Neutrino oscillations in astrophysical environment accounting for neutrino charge radius and anapole moment
Vadim Shakhov, Alexander Studenikin

TL;DR
This paper derives an effective Hamiltonian for neutrino oscillations in astrophysical environments, incorporating effects of neutrino charge radius and anapole moment, with potential astrophysical applications.
Contribution
It introduces a novel Hamiltonian that accounts for neutrino charge radius and anapole moment effects in spin oscillations, expanding the theoretical framework for neutrino behavior in astrophysics.
Findings
Derived an effective Hamiltonian including charge radius and anapole effects
Provided expressions for neutrino spin oscillation probabilities
Discussed potential astrophysical implications
Abstract
We derive an effective neutrino evolution Hamiltonian and corresponding expression for neutrino spin oscillations probabilities accounting for neutrino interactions with external electric current due to neutrino charge radii and anapole moment. The results are interesting for possible applications in astrophysics.
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Taxonomy
TopicsNeutrino Physics Research · Particle accelerators and beam dynamics · Dark Matter and Cosmic Phenomena
