions show Scientists Physics portal Category vte The positive energy theorem (also known as the positive mass theorem) refers to a collection of foundational results dentro general relativity e differential geometry. Its standard form, broadly speakdentrog, asserts that the gravitational energy of an isolated system is nonnegative, and can only be zero when the system has no gravitating objects. Although these statements are often thought of as being primarily physical in nature, they can be formalized as mathematical theorems which can be proven using techniques of differential geometry, partial differential equations, and geometric measure theory.

Richard Schoen and Shing-Tung Yau, in 1979 and 1981, were the first to give proofs of the positive mass theorem. Edward Witten, in 1982, gave the outlines of an alternative proof, which were later filled in rigorously by mathematicians. Witten and Yau were awarded the Fields medal in mathematics in part for their work on this topic.

An imprecise formulation of the Schoen-Yau / Witten positive energy theorem states the following: Given an asymptotically flat initial data set, one can define the energy-momentum of each infinite region as an element of Minkowski space. Provided that the initial data set is geodesically complete and satisfies the dominant energy condition, each such element must be in the causal future of the origin. If any infinite region has null energy-momentum, then the initial data set is trivial in the sense that it can be geometrically embedded in Minkowski space.

The meaning of these terms is discussed below. There are alternative and non-equivalent formulations for different notions of energy-momentum and for different classes of initial data sets. Not all of these formulations have been rigorously proven, and it is currently an open problem whether the above formulation holds for initial data sets of arbitrary dimension.

Conteúdo 1 Historical overview 2 Initial data sets 3 The ends of asymptotically flat initial data sets 4 Formal statements 4.1 Schoen and Yau (1979) 4.2 Schoen and Yau (1981) 4.3 Witten (1981) 4.4 Extensions and remarks 5 Formulários 6 References Historical overview The original proof of the theorem for ADM mass was provided by Richard Schoen and Shing-Tung Yau in 1979 using variational methods and minimal surfaces. Edward Witten gave another proof in 1981 based on the use of spinors, inspired by positive energy theorems in the context of supergravity. An extension of the theorem for the Bondi mass was given by Ludvigsen and James Vickers, Gary Horowitz and Malcolm Perry, and Schoen and Yau.

Gary Gibbons, Stephen Hawking, Horowitz and Perry proved extensions of the theorem to asymptotically anti-de Sitter spacetimes and to Einstein–Maxwell theory. The mass of an asymptotically anti-de Sitter spacetime is non-negative and only equal to zero for anti-de Sitter spacetime. In Einstein–Maxwell theory, for a spacetime with electric charge {estilo de exibição Q} and magnetic charge {estilo de exibição P} , the mass of the spacetime satisfies (in Gaussian units) {displaystyle Mgeq {quadrado {Q^{2}+P^{2}}},} with equality for the Majumdar–Papapetrou extremal black hole solutions.

Initial data sets An initial data set consists of a Riemannian manifold (M, g) and a symmetric 2-tensor field k on M. One says that an initial data set (M, g, k): is time-symmetric if k is zero is maximal if trgk = 0 [1] satisfies the dominant energy condition if {estilo de exibição R^{g}-|k|_{g}^{2}+(nome do operador {tr} _{g}k)^{2}geq 2{grande |}nome do operador {div} ^{g}k-d(nome do operador {tr} _{g}k){grande |}_{g},} where Rg denotes the scalar curvature of g.[2] Note that a time-symmetric initial data set (M, g, 0) satisfies the dominant energy condition if and only if the scalar curvature of g is nonnegative. One says that a Lorentzian manifold (M, g) is a development of an initial data set (M, g, k) if there is a (necessarily spacelike) hypersurface embedding of M into M, together with a continuous unit normal vector field, such that the induced metric is g and the second fundamental form with respect to the given unit normal is k.

