23-27 mayo 2016
Europe/Madrid timezone

Neutralino dark matter and naturalness in the MSSM

27 may. 2016 12:30
20m
Contributed talk SUSY/Higgs/BSM Astro-Neutrino 10

Ponente

Sandra Robles (IFT, UAM-CSIC)

Descripción

Most of the MSSM DM scenarios (well-tempered neutralinos, funnels, co-annihilation) imply some kind of fine-tuning. We have studied this problem in an, as much as possible, exhaustive and rigorous way. I will present a brief discussion about the statistical meaning of the fine-tuning and how it should be computed for the DM abundance, and combined with the EW fine-tuning. Our results are very robust and model-independent and favour some scenarios, like the h-funnel when the neutralino mass is not too close to m_h/2, with respect to others, such as the pure wino case.

Autor primario

Sandra Robles (IFT, UAM-CSIC)

Coautor

Alberto Casas (IFT UAM)

Materiales de la presentación

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