Accelerating universes with scaling dark matter M Chevallier, D Polarski International Journal of Modern Physics D 10 (02), 213-223, 2001 | 2106 | 2001 |

Reconstruction of a scalar-tensor theory of gravity in an accelerating universe B Boisseau, G Esposito-Farese, D Polarski, AA Starobinsky Physical Review Letters 85 (11), 2236, 2000 | 890 | 2000 |

Conditions for the cosmological viability of dark energy models L Amendola, R Gannouji, D Polarski, S Tsujikawa Physical Review D 75 (8), 083504, 2007 | 809 | 2007 |

Semiclassicality and decoherence of cosmological perturbations D Polarski, AA Starobinsky Classical and Quantum Gravity 13 (3), 377, 1996 | 636 | 1996 |

Are f (R) dark energy models cosmologically viable? L Amendola, D Polarski, S Tsujikawa Physical review letters 98 (13), 131302, 2007 | 546 | 2007 |

Scalar-tensor gravity in an accelerating universe G Esposito-Farese, D Polarski Physical Review D 63 (6), 063504, 2001 | 454 | 2001 |

Spectra of perturbations produced by double inflation with an intermediate matter-dominated stage D Polarski, AA Starobinsky Nuclear Physics B 385 (3), 623-650, 1992 | 313 | 1992 |

Scalar–tensor models of normal and phantom dark energy R Gannouji, D Polarski, A Ranquet, AA Starobinsky Journal of Cosmology and Astroparticle Physics 2006 (09), 016, 2006 | 269 | 2006 |

Isocurvature perturbations in multiple inflationary models D Polarski, AA Starobinsky Physical Review D 50 (10), 6123, 1994 | 259 | 1994 |

Quantum-to-classical transition for fluctuations in the early universe C Kiefer, D Polarski, AA Starobinsky International Journal of Modern Physics D 7 (03), 455-462, 1998 | 257 | 1998 |

Why do cosmological perturbations look classical to us? C Kiefer, D Polarski Advanced science letters 2 (2), 164-173, 2009 | 194 | 2009 |

Quantum-to-classical transition of cosmological perturbations for non-vacuum initial states J Lesgourgues, D Polarski, AA Starobinsky Nuclear Physics B 497 (1-2), 479-508, 1997 | 192 | 1997 |

On the growth of linear perturbations D Polarski, R Gannouji Physics Letters B 660 (5), 439-443, 2008 | 167 | 2008 |

Pointer states for primordial fluctuations in inflationary cosmology C Kiefer, I Lohmar, D Polarski, AA Starobinsky Classical and Quantum Gravity 24 (7), 1699, 2007 | 159 | 2007 |

The growth of matter perturbations in f (R) models R Gannouji, B Moraes, D Polarski Journal of Cosmology and Astroparticle Physics 2009 (02), 034, 2009 | 138 | 2009 |

Dispersion of growth of matter perturbations in f (R) gravity S Tsujikawa, R Gannouji, B Moraes, D Polarski Physical Review D 80 (8), 084044, 2009 | 136 | 2009 |

Power-laws f (R) theories are cosmologically unacceptable L Amendola, D Polarski, S Tsujikawa International Journal of Modern Physics D 16 (10), 1555-1561, 2007 | 114 | 2007 |

The growth of matter perturbations in some scalar–tensor DE models R Gannouji, D Polarski Journal of Cosmology and Astroparticle Physics 2008 (05), 018, 2008 | 107 | 2008 |

Structure of primordial gravitational waves spectrum in a double inflationary model D Polarski, AA Starobinsky Physics Letters B 356 (2-3), 196-204, 1995 | 106 | 1995 |

Can primordial black holes be a significant part of dark matter? D Blais, C Kiefer, D Polarski Physics Letters B 535 (1-4), 11-16, 2002 | 105 | 2002 |