Работы, цитирующие эту работу

Работ: 5

Работа: Anisotropic stars of class one space–time in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4009" altimg="si17.svg"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity under the simplest linear functional of the matter–geometry coupling

1. A Brief analysis of isotropic Karmarkar models in modified gravity theory

   Yihu Feng, Tayyab Naseer, Asifa Ashraf +2

   СтатьяCosmology and Gravitation TheoriesChinese Journal of Physics2024Цитирований: 6

   ABIABI:AkademIndex/openalex/2024.article.000022

2. 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

3. Study on physical properties and maximum mass limit of Finch–Skea anisotropic model under Karmarkar condition in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si7.svg" display="inline" id="d1e4516"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>-gravity

   G. Mustafa, Allah Ditta, Saadia Mumtaz +2

   СтатьяCosmology and Gravitation TheoriesChinese Journal of Physics2024Цитирований: 3

   ABIABI:AkademIndex/openalex/2024.article.000183

4. Constraining maximum mass limit and physical properties of Durgapal–Fuloria complexity-free solution under gravitational decoupling approach

   S. K. Maurya, G. Mustafa, Saibal Ray +3

   СтатьяCosmology and Gravitation TheoriesPhysics of the Dark Universe2023Цитирований: 1

   ABIABI:AkademIndex/openalex/2023.article.000544

5. 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