Radiative Corrections to the Direct Detection of Inelastic Scattering of Higgsino-like Neutralino Dark Matter
Abstract
The direct detection (DD) of Higgsino-like dark matter (DM) through inelastic scattering processes may provide a promising avenue, along with the elastic scattering, when the mass splitting between the neutral Higgsino pairs is extremely tiny. The mass splitting can be reduced further by adopting the on-shell renormalization for the neutral and charged Higgsinos in the MSSM. Moreover, all the one-loop electroweak (EW) corrections to the three-point vertices for the neutralino(s)-Higgs interactions have been considered, while both elastic and inelastic DM-nucleon scattering cross-sections have been calculated primarily through Higgs exchange. Subsequently, the expected number of scattering events in the latest LUX-ZEPLIN (LZ) DD experiment are also computed. Our results highlight a few scenarios in which the inelastic component may exceed the corresponding elastic component, leading to enhanced direct detection scattering rates.
Related
- NNLO QED corrections and inelastic two-photon exchange in elastic lepton-proton scattering with McMule
- Power corrections to heavy-quark spin correlations in small-x deep-inelastic scattering
- Radiative Corrections to Elastic Lepton-Proton Scattering with Focus on Two-Photon-Exchange Diagrams
- Dark Matter Inelastic Scattering with Nuclei for Direct Detection
- Neutralino Dark Matter in SU(5) after H.E.S.S. and Direct-Detection Searches
BibTeX
@misc{chatterjee2026radiative,
title = {{Radiative Corrections to the Direct Detection of Inelastic Scattering of Higgsino-like Neutralino Dark Matter}},
author = {Arindam Chatterjee and Debottam Das and Syed Adil Pasha and Alexander Pukhov and Rahul Puri},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.09830},
eprint = {2609.09830},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.09830},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Radiative Corrections to the Direct Detection of Inelastic Scattering of Higgsino-like Neutralino Dark Matter
AU - Arindam Chatterjee
AU - Debottam Das
AU - Syed Adil Pasha
AU - Alexander Pukhov
AU - Rahul Puri
PY - 2026
DA - 2026/09/09
PB - arXiv
DO - 10.48550/arxiv.2609.09830
UR - https://arxiv.org/abs/2609.09830
AB - The direct detection (DD) of Higgsino-like dark matter (DM) through inelastic scattering processes may provide a promising avenue, along with the elastic scattering, when the mass splitting between the neutral Higgsino pairs is extremely tiny. The mass splitting can be reduced further by adopting the on-shell renormalization for the neutral and charged Higgsinos in the MSSM. Moreover, all the one-loop electroweak (EW) corrections to the three-point vertices for the neutralino(s)-Higgs interactions have been considered, while both elastic and inelastic DM-nucleon scattering cross-sections have been calculated primarily through Higgs exchange. Subsequently, the expected number of scattering events in the latest LUX-ZEPLIN (LZ) DD experiment are also computed. Our results highlight a few scenarios in which the inelastic component may exceed the corresponding elastic component, leading to enhanced direct detection scattering rates.
ER -