Investigating Neutralino Annihilations Using DarkSUSY
S. Kamel, E. eSilva
Abstract
Open-access reader
S. Kamel, E. eSilva
Abstract
Open-access reader
Physicists do not fully understand the nature of dark matter although we infer its existence from experimental observation. This project is part of the dark matter detection searches with the Gamma-Ray Large Area Space Telescope (GLAST). We are investigating one of the Weakly Interacting Massive Particles (WIMP) candidates called the neutralino, a particle predicted by the Minimal Supersymmetric Standard Model. In particular, we ran a computer simulation called DarkSUSY that predicts the signature that we expect to see in the data from GLAST that pertains to the detection of the neutralino in the galactic halo.
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Physicists do not fully understand the nature of dark matter although we infer its existence from experimental observation. This project is part of the dark matter detection searches with the Gamma-Ray Large Area Space Telescope (GLAST). We are investigating one of the Weakly Interacting Massive Particles (WIMP) candidates called the neutralino, a particle predicted by the Minimal Supersymmetric Standard Model. In particular, we ran a computer simulation called DarkSUSY that predicts the signature that we expect to see in the data from GLAST that pertains to the detection of the neutralino in the galactic halo.
Key concepts: WIMP, Neutralino, Dark matter, Weakly interacting massive particles, Physics, Galactic halo, Particle physics, Astrophysics