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NESTOR Project

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Aggouras, G.; Anassontzis, E.; Ball, A.; Bourlis, G.; Chinowsky, W.; Fahrun, E.; Grammatikakis, G.; Green, C.; Grieder, P.; Katrivanos, P.; Katrivanos, P.; Koske, P.; Leisos, A.; Markopoulos, E.; Minkowsky, P.; Nygren, D.; Papageorgiou, K.; Przybylski, G.; Resvanis, L. K.; Siotis, I.; Sopher, J.;
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Aggouras, G.; Anassontzis, E.G.; Ball, A.E.; Bourlis, G.; Chinowsky, W.; Fahrun, E.; Grammatikakis, G.; Green, C.; Grieder, P.; Katrivanos, P.; Koske, P.; Leisos, A.; Ludvig, J.; Markopoulos, E.; Minkowsky, P.; Nygren, D.; Papageorgiou, K.; Przybylski, G.; Resvanis, L.K.; Siotis, I.; Sopher, J.;
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was selected for the installation of the telescope for several reasons. It combines deep water with close proximity to the shore, a convenient combination for the installation of the NESTOR towers and the communication and power supply cables. It is also located in an anti-diametric point with
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Because neutrinos are very weakly interacting, neutrino detectors must be very large to detect a significant number of neutrinos. After completion, NESTOR will consist of a large number of glass balls (the "eyes") containing
1168: 38:(Neutrino Extended Submarine Telescope with Oceanographic Research Project) is an international scientific collaboration whose target is the deployment of a neutrino telescope on the sea floor off 1097: 1194: 810: 619: 339: 95:. Since they do not interact with matter via the electromagnetic or gravitational forces, it is extremely difficult to detect them. Since their mass is very small (less than 14 1163: 304:
Staveris-Polikalas, A.; Tsagli, V.; Tsirigotis, A.; Zhukov, V. A. (2005). "A measurement of the cosmic-ray muon flux with a module of the NESTOR neutrino telescope".
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Original surveys of the seafloor were conducted in 1989, 1991, 1992 and scientific conferences of the NESTOR Collaboration were held in the 1990s.
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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Tzamarias, S.E. (2005). "Operation and performance of the NESTOR test detector: A measurement of the atmospheric muon flux".
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frames. Many frames compose a NESTOR tower. The whole construction is placed at the bottom of the sea to reduce noise from
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Staveris, T.; Tsagli, V.; Tsirigotis, A.; Zhukov, V.A. (2005). "Operation and performance of the NESTOR test detector".
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ocean and therefore, it is possible to compare observations and study correlations between the observed neutrino.
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In March 2003, the NESTOR prototype was lowered to the depth of 3800 meters some 30 kilometers off the coast of
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are elementary particles first detected in the 1950s, long after their theoretical prediction by theorist
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In 2014 the project was still applying funding to build the actual telescope.
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This article is about the neutrino observatory. For other projects, see
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and vice versa. Neutrinos do not interact with matter via either the
