High energy neutrino astronomy; past, present and future
The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size neede...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1993 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Nuclear Physics B (Proceedings Supplements) - Amsterdam : Elsevier, 31(1993), Seite 456-473 |
| Übergeordnetes Werk: |
volume:31 ; year:1993 ; pages:456-473 |
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| 520 | |a The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. | ||
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(DE-627)NLEJ181747456 (DE-599)GBVNLZ181747456 DE-627 ger DE-627 rakwb eng High energy neutrino astronomy; past, present and future 1993 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Learned, J.G. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 31(1993), Seite 456-473 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:31 year:1993 pages:456-473 http://dx.doi.org/10.1016/0920-5632(93)90168-6 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 31 1993 456-473 |
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(DE-627)NLEJ181747456 (DE-599)GBVNLZ181747456 DE-627 ger DE-627 rakwb eng High energy neutrino astronomy; past, present and future 1993 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Learned, J.G. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 31(1993), Seite 456-473 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:31 year:1993 pages:456-473 http://dx.doi.org/10.1016/0920-5632(93)90168-6 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 31 1993 456-473 |
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(DE-627)NLEJ181747456 (DE-599)GBVNLZ181747456 DE-627 ger DE-627 rakwb eng High energy neutrino astronomy; past, present and future 1993 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Learned, J.G. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 31(1993), Seite 456-473 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:31 year:1993 pages:456-473 http://dx.doi.org/10.1016/0920-5632(93)90168-6 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 31 1993 456-473 |
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(DE-627)NLEJ181747456 (DE-599)GBVNLZ181747456 DE-627 ger DE-627 rakwb eng High energy neutrino astronomy; past, present and future 1993 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Learned, J.G. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 31(1993), Seite 456-473 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:31 year:1993 pages:456-473 http://dx.doi.org/10.1016/0920-5632(93)90168-6 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 31 1993 456-473 |
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(DE-627)NLEJ181747456 (DE-599)GBVNLZ181747456 DE-627 ger DE-627 rakwb eng High energy neutrino astronomy; past, present and future 1993 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Learned, J.G. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 31(1993), Seite 456-473 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:31 year:1993 pages:456-473 http://dx.doi.org/10.1016/0920-5632(93)90168-6 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 31 1993 456-473 |
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High energy neutrino astronomy; past, present and future |
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The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. |
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The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. |
| abstract_unstemmed |
The nascent field of high energy neutrino astronomy seems to be near to blossoming in the next few years, after decades of speculation and preliminary experimental work. The motivation for the endeavor, anticipated types of sources, consideration of energy regime for first attempts, scale size needed, and techniques are qualitatively reviewed. A summary of relevant current projects is presented with emphasis on the new initiatives with detectors of the 10,000m^2 class. It seems that by the end of the decade there may be a few such new generation instruments in operation, and that with luck the business of high energy neutrino astrophysics will be underway by the turn of the century. |
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