This definition is motivated from Lorentzian geometry. Given a Lorentzian manifold (M, g) of dimension n + 1 and a spacelike immersion f from a connected n-dimensional manifold M into M which has a trivial normal bundle, one may consider the induced Riemannian metric g = f *g as well as the second fundamental form k of f with respect to either of the two choices of continuous unit normal vector field along f. The triple (M, g, k) is an initial data set. According to the Gauss-Codazzi equations, um tem {estilo de exibição {começar{alinhado}{overline {G}}(não ,não )&={fratura {1}{2}}{Grande (}R^{g}-|k|_{g}^{2}+(nome do operador {tr} ^{g}k)^{2}{Grande )}\{overline {G}}(não ,cdot )&=d(nome do operador {tr} ^{g}k)-nome do operador {div} ^{g}k.end{alinhado}}} where G denotes the Einstein tensor Ricg - 1 / 2 Rgg of g and ν denotes the continuous unit normal vector field along f used to define k. So the dominant energy condition as given above is, in this Lorentzian context, identical to the assertion that G(ν, ⋅), when viewed as a vector field along f, is timelike or null and is oriented in the same direction as ν.[3] The ends of asymptotically flat initial data sets In the literature there are several different notions of ">

No entanto, there are some features which are common to virtually all approaches. One considers an initial data set (M, g, k) which may or may not have a boundary; let n denote its dimension. One requires that there is a compact subset K of M such that each connected component of the complement M − K is diffeomorphic to the complement of a closed ball in Euclidean space ℝn. Such connected components are called the ends of M.

Formal statements Schoen and Yau (1979) Deixar (M, g, 0) be a time-symmetric initial data set satisfying the dominant energy condition. Suponha que (M, g) is an oriented three-dimensional smooth Riemannian manifold-with-boundary, and that each boundary component has positive mean curvature. Suppose that it has one end, and it is asymptotically Schwarzschild in the following sense: Suppose that K is an open precompact subset of M such that there is a diffeomorphism Φ : ℝ3 − B1(0) → M − K, and suppose that there is a number m such that the symmetric 2-tensor {estilo de exibição h_{eu j}=(Phi^{ast }g)_{eu j}-delta _{eu j}-{fratura {m}{2|x|}}delta _{eu j}} on ℝ3 − B1(0) is such that for any i, j, p, q, the functions {estilo de exibição |x|^{2}h_{eu j}(x),} {estilo de exibição |x|^{3}parcial _{p}h_{eu j}(x),} e {estilo de exibição |x|^{4}parcial _{p}parcial _{q}h_{eu j}(x)} are all bounded.

Schoen and Yau's theorem asserts that m must be nonnegative. Se, além do que, além do mais, the functions {estilo de exibição |x|^{5}parcial _{p}parcial _{q}parcial _{r}h_{eu j}(x),} {estilo de exibição |x|^{5}parcial _{p}parcial _{q}parcial _{r}parcial _{s}h_{eu j}(x),} e {estilo de exibição |x|^{5}parcial _{p}parcial _{q}parcial _{r}parcial _{s}parcial _{t}h_{eu j}(x)} are bounded for any {estilo de exibição eu,j,p,q,r,s,t,} then m must be positive unless the boundary of M is empty and (M, g) is isometric to ℝ3 with its standard Riemannian metric.

Note that the conditions on h are asserting that h, together with some of its derivatives, are small when x is large. Since h is measuring the defect between g in the coordinates Φ and the standard representation of the t = constant slice of the Schwarzschild metric, these conditions are a quantification of the term "asymptotically Schwarzschild". This can be interpreted in a purely mathematical sense as a strong form of "asymptotically flat", where the coefficient of the |x|−1 part of the expansion of the metric is declared to be a constant multiple of the Euclidean metric, as opposed to a general symmetric 2-tensor.

Note also that Schoen and Yau's theorem, como dito acima, is actually (despite appearances) a strong form of the "multiple ends" caso. Se (M, g) is a complete Riemannian manifold with multiple ends, then the above result applies to any single end, provided that there is a positive mean curvature sphere in every other end. This is guaranteed, por exemplo, if each end is asymptotically flat in the above sense; one can choose a large coordinate sphere as a boundary, and remove the corresponding remainder of each end until one has a Riemannian manifold-with-boundary with a single end.

Schoen and Yau (1981) Deixar (M, g, k) be an initial data set satisfying the dominant energy condition. Suponha que (M, g) is an oriented three-dimensional smooth complete Riemannian manifold (without boundary); suppose that it has finitely many ends, each of which is asymptotically flat in the following sense.

