NDLI: Einstein-Maxwell field equations in isotropic coordinates: an application to neutron star and quark star

Content Provider	Springer Nature Link
Author	Pradhan, N. Pant, Neeraj
Copyright Year	2014
Abstract	We present a new class of static spherically symmetric exact solutions of the Einstein-Maxwell field equations in isotropic coordinates for perfect fluid by considering a specific choice of electrical intensity which involves a parameter K. The resulting solutions represent charged fluid spheres joining smoothly with the Reissner-Nordstrom metric at the pressure free interface. The solutions so obtained are utilized to construct the models for super-dense star like neutron stars (ρ b =2 and 2.7×1014 g/cm3) and Quark stars (ρ b =4.6888×1014 g/cm3). It is observed that the models are well behaved for the restricted value of parameter K (0.141≤K≤0.159999). Corresponding to K max =0.159999 for which, u max =0.259, the resulting Quark star has a maximum mass M=1.618 M ⊙ and radius R=9.263 km and the neutron star modeling based on the particular solution; corresponding to K=0.15, u=0.238 and by assuming the surface density ρ b =2.7×1014 g/cm3 the maximum mass of neutron star M=1.966 M ⊙ and radius R=12.23 km and by assuming the surface density ρ b =2×1014 g/cm3 the resulting well behaved solution has a maximum mass of neutron M=2.284 M ⊙ and radius R=14.21 km. The robustness of our result is that it matches with the recent discoveries.
Starting Page	143
Ending Page	149
Page Count	7
File Format	PDF
ISSN	0004640X
Journal	Astrophysics and Space Science
Volume Number	352
Issue Number	1
e-ISSN	1572946X
Language	English
Publisher	Springer Netherlands
Publisher Date	2014-04-01
Publisher Place	Dordrecht
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Isotropic coordinates General relativity Reissner-Nordstrom Fluid ball Astrophysics and Astroparticles Astronomy, Observations and Techniques Cosmology Extraterrestrial Physics, Space Sciences Astrobiology
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

Sl.	Authority	Responsibilities	Communication Details
1	Ministry of Education (GoI), Department of Higher Education	Sanctioning Authority	https://www.education.gov.in/ict-initiatives
2	Indian Institute of Technology Kharagpur	Host Institute of the Project: The host institute of the project is responsible for providing infrastructure support and hosting the project	https://www.iitkgp.ac.in
3	National Digital Library of India Office, Indian Institute of Technology Kharagpur	The administrative and infrastructural headquarters of the project	Dr. B. Sutradhar bsutra@ndl.gov.in
4	Project PI / Joint PI	Principal Investigator and Joint Principal Investigators of the project	Dr. B. Sutradhar bsutra@ndl.gov.in Prof. Saswat Chakrabarti will be added soon
5	Website/Portal (Helpdesk)	Queries regarding NDLI and its services	support@ndl.gov.in
6	Contents and Copyright Issues	Queries related to content curation and copyright issues	content@ndl.gov.in
7	National Digital Library of India Club (NDLI Club)	Queries related to NDLI Club formation, support, user awareness program, seminar/symposium, collaboration, social media, promotion, and outreach	clubsupport@ndl.gov.in
8	Digital Preservation Centre (DPC)	Assistance with digitizing and archiving copyright-free printed books	dpc@ndl.gov.in
9	IDR Setup or Support	Queries related to establishment and support of Institutional Digital Repository (IDR) and IDR workshops	idr@ndl.gov.in

A family of exact solutions of Einstein-Maxwell field equations in isotropic coordinates: an application to optimization of quark star mass

Anisotropic charged analogue of Heintzmann’s solution

Relativistic model of anisotropic charged fluid sphere in general relativity

A family of charge analogue of Durgapal solution

Some static relativistic compact charged fluid spheres in general relativity

Compact stars with linear equation of state in isotropic coordinates

Some analytical models of anisotropic strange stars

Well-behaved relativistic charged super-dense star models

A class of relativistic anisotropic charged stellar models in isotropic coordinates

Einstein-Maxwell field equations in isotropic coordinates: an application to neutron star and quark star

Similar Documents

A family of exact solutions of Einstein-Maxwell field equations in isotropic coordinates: an application to optimization of quark star mass

Anisotropic charged analogue of Heintzmann’s solution

Relativistic model of anisotropic charged fluid sphere in general relativity

A family of charge analogue of Durgapal solution

Some static relativistic compact charged fluid spheres in general relativity

Compact stars with linear equation of state in isotropic coordinates

Some analytical models of anisotropic strange stars

Well-behaved relativistic charged super-dense star models

A class of relativistic anisotropic charged stellar models in isotropic coordinates

Einstein-Maxwell field equations in isotropic coordinates: an application to neutron star and quark star