Letter of Intent for KM3NeT 2.0
The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The hi...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adrián-Martínez, S [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
High Energy Astrophysical Phenomena |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Journal of physics. G, Nuclear and particle physics - Bristol : IOP Publ., 1975, (2016) |
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| Übergeordnetes Werk: |
year:2016 |
| Links: |
|---|
| DOI / URN: |
10.1088/0954-3899/43/8/084001 |
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| Katalog-ID: |
OLC198495217X |
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| 520 | |a The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. | ||
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10.1088/0954-3899/43/8/084001 doi PQ20161201 (DE-627)OLC198495217X (DE-599)GBVOLC198495217X (PRQ)a981-1296df1268d227587ce40d43fdb88b11245e8344a563a8e7232a59a5fda08d390 (KEY)0073708920160000000000000000letterofintentforkm3net20 DE-627 ger DE-627 rakwb eng 530 DE-600 UA 4720. AVZ rvk Adrián-Martínez, S verfasserin aut Letter of Intent for KM3NeT 2.0 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. High Energy Astrophysical Phenomena Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Astrophysics Experiment Ageron, M oth Aharonian, F oth Aiello, S oth Albert, A oth Ameli, F oth Anassontzis, E oth Andre, M oth Androulakis, G oth Anghinolfi, M oth Anton, G oth Ardid, M oth Avgitas, T oth Barbarino, G oth Barbarito, E oth Baret, B oth Barrios-Martí, J oth Belhorma, B oth Belias, A oth Berbee, E oth Berg, A. van den oth Bertin, V oth Beurthey, S oth van Beveren, V oth Beverini, N oth Biagi, S oth Biagioni, A oth Billault, M oth Bond, M oth Bormuth, R oth Bouhadef, B oth Bourlis, G oth Bourret, S oth Boutonnet, C oth Bouwhuis, M oth Bozza, C oth Bruijn, R oth Brunner, J oth Buis, E oth Busto, J oth Cacopardo, G oth Caillat, L oth Calamai, M oth Calvo, D oth Capone, A oth Caramete, L oth Cecchini, S oth Celli, S oth Champion, C oth Moursli, R. Cherkaoui El oth Cherubini, S oth Chiarusi, T oth Circella, M oth Classen, L oth Cocimano, R oth Coelho, J. A. B oth Coleiro, A oth Colonges, S oth Coniglione, R oth Cordelli, M oth Cosquer, A oth Coyle, P oth Creusot, A oth Cuttone, G oth D'Amico, A oth De Bonis, G oth De Rosa, G oth De Sio, C oth Di Capua, F oth Di Palma, I oth García, A. F. Díaz oth Distefano, C oth Donzaud, C oth Dornic, D oth Dorosti-Hasankiadeh, Q oth Drakopoulou, E oth Drouhin, D oth Drury, L oth Durocher, M oth Eberl, T oth Eichie, S oth van Eijk, D oth Bojaddaini, I. El oth Khayati, N. El oth Elsaesser, D oth Enzenhöfer, A oth Fassi, F oth Favali, P oth Fermani, P oth Ferrara, G oth Frascadore, G oth Filippidis, C oth Fusco, L. A oth Gal, T oth Galatà, S oth Garufi, F oth Gay, P oth Gebyehu, M oth Giordano, V oth Gizani, N oth ... oth Enthalten in Journal of physics. G, Nuclear and particle physics Bristol : IOP Publ., 1975 (2016) (DE-627)129412058 (DE-600)188689-7 (DE-576)014791617 0305-4616 nnns year:2016 http://dx.doi.org/10.1088/0954-3899/43/8/084001 Volltext http://arxiv.org/abs/1601.07459 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_21 GBV_ILN_22 GBV_ILN_70 GBV_ILN_2279 UA 4720. AR 2016 |
| spelling |
