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Иш: Signature flips in time-varying $\Lambda (t)$ cosmological models with observational data
The role of energy conditions in f(R) cosmology
Salvatore Capozzıello, Shin’ichi Nojiri, Sergei D. Odintsov
Мақола20188 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 иқтибосABIPrecision Cosmology? Not Just Yet . . .
Sarah Bridle, O. Lahav, Jeremiah P. Ostriker +1
Мақола20034 иқтибосABIRunning vacuum against the H <sub>0</sub> and σ<sub>8</sub> tensions
Joan Solà, Adrià Gómez-Valent, Javier de Cruz Pérez +1
Мақола20214 иқтибосABI