2,602 research outputs found
Stochastic quantum inflation for a canonical scalar field with linear self-interaction potential
We apply Starobinsky's formalism of stochastic inflation to the case of a
minimally coupled scalar field with linear self-interaction potential. We solve
the corresponding Fokker-Planck equation exactly, and obtain analytical
expressions for the stochastic expectation values.Comment: 5 pages, no figure
Strange stars in theories of gravity in the Palatini formalism
In the present work we study strange stars in theories of gravity in
the Palatini formalism. We consider two concrete well-known cases, namely the
model as well as the model for two different values
of the mass parameter or . We integrate the modified
Tolman-Oppenheimer-Volkoff equations numerically, and we show the mass-radius
diagram for each model separately. The standard case corresponding to the
General Relativity is also shown in the same figure for comparison. Our
numerical results show that the interior solution can be vastly different
depending on the model and/or the value of the parameter of each model. In
addition, our findings imply that i) for the cosmologically interesting values
of the mass scales the effect of modified gravity on strange stars is
negligible, while ii) for the values predicting an observable effect, the
modified gravity models discussed here would be ruled out by their cosmological
effects.Comment: 10 pages, 2 figure
Gravitino dark matter with neutralino NLSP in the constrained NMSSM
The gravitino dark matter with neutralino NLSP hypothesis is investigated in
the framework of NMSSM. We have considered both the thermal and non-thermal
gravitino production mechanisms, and we have taken into account all the
collider and cosmological constraints. The maximum allowed reheating
temperature after inflation, as well as the maximum allowed gravitino mass are
determined.Comment: Proceedings of the 16th International Symposium on Particles, Strings
and Cosmology (PASCOS 2010), Valencia (Spain), July 19-23, 201
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