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Иш: Cosmological dynamics of dark energy in Ricci inverse gravity
<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>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity
Tiberiu Harko, Francisco S. N. Lobo, Shin’ichi Nojiri +1
Мақола201182 иқтибосABIUnified cosmic history in modified gravity: From <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si10.gif" display="inline" overflow="scroll"><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> theory to Lorentz non-invariant models
Shin’ichi Nojiri, Sergei D. Odintsov
Мақола201152 иқтибосABITeleparallel gravity: from theory to cosmology
Sebastián Bahamonde, Konstantinos F. Dialektopoulos, Celia Escamilla‐Rivera +7
Шарҳ мақола202219 иқтибосABICosmological parameters from SDSS and WMAP
Max Tegmark, Michael A. Strauss, Michael R. Blanton +64
Мақола200411 иқтибосABIHydrostatic equilibrium and stellar structure 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
Salvatore Capozzıello, Mariafelicia De Laurentis, Sergei D. Odintsov +1
Мақола201110 иқтибосABIEinasto-inspired non-commutative black holes within dark matter galactic halos in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si8.svg" display="inline" id="d1e849"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="double-struck">Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity
S. Khan, Javlon Rayimbaev, Inomjon Ibragimov +2
ABIParametrization of Deceleration Parameter in f(Q) Gravity
Gaurav N. Gadbail, Sanjay Mandal, P. K. Sahoo
Мақола20228 иқтибосABIInflationary Cosmology in Modified Gravity Theories
Kazuharu Bamba, Sergei Odintsov
Мақола20157 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
Мақола20076 иқтибосABINon-flat pilgrim dark energy FRW models in modified gravity
Shamaila Rani, Abdul Jawad, Ines G. Salako +1
Мақола20166 иқтибосABI