← Назад к работе
Работы, на которые ссылается эта работа
Работ: 237
Работа: Impact of non-conservative gravity on massive compact objects: Insights from MIT bag model
A study of anisotropic spheres in modified gravity via embedding approach
Asifa Ashraf, Zhiyue Zhang, Allah Ditta +1
Статья2020Цитирований: 13ABIPhysically viable solutions of anisotropic spheres in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mrow><mml:mi mathvariant="script">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">G</mml:mi></mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math> gravity satisfying the Karmarkar condition
G. Mustafa, M. Farasat Shamir, Tiecheng Xia
Статья2020Цитирований: 12ABIRealistic stellar anisotropic model satisfying Karmarker condition in f(R, T) gravity
G. Mustafa, M. Zubair, Saira Waheed +1
Статья2020Цитирований: 9ABIDynamical instability for radiating anisotropic collapse
R. Chan, L. Herrera, N. O. Santos
Статья1993Цитирований: 9ABIRelativistic Equations for Adiabatic, Spherically Symmetric Gravitational Collapse
Charles W. Misner, David H. Sharp
Статья1964Цитирований: 8ABIPhysically Acceptable Embedded Class-I Compact Stars in Modified Gravity with Karmarkar Condition
Saira Waheed, G. Mustafa, M. Zubair +1
Статья2020Цитирований: 8ABIRole of pressure anisotropy on relativistic compact stars
S. K. Maurya, Ayan Banerjee, Sudan Hansraj
Статья2018Цитирований: 8ABICosmological and solar system consequences of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math>gravity models
Hamid Shabani, Mehrdad Farhoudi
Статья2014Цитирований: 8ABIRealistic solutions of fluid spheres in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4074" altimg="si284.svg"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">G</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 Karmarkar condition
G. Mustafa, Tiecheng Xia, M. Farasat Shamir
Статья2020Цитирований: 7ABIStudy of anisotropic strange stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math> gravity: An embedding approach under the simplest linear functional of the matter-geometry coupling
S. K. Maurya, Abdelghani Errehymy, Debabrata Deb +2
Статья2019Цитирований: 7ABINeutron stars with an anisotropic equation of state: mass, redshift and stability.
Статья1975Цитирований: 6ABIQuantum de Sitter cosmology and phantom matter
Shin’ichi Nojiri, Sergei D. Odintsov
Статья2003Цитирований: 6ABIANISOTROPIC COMPACT STARS WITH VARIABLE COSMOLOGICAL CONSTANT
Sk. Monowar Hossein, Farook Rahaman, Jayanta Naskar +2
Статья2012Цитирований: 6ABI