Darío Núñez et al JCAP05(2008)003 doi:10.1088/1475-7516/2008/05/003
Darío Núñez1, Jesús Zavala1,4, Lukas Nellen1, Roberto A Sussman1,5, Luis G Cabral-Rosetti2 and Myriam Mondragón3 (For the Instituto Avanzado de Cosmología, IAC)
Show affiliationsWe derive an expression for the entropy of a dark matter halo described using a Navarro–Frenk–White model with a core. The comparison of this entropy with that of dark matter in the freeze-out era allows us to constrain the parameter space in mSUGRA models. Moreover, combining these constraints with the ones obtained from the usual abundance criterion and demanding that these criteria be consistent with the 2σ bounds for the abundance of dark matter: 0.112≤ΩDMh2≤0.122, we are able to clearly identify validity regions among the values of tanβ, which is one of the parameters of the mSUGRA model. We found that for the regions of the parameter space explored, small values of tanβ are not favored; only for
are the two criteria significantly consistent. In the region where the two criteria are consistent we also found a lower bound for the neutralino mass, mχ≥141 GeV.
95.35.+d Dark matter (stellar, interstellar, galactic, and cosmological)
14.80.Ly Supersymmetric partners of known particles
95.30.Tg Thermodynamic processes, conduction, convection, equations of state
Issue 05 (May 2008)
Received 23 October 2007, accepted for publication 18 April 2008
Published 6 May 2008
Darío Núñez et al JCAP05(2008)003
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