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Иш: Global flow reconfiguration and oscillatory phenomenology in Bondi–Hoyle–Lyttleton accretion within non-conservative gravitational frameworks incorporating Euler–Heisenberg electrodynamics
Evolution of non-static fluid for irreversible gravitational radiation in Palatini <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si4.svg" display="inline" id="d1e26"><mml:mrow><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity
H. Asad, M. Yousaf, Bander Almutairi +2
Мақола202412 иқтибосABIExploring compact stars in modified <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si12.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">G</mml:mi> <mml:mo>,</mml:mo> <mml:mi>φ</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> gravity
Zoya Asghar, M. Farasat Shamir, Fatemah Mofarreh +3
ABIDark energy exponential potential models as curvature quintessence
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Мақола20065 иқтибосABITime-dependent matter instability and star singularity in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity
Kazuharu Bamba, Shin’ichi Nojiri, Sergei D. Odintsov
Мақола20114 иқтибосABI