David Polarski

1. Conditions for the cosmological viability off(R)dark energy models
   2006/12/31 by Luca Amendola, Radouane Gannouji, David Polarski +1 · 28 citations
   Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph #gr-qc #hep-ph #hep-th
2. On the growth of linear perturbations
   2007/10/11 by David Polarski, Radouane Gannouji · 11 citations
   Mathematics · Physics and Astronomy · #Advanced Differential Equations and Dynamical Systems #Cosmology and Gravitation Theories #Mathematical Dynamics and Fractals #astro-ph #gr-qc
3. Semiclassicality and Decoherence of Cosmological Perturbations
   1995/04/30 by David Polarski, Alexei A. Starobinsky · 2 citations
   Physics and Astronomy · #gr-qc #astro-ph #hep-th #quant-ph
4. Why do cosmological perturbations look classical to us?
   2008/10/31 by Claus Kiefer, David Polarski · 3 citations
   Physics and Astronomy · #astro-ph #gr-qc #quant-ph
5. Dispersion of growth of matter perturbations inf(R)gravity
   2009/08/19 by Shinji Tsujikawa, Radouane Gannouji, Bruno Moraes +1 · 3 citations
   Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph.CO #gr-qc #hep-ph #hep-th