๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Flux predictions of high-energy neutrinos from pulsars

โœ Scribed by Bennett Link; Fiorella Burgio

Book ID
110840990
Publisher
John Wiley and Sons
Year
2006
Tongue
English
Weight
251 KB
Volume
371
Category
Article
ISSN
0035-8711

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

High energy neutrino emission from young
High energy neutrino emission from young pulsars
โœ G.F. Burgio; B. Link ๐Ÿ“‚ Article ๐Ÿ“… 2006 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 119 KB

We propose that young (t age t10 5 yr), rapidly rotating pulsars can accelerate ions to energies of $1 PeV near the surface of a neutron star. Protons undergo resonant excitation with surface X-rays and produce a beam of m neutrinos with energies of several tens of TeV which could be detectable by c

High-energy radiation from old pulsars
High-energy radiation from old pulsars
โœ ZeJun Jiang; Li Zhang ๐Ÿ“‚ Article ๐Ÿ“… 2010 ๐Ÿ› Science in China Press (SCP) ๐ŸŒ English โš– 433 KB
Neutrino properties from high energy ast
Neutrino properties from high energy astrophysical neutrinos
โœ S. Pakvasa ๐Ÿ“‚ Article ๐Ÿ“… 2004 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 520 KB

It is shown how high energy neutrino beams from very distant sources can be utilized to learn about some properties of neutrinos such as lifetimes, mass hierarchy, etc. Furthermore, even mixing elements such as U e3 and the CPV phase in the neutrino mixing matrix can be measured in principle. Pseudo