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Constraining the mSUGRA (minimal supergravity) parameter space using the entropy of dark matter halos

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)

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We 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 \tan \beta \simeq 50 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.


Keywords

dark matter

structure of galaxies

cosmology of theories beyond the SM

PACS

95.35.+d Dark matter (stellar, interstellar, galactic, and cosmological)

04.65.+e Supergravity

98.62.Gq Galactic halos

14.80.Ly Supersymmetric partners of known particles

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

95.30.Tg Thermodynamic processes, conduction, convection, equations of state

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 05 (May 2008)

Received 23 October 2007, accepted for publication 18 April 2008

Published 6 May 2008



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