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...

Ամբողջական նկարագրություն

Մատենագիտական մանրամասներ
Հիմնական հեղինակներ: Anchordoqui, L, Hooper, D, Sarkar, S, Taylor, A
Ձևաչափ: Journal article
Լեզու:English
Հրապարակվել է: 2007
_version_ 1826284780992331776
author Anchordoqui, L
Hooper, D
Sarkar, S
Taylor, A
author_facet Anchordoqui, L
Hooper, D
Sarkar, S
Taylor, A
author_sort Anchordoqui, L
collection OXFORD
description 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 neutrino flux if cosmic ray sources accelerate not only protons but also significant number of heavier nuclei, as is indicated by recent air shower data. We consider plausible extragalactic sources such as active galactic nuclei, gamma-ray bursts and starburst galaxies and demand consistency with the observed cosmic ray composition and energy spectrum at Earth after allowing for propagation through intergalactic radiation fields. This allows us to calculate the expected neutrino fluxes from the sources, normalised to the observed cosmic ray spectrum. We find that the likely signals are still within reach of next generation neutrino telescopes such as IceCube.
first_indexed 2024-03-07T01:19:00Z
format Journal article
id oxford-uuid:8fb1c8a7-fadd-40fe-bb9e-2d61c346be8c
institution University of Oxford
language English
last_indexed 2024-03-07T01:19:00Z
publishDate 2007
record_format dspace
spelling oxford-uuid:8fb1c8a7-fadd-40fe-bb9e-2d61c346be8c2022-03-26T23:06:10ZHigh-energy neutrinos from astrophysical accelerators of cosmic ray nucleiJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:8fb1c8a7-fadd-40fe-bb9e-2d61c346be8cEnglishSymplectic Elements at Oxford2007Anchordoqui, LHooper, DSarkar, STaylor, AOngoing 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 neutrino flux if cosmic ray sources accelerate not only protons but also significant number of heavier nuclei, as is indicated by recent air shower data. We consider plausible extragalactic sources such as active galactic nuclei, gamma-ray bursts and starburst galaxies and demand consistency with the observed cosmic ray composition and energy spectrum at Earth after allowing for propagation through intergalactic radiation fields. This allows us to calculate the expected neutrino fluxes from the sources, normalised to the observed cosmic ray spectrum. We find that the likely signals are still within reach of next generation neutrino telescopes such as IceCube.
spellingShingle Anchordoqui, L
Hooper, D
Sarkar, S
Taylor, A
High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title_full High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title_fullStr High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title_full_unstemmed High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title_short High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei
title_sort high energy neutrinos from astrophysical accelerators of cosmic ray nuclei
work_keys_str_mv AT anchordoquil highenergyneutrinosfromastrophysicalacceleratorsofcosmicraynuclei
AT hooperd highenergyneutrinosfromastrophysicalacceleratorsofcosmicraynuclei
AT sarkars highenergyneutrinosfromastrophysicalacceleratorsofcosmicraynuclei
AT taylora highenergyneutrinosfromastrophysicalacceleratorsofcosmicraynuclei