Speaker
Seyda Ipek
Description
A pseudo-Dirac bino could be responsible for generating nuetrino masses in R-symmetric MSSM. We show that this bino, which we rename bi$\nu$o can be long lived in certain parameter regions and could be searched for in proposed experiments like MATHUSLA and CODEX-b. These experiments can probe biνo masses of 10 GeV-2 TeV and SUSY messenger scales $10^{2−11}$ TeV for a range of squark masses.
Author
Seyda Ipek
Co-author
Julia Gehrlein