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Silhouettes of invisible black holes

 a, b,  c, d
a Institute for Nuclear Research, Russian Academy of Sciences, prosp. 60-letiya Oktyabrya 7a, Moscow, 117312, Russian Federation
b National Research Nuclear University ‘MEPhI’, Kashirskoe shosse 31, Moscow, 115409, Russian Federation
c The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy
d Scuola Internazionale Superiore di Studi Avanzati, via Bonomea, 265, Trieste, 34136, Italy

In general relativity, isolated black holes are invisible objects due to their intrinsic physical properties. Nevertheless, the dark silhouettes of astrophysical black holes may be visible to a distant observer as a result of emitting matter lensing in the gravitational field of black holes. The most probable astrophysical conditions for the experimental detection of a dark black hole silhouette are either the stationary luminous background behind the black hole or nonstationary hot matter plunging into the black hole and having emissions approaching the black hole horizon. The black hole shadow is observed in the case of a stationary luminous background, which is a projection on the celestial sphere of the photon capture cross section in the black hole gravitational field. Meanwhile, in the case of nonstationary emitting matter in the inner part of the thin accretion disk adjoining the event horizon, a dark silhouette of the event horizon itself would be seen. This dark silhouette of the event horizon is seen in the first image of the supermasive black hole M87* presented by the Event Horizon Telescope international collaboration. The brightness of accretion matter is much higher than the corresponding one of the usual astrophysical stationary background in the form of numerous stars or extensive hot gas clouds. For this reason, it is improbable that a black hole shadow can be observed in the presence of very luminous accretion matter.

Fulltext pdf (958 KB)
Fulltext is also available at DOI: 10.3367/UFNe.2020.01.038717
Keywords: gravitation theory, general relativity, black holes, event horizon, gravitational lensing
PACS: 04.70.Bw, 98.35.Jk, 98.62.Js (all)
DOI: 10.3367/UFNe.2020.01.038717
URL: https://ufn.ru/en/articles/2020/6/d/
000563842900004
2-s2.0-85092023307
2020PhyU...63..583D
Citation: Dokuchaev V I, Nazarova N O "Silhouettes of invisible black holes" Phys. Usp. 63 583–600 (2020)
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Received: 5th, November 2019, revised: 4th, December 2019, 15th, January 2020

Оригинал: Докучаев В И, Назарова Н О «Силуэты невидимых чёрных дыр» УФН 190 627–647 (2020); DOI: 10.3367/UFNr.2020.01.038717

References (339) Cited by (59) Similar articles (20) ↓

  1. V.I. Dokuchaev, Yu.N. Eroshenko “Physical laboratory at the center of the Galaxy” Phys. Usp. 58 772–784 (2015)
  2. N.S. Kardashev, I.D. Novikov et al “Review of scientific topics for Millimetron space observatory” Phys. Usp. 57 1199–1228 (2014)
  3. I.D. Novikov “A new concept of wormholes and the Multiverse” Phys. Usp. 61 280–288 (2018)
  4. I.D. Novikov, V.P. Frolov “Black holes in the Universe” Phys. Usp. 44 291–305 (2001)
  5. V.S. Beskin, Ya.N. Istomin, A.A. Philippov “Radio pulsars: the search for truth” Phys. Usp. 56 164–179 (2013)
  6. B. Heinemann, Y. Nir “The Higgs program and open questions in particle physics and cosmology” Phys. Usp. 62 920–930 (2019)
  7. E.A. Khazanov, S.Yu. Mironov, Mourou Gérard “Nonlinear compression of high-power laser pulses: compression after compressor approach” Phys. Usp. 62 1096–1124 (2019)
  8. E.P. Kurbatov, D.V. Bisikalo, P.V. Kaygorodov “On the possible turbulence mechanism in accretion disks in nonmagnetic binary stars” Phys. Usp. 57 787–798 (2014)
  9. D.I. Kazakov “Prospects of elementary particle physics” Phys. Usp. 62 364–377 (2019)
  10. Yu.N. Efremov, S.B. Novikov, P.V. Shcheglov “Prospects for development of ground-based optical astronomy” Sov. Phys. Usp. 18 151–160 (1975)
  11. V.A. Rubakov “The Null Energy Condition and its violation” Phys. Usp. 57 128–142 (2014)
  12. E.P. Kurbatov, A.G. Zhilkin, D.V. Bisikalo “Modified magnetohydrodynamics model including wave turbulence: astrophysical applications” Phys. Usp. 60 798–817 (2017)
  13. I.M. Dremin “The interaction region of high energy protons” Phys. Usp. 58 61–70 (2015)
  14. V.M. Kuleshov, V.D. Mur et al “Coulomb problem for a Z>Zcr” Phys. Usp. 58 785–791 (2015)
  15. I.M. Dremin, C. Quigg “Clusters in hadron multiple production processes” Sov. Phys. Usp. 21 265–271 (1978)
  16. S.G. Karshenboim “Progress in the accuracy of the fundamental physical constants: 2010 CODATA recommended values” Phys. Usp. 56 883–909 (2013)
  17. D.P. Skulachev “Cosmic microwave background anisotropy data correlation in WMAP and Relikt-1 experiments” Phys. Usp. 53 373–376 (2010)
  18. L.A. Falkovsky “Optical properties of graphene and IV — VI semiconductors” Phys. Usp. 51 887–897 (2008)
  19. M.V. Sazhin “Anisotropy and polarization of cosmic microwave background: state of the art” Phys. Usp. 47 187–194 (2004)
  20. A.N. Adamchuk, S.E. Esipov “Collectively fluctuating assets in the presence of arbitrage opportunities, and option pricing” Phys. Usp. 40 1239–1248 (1997)

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