Pregled bibliografske jedinice broj: 73417
Nonstandard neutrino properties and the high-energy cosmic neutrino flux
Nonstandard neutrino properties and the high-energy cosmic neutrino flux // Physical Review D, 64 (2001), 067302-037306 (međunarodna recenzija, članak, znanstveni)
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Naslov
Nonstandard neutrino properties and the high-energy cosmic neutrino flux
Autori
Horvat, Raul
Izvornik
Physical Review D (0556-2821) 64
(2001);
067302-037306
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
galactic nuclei; gamma-ray sources (astronomical); cosmic ray neutrinos; solar cosmic ray particles; solar interior; high-energy cosmic ray interactions; galactic cosmic rays; neutrino mass; neutrino oscillations; mass differences
Sažetak
Recently, it has been shown that cosmic neutrino flux at the gamma ray burster/active galactic nuclei source, F_nu[sub e]^0:F_nu[sub mu]^0:F_nu[sub tau]^0~=1:2:0, inevitably oscillates (in the three neutrino framework) to 1:1:1, irrespective of the mixing angle relevant to the solar data. It has also been pointed out that the intrinsic flux of the cosmic high-energy neutrinos may not have the standard ratio, in which case the cosmic neutrino flux in the far distance should be dependent on the mixing angle. For neutrinos with nonzero electromagnetic properties, we show in the latter case that matter effects on oscillations of high-energy cosmic neutrinos can substantially modify the vacuum oscillation probability, if the mass-squared difference is <~10^10 eV^2.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- SCI-EXP, SSCI i/ili A&HCI