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27 April 2024
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David Polarski
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1.
Can Primordial Black Holes be a Significant Part of Dark Matter ?
David Blais
;
Claus Kiefer
;
David Polarski
;
29 Mar 2002
/ Phys.Lett. B535 (2002) 11-16
2.
Can Lightcone Fluctuations be Probed with Cosmological Backgrounds?
David Polarski
;
Philippe Roche
;
7 Dec 2004
/ Mod.Phys.Lett. A20 (2005) 499-508
3.
Primordial Black Holes in an Accelerating Universe
David Polarski
;
13 Dec 2001
/ Phys.Lett. B528 (2002) 193-198
4.
Primordial Black Holes from inflationary models with and without Broken Scale Invariance
Torsten Bringmann
;
Claus Kiefer
;
David Polarski
;
24 Sep 2001
/ Phys.Rev. D65 (2002) 024008
5.
Classicality of primordial fluctuations and Primordial Black Holes
David Polarski
;
21 Sep 2001
/ Int.J.Mod.Phys. D10 (2001) 927
6.
Accelerated Expansion: Theory and Observations
David Polarski
;
20 Sep 2001
7.
Primordial Fluctuations from Inflation: a Consistent Histories Approach
David Polarski
;
2 Dec 1998
/ Phys.Lett. B446 (1999) 53-57
8.
On the Phase-Space Volume of Primordial Cosmological Perturbations
Julien Lesgourgues
;
David Polarski
;
Alexei A. Starobinsky
;
15 Jun 1998
/ Class.Quant.Grav. 14 (1997) 881-888
9.
The Coherence of Primordial Fluctuations Produced During Inflation
Claus Kiefer
;
Julien Lesgourgues
;
David Polarski
;
Alexei A. Starobinsky
;
15 Jun 1998
/ Class.Quant.Grav. 15 (1998) L67-L72
10.
Quantum-to-classical Transition of Cosmological Perturbations for Non-vacuum Initial States
Julien Lesgourgues
;
David Polarski
;
Alexei A. Starobinsky
;
7 Nov 1996
/ Nucl.Phys. B497 (1997) 479-510
11.
On the equation of state of Dark Energy
D. Polarski
;
A. Ranquet
;
12 Jul 2005
/ Phys.Lett. B627 (2005) 1-8
12.
Galactic Cosmic Rays from PBHs and Primordial Spectra with a Scale
A. Barrau
;
D. Blais
;
G. Boudoul
;
D. Polarski
;
7 Oct 2002
/ Phys.Lett. B551 (2003) 218-225
13.
Accelerating Universes with Scaling Dark Matter
M. Chevallier
;
D. Polarski
;
4 Sep 2000
/ Int.J.Mod.Phys. D10 (2001) 213-224
14.
Direct Detection of Primordial Gravitational Waves in a BSI Inflationary Model
D. Polarski
;
17 Jun 1999
/ Phys.Lett. B458 (1999) 13-18
15.
Chameleon dark energy models with characteristic signatures
Radouane Gannouji
;
Bruno Moraes
;
David F. Mota
;
David Polarski
;
Shinji Tsujikawa
;
Hans A. Winther
;
19 Oct 2010
16.
Accurate results for primordial black holes from spectra with a distinguished scale
David Blais
;
Torsten Bringmann
;
Claus Kiefer
;
David Polarski
;
16 Jun 2002
/ Phys.Rev. D67 (2003) 024024
17.
Weak gravity on a $Lambda$CDM background
Radouane Gannouji
;
Leandros Perivolaropoulos
;
David Polarski
;
Foteini Skara
;
3 Nov 2020
18.
A negative cosmological constant in the dark sector?
Rodrigo Calderón
;
Radouane Gannouji
;
Benjamin L'Huillier
;
David Polarski
;
24 Aug 2020
19.
Defying the laws of Gravity I: Model-independent reconstruction of the Universe expansion from growth data
Benjamin L'Huillier
;
Arman Shafieloo
;
David Polarski
;
Alexei A. Starobinsky
;
14 Jun 2019
20.
A critical assessment of some inhomogeneous pressure Stephani models
Adam Balcerzak
;
Mariusz P. Dabrowski
;
Tomasz Denkiewicz
;
David Polarski
;
Denis Puy
;
2 Sep 2014
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