High energy neutrino Astronomy

Soebur Razzaque

doi:10.1016/j.nuclphysbps.2011.10.039

High energy neutrino Astronomy

Soebur Razzaque

Pennsylvania State University

Research output: Contribution to journal › Article › peer-review

Abstract

Astrophysical candidate sources of ultra-high energy cosmic rays inevitably produce high-energy neutrinos in and/or around them. While cosmic rays are scattered in the inter-galactic magnetic fields, neutrinos point back to their origin. Hence neutrinos can be used to probe astrophysical sources just like in usual photon astronomy. Here we present the expected neutrino signals from different astrophysical objects and discuss their possible applications to study these intriguing sources.

Original language	English
Pages (from-to)	389
Number of pages	1
Journal	Nuclear Physics B - Proceedings Supplements
Volume	221
DOIs	https://doi.org/10.1016/j.nuclphysbps.2011.10.039
Publication status	Published - Dec 2011
Externally published	Yes

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

Access to Document

10.1016/j.nuclphysbps.2011.10.039

Cite this

@article{81a47da237d04b419e1f4757bf1e4e2d,

title = "High energy neutrino Astronomy",

abstract = "Astrophysical candidate sources of ultra-high energy cosmic rays inevitably produce high-energy neutrinos in and/or around them. While cosmic rays are scattered in the inter-galactic magnetic fields, neutrinos point back to their origin. Hence neutrinos can be used to probe astrophysical sources just like in usual photon astronomy. Here we present the expected neutrino signals from different astrophysical objects and discuss their possible applications to study these intriguing sources.",

author = "Soebur Razzaque",

year = "2011",

month = dec,

doi = "10.1016/j.nuclphysbps.2011.10.039",

language = "English",

volume = "221",

pages = "389",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier",

}

TY - JOUR

T1 - High energy neutrino Astronomy

AU - Razzaque, Soebur

PY - 2011/12

Y1 - 2011/12

N2 - Astrophysical candidate sources of ultra-high energy cosmic rays inevitably produce high-energy neutrinos in and/or around them. While cosmic rays are scattered in the inter-galactic magnetic fields, neutrinos point back to their origin. Hence neutrinos can be used to probe astrophysical sources just like in usual photon astronomy. Here we present the expected neutrino signals from different astrophysical objects and discuss their possible applications to study these intriguing sources.

AB - Astrophysical candidate sources of ultra-high energy cosmic rays inevitably produce high-energy neutrinos in and/or around them. While cosmic rays are scattered in the inter-galactic magnetic fields, neutrinos point back to their origin. Hence neutrinos can be used to probe astrophysical sources just like in usual photon astronomy. Here we present the expected neutrino signals from different astrophysical objects and discuss their possible applications to study these intriguing sources.

UR - http://www.scopus.com/inward/record.url?scp=84859716871&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2011.10.039

DO - 10.1016/j.nuclphysbps.2011.10.039

M3 - Article

AN - SCOPUS:84859716871

SN - 0920-5632

VL - 221

SP - 389

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

ER -

High energy neutrino Astronomy

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this