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20012011
most citedTheoretical predictions for the direct detection of neutralino dark matter in the NMSSM

89 citations · 527 across the 16 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2011★ 36 cited

CLUES on Fermi-LAT prospects for the extragalactic detection of munuSSM gravitino Dark Matter

G. A. Gomez-Vargas, M. Fornasa, F. Zandanel +4

The munuSSM is a supersymmetric model that has been proposed to solve the problems generated by other supersymmetric extensions of the standard model of particle physics. Given tha…

hep-ph2008★ 8 cited

Stau detection at neutrino telescopes in scenarios with supersymmetric dark matter

B. Canadas, D. G. Cerdeno, C. Munoz +1

We have studied the detection of long-lived staus at the IceCube neutrino telescope, after their production inside the Earth through the inelastic scattering of high energy neutrin…

hep-ph2007★ 1 cited

Lepton masses and mixings in orbifold models with three Higgs families

N. Escudero, C. Munoz, A. M Teixeira

We analyse the phenomenological viability of heterotic Z(3) orbifolds with two Wilson lines, which naturally predict three supersymmetric families of matter and Higgs fields. Given…

hep-ph2007★ 9 cited

Prospects for the direct detection of neutralino dark matter in orbifold scenarios

D. G. Cerdeno, T. Kobayashi, C. Munoz

We analyse the phenomenology of orbifold scenarios from the heterotic superstring, and the resulting theoretical predictions for the direct detection of neutralino dark matter. In…

hep-ph2007★ 72 cited

Phenomenological viability of neutralino dark matter in the NMSSM

D. G. Cerdeno, E. Gabrielli, D. E. Lopez-Fogliani +2

The viability of the lightest neutralino as a dark matter candidate in the Next-to-Minimal Supersymmetric Standard Model is analysed. We carry out a thorough analysis of the parame…

hep-ph2005★ 44 cited

Adiabatic compression and indirect detection of supersymmetric dark matter

Y. Mambrini, C. Munoz, E. Nezri +1

Recent developments in the modelling of the dark matter distribution in our Galaxy point out the necessity to consider some physical processes to satisfy observational data. In par…