J.A.S. Fortunato , P.H.R.S. Moraes , E. Brito , J.G. de Lima Júnior , T.S. Guerini
{"title":"Hydrostatic equilibrium configurations of neutron stars in the f(R,L,T) gravity theory","authors":"J.A.S. Fortunato , P.H.R.S. Moraes , E. Brito , J.G. de Lima Júnior , T.S. Guerini","doi":"10.1016/j.dark.2025.101893","DOIUrl":null,"url":null,"abstract":"<div><div>In the present work, we obtain the hydrostatic equilibrium configurations of neutron stars in the recently proposed <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>R</mi><mo>,</mo><mi>L,T</mi><mo>)</mo></mrow></mrow></math></span> theory of gravity, for which <span><math><mi>R</mi></math></span> is the Ricci scalar, <span><math><mi>L</mi></math></span> is the matter lagrangian density, <span><math><mi>T</mi></math></span> is the trace of the energy–momentum tensor and <span><math><mi>f</mi></math></span> is a function of the argument. This theory emerges in the present literature as a generalized geometry-matter coupling theory of gravity. We derive the Tolman–Oppenheimer–Volkoff-like equation for a particular functional form of the <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>R</mi><mo>,</mo><mi>L</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></mrow></math></span> function. Our solutions are obtained from realistic equations of state describing matter inside neutron stars. We obtain stable solutions for neutron stars and we show that for some values of the free parameter of the theory it is possible to be in agreement with both NICER and LIGO/Virgo observational data. We also calculate the surface gravitational redshift for the <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>R</mi><mo>,</mo><mi>L</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></mrow></math></span> gravity neutron stars.</div></div>","PeriodicalId":48774,"journal":{"name":"Physics of the Dark Universe","volume":"48 ","pages":"Article 101893"},"PeriodicalIF":5.0000,"publicationDate":"2025-03-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of the Dark Universe","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S221268642500086X","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
In the present work, we obtain the hydrostatic equilibrium configurations of neutron stars in the recently proposed theory of gravity, for which is the Ricci scalar, is the matter lagrangian density, is the trace of the energy–momentum tensor and is a function of the argument. This theory emerges in the present literature as a generalized geometry-matter coupling theory of gravity. We derive the Tolman–Oppenheimer–Volkoff-like equation for a particular functional form of the function. Our solutions are obtained from realistic equations of state describing matter inside neutron stars. We obtain stable solutions for neutron stars and we show that for some values of the free parameter of the theory it is possible to be in agreement with both NICER and LIGO/Virgo observational data. We also calculate the surface gravitational redshift for the gravity neutron stars.
期刊介绍:
Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact.
The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.