Speaker
Ms.
Asya Aynbund
(MIPT)
Description
Cones of future and past are rigorously constructed under the horizon of black hole by completions of geodesics continued from causally connected space-time regions outside the black hole interior. Treating the Schwarzschild black hole as a zero charge limit of Reissner—Nordsrom black hole reforms the Penrose—Carter diagram into the infinite band that excludes the closed proper-time cycles under the geodesic motion. The marginal trajectories between the cones of future and past compose paths common with a compact non-Hausdorff spherical extension of black hole interior forming the thermal bath for particles fallen to the black hole.
Primary authors
Ms.
Asya Aynbund
(MIPT)
Dr.
Valery V. Kiselev
(MIPT, IHEP NRC «Kurchatov Institute»)
