Asymptotic behavior of null geodesics near future null infinity. III. Photons towards inward directions

Abstract

A new sufficient condition for photons emitted near future null infinity to reach future null infinity is derived by studying null geodesics in the Bondi coordinates in asymptotically flat spacetimes. In our previous works [arXiv:2106.03150, arXiv:2110.10917], such a condition was established for photons emitted in outward or tangential directions to constant radial surfaces. This paper improves our previous result by including photons emitted in inward directions. In four dimensions, imposing the same assumptions on the metric functions as previously, we prove that photons reach future null infinity if their initial values of $|dr/du|$ are smaller than a certain quantity, where $r$ and $u$ are the radial and retarded time coordinates, respectively. This quantity is determined by the asymptotic properties of the metric and is connected to the conjectured maximal luminosity. In higher dimensions, photons emitted with $dr/du>-(1-1/\sqrt{3})\approx -0.423$ are shown to reach future null infinity without the assumptions on the metric functions.

19 pages, no figures

References in corpus (6)

• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• Fundamental photon orbits: black hole shadows and spacetime instabilities
• Asymptotic flatness at null infinity in higher dimensional gravity
• Higher Dimensional Bondi Energy with a Globally Specified Background Structure
• Gravitational Machines
• Asymptotic behavior of null geodesics near future null infinity: Significance of gravitational waves