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Could a real (not virtual) static observer exist outside a Schwarzschild black hole?

2011/06/03 by V. A. Berezin, Victor Berezin · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Back-reaction #Black hole (networking) #Charged black hole #Classical mechanics #Cosmology and Gravitation Theories #Differential geometry #Earth Systems and Cosmic Evolution #General relativity #Geometry #Gravitation #Kerr metric #Measure (data warehouse) #Observer (physics) #Photon sphere #Physics #Quantum mechanics #RADIUS #Relativity and Gravitational Theory #Schwarzschild geodesics #Schwarzschild metric #Schwarzschild radius #Theoretical physics #gr-qc

paper · pdf · doi:10.1007/s10714-012-1356-1

7 pages

arxiv created 2011/06/03 · openalex publication_date 2012/04/06 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The aim of this Letter is rather pedagogical. We considered the static spherically symmetric ensemble of observers, having finite bare mass and trying to measure geometrical and physical properties of the environmental static (Schwarzschild) space-time. It is shown that, using the photon rockets (which the mass together with the mass of their fuel is also taken into account) they can managed to keep themselves on the fixed value of radius. The process of diminishing the total bare mass up to zero lasts infinitely long time. It is important that the problem is solved self-consistently, i.e., with full account for the back reaction of both bare mass and radiation from rockets on the space-time geometry.

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