Suponha que {displaystyle Ksubset M} is an open precompact subset such that {displaystyle Msmallsetminus K} has finitely many connected components {estilo de exibição M_{1},ldots ,M_{n},} and for each {estilo de exibição i=1,ldots ,n} existe um difeomorfismo {displaystyle Phi _{eu}:mathbb {R} ^{3}smallsetminus B_{1}(0)to M_{eu}} such that the symmetric 2-tensor {estilo de exibição h_{eu j}=(Phi^{ast }g)_{eu j}-delta _{eu j}} satisfies the following conditions: {estilo de exibição |x|h_{eu j}(x),} {estilo de exibição |x|^{2}parcial _{p}h_{eu j}(x),} e {estilo de exibição |x|^{3}parcial _{p}parcial _{q}h_{eu j}(x)} are bounded for all {estilo de exibição eu,j,p,q.} Also suppose that {estilo de exibição |x|^{4}R^{Phi _{eu}^{ast }g}} e {estilo de exibição |x|^{5}parcial _{p}R^{Phi _{eu}^{ast }g}} are bounded for any {estilo de exibição p} {estilo de exibição |x|^{2}(Phi _{eu}^{ast }k)_{eu j}(x),} {estilo de exibição |x|^{3}parcial _{p}(Phi _{eu}^{ast }k)_{eu j}(x),} e {estilo de exibição |x|^{4}parcial _{p}parcial _{q}(Phi _{eu}^{ast }k)_{eu j}(x)} para qualquer {estilo de exibição p,q,eu,j} {estilo de exibição |x|^{3}((Phi _{eu}^{ast }k)_{11}(x)+(Phi^{ast }k)_{22}(x)+(Phi _{eu}^{ast }k)_{33}(x))} é limitado.

The conclusion is that the ADM energy of each {estilo de exibição M_{1},ldots ,M_{n},} definido como {estilo de exibição {texto{E}}(M_{eu})={fratura {1}{16pi }}lim_{rto infty }int_{|x|=r}soma _{p=1}^{3}soma _{q=1}^{3}{grande (}parcial _{q}(Phi _{eu}^{ast }g)_{pq}-parcial _{p}(Phi _{eu}^{ast }g)_{qq}{grande )}{fratura {x^{p}}{|x|}},d{matemática {H}}^{2}(x),} is nonnegative. Além disso, supposing in addition that {estilo de exibição |x|^{4}parcial _{p}parcial _{q}parcial _{r}h_{eu j}(x)} e {estilo de exibição |x|^{4}parcial _{p}parcial _{r}parcial _{s}parcial _{t}h_{eu j}(x)} are bounded for any {estilo de exibição eu,j,p,q,r,s,} the assumption that {estilo de exibição {texto{E}}(M_{eu})=0} para alguns {displaystyle iin {1,ldots ,n}} implies that n = 1, that M is diffeomorphic to ℝ3, and that Minkowski space ℝ3,1 is a development of the initial data set (M, g, k).

