David Polarski

3 ta ish

University of Montpellier

1. Are<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

   MaqolaOAOchiq kirish20077 iqtibos

   ABIABI:AkademIndex/2026.other.001657

2. Conditions for the cosmological viability of<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

   Luca Amendola, Radouane Gannouji, David Polarski +1

   MaqolaOAOchiq kirish20072 iqtibos

   ABIABI:AkademIndex/2026.other.001182

3. Reconstruction of a Scalar-Tensor Theory of Gravity in an Accelerating Universe

   B. Boisseau, Gilles Esposito-Farèse, David Polarski +1

   MaqolaOAOchiq kirish20002 iqtibos

   ABIABI:AkademIndex/2026.other.002061