activity
19962011
collaborators

10 papers

astro-ph.CO2011

Spherical `Top-Hat' Collapse in general Chaplygin gas dominated universes

R. A. A. Fernandes, J. P. M. de Carvalho, A. Yu. Kamenshchik +2

We expand previous works on the spherical `top-hat' collapse (SC-TH) framework in generalized Chaplygin gas (gCg) dominated universes. Here we allow the collapse in all energetic c…

astro-ph2008

Dark matter from cosmic defects on galactic scales?

N. Guerreiro, P. P. Avelino, J. P. M. de Carvalho +1

We discuss the possible dynamical role of extended cosmic defects on galactic scales, specifically focusing on the possibility that they may provide the dark matter suggested by th…

astro-ph2002

Alternatives to Quintessence Model Building

P. P. Avelino, L. M. G. Beca, J. P. M. de Carvalho +2

We discuss the issue of toy model building for the dark energy component of the universe. Specifically, we consider two generic toy models recently proposed as alternatives to quin…

astro-ph2001

CMB constraints on spatial variations of the vacuum energy density

P. P. Avelino, A. Canavezes, J. P. M. de Carvalho +1

In a recent article, a simple `spherical bubble' toy model for a spatially varying vacuum energy density was introduced, and type Ia supernovae data was used to constrain it. Here…

astro-ph2001

Supernova constraints on spatial variations of the vacuum energy density

P. P. Avelino, J. P. M. de Carvalho, C. J. A. P. Martins

We consider a very simple toy model for a spatially varying `cosmological constant', where we are inside a spherical bubble (with a given set of cosmological parameters) that is su…

astro-ph2000

Can our Universe be inhomogeneous on large sub-horizon scales ?

P. P. Avelino, J. P. M. de Carvalho, C. J. A. P. Martins +1

We show that our Universe may be inhomogeneous on large sub-horizon scales without us being able to realise it. We assume that a network of domain walls permeates the universe divi…