Quantum coherence in neutrino spin-flavor oscillations

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Alok, Ashutosh Kumar, Chall, Trambak Jyoti, Chundawat, Neetu Raj Singh, Gangal, Shireen, Lambiase, Gaetano
Format: Preprint
Published: 2024
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866910833552916480
author Alok, Ashutosh Kumar
Chall, Trambak Jyoti
Chundawat, Neetu Raj Singh
Gangal, Shireen
Lambiase, Gaetano
author_facet Alok, Ashutosh Kumar
Chall, Trambak Jyoti
Chundawat, Neetu Raj Singh
Gangal, Shireen
Lambiase, Gaetano
contents Coherence, which represents the superposition of orthogonal states, is a fundamental concept in quantum mechanics and can also be precisely defined within quantum resource theory. Thus exploring quantum coherence in neutrino oscillations can not only help in examining the intrinsic quantum nature but can also explore their potential applications in quantum information technologies. Previous studies on quantum coherence have focused on neutrino flavor oscillations (FO). However, FO imply that neutrinos have mass and this can lead to the generation of a tiny but finite magnetic dipole moment of neutrinos through quantum loop diagrams at higher orders of perturbative expansion of the interaction. This electromagnetic property of neutrinos can induce spin flavor oscillations (SFO) in the presence of an external magnetic field and hence is expected to enrich the study of coherence. In this work, we investigate quantum coherence in neutrino SFO with three flavor mixing within the interstellar as well as intergalactic magnetic fields, quantified by the $l_1$ norm and the relative entropy of coherence, and express these measures in terms of neutrino SFO probabilities. For FO, coherence measures can sustain higher values (say, within 50% of the maximum) over distances of several kilometers, which are relevant for terrestrial experiments like reactor and accelerator neutrinos. However, for SFO, we find that the coherence scale can extend to astrophysical distances, spanning from kiloparsecs to gigaparsecs.
format Preprint
id arxiv_https___arxiv_org_abs_2407_16742
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Quantum coherence in neutrino spin-flavor oscillations
Alok, Ashutosh Kumar
Chall, Trambak Jyoti
Chundawat, Neetu Raj Singh
Gangal, Shireen
Lambiase, Gaetano
High Energy Physics - Phenomenology
Quantum Physics
Coherence, which represents the superposition of orthogonal states, is a fundamental concept in quantum mechanics and can also be precisely defined within quantum resource theory. Thus exploring quantum coherence in neutrino oscillations can not only help in examining the intrinsic quantum nature but can also explore their potential applications in quantum information technologies. Previous studies on quantum coherence have focused on neutrino flavor oscillations (FO). However, FO imply that neutrinos have mass and this can lead to the generation of a tiny but finite magnetic dipole moment of neutrinos through quantum loop diagrams at higher orders of perturbative expansion of the interaction. This electromagnetic property of neutrinos can induce spin flavor oscillations (SFO) in the presence of an external magnetic field and hence is expected to enrich the study of coherence. In this work, we investigate quantum coherence in neutrino SFO with three flavor mixing within the interstellar as well as intergalactic magnetic fields, quantified by the $l_1$ norm and the relative entropy of coherence, and express these measures in terms of neutrino SFO probabilities. For FO, coherence measures can sustain higher values (say, within 50% of the maximum) over distances of several kilometers, which are relevant for terrestrial experiments like reactor and accelerator neutrinos. However, for SFO, we find that the coherence scale can extend to astrophysical distances, spanning from kiloparsecs to gigaparsecs.
title Quantum coherence in neutrino spin-flavor oscillations
topic High Energy Physics - Phenomenology
Quantum Physics
url https://arxiv.org/abs/2407.16742