pseudo riemannian manifold
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Pseudo Riemannian ManifoldPseudo Riemannian ManifoldPseudo Riemannian ManifoldPseudo Riemannian ManifoldPseudo Riemannian ManifoldTRANSCRIPT
Pseudo-Riemannian manifold
In differential geometry, a pseudo-Riemannian mani-fold[1][2] (also called a semi-Riemannian manifold) isa generalization of a Riemannian manifold in which themetric tensor need not be positive-definite. Instead aweaker condition of nondegeneracy is imposed on themetric tensor.The tangent space of a pseudo-Riemannian manifoldis a pseudo-Euclidean space described by an isotropicquadratic form.A special case of great importance to general relativityis a Lorentzian manifold, in which one dimension hasa sign opposite to that of the rest. This allows tangentvectors to be classified into timelike, null, and spacelike.Spacetime can be modeled as a 4-dimensional Lorentzianmanifold.
1 Introduction
1.1 Manifolds
Main articles: Manifold and Differentiable manifold
In differential geometry, a differentiable manifold is aspace which is locally similar to a Euclidean space. Inan n-dimensional Euclidean space any point can be spec-ified by n real numbers. These are called the coordinatesof the point.An n-dimensional differentiable manifold is a generalisa-tion of n-dimensional Euclidean space. In a manifold itmay only be possible to define coordinates locally. Thisis achieved by defining coordinate patches: subsets of themanifold which can be mapped into n-dimensional Eu-clidean space.See Manifold, differentiable manifold, coordinate patchfor more details.
1.2 Tangent spaces and metric tensors
Main articles: Tangent space and metric tensor
Associated with each point p in an n -dimensional dif-ferentiable manifold M is a tangent space (denoted TpM
). This is an n -dimensional vector space whose elementscan be thought of as equivalence classes of curves passingthrough the point p .
A metric tensor is a non-degenerate, smooth, symmetric,bilinear map which assigns a real number to pairs of tan-gent vectors at each tangent space of the manifold. De-noting the metric tensor by g we can express this as
g : TpM × TpM → R.
The map is symmetric and bilinear so if X,Y,Z∈TpM aretangent vectors at a point p to the manifold M then wehave
• g(X,Y ) = g(Y,X)
• g(aX + Y,Z) = ag(X,Z) + g(Y, Z)
for any real number a∈R .That g is non-degenerate means there are no non-zeroX ∈ TpM such that g(X,Y ) = 0 for all Y ∈ TpM.
1.3 Metric signatures
Main article: Metric signature
Given a metric tensor g on an n-dimensional real mani-fold, the quadratic form q(x) = g(x, x) associated with themetric tensor applied to each vector of any orthogonalbasis produces n real values. By Sylvester’s law of iner-tia, the number of each positive, negative and zero valuesproduced in this manner are invariants of the metric ten-sor, independent of the choice of orthogonal basis. Thesignature (p, q, r) of the metric tensor gives these num-bers, shown in the same order. A non-degenerate metrictensor has r = 0 and the signature may be denoted (p, q),where p + q = n.
2 Definition
A pseudo-Riemannian manifold (M, g) is adifferentiable manifold M equipped with a non-degenerate, smooth, symmetric metric tensor g .Such a metric is called a pseudo-Riemannian metricand its values can be positive, negative or zero.The signature of a pseudo-Riemannian metric is (p, q),where both p and q are non-negative.
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2 7 REFERENCES
3 Lorentzian manifold
A Lorentzian manifold is an important special case ofa pseudo-Riemannian manifold in which the signature ofthe metric is (1, n−1) (or sometimes (n−1, 1), see signconvention). Such metrics are called Lorentzian met-rics. They are named after the physicist Hendrik Lorentz.
3.1 Applications in physics
After Riemannian manifolds, Lorentzian manifolds formthe most important subclass of pseudo-Riemannian man-ifolds. They are important in applications of general rel-ativity.A principal basis of general relativity is that spacetimecan be modeled as a 4-dimensional Lorentzian manifoldof signature (3, 1) or, equivalently, (1, 3). Unlike Rie-mannianmanifolds with positive-definitemetrics, a signa-ture of (p, 1) or (1, q) allows tangent vectors to be classi-fied into timelike, null or spacelike (see Causal structure).
4 Properties of pseudo-Riemannian manifolds
Just as Euclidean spaceRn can be thought of as themodelRiemannian manifold, Minkowski spaceRn−1,1 with theflat Minkowski metric is the model Lorentzian mani-fold. Likewise, themodel space for a pseudo-Riemannianmanifold of signature (p, q) is Rp,q with the metric
g = dx21 + · · ·+ dx2
p − dx2p+1 − · · · − dx2
p+q
Some basic theorems of Riemannian geometry can begeneralized to the pseudo-Riemannian case. In particu-lar, the fundamental theorem of Riemannian geometryis true of pseudo-Riemannian manifolds as well. Thisallows one to speak of the Levi-Civita connection on apseudo-Riemannian manifold along with the associatedcurvature tensor. On the other hand, there are many the-orems in Riemannian geometry which do not hold in thegeneralized case. For example, it is not true that everysmooth manifold admits a pseudo-Riemannian metric ofa given signature; there are certain topological obstruc-tions. Furthermore, a submanifold does not always in-herit the structure of a pseudo-Riemannian manifold; forexample, the metric tensor becomes zero on any light-like curve. The Clifton–Pohl torus provides an exam-ple of a pseudo-Riemannian manifold that is compact butnot complete, a combination of properties that the Hopf–Rinow theorem disallows for Riemannian manifolds.[3]
5 See also• Spacetime
• Hyperbolic partial differential equation
• Causality conditions
• Globally hyperbolic manifold
6 Notes[1] Benn & Tucker (1987), p. 172.
[2] Bishop & Goldberg (1968), p. 208
[3] O'Neill (1983), p. 193.
7 References• Benn, I.M.; Tucker, R.W. (1987), An introduction toSpinors and Geometry with Applications in Physics(First published 1987 ed.), Adam Hilger, ISBN 0-85274-169-3
• Bishop, Richard L.; Goldberg, Samuel I. (1968),Tensor Analysis on Manifolds (First Dover 1980ed.), The Macmillan Company, ISBN 0-486-64039-6
• Chen, Bang-Yen (2011), Pseudo-Riemannian Ge-ometry, [delta]-invariants and Applications, WorldScientific Publisher, ISBN 978-981-4329-63-7
• O'Neill, Barrett (1983), Semi-Riemannian Geome-try With Applications to Relativity, Pure and Ap-plied Mathematics 103, Academic Press, ISBN9780080570570
• Vrănceanu, G.; Roşca, R. (1976), Introduction toRelativity and Pseudo-Riemannian Geometry, Bu-carest: Editura Academiei Republicii SocialisteRomânia.
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