FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea
The observation of high-energy extraterrestrial neutrinos is one of the most promising future options to increase our knowledge on non-thermal processes in the universe. Neutrinos are e.g. unavoidably produced in environments where high-energy hadrons collide; in particular this almost certainly mus...
Main Author: | |
---|---|
Other Authors: | |
Format: | Text |
Language: | English |
Published: |
2008
|
Subjects: | |
Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.5641 http://arxiv.org/pdf/astro-ph/0601012v1.pdf |
id |
ftciteseerx:oai:CiteSeerX.psu:10.1.1.257.5641 |
---|---|
record_format |
openpolar |
spelling |
ftciteseerx:oai:CiteSeerX.psu:10.1.1.257.5641 2023-05-15T14:00:02+02:00 FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea Ulrich F. Katz The Pennsylvania State University CiteSeerX Archives 2008 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.5641 http://arxiv.org/pdf/astro-ph/0601012v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.5641 http://arxiv.org/pdf/astro-ph/0601012v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0601012v1.pdf text 2008 ftciteseerx 2016-01-07T20:00:50Z The observation of high-energy extraterrestrial neutrinos is one of the most promising future options to increase our knowledge on non-thermal processes in the universe. Neutrinos are e.g. unavoidably produced in environments where high-energy hadrons collide; in particular this almost certainly must be true in the astrophysical accelerators of cosmic rays, which thus could be identified unambiguously by sky observations in “neutrino light”. On the one hand, neutrinos are ideal messengers for astrophysical observations since they are not deflected by electromagnetic fields and interact so weakly that they are able to escape even from very dense production regions and traverse large distances in the universe without attenuation. On the other hand, their weak interaction poses a significant problem for detecting neutrinos. Huge target masses up to gigatons must be employed, requiring to instrument natural abundances of media such as sea water or antarctic ice. The first generation of such neutrino telescopes is taking data or will do so in the near future, while the second-generation projects with cubic-kilometre size is under construction or being prepared. This report focuses on status and prospects of current (ANTARES, NEMO, NESTOR) and future (KM3NeT) neutrino telescope projects in the Mediterranean Sea. 1 Current neutrino telescope projects in the Mediterranean Sea Text Antarc* Antarctic Unknown Antarctic Nestor ENVELOPE(-63.435,-63.435,-64.415,-64.415) |
institution |
Open Polar |
collection |
Unknown |
op_collection_id |
ftciteseerx |
language |
English |
description |
The observation of high-energy extraterrestrial neutrinos is one of the most promising future options to increase our knowledge on non-thermal processes in the universe. Neutrinos are e.g. unavoidably produced in environments where high-energy hadrons collide; in particular this almost certainly must be true in the astrophysical accelerators of cosmic rays, which thus could be identified unambiguously by sky observations in “neutrino light”. On the one hand, neutrinos are ideal messengers for astrophysical observations since they are not deflected by electromagnetic fields and interact so weakly that they are able to escape even from very dense production regions and traverse large distances in the universe without attenuation. On the other hand, their weak interaction poses a significant problem for detecting neutrinos. Huge target masses up to gigatons must be employed, requiring to instrument natural abundances of media such as sea water or antarctic ice. The first generation of such neutrino telescopes is taking data or will do so in the near future, while the second-generation projects with cubic-kilometre size is under construction or being prepared. This report focuses on status and prospects of current (ANTARES, NEMO, NESTOR) and future (KM3NeT) neutrino telescope projects in the Mediterranean Sea. 1 Current neutrino telescope projects in the Mediterranean Sea |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Ulrich F. Katz |
spellingShingle |
Ulrich F. Katz FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
author_facet |
Ulrich F. Katz |
author_sort |
Ulrich F. Katz |
title |
FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
title_short |
FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
title_full |
FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
title_fullStr |
FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
title_full_unstemmed |
FAU-PI1-05-01 Neutrino Telescopy in the Mediterranean Sea |
title_sort |
fau-pi1-05-01 neutrino telescopy in the mediterranean sea |
publishDate |
2008 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.5641 http://arxiv.org/pdf/astro-ph/0601012v1.pdf |
long_lat |
ENVELOPE(-63.435,-63.435,-64.415,-64.415) |
geographic |
Antarctic Nestor |
geographic_facet |
Antarctic Nestor |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
http://arxiv.org/pdf/astro-ph/0601012v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.5641 http://arxiv.org/pdf/astro-ph/0601012v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
_version_ |
1766269009473306624 |