Speaker
Mr
German Gomez-Vargas
(IFT UAM/CSIC Madrid - INFN Roma Tor Vergata)
Description
The munuSSM is a supersymmetric model that has been proposed to solve the problems of
other supersymmetric extensions of the standard model. The gravitino is a natural
candidate for dark matter in the munuSSM and could be detectable through the emission
of a monochromatic gamma ray in a two-body decay.
We study the prospects of the Fermi-LAT telescope to detect such monochromatic lines
in 5 years of observations of the most massive extragalactic objects.
The dark matter halo around the Virgo galaxy cluster is selected as a reference case,
since it is associated to a particularly high signal-to-noise ratio and is located in
a region scarcely affected by the presence of astrophysical point sources.
The simulation of both signal and background gamma-ray events is carried out with the
Fermi Science Tools, and the dark matter distribution around Virgo is taken from a
$N$-body simulation with constrained initial conditions provided by the CLUES project.
We find that a gravitino with a mass range of 0.5--10 GeV approximately, and with a
lifetime of about 5e27 s (1e28 s) would be detectable by the Fermi-LAT with a
signal-to-noise of 5 (3).
Primary author
Mr
German Gomez-Vargas
(IFT UAM/CSIC Madrid - INFN Roma Tor Vergata)
Co-authors
Antonio Cuesta
(Yale University)
Carlos Munoz
(IFT UAM/CSIC Madrid)
Fabio Zandanel
(Instituto de Astrofisica de Andalucia (IAA - CSIC))
Francisco Prada
(Instituto de Astrofisica de Andalucia (IAA - CSIC))
Gustavo Yepes
(Universidad Aut ́noma de Madrid)
Mattia Fornasa
(Instituto de Astrofisica de Andalucia (IAA - CSIC))
