๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

High energy neutrino emission from young pulsars

โœ Scribed by G.F. Burgio; B. Link


Publisher
Elsevier Science
Year
2006
Tongue
English
Weight
119 KB
Volume
567
Category
Article
ISSN
0168-9002

No coin nor oath required. For personal study only.

โœฆ Synopsis


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 current technology. Detection of these neutrinos would further our understanding of high-energy processes that take place in the stellar magnetosphere.


๐Ÿ“œ SIMILAR VOLUMES


Production of high-energy ฮผ neutrinos fr
โœ G.F. Burgio; B. Link ๐Ÿ“‚ Article ๐Ÿ“… 2007 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 343 KB

Young, rapidly rotating neutron stars could accelerate protons to energies of โˆผ 1 PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the ฮ” resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum o

Neutrino properties from high energy ast
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

High-energy neutrinos from extragalactic
โœ Karl Mannheim ๐Ÿ“‚ Article ๐Ÿ“… 1995 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 778 KB

In this paper I calculate the diffuse background of high-energy neutrinos from extragalactic jets emerging from active galactic nuclei ( AGN) \_ I assume that radio-quiet AGN have jets that are disrupted by turbulence in the vicinity of an accretion disk surrounding a central black hole and remain i