Energy Momentum Squared Gravity in Doneva-Jazadjiev anisotropic pressure model of non-rotating neutron stars

Hanifa, M. D. Danarianto, A. Sulaksono

Research output: Contribution to journalConference articlepeer-review

Abstract

We implement the Doneva-Yazadjiev (DY) anisotropic model of neutron stars into Energy Momentum Squared Gravity (EMSG) theory. We have shown that the Tolmann-Oppenheimer-Volkoff (TOV) equation within this model can be expressed in the terms of effective pressure and energy density. The structure of neutron stars (NS) is then calculated by using Basic Standard Parameter equation of state with hyperons in the center. We found that the combined model is able to adjust the mass-radius relation of the NS. We also found that this model could affect boundary limit of EMSG parameter, α, in the term of stability.

Original languageEnglish
Article number012003
JournalJournal of Physics: Conference Series
Volume2214
Issue number1
DOIs
Publication statusPublished - 15 Mar 2022
Event2nd International Symposium on Space Science 2021, ISSS 2021 - Virtual, Online
Duration: 14 Nov 202115 Nov 2021

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