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Иш: Linear redshift parametrization of deceleration parameter in f(R,Lm) gravity
Cosmology in f(R,Lm) gravity
Lakhan V. Jaybhaye, Raja Solanki, Sanjay Mandal +1
Мақола20225 иқтибосABIAre<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>Dark Energy Models Cosmologically Viable?
Luca Amendola, David Polarski, Shinji Tsujikawa
Мақола20074 иқтибосABISolar system and equivalence principle constraints on<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 by the chameleon approach
Salvatore Capozzıello, Shinji Tsujikawa
Мақола20084 иқтибосABILow-lying doubly heavy baryons: Regge relation and mass scaling
Yongxin Song, Duojie Jia, Wen-Xuan Zhang +1
Мақола20234 иқтибосABINon-minimal geometry–matter couplings in Weyl–Cartan space–times: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1253" altimg="si4.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:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>T</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity
Tiberiu Harko, N. Myrzakulov, Ratbay Myrzakulov +1
Мақола20213 иқтибосABIConstraining f(R) gravity in solar system, cosmology and binary pulsar systems
Мақола20172 иқтибосABI