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Иш: Linear redshift parametrization of deceleration parameter in f(R,Lm) gravity
Class of viable modified<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>gravities describing inflation and the onset of accelerated expansion
Guido Cognola, E. Elizalde, Shin’ichi Nojiri +3
Мақола20087 иқтибосABIUnifying inflation with ΛCDM epoch in modified <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 consistent with Solar System tests
Shin’ichi Nojiri, Sergei D. Odintsov
Мақола20077 иқтибосABIFitting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4298" altimg="si614.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 models with a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4315" altimg="si606.svg"> <mml:mi>Λ</mml:mi> </mml:math> CDM limit using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4320" altimg="si18.svg"> <mml:mrow> <mml:mi>H</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>z</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> and Pantheon data
José Antonio Nájera, Amanda Fajardo
Мақола20217 иқтибосABIGeneralized Curvature-Matter Couplings in Modified Gravity
Tiberiu Harko, Francisco S. N. Lobo
Мақола20146 иқтибосABIConstraining effective equation of state in f(Q, T) gravity
Simran Arora, Abhishek Parida, P. K. Sahoo
Мақола20216 иқтибосABIThe dynamics of matter bounce cosmology in Weyl-type <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si248.svg" display="inline" id="d1e71"><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
A. Zhadyranova, M. Koussour, S. Bekkhozhayev
Мақола20246 иқтибосABIDo consistent models mimic general relativity plus Λ?
Stephen Appleby, Richard A. Battye
Мақола20075 иқтибосABIModified<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 unifying<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>R</mml:mi><mml:mi>m</mml:mi></mml:msup></mml:math>inflation with the<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>epoch
Shin’ichi Nojiri, Sergei D. Odintsov
Мақола20085 иқтибосABIStellar content of extremely red quiescent galaxies at<i>z</i>> 2
M. López‐Corredoira, A. Vazdekis, C. M. Gutiérrez +1
Мақола20175 иқтибосABI