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Extended phase space thermodynamics of regular-AdS black hole. [PDF]
Rehan M, Islam SU, Ghosh SG.
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Correction: Bianconi, G. The Quantum Relative Entropy of the Schwarzschild Black Hole and the Area Law. <i>Entropy</i> 2025, <i>27</i>, 266. [PDF]
Bianconi G.
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Modification of Premises for the Black Hole Information Paradox Caused by Topological Constraints in the Event Horizon Vicinity. [PDF]
Jacak JE.
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2009
Abstract A black hole is an object that is inside its event horizon at r=r*: a one-way surface that particles and light can only traverse inward. This chapter studies the spherically symmetric nonrotating Schwarzschild black hole. The metric elements change their respective signs when crossing from r>r∗ to r<r*, leading to ...
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Abstract A black hole is an object that is inside its event horizon at r=r*: a one-way surface that particles and light can only traverse inward. This chapter studies the spherically symmetric nonrotating Schwarzschild black hole. The metric elements change their respective signs when crossing from r>r∗ to r<r*, leading to ...
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Mathematical Physics, 2005
Black holes are predicted by General Relativity and there has been a long search for them. Now they have been observed. General Relativity also predicts effects of high spin of the black hole. There is good reason to believe that the best known black hole is spinning more or less as rapidly as it is allowed to. Now, the search is on for the spin of the
DE PAOLIS, Francesco +3 more
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Black holes are predicted by General Relativity and there has been a long search for them. Now they have been observed. General Relativity also predicts effects of high spin of the black hole. There is good reason to believe that the best known black hole is spinning more or less as rapidly as it is allowed to. Now, the search is on for the spin of the
DE PAOLIS, Francesco +3 more
openaire +2 more sources
2000
According to the generalized second law of thermodynamics, the quantity that never decreases in irreversible processes involving gravity is the sum of the entropy content of ordinary matter plus the entropy provided by the black holes. As the entropy of matter has a statistical description in terms of microscopic degrees of freedom, it seems that the ...
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According to the generalized second law of thermodynamics, the quantity that never decreases in irreversible processes involving gravity is the sum of the entropy content of ordinary matter plus the entropy provided by the black holes. As the entropy of matter has a statistical description in terms of microscopic degrees of freedom, it seems that the ...
openaire +3 more sources
Cancer statistics for African American/Black People 2022
Ca-A Cancer Journal for Clinicians, 2022Angela Giaquinto +2 more
exaly
Coalescence of black hole–neutron star binaries
Living Reviews in Relativity, 2021Koutarou Kyutoku +2 more
exaly

