Sfoglia per Autore TROISI, Antonio
Quintessence without scalar fields. In: Recent Research Developments in Astronomy and Astrophysics
2003-01-01 Capozziello, S.; Carloni, S.; Troisi, A.
Matching torsion A-term with observations
2003-01-01 Capozziello, S; Cardone, Vf; Piedipalumbo, E; Sereno, M; Troisi, A
Cosmological consequences of an inhomogeneous space-time
2004-01-01 Canfora, F; Troisi, A
Unified dark energy models: A phenomenological approach
2004-01-01 Cardone, V. F.; Troisi, A.; Capozziello, S.
Can higher order curvature theories explain rotation curves of galaxies?
2004-01-01 Capozziello, S; Cardone, Vf; Carloni, S; Troisi, A
Phenomenological model for inflationary quintessence
2005-01-01 Cardone, Vf; Troisi, A; Capozziello, S
Higher order curvature theories of gravity matched with observations: a bridge between dark energy and dark matter problems
2005-01-01 Capozziello, S; Cardone, Vf; Carloni, S; Troisi, A
Parametrized post-Newtonian limit of fourth order gravity inspired by scalar-tensor gravity
2005-01-01 Capozziello, S.; Troisi, A.
Reconciling dark energy models with f(R) theories
2005-01-01 Capozziello, S.; Cardone, V. F.; Troisi, A.
Constraining Van der Waals quintessence with observations
2005-01-01 Capozziello, S; F Cardone, V; Carloni, S; De Martino, S; Falanga, M; Troisi, A; Bruni, M
Cosmological dynamics of R n gravity
2005-01-01 Carloni, S; S Dunsby, P K; Capozziello, S; Troisi, A
Beyond the perfect fluid hypothesis for the dark energy equation of state
2006-01-01 Cardone, V. F.; Tortora, C.; Troisi, A.; Capozziello, S.
Gravitational lensing in fourth order gravity
2006-01-01 Capozziello, S.; Cardone, V. F.; Troisi, A.
Dark energy and dark matter as curvature effects?
2006-01-01 Capozziello, S; F Cardone, V; Troisi, A
A fluid of strings as a viable candidate for the dark side of the universe
2006-01-01 Capozziello, S; Cardone, Vf; Lambiase, G; Troisi, A
FOURTH-ORDER GRAVITY AND EXPERIMENTAL CONSTRAINTS ON EDDINGTON PARAMETERS
2006-01-01 Capozziello, S.; Stabile, A.; Troisi, A.
Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
2006-01-01 Capozziello, S.; Nojiri, S.; Odintsov, S. D.; Troisi, A.
Structure formation and CMBR anisotropy spectrum in the inflessence model
2006-01-01 Sen, Aa; Cardone, Vf; Capozziello, S; Troisi, A
Cosmological model with born-infeld type scalar field
2007-01-01 Troisi, A; Serie, E; Kerner, R
Newtonian limit of f(R) gravity
2007-01-01 Capozziello, S.; Stabile, A.; Troisi, A.
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