• Radial oscillations of magnetized proto strange stars in temperature- and density-dependent quark mass model

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    • Keywords


      Proto strange stars; magnetic field; radial oscillations

    • Abstract


      We report on the study of the mass-radius (M–R) relation and the radial oscillations of magnetized proto strange stars. For the quark matter we have employed the very recent modification, the temperature- and density-dependent quark mass model of the well-known density-dependent quark mass model. We find that the effect of magnetic field, both on the maximum mass and radial frequencies, is rather small. Also a proto strange star, whether magnetized or otherwise, is more likely to evolve into a strange star rather than transform into a black hole.

    • Author Affiliations


      V K Gupta1 2 Asha Gupta1 S Singh1 2 J D Anand1

      1. Department of Physics and Astrophysics, University of Delhi, Delhi - 110 007, India
      2. Inter-University Centre for Astronomy and Astrophysics, Ganeshkhind, Pune - 411 007, India
    • Dates

  • Pramana – Journal of Physics | News

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