Spin precession and neutrino helicity flip in various spacetimes
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866908295268139008 |
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| author | Saadati, Reza Hammad, Fayçal Novoa-Cattivelli, Santiago Simard, Mathieu Fleury, Nicolas |
| author_facet | Saadati, Reza Hammad, Fayçal Novoa-Cattivelli, Santiago Simard, Mathieu Fleury, Nicolas |
| contents | We systematically study spin precession of neutral particles freely moving in spacetime. We first derive the formula describing spin precession within a general stationary and axisymmetric spacetime. We then apply our formula to study spin precession of neutral spinning particles moving within various spacetimes that are among the most ubiquitous ones found in the literature. Our results are then used to extract the helicity flip probability for neutrinos propagating in each one of those selected spacetimes. It is found that low-energy neutrinos acquire a spin-flip probability that is as large as unity in all the spacetimes considered here. The remarkable result, however, is that while spin-flip probability for high-energy neutrinos remains insignificant in most of these spacetimes, some of them do allow spin-flip probability to reach unity even for high-energy neutrinos. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2502_15593 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Spin precession and neutrino helicity flip in various spacetimes Saadati, Reza Hammad, Fayçal Novoa-Cattivelli, Santiago Simard, Mathieu Fleury, Nicolas High Energy Physics - Phenomenology General Relativity and Quantum Cosmology We systematically study spin precession of neutral particles freely moving in spacetime. We first derive the formula describing spin precession within a general stationary and axisymmetric spacetime. We then apply our formula to study spin precession of neutral spinning particles moving within various spacetimes that are among the most ubiquitous ones found in the literature. Our results are then used to extract the helicity flip probability for neutrinos propagating in each one of those selected spacetimes. It is found that low-energy neutrinos acquire a spin-flip probability that is as large as unity in all the spacetimes considered here. The remarkable result, however, is that while spin-flip probability for high-energy neutrinos remains insignificant in most of these spacetimes, some of them do allow spin-flip probability to reach unity even for high-energy neutrinos. |
| title | Spin precession and neutrino helicity flip in various spacetimes |
| topic | High Energy Physics - Phenomenology General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2502.15593 |