| Accelerating universes with scaling dark matter M Chevallier, D Polarski International Journal of Modern Physics D 10 (02), 213-223, 2001 | 2653 | 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 | 964 | 2000 |
| Conditions for the cosmological viability of dark energy models L Amendola, R Gannouji, D Polarski, S Tsujikawa Physical Review D—Particles, Fields, Gravitation, and Cosmology 75 (8), 083504, 2007 | 935 | 2007 |
| Semiclassicality and decoherence of cosmological perturbations D Polarski, AA Starobinsky Classical and Quantum Gravity 13 (3), 377, 1996 | 746 | 1996 |
| Are f (R) dark energy models cosmologically viable? L Amendola, D Polarski, S Tsujikawa Physical review letters 98 (13), 131302, 2007 | 619 | 2007 |
| Scalar-tensor gravity in an accelerating universe G Esposito-Farese, D Polarski Physical Review D 63 (6), 063504, 2001 | 499 | 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 | 342 | 1992 |
| 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 | 318 | 1998 |
| 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 | 292 | 2006 |
| Isocurvature perturbations in multiple inflationary models D Polarski, AA Starobinsky Physical Review D 50 (10), 6123, 1994 | 274 | 1994 |
| Why do cosmological perturbations look classical to us? C Kiefer, D Polarski Advanced science letters 2 (2), 164-173, 2009 | 255 | 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 | 254 | 2007 |
| 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 | 233 | 1997 |
| Pointer states for primordial fluctuations in inflationary cosmology C Kiefer, I Lohmar, D Polarski, AA Starobinsky Classical and Quantum Gravity 24 (7), 1699, 2007 | 193 | 2007 |
| On the growth of linear perturbations D Polarski, R Gannouji Physics Letters B 660 (5), 439-443, 2008 | 185 | 2008 |
| 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 | 163 | 2009 |
| Dispersion of growth of matter perturbations in gravity S Tsujikawa, R Gannouji, B Moraes, D Polarski Physical Review D—Particles, Fields, Gravitation, and Cosmology 80 (8), 084044, 2009 | 154 | 2009 |
| Generalizing the running vacuum energy model and comparing<? format?> with the entropic-force models S Basilakos, D Polarski, J Sola Physical Review D—Particles, Fields, Gravitation, and Cosmology 86 (4), 043010, 2012 | 117 | 2012 |
| 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 | 116 | 2002 |
| Emergence of classicality for primordial fluctuations: Concepts and analogies C Kiefer, D Polarski Annalen der Physik 510 (3), 137-158, 1998 | 116 | 1998 |
