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85 та иш
Иш: Late-time acceleration in extended and unified f(R,Lm,T) gravity with observational data
Constant-roll and primordial black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1888" altimg="si282.svg"> <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
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Мақола202312 иқтибосABIIs cosmic speed-up due to new gravitational physics?
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Мақола200411 иқтибосABIGaussian process estimation of transition redshift
J. F. Jesus, R. Valentim, A. A. Escobal +1
Мақола202011 иқтибосABICosmological implications of the constant jerk parameter in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si275.svg" display="inline" id="d1e952"><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 theory
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Мақола202311 иқтибосABIConstruction of cosmologically viable gravity models
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Мақола200911 иқтибосABIInference from Iterative Simulation Using Multiple Sequences
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Мақола199210 иқтибосABIObservational constraints on the equation of state of viscous fluid in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si250.svg" display="inline" id="d1e314"><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
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ABIKinetically driven quintessence
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Мақола20009 иқтибосABILate-time acceleration in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e175" altimg="si19.svg"><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: Analysis and constraints in an anisotropic background
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Мақола20229 иқтибосABINeutron stars in $$f(R,L_m,T)$$ gravity
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Препринт20249 иқтибосABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Λ</mml:mi><mml:mi>CDM</mml:mi></mml:math>universe in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><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
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Мақола20108 иқтибосABICoexistence of matter dominated and accelerating solutions in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity
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Мақола20098 иқтибосABIEnergy conditions in modified f(G) gravity
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Мақола20178 иқтибосABIEnergy conditions in the f(R, L, T) theory of gravity
Simran Arora, P. H. R. S. Moraes, P. K. Sahoo
Препринт20245 иқтибосABI