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PTOLEMY's test of generalized neutrino interactions: unveiling challenges and constraints
Unanswered questions surrounding neutrinos have motivated investigations into physics beyond the standard model (SM) of particle physics. In particular, generalized neutrino interactions (GNI) provide a broader framework for studying these effects compared to the commonly studied non-standard neutri...
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Published in: | Journal of cosmology and astroparticle physics 2024-04, Vol.2024 (4), p.2 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Unanswered questions surrounding neutrinos have motivated investigations into physics
beyond the standard model (SM) of particle physics. In particular, generalized neutrino
interactions (GNI) provide a broader framework for studying these effects compared to the commonly
studied non-standard neutrino interactions. These interactions are described by higher dimensional
operators while maintaining the gauge symmetries of the SM. Furthermore, the cosmic neutrino
background, a predicted component of the SM and standard cosmology, has yet to be directly
detected. To shed light on this elusive phenomenon, we conduct a comprehensive analysis of the
relevant GNI, specifically focusing on their implications for the proposed cosmic neutrino
detector PTOLEMY. We make an attempt to see the capabilities and the limitations of PTOLEMY in
sensing GNI while remaining optimistic regarding PTOLEMY's experimental resolution. These
interactions play a significant role in modifying the electron spectrum resulting from the capture
of cosmic neutrinos on radioactive tritium. This work also explores how the presence of these
interactions influences the differential electron spectrum, taking into account factors such as
finite experimental resolution, the mass of the lightest neutrino eigenstate, the strength of the
interactions, and the ordering of neutrino mass. |
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ISSN: | 1475-7516 1475-7516 |
DOI: | 10.1088/1475-7516/2024/04/002 |