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Luca Amendola
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1.
Dark Matter from an ultra-light pseudo-Goldsone-boson
Luca Amendola
;
Riccardo Barbieri
;
23 Sep 2005
2.
Phantom energy mediates a long-range repulsive force
Luca Amendola
;
22 Sep 2004
/ Phys.Rev.Lett. 93 (2004) 181102
3.
Supernovae type Ia data favour coupled phantom energy
Elisabetta Majerotto
;
Domenico Sapone
;
Luca Amendola
;
22 Oct 2004
4.
Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
Luca Amendola
;
Claudia Quercellini
;
Emanuele Giallongo
;
30 Apr 2004
/ Mon.Not.Roy.Astron.Soc. 357 (2005) 429-439
5.
Skewness as a test of the equivalence principle
Luca Amendola
;
Claudia Quercellini
;
1 Mar 2004
/ Phys.Rev.Lett. 92 (2004) 181102
6.
Linear and non-linear perturbations in dark energy models
Luca Amendola
;
7 Nov 2003
/ Phys.Rev. D69 (2004) 103524
7.
Acceleration at z>1?
Luca Amendola
;
24 Sep 2002
/ Mon.Not.Roy.Astron.Soc. 342 (2003) 221-226
8.
Constraints on the interaction and self-interaction of dark energy from cosmic microwave background
Luca Amendola
;
Claudia Quercellini
;
Domenico Tocchini-Valentini
;
Alessandro Pasqui
;
7 May 2002
/ Astrophys.J. 583 (2003) L53
9.
Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
Domenico Tocchini-Valentini
;
Luca Amendola
;
8 Aug 2001
/ Phys.Rev. D65 (2002) 063508
10.
The dependence of cosmological parameters estimated from the microwave background on non-gaussianity
Luca Amendola
;
27 Jul 2001
/ Astrophys.J. 569 (2002) 595-599
11.
Stationary dark energy: the present universe as a global attractor
Luca Amendola
;
Domenico Tocchini-Valentini
;
13 Nov 2000
/ Phys.Rev. D64 (2001) 043509
12.
The Dyer-Roeder distance in quintessence cosmology and the estimation of H_0 through time-delays
Fabio Giovi
;
Franco Occhionero
;
Luca Amendola
;
5 Nov 2000
/ Mon.Not.Roy.Astron.Soc. 325 (2001) 1097
13.
Dark energy and the Boomerang data
Luca Amendola
;
21 Jun 2000
/ Phys.Rev.Lett. 86 (2001) 196-199
14.
Coupled Quintessence
Luca Amendola
;
3 Aug 1999
/ Phys.Rev. D62 (2000) 043511
15.
Time variability of the gravitational constant and Type Ia supernovae
Luca Amendola
;
Stefano Corasaniti
;
Franco Occhionero
;
16 Jul 1999
16.
Perturbations in a coupled scalar field cosmology
Luca Amendola
;
4 Jun 1999
/ Mon.Not.Roy.Astron.Soc. 312 (2000) 521
17.
The scale of homogeneity in the Las Campanas Redshift Survey
Luca Amendola
;
Emilia Palladino
;
29 Dec 1998
/ Astrophys.J. 514 (1999) L1
18.
Non-Gaussian Chi-squared method with the multivariate Edgeworth expansion
Luca Amendola
;
13 Oct 1998
/ Astro. Lett. and Communications, 1996, 33, 63
19.
Reconstruction of the bubble nucleating potential
Luca Amendola
;
Carlo Baccigalupi
;
Rostislav Konoplich
;
Franco Occhionero
;
Sergei Rubin
;
4 Oct 1996
/ Phys.Rev. D54 (1996) 7199-7206
20.
Non-Gaussian Likelihood Function
Luca Amendola
;
9 Apr 1995
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