Estimating Microscopic Nuclear Data by Compact Star Observations

Balázs Endre Szigeti; Gergely Gábor Barnaföldi; Péter Pósfay; Antal Jakovác

Estimating Microscopic Nuclear Data by Compact Star Observations

Nuclear Theory 2021-07-29 v1 High Energy Astrophysical Phenomena High Energy Physics - Phenomenology

Authors: Balázs Endre Szigeti , Gergely Gábor Barnaföldi , Péter Pósfay , Antal Jakovác

Abstract

We studied recent observation data of pulsar masses and radii of PSR J0740 $+$ 6620, PSR J0348 $+$ 0432, and PSR J1614 $-$ 2230 from different measurements, based on the extended version of $\sigma$ - $\omega$ model. Throughout our analysis, we assumed that these pulsars are maximal-mass compact stars, thus we applied the core approximation. Based on the linear relation between the microscopic and macroscopic parameters of compact stars evaluated by our model, we estimated the average Landau mass $m_L = 752.46^{+49.1}_{-42.5}$ MeV and compressibility $K = 261.7^{+57.2}_{-28.0}$ MeV.

Keywords

pulsar astronomy pulsars neutron stars

Cite

@article{arxiv.2107.13476,
  title  = {Estimating Microscopic Nuclear Data by Compact Star Observations},
  author = {Balázs Endre Szigeti and Gergely Gábor Barnaföldi and Péter Pósfay and Antal Jakovác},
  journal= {arXiv preprint arXiv:2107.13476},
  year   = {2021}
}

Comments

4 paghes 1 table, 1 figue. arXiv admin note: substantial text overlap with arXiv:2006.03710

Estimating Microscopic Nuclear Data by Compact Star Observations

Abstract

Keywords

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