TY  - JOUR
AU  - Kim, J. S.
AU  - Lopez-Fogliani, D. E.
AU  - Perez, A. D.
AU  - Ruiz de Austri, R.
PY  - 2022
DA  - 2022//
TI  - The new (g-2)(mu) and right-handed sneutrino dark matter
T2  - Nucl. Phys. B
JO  - Nuclear Physics B
SP  - 115637
EP  - 23pp
VL  - 974
PB  - Elsevier
AB  - In this paper we investigate the (g – 2)(mu) discrepancy in the context of the R-parity conserving next-to minimal supersymmetric Standard Model plus right-handed neutrinos superfields. The model has the ability to reproduce neutrino physics data and includes the interesting possibility to have the right-handed sneutrino as the lightest supersymmetric particle and a viable dark matter candidate. Since right-handed sneutrinos are singlets, no new contributions for delta a(mu) with respect to the MSSM and NMSSM are present. However, the possibility to have the right-handed sneutrino as the lightest supersymmetric particle opens new ways to escape Large Hadron Collider and direct detection constraints. In particular, we find that dark matter masses within 10 less than or similar to m((upsilon) over tildeR) less than or similar to 600 GeV are fully compatible with current experimental constraints. Remarkably, not only spectra with light sleptons are needed, but we obtain solutions with m((mu) over tilde) greater than or similar to 600 GeV in the entire dark matter mass range that could be probed by new (g – 2)(mu) data in the near future. In addition, dark matter direct detection experiments will be able to explore a sizable portion of the allowed parameter space with mvR < 300 GeV, while indirect detection experiments will be able to probe a much smaller fraction within 200 less than or similar to m((nu)over tilde>R) less than or similar to 350 GeV.
SN  - 0550-3213
UR  - https://arxiv.org/abs/2107.02285
UR  - https://doi.org/10.1016/j.nuclphysb.2021.115637
DO  - 10.1016/j.nuclphysb.2021.115637
LA  - English
N1  - WOS:000760320700019
ID  - Kim_etal2022
ER  -