Ушбу иш иқтибос қилган ишлар
77 та иш
Иш: Constraining <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
Study 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
Мақола201910 иқтибосABINeutron stars in $$f(R,L_m,T)$$ gravity
Clésio E. Mota, Juan M. Z. Pretel, César O. V. Flores
Препринт202410 иқтибосABIGravitational decoupling minimal geometric deformation model in modified <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e2140" altimg="si513.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>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity theory
S. K. Maurya, Abdelghani Errehymy, Ksh. Newton Singh +2
Мақола20209 иқтибосABIAnisotropic compact stars in f(R) gravity
G. G. L. Nashed, Salvatore Capozzıello
Мақола20218 иқтибосABICosmology in f(R,Lm) gravity
Lakhan V. Jaybhaye, Raja Solanki, Sanjay Mandal +1
Мақола20227 иқтибосABIAnisotropic compact stars in the Buchdahl model: A comprehensive study
S. K. Maurya, Ayan Banerjee, M. K. Jasim +3
Мақола20197 иқтибосABISupermassive neutron stars in axion F(R) gravity
Artyom V. Astashenok, Sergei D. Odintsov
Мақола20207 иқтибосABIOn the nature and evolution of the unique binary pulsar J1903+0327
P. C. C. Freire, C. G. Bassa, N. Wex +16
Мақола20115 иқтибосABIComplexity factors for axially symmetric static sources
L. Herrera, A. Di Prisco, J. Ospino
Мақола20194 иқтибосABIPhysical properties of class I compact star model for linear and Starobinsky <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1207" altimg="si25.svg"> <mml:mrow> <mml:mo>−</mml:mo> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> functions
Ksh. Newton Singh, S. K. Maurya, Abdelghani Errehymy +2
Мақола20203 иқтибосABIBuchdahl model in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e9177" altimg="si187.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>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity: A comparative study with standard Einstein’s gravity
S.K. Maurya, Ayan Banerjee, Francisco Tello-Ortiz
Мақола20193 иқтибосABI