2018/04/30 by V. I. Dokuchaev, N. O. Nazarova · 30 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysical Phenomena and Observations #Binary black hole #Black hole (networking) #Earth Systems and Cosmic Evolution #Event (particle physics) #Event horizon #Hawking radiation #Horizon #Primordial black hole #Relativity and Gravitational Theory #Shadow (psychology) #White hole #astro-ph.HE #gr-qc
paper · pdf · doi:10.1134/s1063776119030026
published in Journal of Experimental and Theoretical Physics 128(4), 578-585 (Pleiades Publishing) · 7 pages, 9 figures, new references added
openalex created_date 2018/05/07 · openalex publication_date 2019/04/01 · arxiv created 2019/06/07 · arxiv updated 2019/06/11 · openalex updated_date 2026/08/05
Abstract We argue that a genuine image of the black hole viewed by a distant observer is not its shadow, but a more compact event horizon image probed by the luminous matter plunging into black hole. The external border of the black hole shadow is washed out by radiation from matter plunging into black hole and approaching the event horizon. This effect will crucially influence the results of future observations by the Event Horizon Telescope. We show that gravitational lensing of the luminous matter plunging into black hole provides the possibility for visualization of the event horizon. The lensed image of the event horizon is formed by the highly red-shifted photons emitted by the plunging matter very near the black hole event horizon and detected by a distant observer. The resulting event horizon image is a gravitationally lensed projection on the celestial sphere of the whole black hole event horizon sphere. Seemingly, black holes are the unique objects in the Universe which may be viewed by distant observers at once from both the front and back sides.