Future galactic supernova neutrino signal: What can we learn?

Details Future galactic supernova neutrino signal: What can we learn? Future galactic supernova neutrino signal: What can we learn?

2001-11-07

arxiv.org/abs/nucl-th/0111016v1

Prog.Part.Nucl.Phys. 48 (2002) 29-37

Physics

Nuclear Physics

Nuclear Theory

10 pages, 5 figures, Talk at the School `Neutrinos in Astro, Particle and Nuclear Physics', Erice, September 18-26, 2001

Scientific paper

10.1016/S0146-6410(02)00108-4

The next supernova in our galaxy will be detected by a variety of neutrino detectors. In this lecture I discuss the set of observables needed to constrain the models of supernova neutrino emission. They are the flux normalizations, and average energies, of each of the three expected components of the neutrino flux: $\nu_e$, $\bar{\nu}_e$, and $\nu_x$ (all the other four flavors combined). I show how the existing, or soon to be operational, neutrino detectors will be able to determine the magnitude of these observables, and estimate the corresponding rates.

Affiliated with

Also associated with

No associations

Rating

Future galactic supernova neutrino signal: What can we learn? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Future galactic supernova neutrino signal: What can we learn?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Future galactic supernova neutrino signal: What can we learn? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-102930