Работы, цитирующие эту работу

Работ: 2

Работа: Self bound compact stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si13.svg" display="inline" id="d1e1787"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity admitting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si179.svg" display="inline" id="d1e1804"><mml:mrow><mml:mi>C</mml:mi><mml:mi>F</mml:mi><mml:mi>L</mml:mi></mml:mrow></mml:math> equation of state in presence of non-minimal <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si542.svg" display="inline" id="d1e1814"><mml:mrow><mml:mi>Q</mml:mi><mml:mi>C</mml:mi><mml:mi>D</mml:mi></mml:mrow></mml:math> correction factor

1. Implication of f(Q,T) gravity on the formation of the charge compact stars and constraining their mass-radius relations in lower mass gap region

   S. K. Maurya, Abdelghani Errehymy, Zhanbala Umbetova +4

   СтатьяCosmology and Gravitation TheoriesJournal of High Energy Astrophysics2025Цитирований: 4

   ABIABI:AkademIndex/openalex/2026.other.109622

2. Testing linear non-minimal coupling in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si447.svg" display="inline" id="d1e4384"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity using X-ray binary pulsars constrained by NICER observations

   Abdelghani Errehymy, S. K. Maurya, Orhan Dönmez +4

   СтатьяPulsars and Gravitational Waves ResearchPhysics of the Dark Universe2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.001332