High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the expectation that astrophysical accelerators of cosmic ray protons would also generate neutrinos through interactions with ambient matter and/or photons. However there will be a reduction in the predicted...
Egile Nagusiak: | Anchordoqui, L, Hooper, D, Sarkar, S, Taylor, A |
---|---|
Formatua: | Journal article |
Hizkuntza: | English |
Argitaratua: |
2007
|
Antzeko izenburuak
-
Neutrino diagnostics of ultra-high energy cosmic ray protons
nork: Ahlers, M, et al.
Argitaratua: (2009) -
The intergalactic propagation of ultra-high energy cosmic ray nuclei
nork: Hooper, D, et al.
Argitaratua: (2006) -
Astrophysical neutrinos and cosmic rays observed by IceCube
nork: Aartsen, MG, et al.
Argitaratua: (2017) -
Astrophysical neutrinos and cosmic rays observed by IceCube
nork: Aartsen, MG, et al.
Argitaratua: (2017) -
Astrophysical origin of high-energy cosmic neutrinos
nork: Murase Kohta
Argitaratua: (2015-01-01)