Experimental status of high energy neutrino astronomy
Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1990 |
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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, 14(1990), 1, Seite 97-102 |
| Übergeordnetes Werk: |
volume:14 ; year:1990 ; number:1 ; pages:97-102 |
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| 520 | |a Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. | ||
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(DE-627)NLEJ181733986 (DE-599)GBVNLZ181733986 DE-627 ger DE-627 rakwb eng Experimental status of high energy neutrino astronomy 1990 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Svoboda, R. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 14(1990), 1, Seite 97-102 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:14 year:1990 number:1 pages:97-102 http://dx.doi.org/10.1016/0920-5632(90)90405-J GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1990 1 97-102 |
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(DE-627)NLEJ181733986 (DE-599)GBVNLZ181733986 DE-627 ger DE-627 rakwb eng Experimental status of high energy neutrino astronomy 1990 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Svoboda, R. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 14(1990), 1, Seite 97-102 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:14 year:1990 number:1 pages:97-102 http://dx.doi.org/10.1016/0920-5632(90)90405-J GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1990 1 97-102 |
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(DE-627)NLEJ181733986 (DE-599)GBVNLZ181733986 DE-627 ger DE-627 rakwb eng Experimental status of high energy neutrino astronomy 1990 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Svoboda, R. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 14(1990), 1, Seite 97-102 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:14 year:1990 number:1 pages:97-102 http://dx.doi.org/10.1016/0920-5632(90)90405-J GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1990 1 97-102 |
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(DE-627)NLEJ181733986 (DE-599)GBVNLZ181733986 DE-627 ger DE-627 rakwb eng Experimental status of high energy neutrino astronomy 1990 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Svoboda, R. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 14(1990), 1, Seite 97-102 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:14 year:1990 number:1 pages:97-102 http://dx.doi.org/10.1016/0920-5632(90)90405-J GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1990 1 97-102 |
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(DE-627)NLEJ181733986 (DE-599)GBVNLZ181733986 DE-627 ger DE-627 rakwb eng Experimental status of high energy neutrino astronomy 1990 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Svoboda, R. oth in Nuclear Physics B (Proceedings Supplements) Amsterdam : Elsevier 14(1990), 1, Seite 97-102 (DE-627)NLEJ181551780 (DE-600)1466572-4 0920-5632 nnns volume:14 year:1990 number:1 pages:97-102 http://dx.doi.org/10.1016/0920-5632(90)90405-J GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1990 1 97-102 |
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Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. |
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Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. |
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Current status of high energy astronomy is reviewed from an experimental point of view. Present data from the Baksan, Kamiokande, and IMB detectors constrain neutrino flux enhancement factors (λ) to be less than about 400, based on extrapolations from reported ultrahigh energy (UHE) ''D.C.'' gamma ray observations. |
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