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Theoretical predictions for the direct detection of neutralino dark matter in the NMSSM

David G. Cerdeño1, Cyril Hugonie2, Daniel E. López-Fogliani3, Carlos Muñoz3 and Ana M. Teixeira3

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We analyse the direct detection of neutralino dark matter in the framework of the Next-to-Minimal Supersymmetric Standard Model. After performing a detailed analysis of the parameter space, taking into account all the available constraints from LEPII, we compute the neutralino-nucleon cross section, and compare the results with the sensitivity of detectors. We find that sizable values for the detection cross section, within the reach of dark matter detectors, are attainable in this framework. For example, neutralino-proton cross sections compatible with the sensitivity of present experiments can be obtained due to the exchange of very light Higgses with mh10lesssim70 GeV. Such Higgses have a significant singlet composition, thus escaping detection and being in agreement with accelerator data. The lightest neutralino in these cases exhibits a large singlino-Higgsino composition, and a mass in the range 50lesssimmtilde chi10lesssim100 GeV.


Keywords

Supersymmetry Phenomenology

Supersymmetric Standard Model

Supersymmetric Effective Theories

Cosmology of Theories beyond the SM

PACS

12.60.Jv Supersymmetric models

12.39.-x Phenomenological quark models

11.15.-q Gauge field theories

11.10.-z Field theory

Subjects

Particle physics and field theory

Dates

Issue 12 (December 2004)

Received 28 October 2004, accepted for publication 18 December 2004

Published 17 January 2005



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