Oddziaływania czarnych dziur-Reference-Cited by-同舟云学术

Oddziaływania czarnych dziur

Published:2023-09-20 Issue:3 Volume:74 Page:15-23
ISSN:0032-5430
Container-title:Postępy Fizyki
language:
Short-container-title:PF

Author:

Szybka Sebastian J.,

Abstract

The final stage of an unrestrained gravitational collapse is a single object known as a black hole. Do black holes always have the same universal form? Although the uniqueness theorem provides a positive answer to this question, every theorem is only as strong as its assumptions. For many years physicists were unable to exclude the existence of stationary configurations of two black holes that could form together a more complex object. Currently, we know the solution to this problem.

Publisher

University of Warsaw

Reference45 articles.

1. [1] LIGO Scientific Collaboration and Virgo Collaboration, "Observation of GravitationalWaves from a Binary Black Hole Merger", Physical Review Letters,116 (6): 061102 (2016).

2. [2] The Event Horizon Telescope Collaboration, "First M87 Event Horizon Telescope Results. I.The Shadow of the Supermassive Black Hole",The Astrophysical Journal Letters. 875 (1): L1 (2019).

3. [3] Szybka S. J., "On gravitational interactions between two bodies" w: Mathematical Structures of the Universe, red. M. Eckstein, M. Heller, S.J. Szybka,CCPress, 2014, 137-151.

4. [4] Liu F. K., "X-shaped radio galaxies as observational evidence for the interaction of supermassive binary black holes and accretion disc at parsec scale",Monthly Notices of the Royal Astronomical Society, 347,4:1357-1369 (2004).

5. [5] Deane R. P. , Paragi Z., Jarvis M. J. , Coriat M., Bernardi G., Fender R. P. ,Frey S., Heywood I., Klockner H.-R., Grainge K., Rumsey C., "A close-pair binary in a distant triple supermassive black hole system", Nature, 511, 57 (2014).