Pseudo-Riemannian manifold

(Redirected from Lorentzian manifolds)

In differential geometry, a pseudo-Riemannian manifold[1][2] (also called a semi-Riemannian manifold) is a generalization of a Riemannian manifold in which the metric tensor need not be positive-definite, but is instead only required to be nondegenerate, which is a weaker condition.

Every tangent space of a pseudo-Riemannian manifold is a pseudo-Euclidean space described by a quadratic form, which may be isotropic.

A special case of great importance to general relativity is a Lorentzian manifold, in which one dimension has a sign opposite to that of the rest. This allows tangent vectors to be classified into timelike, null, and spacelike. Spacetime can be modeled as a 4-dimensional Lorentzian manifold.

Introduction

Manifolds

In differential geometry, a differentiable manifold is a space which is locally similar to a Euclidean space. In an n-dimensional Euclidean space any point can be specified by n real numbers. These are called the coordinates of the point.

An n-dimensional differentiable manifold is a generalisation of n-dimensional Euclidean space. In a manifold it may only be possible to define coordinates locally. This is achieved by defining coordinate patches: subsets of the manifold which can be mapped into n-dimensional Euclidean space.

See Manifold, differentiable manifold, coordinate patch for more details.

Tangent spaces and metric tensors

Associated with each point ${\displaystyle p}$ in an ${\displaystyle n}$-dimensional differentiable manifold ${\displaystyle M}$ is a tangent space (denoted ${\displaystyle T_{p}M}$). This is an ${\displaystyle n}$-dimensional vector space whose elements can be thought of as equivalence classes of curves passing through the point ${\displaystyle p}$.

A metric tensor is a non-degenerate, smooth, symmetric, bilinear map that assigns a real number to pairs of tangent vectors at each tangent space of the manifold. Denoting the metric tensor by ${\displaystyle g}$ we can express this as

${\displaystyle g:T_{p}M\times T_{p}M\to \mathbb {R} .}$

The map is symmetric and bilinear so if ${\displaystyle X,Y,Z\in T_{p}M}$ are tangent vectors at a point ${\displaystyle p}$ to the manifold ${\displaystyle M}$ then we have

• ${\displaystyle \,g(X,Y)=g(Y,X)}$
• ${\displaystyle \,g(aX+Y,Z)=ag(X,Z)+g(Y,Z)}$

for any real number ${\displaystyle a\in \mathbb {R} }$.

That ${\displaystyle g}$ is non-degenerate means there are no non-zero ${\displaystyle X\in T_{p}M}$ such that ${\displaystyle \,g(X,Y)=0}$ for all ${\displaystyle Y\in T_{p}M}$.

Metric signatures

Given a metric tensor g on an n-dimensional real manifold, the quadratic form q(x) = g(x, x) associated with the metric tensor applied to each vector of any orthogonal basis produces n real values. By Sylvester's law of inertia, the number of each positive, negative and zero values produced in this manner are invariants of the metric tensor, independent of the choice of orthogonal basis. The signature (p, q, r) of the metric tensor gives these numbers, shown in the same order. A non-degenerate metric tensor has r = 0 and the signature may be denoted (p, q), where p + q = n.

Definition

A pseudo-Riemannian manifold ${\displaystyle (M,g)}$ is a differentiable manifold ${\displaystyle M}$ equipped with a non-degenerate, smooth, symmetric metric tensor ${\displaystyle g}$.

Such a metric is called a pseudo-Riemannian metric. Applied to a vector field, its value can be positive, negative or zero.

The signature of a pseudo-Riemannian metric is (p, q), where both p and q are non-negative.

Lorentzian manifold

A Lorentzian manifold is an important special case of a pseudo-Riemannian manifold in which the signature of the metric is (1, n−1) (equivalently, (n−1, 1); see sign convention). Such metrics are called Lorentzian metrics. They are named after the physicist Hendrik Lorentz.

Applications in physics

After Riemannian manifolds, Lorentzian manifolds form the most important subclass of pseudo-Riemannian manifolds. They are important in applications of general relativity.

A principal basis of general relativity is that spacetime can be modeled as a 4-dimensional Lorentzian manifold of signature (3, 1) or, equivalently, (1, 3). Unlike Riemannian manifolds with positive-definite metrics, a signature of (p, 1) or (1, q) allows tangent vectors to be classified into timelike, null or spacelike (see Causal structure).

Properties of pseudo-Riemannian manifolds

Just as Euclidean space ${\displaystyle \mathbb {R} ^{n}}$ can be thought of as the model Riemannian manifold, Minkowski space ${\displaystyle \mathbb {R} ^{n-1,1}}$ with the flat Minkowski metric is the model Lorentzian manifold. Likewise, the model space for a pseudo-Riemannian manifold of signature (p, q) is ${\displaystyle \mathbb {R} ^{p,q}}$ with the metric

${\displaystyle g=dx_{1}^{2}+\cdots +dx_{p}^{2}-dx_{p+1}^{2}-\cdots -dx_{p+q}^{2}}$

Some basic theorems of Riemannian geometry can be generalized to the pseudo-Riemannian case. In particular, the fundamental theorem of Riemannian geometry is true of pseudo-Riemannian manifolds as well. This allows one to speak of the Levi-Civita connection on a pseudo-Riemannian manifold along with the associated curvature tensor. On the other hand, there are many theorems in Riemannian geometry which do not hold in the generalized case. For example, it is not true that every smooth manifold admits a pseudo-Riemannian metric of a given signature; there are certain topological obstructions. Furthermore, a submanifold does not always inherit the structure of a pseudo-Riemannian manifold; for example, the metric tensor becomes zero on any light-like curve. The Clifton–Pohl torus provides an example of a pseudo-Riemannian manifold that is compact but not complete, a combination of properties that the Hopf–Rinow theorem disallows for Riemannian manifolds.[3]