Searching for the Origin of Neutrinos Coming from the Galactic Plane
Diffuse intergalactic magnetic fields and constraints for observations by CTA and ...
Prospects for using future detectors to study diffuse neutrinos from relic supernova
Full text | |
Author(s): |
Esmaili, Arman
;
Peres, O. L. G.
;
Serpico, Pasquale Dario
Total Authors: 3
|
Document type: | Journal article |
Source: | Physical Review D; v. 90, n. 3, p. 20-pg., 2014-08-20. |
Abstract | |
We study the impact of the existence of an eV-mass scale sterile neutrino-with parameters in the ballpark of what is required to fit the laboratory anomalies-on the early time profile of the electron neutrino and antineutrino fluxes associated to a core-collapse supernova (SN). In particular, we focus on the universal feature of neutronization burst expected in the first tens of ms of the signal: Provided that a detector with sufficient sensitivity is available, it is well known that in the three-neutrino framework the detection of the neutronization burst in neutrino channel would signal inverted mass hierarchy. This conclusion is dramatically altered in the presence of a sterile neutrino: We study here, both analytically and numerically, the region in parameter space where this characteristic signal disappears, mimicking normal hierarchy expectations. Conversely, the detection of a peak consistent with expectations for inverted mass hierarchy would exclude the existence of a sterile state over a much wider parameter space than what is required by laboratory anomaly fits, or is even probed by detectors coming on-line in the near future. Additionally, we show the peculiar alteration in the energy-time double differential flux, with a delayed peak appearing for kinematical reasons, which might offer a remarkable signature in the case of favorable parameters and for a high statistics detection of a Galactic SN. We also comment on additional potentially interesting effects in the electron antineutrino channel, if more than one angle in the active-sterile sector is nonvanishing. As an ancillary result that we derived in the technical resolution of the equations, in an Appendix we report the Cayley-Hamilton formalism for the evolution of a four-neutrino system in matter, generalizing existing results in the literature. (AU) | |
FAPESP's process: | 09/17924-5 - Neutrino phenomenology in neutrino telescopes |
Grantee: | Arman Esmaili Taklimi |
Support Opportunities: | Scholarships in Brazil - Post-Doctoral |
FAPESP's process: | 12/08208-7 - Astroparticle tests of beyond standard model light degrees of freedom |
Grantee: | Orlando Luis Goulart Peres |
Support Opportunities: | Research Grants - Visiting Researcher Grant - International |
FAPESP's process: | 12/16389-1 - Neutrino phenomenology |
Grantee: | Orlando Luis Goulart Peres |
Support Opportunities: | Regular Research Grants |