Does particle creation mechanism favour formation of black hole or naked singularity?
Abstract The paper deals with collapse dynamics of a spherically symmetric massive star in the framework of non-equilibrium thermodynamic prescription through particle creation mechanism. The matter content in the star is in the form of perfect fluid with barotropic equation of state, and the dissip...
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2018-06-01
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-5965-z |
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doaj-ab4116e5425849af8b2e0d8643cef85e2020-11-25T02:12:18ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-06-0178611810.1140/epjc/s10052-018-5965-zDoes particle creation mechanism favour formation of black hole or naked singularity?Sudipto Bhattacharjee0Subhajit Saha1Subenoy Chakraborty2Department of Mathematics, Jadavpur UniversityDepartment of Mathematics, Panihati MahavidyalayaDepartment of Mathematics, Jadavpur UniversityAbstract The paper deals with collapse dynamics of a spherically symmetric massive star in the framework of non-equilibrium thermodynamic prescription through particle creation mechanism. The matter content in the star is in the form of perfect fluid with barotropic equation of state, and the dissipative phenomena due to non-equilibrium thermodynamics is in the form of bulk viscosity. For simplicity, the thermodynamic system is chosen to be adiabatic so that the effective bulk viscous pressure is linearly related to the particle creation rate. As a result, the evolution of the collapsing star also depends on the particle creation rate. By proper choice of creation rate as a function of the Hubble parameter, it is found that the end state of the collapse may be either a black hole (BH) or a naked singularity (NS).http://link.springer.com/article/10.1140/epjc/s10052-018-5965-z |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Sudipto Bhattacharjee Subhajit Saha Subenoy Chakraborty |
spellingShingle |
Sudipto Bhattacharjee Subhajit Saha Subenoy Chakraborty Does particle creation mechanism favour formation of black hole or naked singularity? European Physical Journal C: Particles and Fields |
author_facet |
Sudipto Bhattacharjee Subhajit Saha Subenoy Chakraborty |
author_sort |
Sudipto Bhattacharjee |
title |
Does particle creation mechanism favour formation of black hole or naked singularity? |
title_short |
Does particle creation mechanism favour formation of black hole or naked singularity? |
title_full |
Does particle creation mechanism favour formation of black hole or naked singularity? |
title_fullStr |
Does particle creation mechanism favour formation of black hole or naked singularity? |
title_full_unstemmed |
Does particle creation mechanism favour formation of black hole or naked singularity? |
title_sort |
does particle creation mechanism favour formation of black hole or naked singularity? |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2018-06-01 |
description |
Abstract The paper deals with collapse dynamics of a spherically symmetric massive star in the framework of non-equilibrium thermodynamic prescription through particle creation mechanism. The matter content in the star is in the form of perfect fluid with barotropic equation of state, and the dissipative phenomena due to non-equilibrium thermodynamics is in the form of bulk viscosity. For simplicity, the thermodynamic system is chosen to be adiabatic so that the effective bulk viscous pressure is linearly related to the particle creation rate. As a result, the evolution of the collapsing star also depends on the particle creation rate. By proper choice of creation rate as a function of the Hubble parameter, it is found that the end state of the collapse may be either a black hole (BH) or a naked singularity (NS). |
url |
http://link.springer.com/article/10.1140/epjc/s10052-018-5965-z |
work_keys_str_mv |
AT sudiptobhattacharjee doesparticlecreationmechanismfavourformationofblackholeornakedsingularity AT subhajitsaha doesparticlecreationmechanismfavourformationofblackholeornakedsingularity AT subenoychakraborty doesparticlecreationmechanismfavourformationofblackholeornakedsingularity |
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1724910137137692672 |