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20042006
most citedCMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe

148 citations · 270 across the 4 of their papers we have counts for

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astro-ph2006103 cited

The supernova Hubble diagram for off-center observers in a spherically symmetric inhomogeneous universe

Havard Alnes, Morad Amarzguioui

We have previously shown that spherically symmetric, inhomogeneous universe models can explain both the supernova data and the location of the first peak in the CMB spectrum withou…

astro-ph2006148 cited

CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe

Havard Alnes, Morad Amarzguioui

The current authors have previously shown that inhomogeneous, but spherically symmetric universe models containing only matter can yield a very good fit to the SNIa data and the po…

astro-ph2005

An inhomogeneous alternative to dark energy?

Havard Alnes, Morad Amarzguioui, Oyvind Gron

Recently, there have been suggestions that the apparent accelerated expansion of the universe is not caused by repulsive gravitation due to dark energy, but is rather a result of i…

astro-ph2005

Cosmological constraints on f(R) gravity theories within the Palatini approach

M. Amarzguioui, O. Elgaroy, D. F. Mota +1

We investigate f(R) theories of gravity within the Palatini approach and show how one can determine the expansion history, H(a), for an arbitrary choice of f(R). As an example, we…

astro-ph2005

Can a dust dominated universe have accelerated expansion?

H. Alnes, M. Amarzguioui, O. Gron

Recently, there has been suggestions that the apparent accelerated expansion of the universe is due not to a cosmological constant, but rather to inhomogeneities in the distributio…

astro-ph2004

Combined constraints on Cardassian models from supernovae, CMB and large-scale structure observations

Morad Amarzguioui, Oystein Elgaroy, Tuomas Multamaki

We confront Cardassian models with recent observational data. These models can be viewed either as purely phenomenological modifications of the Friedmann equation, or as arising fr…