Charged anisotropic spherical collapse with heat flow
In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse for the charged stars are known to give rise to a high degree of non-linearity in the ordinary differential equation coming from junction conditions. Th...
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Published in | The European physical journal. C, Particles and fields Vol. 81; no. 1; pp. 1 - 11 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
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Berlin/Heidelberg
Springer Berlin Heidelberg
01.01.2021
Springer Springer Nature B.V SpringerOpen |
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Online Access | Get full text |
ISSN | 1434-6044 1434-6052 |
DOI | 10.1140/epjc/s10052-021-08865-8 |
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Abstract | In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse for the charged stars are known to give rise to a high degree of non-linearity in the ordinary differential equation coming from junction conditions. The attempts to solve it analytically proved to be unfortunate. Numerical methods have been suggested in the past. However, the high degree of non-linearity tends to introduce fluctuations and large round off errors in the numerical calculation. A new ansatz is proposed in the present work to reduce the degree of non-linearity. An ordinary differential equation is derived by satisfying junction conditions, and its numerical solution is demonstrated. Physical quantities associated with the collapse process are plotted to observe the effect of charge on these quantities. It is concluded that the charge can delay the collapse of a star and can even prevent it depending upon the amount of charge. It is also verified that the solution satisfies all the energy conditions. |
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AbstractList | In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse for the charged stars are known to give rise to a high degree of non-linearity in the ordinary differential equation coming from junction conditions. The attempts to solve it analytically proved to be unfortunate. Numerical methods have been suggested in the past. However, the high degree of non-linearity tends to introduce fluctuations and large round off errors in the numerical calculation. A new ansatz is proposed in the present work to reduce the degree of non-linearity. An ordinary differential equation is derived by satisfying junction conditions, and its numerical solution is demonstrated. Physical quantities associated with the collapse process are plotted to observe the effect of charge on these quantities. It is concluded that the charge can delay the collapse of a star and can even prevent it depending upon the amount of charge. It is also verified that the solution satisfies all the energy conditions. Abstract In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse for the charged stars are known to give rise to a high degree of non-linearity in the ordinary differential equation coming from junction conditions. The attempts to solve it analytically proved to be unfortunate. Numerical methods have been suggested in the past. However, the high degree of non-linearity tends to introduce fluctuations and large round off errors in the numerical calculation. A new ansatz is proposed in the present work to reduce the degree of non-linearity. An ordinary differential equation is derived by satisfying junction conditions, and its numerical solution is demonstrated. Physical quantities associated with the collapse process are plotted to observe the effect of charge on these quantities. It is concluded that the charge can delay the collapse of a star and can even prevent it depending upon the amount of charge. It is also verified that the solution satisfies all the energy conditions. |
ArticleNumber | 60 |
Audience | Academic |
Author | Yadav, Om Prakash Charan, Kali Tewari, B. C. |
Author_xml | – sequence: 1 givenname: Kali surname: Charan fullname: Charan, Kali organization: Department of Mathematical and Statistical Sciences, Institute of Natural Sciences, Shri Ramswaroop Memorial University Lucknow – sequence: 2 givenname: Om Prakash surname: Yadav fullname: Yadav, Om Prakash email: opyadav@nith.ac.in organization: Department of Mathematics and Scientific Computing, National Institute of Technology Hamirpur – sequence: 3 givenname: B. C. surname: Tewari fullname: Tewari, B. C. organization: Department of Mathematics, SSJ Campus Almora, Kumaun University Nainital |
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CitedBy_id | crossref_primary_10_1140_epjc_s10052_021_09163_z crossref_primary_10_1140_epjc_s10052_021_09589_5 crossref_primary_10_1007_s10714_023_03161_0 crossref_primary_10_3390_e23111539 crossref_primary_10_1016_j_cjph_2022_07_016 crossref_primary_10_1007_s10714_024_03338_1 crossref_primary_10_1002_prop_202300250 crossref_primary_10_1093_ptep_ptab116 crossref_primary_10_1142_S0219887822501857 crossref_primary_10_3390_e23111400 |