Witten (1981) Deixar {estilo de exibição (M,g)} be an oriented three-dimensional smooth complete Riemannian manifold (without boundary). Deixar {estilo de exibição k} be a smooth symmetric 2-tensor on {estilo de exibição M} de tal modo que {estilo de exibição R^{g}-|k|_{g}^{2}+(nome do operador {tr} _{g}k)^{2}geq 2{grande |}nome do operador {div} ^{g}k-d(nome do operador {tr} _{g}k){grande |}_{g}.} Suponha que {displaystyle Ksubset M} is an open precompact subset such that {displaystyle Msmallsetminus K} has finitely many connected components {estilo de exibição M_{1},ldots ,M_{n},} and for each {displaystyle alpha =1,ldots ,n} existe um difeomorfismo {displaystyle Phi _{alfa }:mathbb {R} ^{3}smallsetminus B_{1}(0)to M_{eu}} such that the symmetric 2-tensor {estilo de exibição h_{eu j}=(Phi _{alfa }^{ast }g)_{eu j}-delta _{eu j}} satisfies the following conditions: {estilo de exibição |x|h_{eu j}(x),} {estilo de exibição |x|^{2}parcial _{p}h_{eu j}(x),} e {estilo de exibição |x|^{3}parcial _{p}parcial _{q}h_{eu j}(x)} are bounded for all {estilo de exibição eu,j,p,q.} {estilo de exibição |x|^{2}(Phi _{alfa }^{ast }k)_{eu j}(x)} e {estilo de exibição |x|^{3}parcial _{p}(Phi _{alfa }^{ast }k)_{eu j}(x),} are bounded for all {estilo de exibição eu,j,p.} For each {displaystyle alpha =1,ldots ,n,} define the ADM energy and linear momentum by {estilo de exibição {texto{E}}(M_{alfa })={fratura {1}{16pi }}lim_{rto infty }int_{|x|=r}soma _{p=1}^{3}soma _{q=1}^{3}{grande (}parcial _{q}(Phi _{alfa }^{ast }g)_{pq}-parcial _{p}(Phi _{alfa }^{ast }g)_{qq}{grande )}{fratura {x^{p}}{|x|}},d{matemática {H}}^{2}(x),} {estilo de exibição {texto{P}}(M_{alfa })_{p}={fratura {1}{8pi }}lim_{rto infty }int_{|x|=r}soma _{q=1}^{3}{grande (}(Phi _{alfa }^{ast }k)_{pq}-{grande (}(Phi _{alfa }^{ast }k)_{11}+(Phi _{alfa }^{ast }k)_{22}+(Phi _{alfa }^{ast }k)_{33}{grande )}delta _{pq}{grande )}{fratura {x^{q}}{|x|}},d{matemática {H}}^{2}(x).} For each {displaystyle alpha =1,ldots ,n,} consider this as a vector {estilo de exibição ({texto{P}}(M_{alfa })_{1},{texto{P}}(M_{alfa })_{2},{texto{P}}(M_{alfa })_{3},{texto{E}}(M_{alfa }))} in Minkowski space. Witten's conclusion is that for each {alfa de estilo de exibição } it is necessarily a future-pointing non-spacelike vector. If this vector is zero for any {alfa de estilo de exibição ,} então {estilo de exibição n=1,} {estilo de exibição M} is diffeomorphic to {estilo de exibição mathbb {R} ^{3},} and the maximal globally hyperbolic development of the initial data set {estilo de exibição (M,g,k)} has zero curvature.

Extensions and remarks According to the above statements, Witten's conclusion is stronger than Schoen and Yau's. No entanto, a third paper by Schoen and Yau[4] shows that their 1981 result implies Witten's, retaining only the extra assumption that {estilo de exibição |x|^{4}R^{Phi _{eu}^{ast }g}} e {estilo de exibição |x|^{5}parcial _{p}R^{Phi _{eu}^{ast }g}} are bounded for any {displaystyle p.} It also must be noted that Schoen and Yau's 1981 result relies on their 1979 resultado, which is proved by contradiction; therefore their extension of their 1981 result is also by contradiction. Por contraste, Witten's proof is logically direct, exhibiting the ADM energy directly as a nonnegative quantity. Além disso, Witten's proof in the case {nome do operador de estilo de exibição {tr} _{g}k=0} can be extended without much effort to higher-dimensional manifolds, under the topological condition that the manifold admits a spin structure.[5] Schoen and Yau's 1979 result and proof can be extended to the case of any dimension less than eight.[6] Mais recentemente, Witten's result, using Schoen and Yau (1981)'s methods, has been extended to the same context.[7] Resumindo: following Schoen and Yau's methods, the positive energy theorem has been proven in dimension less than eight, while following Witten, it has been proven in any dimension but with a restriction to the setting of spin manifolds.

As of April 2017, Schoen and Yau have released a preprint which proves the general higher-dimensional case in the special case {nome do operador de estilo de exibição {tr} _{g}k=0,} without any restriction on dimension or topology. No entanto, it has not yet (as of May 2020) appeared in an academic journal.

