International Journal of Astronomy and Astrophysics

International Journal of Astronomy and Astrophysics

ISSN Print: 2161-4717
ISSN Online: 2161-4725
www.scirp.org/journal/ijaa
E-mail: ijaa@scirp.org
"Kruskal Coordinates and Mass of Schwarzschild Black Holes: No Finite Mass Black Hole at All"
written by Abhas Mitra,
published by International Journal of Astronomy and Astrophysics, Vol.2 No.4, 2012
has been cited by the following article(s):
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[2] Consequences of a Generalized Newtonian Gravity with an Exponential Factor
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[3] Half Truths and Rant Against ECO Paradigm by Chandra Prakash
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[4] О свойствах гравитационного поля, обусловленного обобщенно-ньютоновой силой всемирного тяготения
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[5] The Consequences of a Strengthened Newtonian Gravity at Short Distances
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[6] Mass of Schwarzschild Black Holes Is Indeed Zero And Black Hole Candidates Are Quasi Black Holes
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[7] Is the Schwarzschild radius truly a radius
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[8] Horizon free eternally collapsing anisotropic radiating star
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[9] EINSTEINIAN REVOLUTION’S MISINTERPRETATION: NO TRUE BLACK HOLES, NO INFORMATION PARADOX: JUST QUASI-STATIC BALLS OF QUARK GLUON PLASMA
New Results and Actual Problems in Particle & Astroparticle Physics and Cosmology-Proceedings of XXIXth International Workshop on High Energy Physics. Edited by RYUTIN ROMAN, PETROV VLADIMIR & KISELEV V. Published by World Scientific Publishing Co. Pte. Ltd., 2014. ISBN# 9789814578745, pp. 153-163, 2014
[10] Modeling quasar central engine as a relativistic radiating star
Astrophysics and Space Science, 2014
[11] Einsteinian Revolution's Misinterpretation: no True Black Holes, no Information Paradox: Just Quasi-Static Balls of Quark Gluon Plasma
New Results and Actual Problems in Particle & Astroparticle Physics and Cosmology, 2014
[12] Does Pressure Accentuate General Relativistic Gravitational Collapse and Formation of Trapped Surfaces?
International Journal of Modern Physics D, 2013
[13] THE MASS OF THE OPPENHEIMER–SNYDER-BLACK HOLE: ONLY FINITE MASS QUASI-BLACK HOLES
International Journal of Modern Physics D, 2013
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