10.1088/0954-3899/43/8/084001 doi PQ20161201 (DE-627)OLC198495217X (DE-599)GBVOLC198495217X (PRQ)a981-1296df1268d227587ce40d43fdb88b11245e8344a563a8e7232a59a5fda08d390 (KEY)0073708920160000000000000000letterofintentforkm3net20 DE-627 ger DE-627 rakwb eng 530 DE-600 UA 4720. AVZ rvk Adrián-Martínez, S verfasserin aut Letter of Intent for KM3NeT 2.0 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. High Energy Astrophysical Phenomena Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Astrophysics Experiment Ageron, M oth Aharonian, F oth Aiello, S oth Albert, A oth Ameli, F oth Anassontzis, E oth Andre, M oth Androulakis, G oth Anghinolfi, M oth Anton, G oth Ardid, M oth Avgitas, T oth Barbarino, G oth Barbarito, E oth Baret, B oth Barrios-Martí, J oth Belhorma, B oth Belias, A oth Berbee, E oth Berg, A. van den oth Bertin, V oth Beurthey, S oth van Beveren, V oth Beverini, N oth Biagi, S oth Biagioni, A oth Billault, M oth Bond, M oth Bormuth, R oth Bouhadef, B oth Bourlis, G oth Bourret, S oth Boutonnet, C oth Bouwhuis, M oth Bozza, C oth Bruijn, R oth Brunner, J oth Buis, E oth Busto, J oth Cacopardo, G oth Caillat, L oth Calamai, M oth Calvo, D oth Capone, A oth Caramete, L oth Cecchini, S oth Celli, S oth Champion, C oth Moursli, R. Cherkaoui El oth Cherubini, S oth Chiarusi, T oth Circella, M oth Classen, L oth Cocimano, R oth Coelho, J. A. B oth Coleiro, A oth Colonges, S oth Coniglione, R oth Cordelli, M oth Cosquer, A oth Coyle, P oth Creusot, A oth Cuttone, G oth D'Amico, A oth De Bonis, G oth De Rosa, G oth De Sio, C oth Di Capua, F oth Di Palma, I oth García, A. F. Díaz oth Distefano, C oth Donzaud, C oth Dornic, D oth Dorosti-Hasankiadeh, Q oth Drakopoulou, E oth Drouhin, D oth Drury, L oth Durocher, M oth Eberl, T oth Eichie, S oth van Eijk, D oth Bojaddaini, I. El oth Khayati, N. El oth Elsaesser, D oth Enzenhöfer, A oth Fassi, F oth Favali, P oth Fermani, P oth Ferrara, G oth Frascadore, G oth Filippidis, C oth Fusco, L. A oth Gal, T oth Galatà, S oth Garufi, F oth Gay, P oth Gebyehu, M oth Giordano, V oth Gizani, N oth ... oth Enthalten in Journal of physics. G, Nuclear and particle physics Bristol : IOP Publ., 1975 (2016) (DE-627)129412058 (DE-600)188689-7 (DE-576)014791617 0305-4616 nnns year:2016 http://dx.doi.org/10.1088/0954-3899/43/8/084001 Volltext http://arxiv.org/abs/1601.07459 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_21 GBV_ILN_22 GBV_ILN_70 GBV_ILN_2279 UA 4720. AR 2016 |
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10.1088/0954-3899/43/8/084001 doi PQ20161201 (DE-627)OLC198495217X (DE-599)GBVOLC198495217X (PRQ)a981-1296df1268d227587ce40d43fdb88b11245e8344a563a8e7232a59a5fda08d390 (KEY)0073708920160000000000000000letterofintentforkm3net20 DE-627 ger DE-627 rakwb eng 530 DE-600 UA 4720. AVZ rvk Adrián-Martínez, S verfasserin aut Letter of Intent for KM3NeT 2.0 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. High Energy Astrophysical Phenomena Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Astrophysics Experiment Ageron, M oth Aharonian, F oth Aiello, S oth Albert, A oth Ameli, F oth Anassontzis, E oth Andre, M oth Androulakis, G oth Anghinolfi, M oth Anton, G oth Ardid, M oth Avgitas, T oth Barbarino, G oth Barbarito, E oth Baret, B oth Barrios-Martí, J oth Belhorma, B oth Belias, A oth Berbee, E oth Berg, A. van den oth Bertin, V oth Beurthey, S oth van Beveren, V oth Beverini, N oth Biagi, S oth Biagioni, A oth Billault, M oth Bond, M oth Bormuth, R oth Bouhadef, B oth Bourlis, G oth Bourret, S oth Boutonnet, C oth Bouwhuis, M oth Bozza, C oth