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Peer-reviewedCC BY 4.0Journal of High Energy Physics

Stodolsky effect in the framework of generalised neutrino interactions

  • Siddhartha Bandyopadhyay1,2
  • Ujjal Kumar Dey2
  1. 1Indian Institute of Technology Kanpur
  2. 2Indian Institute of Science Education and Research Berhampur
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Abstract

A bstract : We study the Stodolsky effect utilizing the most general form of neutrino interactions with electrons below the electroweak scale by considering all possible Lorentz invariant operators respecting SU(3) ⨂ U(1) symmetry. We perform our calculation for both Dirac and Majorana neutrinos and find that in the most general setting, only the non-standard neutrino interactions and the tensor interaction terms provide a non-zero contribution, apart from the Standard Model contribution. We investigate the implications for the possible detection of the cosmic neutrino background (C ν B) by analysing the energy shifts that are characteristic of the Stodolsky effect. We also discuss the implication of considerable asymmetry in the C ν B on the present scenario.

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Cite

BibTeXRIS
BibTeX
@article{bandyopadhyay2026stodolsky,
  title = {{Stodolsky effect in the framework of generalised neutrino interactions}},
  author = {Siddhartha Bandyopadhyay and Ujjal Kumar Dey},
  journal = {Journal of High Energy Physics},
  year = {2026},
  month = oct,
  doi = {10.1007/jhep10(2026)024},
  url = {https://link.springer.com/10.1007/JHEP10(2026)024},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Stodolsky effect in the framework of generalised neutrino interactions
AU  - Siddhartha Bandyopadhyay
AU  - Ujjal Kumar Dey
PY  - 2026
DA  - 2026/10/02
JO  - Journal of High Energy Physics
DO  - 10.1007/jhep10(2026)024
UR  - https://link.springer.com/10.1007/JHEP10(2026)024
AB  - A bstract : We study the Stodolsky effect utilizing the most general form of neutrino interactions with electrons below the electroweak scale by considering all possible Lorentz invariant operators respecting SU(3) ⨂ U(1) symmetry. We perform our calculation for both Dirac and Majorana neutrinos and find that in the most general setting, only the non-standard neutrino interactions and the tensor interaction terms provide a non-zero contribution, apart from the Standard Model contribution. We investigate the implications for the possible detection of the cosmic neutrino background (C ν B) by analysing the energy shifts that are characteristic of the Stodolsky effect. We also discuss the implication of considerable asymmetry in the C ν B on the present scenario.
SN  - 1029-8479
ER  -