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XIX International Conference on Neutrino Physics & Astrophysics
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Feder, T. (2002). "Deep-Sea Km Neutrino Detector Gets Thumbs Up".
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forces, since they are electrically neutral leptons and their
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They interact with the 448: 373: 162:The spokesperson for the project is 326:10.1016/j.astropartphys.2005.02.001 106: 24: 367: 25: 1298: 1200:Long Baseline Neutrino Experiment 419: 254:10.1016/j.nuclphysbps.2005.01.129 91:(neutrons and protons) only via 346: 332: 296: 260: 225: 207: 13: 1: 517:Lederman–Schwartz–Steinberger 200: 1256:List of neutrino experiments 134:cable for data collection. 7: 183: 45: 10: 1303: 290:10.1016/j.nima.2005.06.083 145:neutrino telescope in the 110: 49: 26: 1228: 1182: 1106: 925: 869: 844: 786: 765: 709: 678: 600: 585: 482: 93:weak nuclear interactions 79:, the strong nuclear, or 29:Nestor (disambiguation) 1277:Neutrino observatories 438:experiment record on 306:Astroparticle Physics 71:are transformed into 1287:Particle experiments 571:Neutrino oscillation 168:University of Athens 1241:Kamioka Observatory 390:2002PhT....55j..20F 318:2005APh....23..377N 282:2005NIMPA.552..420A 246:2005NuPhS.143..355T 1282:Neutrino astronomy 414:. 24 October 2002. 1264: 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983:Gargamelle 887:Baikal-GVD 742:NA61/SHINE 727:MicroBooNE 201:References 1183:Cancelled 1003:Homestake 953:Cuoricino 917:SuperNEMO 737:MiniBooNE 586:Operating 85:rest mass 57:Neutrinos 1229:See also 1174:WATCHMAN 1124:JEM-EUSO 1107:Proposed 1093:Soudan 2 1083:SciBooNE 816:MAJORANA 766:Collider 686:Daya Bay 630:Borexino 592:neutrino 184:See also 124:titanium 89:nucleons 73:neutrons 67:, where 52:Neutrino 46:Neutrino 1154:Nucifer 973:EXO-200 926:Retired 882:ARIANNA 778:SND@LHC 732:MINERνA 691:KamLAND 679:Reactor 645:IceCube 615:ANTARES 594:source) 590:primary 576:SN 1987 386:Bibcode 314:Bibcode 278:Bibcode 242:Bibcode 195:ANTARES 147:Pacific 69:protons 1251:SNOLAB 1195:LAGUNA 1139:LEGEND 1058:MINOS+ 1033:KARMEN 1008:ICARUS 978:GALLEX 933:AMANDA 912:KM3NeT 852:KATRIN 826:PandaX 701:STEREO 561:τ 556:ν 534:μ 529:ν 502:ν 436:NESTOR 178:KM3NeT 157:Greece 143:DUMAND 101:vacuum 1220:BOREX 1159:P-ONE 1129:GRAND 1114:CUPID 1073:OPERA 1053:MINOS 1048:MACRO 988:GERDA 958:DONUT 943:Chooz 857:WITCH 845:Other 836:XMASS 806:CUORE 801:COBRA 796:AMoRE 773:FASER 717:ANNIE 670:SNEWS 655:NEVOD 625:BDUNT 610:ANITA 544:DONUT 357:(PDF) 166:from 138:Pylos 1246:LNGS 1164:SBND 1144:LENA 1119:nEXO 1098:Utah 1078:RICE 1068:NEMO 1063:NARC 1043:LSND 1013:IGEX 968:ERPM 948:CNGS 938:CDHS 907:JUNO 897:DUNE 892:BEST 831:SNO+ 821:NEXT 788:0νββ 752:NuMI 747:NOvA 696:RENO 660:SAGE 640:HALO 635:BUST 34:The 1215:SOX 1169:UNO 1134:INO 1088:SNO 1038:KGF 1023:K2K 1018:IMB 993:GNO 877:ARA 757:T2K 650:LVD 620:ASD 394:doi 322:doi 286:doi 274:552 250:doi 238:143 1273:: 408:. 392:. 382:55 380:. 320:. 310:23 308:. 284:. 272:. 248:. 236:. 217:. 170:. 103:. 97:eV 42:. 567:) 546:( 540:) 519:( 513:) 507:e 492:( 468:e 461:t 454:v 400:. 396:: 388:: 359:. 328:. 324:: 316:: 292:. 288:: 280:: 256:. 252:: 244:: 31:. 20:)

Index

Nestor Project
Nestor (disambiguation)
Pylos, Greece
Neutrino
Neutrinos
Wolfgang Pauli
nuclear reactions
protons
neutrons
electromagnetic
gravitational
rest mass
nucleons
weak nuclear interactions
eV
vacuum
Neutrino detector
photomultiplier
titanium
cosmic radiation
optic fiber
Pylos
DUMAND
Pacific
Greece
Leonidas Resvanis
University of Athens
KM3NeT
Project DUMAND
ANTARES

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