๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Astrophysical sources of high-energy neutrinos

โœ Scribed by Karl Mannheim

Book ID
108227797
Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
155 KB
Volume
143
Category
Article
ISSN
0920-5632

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Astrophysical sources of high energy neu
Astrophysical sources of high energy neutrinos
โœ E. Waxman ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 998 KB

Several high energy, > 100 GeV, neutrino telescopes are currently operating or under construction. Their main motivation is the extension of the horizon of neutrino astronomy to cosmological scales. We show that general, model independent, arguments imply that N 1 Gton detectors are required to det

High energy neutrino astrophysics
High energy neutrino astrophysics
โœ Teresa Montaruli ๐Ÿ“‚ Article ๐Ÿ“… 2005 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 216 KB

Astroparticle physics is a field rich in perspectives in investigating the ultra high energy region which will never be accessible to man-made machines. Many efforts are underway in order to detect the first cosmic neutrinos, messengers of the unobserved universe. The motivations of this field of re

High energy neutrino astrophysics
High energy neutrino astrophysics
โœ R.J. Protheroe ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 685 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