Abstract
AbstractWe studied five methods to include anisotropy, or unequal stress distributions, in general relativistic matter configurations. We used nine acceptability conditions that the metric and physical variables must meet to determine if our models were astrophysically viable. Our analysis found the most effective way to introduce anisotropy while keeping a simple density profile. We also found a practical “rule of thumb” that relates the density at the boundary to the density at the centre of relativistic matter distributions. Additionally, we calculated the configuration radius and encountered that values observed by NICER for PSR J0740+6620 are consistent with several acceptable matter configurations, both isotropic and anisotropic.
Funder
Ministerio de Ciencia e Innovación
Erasmus+
Junta de Castilla y León
Vicerrectoría de Investigación y Extensión, Universidad Industrial de Santander
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference65 articles.
1. B.P. Abbott, R. Abbott, T.D. Abbott et al., LIGO Scientific Collaboration, and Virgo Collaboration, Properties of the binary neutron star merger gw170817. Phys. Rev. X 9, 011001 (2019)
2. K. Gendreau, Z. Arzoumanian, E. Ferrara, C.B. Markwardt, NICER: The Neutron Star Interior Composition Explorer (Springer Nature Singapore, Singapore, 2022), pp.1–21
3. M.S.R. Delgaty, K. Lake, Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein’s equations. Comput. Phys. Commun. 115, 395 (1998)
4. B.V. Ivanov, Analytical study of anisotropic compact star models. Eur. Phys. J. C 77(11), 738 (2017)
5. B.V. Ivanov, A conformally flat realistic anisotropic model for a compact star. Eur. Phys. J. C 78(4), 332 (2018)
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