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22 CHRISTIAN KETTERER

speration function

\tau_{B\times_fF}((p,x),(q,y)):=\sup L(\gamma)

where the sup is w.r.t. all future directed causal curves \gamma that connect (p,x) and (q,y) . If there is no such curve, one sets \tau((p,x),(q,y))=0 . \tau_{B\times_fF} satisfies the reverse \triangle -inequality

\tau_{B\times_fF}((p,x),(q,y))\ge\tau_{B\times_fF}((p,x),(r,z))+\tau_{B\times_fF}((r,z),(q,y)).

For all (p,x),(q,y),(r,z)\in I\times F . In the following we write also \tau_{B\times_fF}=\tau .

The time seperation function has the following properties:

  • \tau(y,y')=0 if y' and y are not cuassally related,
  • \tau(y,y')>0 if y\ll y' .

The generalized Lorentzian cone w.r.t. -I , the metric space F and the function f:I\to(0,\infty) is

(I\times F,D,\ll,\le,\tau)=:-I\times_fF.

If F is an intrinsic metric space, then -I\times_fF is a Lorentzian pre-length space in the sense of [KS18].

Here we collect some properties of -I\times_fF . We always assume that F is intrinsic.

  • -I\times_fF has the push-up property: if (s,x)\ll(t,y) if and only if there exists a future directed causal curve from (s,x) to (t,y) with positive length. Moreover I^{+/-}((s,x)) is open for all (s,t)\in I\times F .
  • If F is geodesic, then J^\pm((s,x)) is closed for all (s,x)\in I\times F .

The next theorem is the Lorentzian analogue of Theorem 2.5 above.

Theorem 3.1 (Kunzinger, Saemann, Graf, Alexander). Let X be a strictly intrinsic metric space and let \gamma=(\alpha,\beta) be a future directed, causal curve that is a maximizer w.r.t. L in -I\times_fF and parametrized proportional to arclength. Then

  1. \beta is a minimizer in F ;
  2. (Fiber independence) \alpha is independent of F , except for the total height, i.e. the length L^F(\beta) of \beta . More precisely, if \hat{F} is another strictly intrinsic metric space and \hat{\beta} is a minimizing geodesic in \hat{F} with the same length and speed as \beta , then (\alpha,\hat{\beta}) is a minimizer in -I\times_f\hat{F} .
  3. If \gamma is timelike, then \beta has speed \frac{c_\gamma}{2f^2\circ\alpha} for a constant c_\gamma .
  4. If \gamma is timelike, then -\frac{1}{2}(\alpha')^2+\frac{1}{2f^2\circ\alpha}=E for a constant E .

We stated above that a generalized cone -I\times_fF over an intrinsic metric space F is a Lorentzian pre-length space. If F is locally compact, it was shown in [AGKS23] that -I\times_fF is even a Lorentzian length space.

Theorem 3.2. Let F be a locally compact length space. Then -I\times_fF is a strongly causal Lorentzian length space.