activity
20002009
most citedSpherically symmetric solutions of modified field equations in f(R) theories of gravity

352 citations · 819 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2009★ 40 cited

Gravitational waves from the fragmentation of a supersymmetric condensate

Alexander Kusenko, Anupam Mazumdar, Tuomas Multamaki

We discuss the production of gravity waves from the fragmentation of a supersymmetric condensate in the early universe. Supersymmetry predicts the existence of flat directions in t…

hep-th2008★ 20 cited

Fitting oscillating string gas cosmology to supernova data

Francesc Ferrer, Tuomas Multamaki, Syksy Rasanen

In string gas cosmology, extra dimensions are stabilised by a gas of strings. In the matter-dominated era, competition between matter pushing the extra dimensions to expand and the…

astro-ph2008★ 17 cited

Non-Gaussianity in three fluid curvaton model

Tuomas Multamaki, Jani Sainio, Iiro Vilja

The generation of non-gaussianity is studied in a three fluid curvaton model. By utilizing second order perturbation theory we derive general formulae for the large scale temperatu…

astro-ph2007★ 6 cited

Large tensor-to-scalar ratio and low scale inflation

Rouzbeh Allahverdi, Anupam Mazumdar, Tuomas Multamaki

It is plausible that the scalar density perturbations are created by a relatively low scale model of inflation which predicts the CMB anisotropy and excites Standard Model baryon a…

astro-ph2007★ 82 cited

On using the CMB shift parameter in tests of models of dark energy

Oystein Elgaroy, Tuomas Multamaki

The so-called shift parameter is related to the position of the first acoustic peak in the power spectrum anisotropies of the cosmic microwave background (CMB) anisotropies. It is…

astro-ph2006★ 2 cited

Suppression of the large scale curvature perturbation by interacting fluids

T. Multamaki, J. Sainio, I. Vilja

The large-scale dynamics of a two-fluid system with a time dependent interaction is studied analytically and numerically. We show how a rapid transition can significantly suppress…