Astrophysical neutrino oscillations after pulsar timing array analyses

Gaetano Lambiase, Leonardo Mastrototaro, and Luca Visinelli
Phys. Rev. D 108, 123028 – Published 18 December 2023

Abstract

The pattern of neutrino flavor oscillations could be altered by the influence of noisy perturbations such as those arising from a gravitational wave background (GWB). A stochastic process that is consistent with a GWB has been recently reported by the independent analyses of pulsar timing array (PTA) datasets collected over a decadal timescale by the North American Nanohertz Observatory for gravitational waves, the European PTA jointly with the Indian Pulsar Timing Array, the Parkes PTA, and the Chinese PTA collaborations. We investigate the modifications in the neutrino flavor oscillations under the influence of the GWB reported by the PTA collaborations and we discuss how such effects could be potentially revealed in near-future neutrino detectors, possibly helping the discrimination of different models for the GWB below the nHz frequency range.

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  • Received 7 July 2023
  • Accepted 29 November 2023

DOI:https://doi.org/10.1103/PhysRevD.108.123028

© 2023 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Gaetano Lambiase1,2,*, Leonardo Mastrototaro1,2,†, and Luca Visinelli3,4,‡

  • 1Dipartimento di Fisica “E.R. Caianiello,” Università degli Studi di Salerno, Via Giovanni Paolo II, 132-84084 Fisciano (SA), Italy
  • 2Istituto Nazionale di Fisica Nucleare—Gruppo Collegato di Salerno—Sezione di Napoli, Via Giovanni Paolo II, 132-84084 Fisciano (SA), Italy
  • 3Tsung-Dao Lee Institute (TDLI), 520 Shengrong Road, 201210 Shanghai, People’s Republic of China
  • 4School of Physics and Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Road, 200240 Shanghai, People’s Republic of China

  • *lambiase@sa.infn.it
  • lmastrototaro@unisa.it
  • luca.visinelli@sjtu.edu.cn

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Issue

Vol. 108, Iss. 12 — 15 December 2023

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