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 inThe European physical journal. C, Particles and fields Vol. 81; no. 1; pp. 1 - 11
Main Authors Charan, Kali, Yadav, Om Prakash, Tewari, B. C.
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.01.2021
Springer
Springer Nature B.V
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ISSN1434-6044
1434-6052
DOI10.1140/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.
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
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  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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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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