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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/018/01/0015-0021

    • Keywords

       

      Dwarf stars; neutron stars; C-field

    • Abstract

       

      The effect of C-field in high density matter has been studied. We find that the negative energy and negative pressure of the C-field helps in formation of massive compact stable neutron stars of mass ∼ 0.5 solar mass which is in the range of 0.01 to 1.0 solar mass of recently observed dwarf stars.

    • Author Affiliations

       

      L. P. Singh1 P. K. Sahu2

      1. Physics Department, Utkal University, Bhubaneswar - 751 004, India
      2. Theory Group, Physical Research Laboratory, Navarangpura, Ahmedabad - 380 009, India
    • Dates

       
  • Journal of Astrophysics and Astronomy | News

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      Posted on January 27, 2016

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