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References_xml | – reference: BonnorWBThe equilibrium of a charged sphereMon. Not. R. Astron. Soc.196512964434461965MNRAS.129..443B184695 – reference: IvanovBVCollapsing shear-free perfect fluid spheres with heat flowGen. Relativ. Gravit.2012447183518552012GReGr..44.1835I29352081246.83154 – reference: BonnorWBDe OliveiraASantosNORadiating spherical collapsePhys. Rep.198918152693261989PhR...181..269B1020461 – reference: OlsonEBailynMCharge effects in a static, spherically symmetric, gravitating fluidPhys. Rev. D197613822041976PhRvD..13.2204O – reference: CahillMEMcVittieGCSpherical symmetry and mass–energy in general relativity. I. General theoryJ. Math. Phys.1970114138213911970JMP....11.1382C2603760195.56301 – reference: SantosNNon-adiabatic radiating collapseMon. Not. R. Astron. Soc.19852164034101985MNRAS.216..403S – reference: IvanovBVAll solutions for geodesic anisotropic spherical collapse with shear and heat radiationAstrophys. Space Sci.20163611182016Ap&SS.361...18I3507873 – reference: EddingtonASThe Internal Constitution of the Stars1926BerlinNature Publishing Group52.1021.05 – reference: K. Schwarzschild, About the gravitational field of a mass point according to Einstein’s theory, in Berlin. Session Reports, vol. 18 (1916) – reference: TewariBCCharanKHorizon free eternally collapsing anisotropic radiating starAstrophys. Space Sci.201535721072015Ap&SS.357..107T – reference: HerreraLDi PriscoAOspinoJDefinition of complexity for dynamical spherically symmetric dissipative self-gravitating fluid distributionsPhys. Rev. D201898101040592018PhRvD..98j4059H3954714 – reference: GhezziCRRelativistic structure, stability, and gravitational collapse of charged neutron starsPhys. Rev. D200572101040172005PhRvD..72j4017G – reference: PinheiroGChanRRadiating shear-free gravitational collapse with chargeGen. Relativ. Gravit.20134512432612013GReGr..45..243P30117131260.83025 – reference: ThirukkaneshSGovenderMThe role of the electromagnetic field in dissipative collapseInt. J. Mod. Phys. D2013221413500872013IJMPD..2250087T1284.83038 – reference: SharifMIftikharSCharged dissipative collapse of shearing viscous starAstrophys. Space Sci.20153571792015Ap&SS.357...79S – reference: De OliveiraASantosNNonadiabatic gravitational collapseAstrophys. J.19873126406451987ApJ...312..640D – reference: PantNTewariBHorizon-free gravitational collapse of radiating fluid sphereAstrophys. Space Sci.201133126456502011Ap&SS.331..645P1209.83032 – reference: LindquistRSchwartzRMisnerCVaidya’s radiating Schwarzschild metricPhys. Rev.19651375BB13641965PhRv..137.1364L1989380132.43203 – reference: SherifAGoswamiRMaharajSProperties of expansion-free dynamical starsPhys. Rev. D201910040440392019PhRvD.100d4039S4022994 – reference: GlassEShear-free collapse with heat flowPhys. Lett. A1981866–73513521981PhLA...86..351G – reference: MitraAWhy gravitational contraction must be accompanied by emission of radiation in both Newtonian and Einstein gravityPhys. Rev. D20067420240102006PhRvD..74b4010M – reference: PriscoAHerreraLDenmatGMacCallumMSantosNNonadiabatic charged spherical gravitational collapsePhys. Rev. D20077660640172007PhRvD..76f4017D – reference: BekensteinJDHydrostatic equilibrium and gravitational collapse of relativistic charged fluid ballsPhys. Rev. D19714821851971PhRvD...4.2185B – reference: P.C. Vaidya, The gravitational field of a radiating star, in Proceedings of the Indian Academy of Sciences-Section A, vol. 33, p. 264 (Springer 1951) – reference: TewariBCRadiating Fluid Balls in General Relativity2010MuellerVDM Publishing – reference: GlassEShear-free gravitational collapseJ. Math. Phys.1979207150815131979JMP....20.1508G – reference: OppenheimerJRSnyderHOn continued gravitational contractionPhys. 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Snippet | In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse for the... Abstract In this article, we study the shear-free gravitational collapse of a charged radiating star. The Einstein field equations of gravitational collapse... |
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SubjectTerms | Anisotropy Astronomy Astrophysics and Cosmology Differential equations Differential thermal analysis Einstein equations Elementary Particles Gravitation Gravitational collapse Hadrons Heat transmission Heavy Ions Linearity Measurement Science and Instrumentation Nonlinearity Nuclear Energy Nuclear Physics Numerical methods Ordinary differential equations Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article – Theoretical Physics Roundoff error String Theory |
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Title | Charged anisotropic spherical collapse with heat flow |
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