Bruijn, R oth Brunner, J oth Buis, E oth Busto, J oth Cacopardo, G oth Caillat, L oth Calamai, M oth Calvo, D oth Capone, A oth Caramete, L oth Cecchini, S oth Celli, S oth Champion, C oth Moursli, R. Cherkaoui El oth Cherubini, S oth Chiarusi, T oth Circella, M oth Classen, L oth Cocimano, R oth Coelho, J. A. B oth Coleiro, A oth Colonges, S oth Coniglione, R oth Cordelli, M oth Cosquer, A oth Coyle, P oth Creusot, A oth Cuttone, G oth D'Amico, A oth De Bonis, G oth De Rosa, G oth De Sio, C oth Di Capua, F oth Di Palma, I oth García, A. F. Díaz oth Distefano, C oth Donzaud, C oth Dornic, D oth Dorosti-Hasankiadeh, Q oth Drakopoulou, E oth Drouhin, D oth Drury, L oth Durocher, M oth Eberl, T oth Eichie, S oth van Eijk, D oth Bojaddaini, I. El oth Khayati, N. El oth Elsaesser, D oth Enzenhöfer, A oth Fassi, F oth Favali, P oth Fermani, P oth Ferrara, G oth Frascadore, G oth Filippidis, C oth Fusco, L. A oth Gal, T oth Galatà, S oth Garufi, F oth Gay, P oth Gebyehu, M oth Giordano, V oth Gizani, N oth ... oth Enthalten in Journal of physics. G, Nuclear and particle physics Bristol : IOP Publ., 1975 (2016) (DE-627)129412058 (DE-600)188689-7 (DE-576)014791617 0305-4616 nnns year:2016 http://dx.doi.org/10.1088/0954-3899/43/8/084001 Volltext http://arxiv.org/abs/1601.07459 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_21 GBV_ILN_22 GBV_ILN_70 GBV_ILN_2279 UA 4720. AR 2016 |
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10.1088/0954-3899/43/8/084001 doi PQ20161201 (DE-627)OLC198495217X (DE-599)GBVOLC198495217X (PRQ)a981-1296df1268d227587ce40d43fdb88b11245e8344a563a8e7232a59a5fda08d390 (KEY)0073708920160000000000000000letterofintentforkm3net20 DE-627 ger DE-627 rakwb eng 530 DE-600 UA 4720. AVZ rvk Adrián-Martínez, S verfasserin aut Letter of Intent for KM3NeT 2.0 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. High Energy Astrophysical Phenomena Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Astrophysics Experiment Ageron, M oth Aharonian, F oth Aiello, S oth Albert, A oth Ameli, F oth Anassontzis, E oth Andre, M oth Androulakis, G oth Anghinolfi, M oth Anton, G oth Ardid, M oth Avgitas, T oth Barbarino, G oth Barbarito, E oth Baret, B oth Barrios-Martí, J oth Belhorma, B oth Belias, A oth Berbee, E oth Berg, A. van den oth Bertin, V oth Beurthey, S oth van Beveren, V oth Beverini, N oth Biagi, S oth Biagioni, A oth Billault, M oth Bond, M oth Bormuth, R oth Bouhadef, B oth Bourlis, G oth Bourret, S oth Boutonnet, C oth Bouwhuis, M oth Bozza, C oth Bruijn, R oth Brunner, J oth Buis, E oth Busto, J oth Cacopardo, G oth Caillat, L oth Calamai, M oth Calvo, D oth Capone, A oth Caramete, L oth Cecchini, S oth Celli, S oth Champion, C oth Moursli, R. Cherkaoui El oth Cherubini, S oth Chiarusi, T oth Circella, M oth Classen, L oth Cocimano, R oth Coelho, J. A. B oth Coleiro, A oth Colonges, S oth Coniglione, R oth Cordelli, M oth Cosquer, A oth Coyle, P oth Creusot, A oth Cuttone, G oth D'Amico, A oth De Bonis, G oth De Rosa, G oth De Sio, C oth Di Capua, F oth Di Palma, I oth García, A. F. Díaz oth Distefano, C oth Donzaud, C oth Dornic, D oth Dorosti-Hasankiadeh, Q oth Drakopoulou, E oth Drouhin, D oth Drury, L oth Durocher, M oth Eberl, T oth Eichie, S oth van Eijk, D oth Bojaddaini, I. El oth Khayati, N. El oth Elsaesser, D oth Enzenhöfer, A oth Fassi, F oth Favali, P oth Fermani, P oth Ferrara, G oth Frascadore, G oth Filippidis, C oth Fusco, L. A oth Gal, T oth Galatà, S oth Garufi, F oth Gay, P oth Gebyehu, M oth Giordano, V oth Gizani, N oth ... oth Enthalten in Journal of physics. G, Nuclear and particle physics Bristol : IOP Publ., 1975 (2016) (DE-627)129412058 (DE-600)188689-7 (DE-576)014791617 0305-4616 nnns year:2016 http://dx.doi.org/10.1088/0954-3899/43/8/084001 Volltext http://arxiv.org/abs/1601.07459 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_21 GBV_ILN_22 GBV_ILN_70 GBV_ILN_2279 UA 4720. AR 2016 |
