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Direct detection of neutralino dark matter in supergravity

Seungwon Baek1, David G. Cerdeño2, Yeong Gyun Kim3, Pyungwon Ko4 and Carlos Muñoz5,6

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The direct detection of neutralino dark matter is analysed in general supergravity scenarios, where non-universal soft scalar and gaugino masses can be present. In particular, the theoretical predictions for the neutralino-nucleon cross section are studied and compared with the sensitivity of dark matter detectors. We take into account the most recent astrophysical and experimental constraints on the parameter space, including the current limit on B(Bs0μ+μ). The latter puts severe limitations on the dark matter scattering cross section, ruling out most of the regions that would be within the reach of present experiments. We show how this constraint can be softened with the help of appropriate choices of non-universal parameters which increase the Higgsino composition of the lightest neutralino and minimise the chargino contribution to the bs transition.

Keywords

Supersymmetry Phenomenology

Supergravity Models

Cosmology of Theories beyond the SM

 

E-print Number: hep-ph/0505019

Cited: by |

Refers: to

PACS

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.)

14.65.Fy Bottom quarks

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

04.65.+e Supergravity

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 06 (June 2005)

Received 12 May 2005, accepted for publication 12 May 2005

Published 10 June 2005



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