Analysis of the Forming for Black Hole and Connections with Timespace
DOI:
https://doi.org/10.61173/tbx92e27Keywords:
Event horizon, Schwarzschild radius formulae, accretion disk, relativistic jetsAbstract
Black holes remain the most popular topic in astronomy to this day because of the mystery that makes it so thoughtprovoking. It forms when a star collapses or a huge mass gather. The greater the mass of the black hole, the greater the gravitational field and the faster the galaxies contract, and eventually a massive galaxy will be swallowed up by this black hole and form a singularity. Their immense mass can bend and distort the space-time around them, and this distorting effect leads to a gravitational trap that makes it impossible for anything approaching the black hole to escape its gravitational pull, not even light or radiation. This study begins with an introduction to the basic formation principles and structure of black holes and introduces why it is related to space-time, followed by a description of how black holes are observed, their limitations, and future prospects. According to the analysis, one can acquire more knowledge about this mysterious object and lay the foundation for future research on black holes.
References
[1] Michell J. Vii. on the means of discovering the distance, magnitude, &c. of the fixed stars, in consequence of the diminution of the velocity of their light, in case such a diminution should be found to take place in any of them, and such other data should be procured from observations, as would be farther necessary for that purpose. by the rev. john michell, bdfrs in a letter to henry cavendish, esq. frs and as. Philosophical transactions of the Royal Society of London, 1784 (74): 35-57.
[2] Phillips J. Geology of Oxford and the Valley of the Thames. Clarendon Press, 1871.
[3] LaPlace P S. Exposition du Syste`m du Monde. Paris, 1796.
[4] Luminet J P. An illustrated history of black hole imaging: Personal recollections (1972-2002). arXiv preprint arXiv:1902.11196, 2019.
[5] Panuzzo P, Mazeh T, Arenou F, et al. Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry. Astronomy & Astrophysics, 2024, 686: L2.
[6] Natarajan P, Pacucci F, Ricarte A, et al. First Detection of an Overmassive Black Hole Galaxy UHZ1: Evidence for Heavy Black Hole Seed Formation from Direct Collapse. The Astrophysical Journal Letters, 2023, 960(1): L1.
[7] Fryer C L, Kalogera V. Theoretical black hole mass distributions. The Astrophysical Journal, 2001, 554(1): 548.
[8] Volonteri M. Formation of supermassive black holes. The Astronomy and Astrophysics Review, 2010, 18: 279-315.
[9] Bambi C. Astrophysical black holes: a review. arXiv preprint arXiv:1906.03871, 2019.
[10] Konoplya R A, Zhidenko A. Quasinormal modes of black holes: From astrophysics to string theory. Reviews of Modern Physics, 2011, 83(3): 793-836.
[11] Abramowicz M A, Kluźniak W, Lasota J P. No observational proof of the black-hole event-horizon. Astronomy & Astrophysics, 2002, 396(3): L31-L34.
[12] Gadioux M, Reall H S. Creases, corners, and caustics: Properties of nonsmooth structures on black hole horizons. Physical Review D, 2023, 108(8): 084021.
[13] de Paula M A A, Leite L C S, Dolan S R, et al. Absorption and unbounded superradiance in a static regular black hole spacetime. Physical Review D, 2024, 109(6): 064053.
[14] Akiyama K, Alberdi A, Alef W, et al. First M87 event horizon telescope results. IV. Imaging the central supermassive black hole. The Astrophysical Journal Letters, 2019, 875(1): L4.
[15] DeBenedictis A. Developments in black hole research: Classical, semi-classical, and quantum. arXiv preprint arXiv:0711.2279, 2007.
[16] Anchordoqui L A, Antoniadis I, Lüst D. More on black holes perceiving the dark dimension. Physical Review D, 2024, 110(1): 015004.
[17] Korwar M, Profumo S. Updated constraints on primordial black hole evaporation. Journal of Cosmology and Astroparticle Physics, 2023, 2023(05): 054.
[18] Reynolds C S. Observing black holes spin. Nature Astronomy, 2019, 3(1): 41-47.
[19] Chartas G, Krawczynski H, Zalesky L, et al. Measuring the innermost stable circular orbits of supermassive black holes. The Astrophysical Journal, 2017, 837(1): 26.
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