University of Cambridge > > HEP phenomenology joint Cavendish-DAMTP seminar > MSSM4G scenario

MSSM4G scenario

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Dr Maria Ubiali.

We discuss an extension to the MSSM , so-called MSSM4G scenario, which realises Bino dark matter compatible with the observed relic density by introducing 4th-generation particles. This scenario has many implications for current and future BSM searches. In particular, it will provide characteristic signals in gamma-ray observations and/or LHC experiments. We will see that the two types of searches work complementarily, and the combination will allow us to discover or exclude the MSSM4G models in the next few years.

This talk is part of the HEP phenomenology joint Cavendish-DAMTP seminar series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.


© 2006-2023, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity