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14 ta ish
Ish: Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
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
MaqolaOchiq kirishCosmology and Gravitation TheoriesJournal of High Energy Astrophysics20254 iqtibosABIStudy 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
ABINonmetric geometry and its role in the isotropization of self-Gravitating stellar models
S. Sudheer Khan, Sardor Murodov, Javlon Rayimbaev +3
MaqolaOchiq kirish20252 iqtibosABIConstraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mi mathvariant="script">L</mml:mi> <mml:mi>m</mml:mi> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> gravity with millisecond pulsar observations
S.K. Maurya, A. Errehymy, K.N. Singh +4
MaqolaOchiq kirish20261 iqtibosABIAnisotropic compact stars in quadratic f(R) gravity and influence of quadratic parameter on properties of compact stars
Rajesh Kumar, S. K. Maurya, Yassine Sekhmani +2
MaqolaOchiq kirish20251 iqtibosABISome Stable Hybrid Neutron Stars through MIT Bag Model
S. Khan, J. Rayimbaev, T. Ganesan +2
Maqola20260 iqtibosABI