Astrophysical neutrino oscillations after pulsar timing array analyses

被引：7
作者：
Lambiase, Gaetano [1 ,2 ]
Mastrototaro, Leonardo [1 ,2 ]
Visinelli, Luca [3 ,4 ]
机构：
[1] Univ Salerno, Dipartimento Fis ER Caianiello, Via Giovanni Paolo II 132, I-84084 Fisciano, SA, Italy
[2] Ist Nazl Fis Nucl, Grp Collegato Salerno, Sez Napoli, Via Giovanni Paolo II 132, I-84084 Fisciano, SA, Italy
[3] Tsung Dao Lee Inst TDLI, 520 Shengrong Rd, Shanghai 201210, Peoples R China
[4] Shanghai Jiao Tong Univ, Sch Phys & Astron, 800 Dongchuan Rd, Shanghai 200240, Peoples R China
来源：
PHYSICAL REVIEW D | 2023年 / 108卷 / 12期
关键词：
BLACK-HOLE BINARIES; DATA SET SEARCH; GRAVITATIONAL-WAVES; FLAVOR OSCILLATIONS; 1ST; RADIATION; SPECTRUM; LIMITS;
D O I：
10.1103/PhysRevD.108.123028
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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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页数：8
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