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Setting Limits on Supersymmetry Using Simplified Models
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Compact stars with non-uniform relativistic polytrope.

Mohamed I Nouh1, Mona M Foda2, Mohamed S Aboueisha3

  • 1Astronomy Department, National Research Institute of Astronomy and Geophysics, Helwan, Cairo, 11421, Egypt. mohamed.nouh@nriag.sci.eg.

Scientific Reports
|July 14, 2024
PubMed
Summary

This study introduces new relativistic composite polytropic models for compact stars, accurately simulating their structure and predicting core radii consistent with observations. These models offer a novel approach to understanding neutron star properties.

Keywords:
Compact starsComposite polytropeGeneral relativityMass-radius relationRelativistic effects

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Area of Science:

  • Astrophysics
  • General Relativity
  • Stellar Structure

Background:

  • Compact stars, such as neutron stars, require relativistic models due to strong gravitational fields.
  • Polytropic equations of state are commonly used to approximate stellar matter, but relativistic composite models offer enhanced accuracy.

Purpose of the Study:

  • To develop and analyze new relativistic composite polytropic models for compact stars.
  • To simulate spherically symmetric, static matter distributions by solving Einstein field equations.
  • To investigate the internal structure, mass, and radius of neutron star candidates.

Main Methods:

  • Simultaneously solving Einstein field equations with a polytropic state equation.
  • Deriving and numerically solving the composite Tolman-Oppenheimer-Volkoff (CTOV) equation.
  • Computing Emden and mass functions for various relativistic parameters and polytropic indices.

Main Results:

  • The models successfully simulate compact star structures, with relativistic parameters approaching zero recovering Newtonian polytropic models.
  • Calculated core radii for neutron star candidates Cen X-3 and PSR J1614-22304 are 50-60% of their total radii.
  • The core radius for SAXJ1808.4-3658 is found to be approximately 30% of its total radius, consistent with observations.

Conclusions:

  • The composite relativistic polytrope model provides a robust approximation for neutron star structure.
  • The developed models yield masses and radii consistent with observational data for compact stars.
  • This work validates the computational code by comparing Newtonian and relativistic models.