https://doi.org/10.1140/epjc/s10052-024-13530-x
Regular Article
Probing chiral and flavored 
from cosmic bursts through neutrino interactions
1
Department of Physics, Hokkaido University, 060-0810, Sapporo, Japan
2
Institute for the Advancement of Higher Education, Hokkaido University, 060-0817, Sapporo, Japan
3
Dipartimento di Fisica “E.R Caianiello”, Università degli Studi di Salerno, Via Giovanni Paolo II, 132, 84084, Fisciano (SA), Italy
4
Istituto Nazionale di Fisica Nucleare, Gruppo Collegato di Salerno, Sezione di Napoli, Via Giovanni Paolo II, 132, 84084, Fisciano (SA), Italy
5
College of Physics, Sichuan University, 610065, Chengdu, China
6
Institute of Experimental and Applied Physics, Czech Technical University in Prague, Husova 240/5, 110 00, Prague 1, Czech Republic
b
adas@particle.sci.hokudai.ac.jp
Received:
1
May
2024
Accepted:
24
October
2024
Published online:
26
November
2024
The origin of tiny neutrino mass is an unsolved puzzle leading to a variety of phenomenological aspects beyond the Standard Model (BSM). We consider U(1) gauge extension of the Standard Model (SM) where so-called seesaw mechanism is incarnated with the help of thee generations of Majorana type right-handed neutrinos followed by the breaking of U(1) and electroweak gauge symmetries providing anomaly free structure. In this framework, a neutral BSM gauge boson is evolved. To explore the properties of its interactions we consider chiral (flavored) frameworks where interactions depend on the handedness (generations) of the fermions. In this paper we focus on -neutrino interactions which could be probed from cosmic explosions. We consider 
process which can energize gamma-ray burst (GRB221009A, so far the highest energy) through energy deposition. Hence estimating these rates we constrain U(1) gauge coupling 
and mass 
under Schwarzchild (Sc) and Hartle-Thorne (HT) scenarios. We also study 
-DM scattering through to constrain 
plane using IceCube data considering high energy neutrinos from cosmic blazar (TXS0506+056), active galaxy (NGC1068), the Cosmic Microwave Background (CMB) and the Lyman-
data, respectively. Finally highlighting complementarity we compare our results with current and prospective bounds on plane from scattering, beam-dump and 
experiments. [PICS code].
© The Author(s) 2024
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Funded by SCOAP3.