Applications In 1984 Schoen used the positive mass theorem in his work which completed the solution of the Yamabe problem. The positive mass theorem was used in Hubert Bray's proof of the Riemannian Penrose inequality. References ^ In local coordinates, this says gijkij = 0 ^ In local coordinates, this says R - gikgjlkijkkl + (gijkij)2 ≥ 2(gpq(gijkpi;j - (gijkij);p)(gklkqk;eu - (gklkkl);q))1/2 ou, in the usual "raised and lowered index" notation, this says R - kijkij + (kii)2 ≥ 2((kpi;eu - (kii);p)(kpj;j - (kjj);p))1/2 ^ It is typical to assume M to be time-oriented and for ν to be then specifically defined as the future-pointing unit normal vector field along f; in this case the dominant energy condition as given above for an initial data set arising from a spacelike immersion into M is automatically true if the dominant energy condition in its usual spacetime form is assumed. ^ Schoen, Ricardo; Hoje, Shing Tung (1981). "The energy and the linear momentum of space-times in general relativity". Comunicação. Matemática. Física. 79 (1): 47–51. doi:10.1007/BF01208285. S2CID 120151656. ^ Bartnik, Roberto (1986). "The mass of an asymptotically flat manifold". Comunicação. Pure Appl. Matemática. 39 (5): 661–693. doi:10.1002/cpa.3160390505. ^ Schoen, Ricardo M. (1989). "Variational theory for the total scalar curvature functional for Riemannian metrics and related topics". Topics in calculus of variations (Montecatini Terme, 1987). Notas de aula em matemática. Volume. 1365. Berlim: Springer. pp. 120–154. ^ Eichmair, Michael; Huang, Lan-Hsuan; Lee, Dan A.; Schoen, Ricardo (2016). "The spacetime positive mass theorem in dimensions less than eight". J. Eur. Matemática. Soc. 18 (1): 83–121. arXiv:1110.2087. doi:10.4171/JEMS/584. S2CID 119633794. Schoen, Ricardo; Hoje, Shing-Tung (1979). "On the proof of the positive mass conjecture in general relativity". Communications in Mathematical Physics. 65 (1): 45–76. doi:10.1007/bf01940959. ISSN 0010-3616. S2CID 54217085. Schoen, Ricardo; Hoje, Shing-Tung (1981). "Proof of the positive mass theorem. II". Communications in Mathematical Physics. 79 (2): 231-260. doi:10.1007/bf01942062. ISSN 0010-3616. S2CID 59473203. Witten, Eduardo (1981). "A new proof of the positive energy theorem". Communications in Mathematical Physics. 80 (3): 381–402. doi:10.1007/bf01208277. ISSN 0010-3616. S2CID 1035111. Ludvigsen, M; Vickers, J A G (1981-10-01). "The positivity of the Bondi mass". Revista de Física A: Matemática e Geral. 14 (10): L389–L391. doi:10.1088/0305-4470/14/10/002. ISSN 0305-4470. Horowitz, Gary T.; Perry, Malcolm J. (1982-02-08). "Gravitational Energy Cannot Become Negative". Cartas de Revisão Física. 48 (6): 371–374. doi:10.1103/physrevlett.48.371. ISSN 0031-9007. Schoen, Ricardo; Hoje, Shing Tung (1982-02-08). "Proof That the Bondi Mass is Positive". Cartas de Revisão Física. 48 (6): 369-371. doi:10.1103/physrevlett.48.369. ISSN 0031-9007. Gibbons, G. C.; Hawking, S. C.; Horowitz, G. T.; Perry, M. J. (1983). "Positive mass theorems for black holes". Communications in Mathematical Physics. 88 (3): 295-308. doi:10.1007/BF01213209. MR 0701918. S2CID 121580771.

Textbooks Choquet-Bruhat, Yvonne. General relativity and the Einstein equations. Monografias Matemáticas Oxford. imprensa da Universidade de Oxford, Oxford, 2009. xxvi+785 pp. ISBN 978-0-19-923072-3 Wald, Roberto M. Relatividade geral. Imprensa da Universidade de Chicago, Chicago, IL, 1984. xiii+491 pp. ISBN 0-226-87032-4 Categorias: Mathematical methods in general relativityTheorems in general relativity

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