Acceleration and radiation: classical and quantum electromagnetic and gravitational
Spontaneous Baryogenesis from effective U(1) symmetries in beyond standard model e...
Full text | |
Author(s): |
Ahluwalia, Dharam Vir
;
Labun, Lance
;
Torrieri, Giorgio
Total Authors: 3
|
Document type: | Journal article |
Source: | EUROPEAN PHYSICAL JOURNAL A; v. 52, n. 7 JUL 19 2016. |
Web of Science Citations: | 6 |
Abstract | |
We discuss the inverse beta-decay of accelerated protons in the context of neutrino flavor superpositions (mixings) in mass eigenstates. The process p -> nl(+) v(l) is kinematically allowed because the accelerating field provides the rest energy difference between initial and final states. The rate of p -> n conversions can be evaluated in either the laboratory frame (where the proton is accelerating) or the co-moving frame (where the proton is at rest and interacts with an effective thermal bath of l and v(l) due to the Unruh effect). By explicit calculation, we show that the rates in the two frames disagree when taking into account neutrino mixings, because the weak interaction couples to charge eigenstates whereas gravity couples to neutrino mass eigenstates (D.V. Ahluwalia et al., arXiv:1505.04082 {[} hep-ph]). The contradiction could be resolved experimentally, potentially yielding new information on the origins of neutrino masses. (AU) | |
FAPESP's process: | 14/13120-7 - Scaling of azimuthal correlations in hadronic collisions across system sizes, energies and rapidities: theory and phenomenology |
Grantee: | Donato Giorgio Torrieri |
Support Opportunities: | Regular Research Grants |