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10.1088/0954-3899/43/8/084001 doi PQ20161201 (DE-627)OLC198495217X (DE-599)GBVOLC198495217X (PRQ)a981-1296df1268d227587ce40d43fdb88b11245e8344a563a8e7232a59a5fda08d390 (KEY)0073708920160000000000000000letterofintentforkm3net20 DE-627 ger DE-627 rakwb eng 530 DE-600 UA 4720. AVZ rvk Adrián-Martínez, S verfasserin aut Letter of Intent for KM3NeT 2.0 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. High Energy Astrophysical Phenomena Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Astrophysics Experiment Ageron, M oth Aharonian, F oth Aiello, S oth Albert, A oth Ameli, F oth Anassontzis, E oth Andre, M oth Androulakis, G oth Anghinolfi, M oth Anton, G oth Ardid, M oth Avgitas, T oth Barbarino, G oth Barbarito, E oth Baret, B oth Barrios-Martí, J oth Belhorma, B oth Belias, A oth Berbee, E oth Berg, A. van den oth Bertin, V oth Beurthey, S oth van Beveren, V oth Beverini, N oth Biagi, S oth Biagioni, A oth Billault, M oth Bond, M oth Bormuth, R oth Bouhadef, B oth Bourlis, G oth Bourret, S oth Boutonnet, C oth Bouwhuis, M oth Bozza, C oth Bruijn, R oth Brunner, J oth Buis, E oth Busto, J oth Cacopardo, G oth Caillat, L oth Calamai, M oth Calvo, D oth Capone, A oth Caramete, L oth Cecchini, S oth Celli, S oth Champion, C oth Moursli, R. Cherkaoui El oth Cherubini, S oth Chiarusi, T oth Circella, M oth Classen, L oth Cocimano, R oth Coelho, J. A. B oth Coleiro, A oth Colonges, S oth Coniglione, R oth Cordelli, M oth Cosquer, A oth Coyle, P oth Creusot, A oth Cuttone, G oth D'Amico, A oth De Bonis, G oth De Rosa, G oth De Sio, C oth Di Capua, F oth Di Palma, I oth García, A. F. Díaz oth Distefano, C oth Donzaud, C oth Dornic, D oth Dorosti-Hasankiadeh, Q oth Drakopoulou, E oth Drouhin, D oth Drury, L oth Durocher, M oth Eberl, T oth Eichie, S oth van Eijk, D oth Bojaddaini, I. El oth Khayati, N. El oth Elsaesser, D oth Enzenhöfer, A oth Fassi, F oth Favali, P oth Fermani, P oth Ferrara, G oth Frascadore, G oth Filippidis, C oth Fusco, L. A oth Gal, T oth Galatà, S oth Garufi, F oth Gay, P oth Gebyehu, M oth Giordano, V oth Gizani, N oth ... oth Enthalten in Journal of physics. G, Nuclear and particle physics Bristol : IOP Publ., 1975 (2016) (DE-627)129412058 (DE-600)188689-7 (DE-576)014791617 0305-4616 nnns year:2016 http://dx.doi.org/10.1088/0954-3899/43/8/084001 Volltext http://arxiv.org/abs/1601.07459 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_21 GBV_ILN_22 GBV_ILN_70 GBV_ILN_2279 UA 4720. AR 2016 |
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The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. |
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The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. |
| abstract_unstemmed |
The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. |
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Letter of Intent for KM3NeT 2.0 |
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