High energy neutrino astronomy

Soebur Razzaque

High energy neutrino astronomy

Pennsylvania State University

Research output: Contribution to conference › Paper › 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	470
Number of pages	1
Publication status	Published - 2006
Externally published	Yes
Event	22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006 - Santa Fe, NM, United States Duration: 13 Jun 2006 → 19 Jun 2006

Conference

Conference	22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006
Country/Territory	United States
City	Santa Fe, NM
Period	13/06/06 → 19/06/06

ASJC Scopus subject areas

Astronomy and Astrophysics

Cite this

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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 = "2006",

language = "English",

pages = "470",

note = "22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006 ; Conference date: 13-06-2006 Through 19-06-2006",

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TY - CONF

T1 - High energy neutrino astronomy

AU - Razzaque, Soebur

PY - 2006

Y1 - 2006

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.

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M3 - Paper

AN - SCOPUS:84884387315

SP - 470

T2 - 22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006

Y2 - 13 June 2006 through 19 June 2006

ER -

High energy neutrino astronomy

Abstract

Conference

ASJC Scopus subject areas

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