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would have combined the signals from many optical and acoustic sensors, allowing scientists to determine the direction from which the neutrino arrived, and to rule out
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144:, but the project cancelled in 1995 due to technical difficulties. Although it was never completed, DUMAND was in a sense a precursor of the
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74:, five kilometers beneath the surface. It would have included thousands of strings of instruments occupying a cubic kilometer of the
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164:). The DUMAND hardware was also donated to NESTOR, to reduce costs and cut on development and construction time.
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Diagram illustrating the strings of sensors and detail of one of the sensors
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183:; Spencer R. Klein (2008). "Astronomy and astrophysics with neutrinos".
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between neutrinos and protons, DUMAND would have been most sensitive to
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148:(AMANDA), and the water Cherenkov neutrino telescopes in the
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89:The proposal called for two types of detectors:
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240:Neutrino Telescopes Launch New Era of Astronomy
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113:generated by the interactions. Sophisticated
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1056:BNO (Baksan or Baxan Neutrino Observatory)
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146:Antarctic Muon And Neutrino Detector Array
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101:in water, resulting from collisions by
27:Proposed underwater neutrino telescope
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221:"DUMAND at the University of Hawaii"
125:or acoustic sources. Because of the
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1020:Long Baseline Neutrino Experiment
237:Tanya Lewis (January 20, 2014),
133:, and completely insensitive to
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337:Lederman–Schwartz–Steinberger
140:Work began in about 1976, at
1076:List of neutrino experiments
62:) was a proposed underwater
131:ultra-high energy neutrinos
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127:nature of the interaction
70:, off the shore of the
1102:Neutrino observatories
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259:experiment record on
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1107:Particle experiments
391:Neutrino oscillation
1061:Kamioka Observatory
199:2008PhT....61e..29H
121:arising from other
95:Cherenkov radiation
66:to be built in the
109:to listen for the
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64:neutrino telescope
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818:Heidelberg-Moscow
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542:ICARUS (Fermilab)
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115:signal processing
91:optical detectors
16:(Redirected from
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969:Neutrino Factory
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150:Mediterranean
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142:Keahole Point
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119:false signals
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783:Double Chooz
690:Construction
422:Astronomical
310:Cowan–Reines
255:
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193:(5): 29–35.
190:
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93:to find the
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59:
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51:
47:
43:
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35:
31:
29:
631:KamLAND-Zen
530:Accelerator
408:(divided by
303:Discoveries
261:INSPIRE-HEP
107:hydrophones
1091:Categories
848:Kamiokande
803:Gargamelle
707:Baikal-GVD
562:NA61/SHINE
547:MicroBooNE
168:References
42:nderwater
1003:Cancelled
823:Homestake
773:Cuoricino
737:SuperNEMO
557:MiniBooNE
406:Operating
245:Space.com
123:particles
103:neutrinos
1049:See also
994:WATCHMAN
944:JEM-EUSO
927:Proposed
913:Soudan 2
903:SciBooNE
636:MAJORANA
586:Collider
506:Daya Bay
450:Borexino
412:neutrino
160:and the
58:etector
54:eutrino
974:Nucifer
793:EXO-200
746:Retired
702:ARIANNA
598:SND@LHC
552:MINERνA
511:KamLAND
499:Reactor
465:IceCube
435:ANTARES
414:source)
410:primary
396:SN 1987
195:Bibcode
154:ANTARES
60:Project
1071:SNOLAB
1015:LAGUNA
959:LEGEND
878:MINOS+
853:KARMEN
828:ICARUS
798:GALLEX
753:AMANDA
732:KM3NeT
672:KATRIN
646:PandaX
521:STEREO
381:τ
376:ν
354:μ
349:ν
322:ν
257:DUMAND
105:, and
1040:BOREX
979:P-ONE
949:GRAND
934:CUPID
893:OPERA
873:MINOS
868:MACRO
808:GERDA
778:DONUT
763:Chooz
677:WITCH
665:Other
656:XMASS
626:CUORE
621:COBRA
616:AMoRE
593:FASER
537:ANNIE
490:SNEWS
475:NEVOD
445:BDUNT
430:ANITA
364:DONUT
76:ocean
1066:LNGS
984:SBND
964:LENA
939:nEXO
918:Utah
898:RICE
888:NEMO
883:NARC
863:LSND
833:IGEX
788:ERPM
768:CNGS
758:CDHS
727:JUNO
717:DUNE
712:BEST
651:SNO+
641:NEXT
608:0νββ
572:NuMI
567:NOvA
516:RENO
480:SAGE
460:HALO
455:BUST
158:NEMO
46:uon
38:eep
30:The
1035:SOX
989:UNO
954:INO
908:SNO
858:KGF
843:K2K
838:IMB
813:GNO
697:ARA
577:T2K
470:LVD
440:ASD
203:doi
50:nd
1093::
243:,
201:.
191:61
189:.
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137:.
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366:(
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339:(
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327:e
312:(
288:e
281:t
274:v
223:.
209:.
205::
197::
152:(
56:D
52:N
48:A
44:M
40:U
36:D
34:(
20:)
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