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Astrophysics and Space Science

, Volume 84, Issue 2, pp 409–419 | Cite as

Neutron stars and general equation of nuclear matter

  • M. C. Durgapal
  • R. Bannerji
Article
  • 26 Downloads

Abstract

It has been shown that the mass of neutron stars obtained from equations of state based on nuclear theory depend upon the number of baryons assembled in it but not on the type of interactions considered. On examining the behaviour of different equations of state based on nuclear theories, a simple polytropic equation of state,P = (K/N)(pps)N is proposed. The results obtained forN=1.75 cover the entire range of neutron star masses obtained from the equations of state based on nuclear theories and give a maximum mass of 2.8M. Depending upon various mechanisms for energy output the mass of Crab pulsar is estimated to range from 0.32M to 1.5M. The relation connecting the coordinate mass,M, and the rest mass,M0, may be written asM/M≅0.93 (M0/M)0.9.

Keywords

Neutron Star Entire Range General Equation Energy Output Nuclear Matter 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Co 1982

Authors and Affiliations

  • M. C. Durgapal
    • 1
  • R. Bannerji
    • 1
  1. 1.Department of Physics, DSB Constituent CollegeKumaun UniversityNainitalIndia

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