829:
microseconds; the distance between the vertices of the two signals should be less than 100 cm; and no other signals (except for the delayed signal) are found 200 microseconds before or 600 microseconds after the prompt signal. Detection of the prompt signal has reached nearly 100% efficiency, however it is not as easy to detect the delayed signal due to issues such as Gd-concentration and neutron scattering models.
17:
106:
The inner veto surrounded the buffer vessel with a 50 cm thick layer of scintillating mineral oil. In addition, it had 78 8-inch PMTs distributed on the top, bottom and sides. This inner veto layer served as an active veto layer for muons and fast neutrons. The surrounding 15 cm thick steel
67:
Double Chooz used two identical gadolinium-doped liquid scintillator detectors placed in vicinity of two 4.25 GW thermal power reactors to measure antineutrino disappearance. The two detectors were referred to as "near", 400 meters from the reactor; and "far", 1,050 meters from the reactor. The far
828:
Since there are backgrounds to consider, candidates for (IBD) are determined by the following: visible energy from the prompt signal must be between 0.5 and 20 MeV; the delayed signal must have an energy between 4 and 10 MeV; the time difference between those two signals must be between 0.5 and 150
860:
oscillation hypothesis was excluded at 2.9 sigma by combining the Double Chooz experiment disappearance data and the T2K experiment appearance data, that had been released only some months before. This result became both the most important evidence at the time and the first accurate measurement of
84:
and had a diameter of 230 cm, a height of 245.8 cm, and a thickness of 0.8 cm. This chamber was filled with 10,000 liters of gadolinium (Gd) loaded (1 gram/liter) liquid scintillator; it was the neutrino target. The next layer out was the γ-catcher. It surrounded the neutrino target
93:
The buffer vessel was made of stainless steel 304L with dimensions of 552.2 cm wide by 568.0 cm tall and 0.3 cm thick. The remainder of the interior space that wasn't occupied by the acrylic double vessel was filled with a non-scintillating mineral oil. On the inner surface of the
58:
experiment; one of its detectors occupies the same site as its predecessor. Until
January 2015 all data had been collected using only the far detector. The near detector was completed in September 2014, after construction delays, and started taking data at the beginning of 2015. Both detectors
85:
with a 55 cm thick layer of Gd-free liquid scintillator. The casing for the γ-catcher was 12 cm thick and made of the same material as the neutrino catcher. The materials were chosen so that both of these vessels are transparent to photons with a wavelength greater than 400 nm.
658:
1223:
annihilation and distorts the scintillation signal. A tagging algorithm was developed that could be used in neutrino detectors for improved background rejection, which was similarly done by
Borexino for cosmogenic C background. An ortho-positronium lifetime of
1117:
993:
138:
are electrically neutral, extremely light particles that only interact weakly, meaning they can travel vast distances without ever being noticed. One of the properties of neutrinos is that as the propagate they have a chance to
53:
reactors as a neutrino source and measured the flux of neutrinos from them. To accomplish this, Double Chooz had a set of two detectors situated 400 meters and 1050 meters from the reactors. Double Chooz was a successor to the
98:. The purpose of the buffer layer was to shield from radioactivity in the PMTs and the surrounding rock. These two layers in addition to the neutrino target and γ-catcher were collectively referred to as the "inner detector."
484:
876:) so far. A similar analysis combination technique as done by the Double Chooz experiment in 2012 has been employed by the T2K experiment to yield the first constraints on the non-zero CP-violation phase in 2020.
2710:
1205:
107:
casing further served to shield against external γ-rays. The outer veto covered the top of the detector tank. It consisted of strips with a 5 cm x 1 cm cross section laid in orthogonal directions.
389:
823:
295:
119:
electronics with a sampling rate of 500 MHz. The trigger threshold for the detectors was set to 350 keV, much lower than the 1.02 MeV expected of the electron anti-neutrinos.
744:
468:
428:
2232:
1010:
886:
325:
234:
200:
173:
2563:
2326:
2206:
1588:
Y, Abe; et al. (Double Chooz collaboration) (28 March 2012). "Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment".
708:
68:
detector was placed inside a hill such that there was a 300 meters of water equivalent of shielding from cosmic muons. The detector itself was a calorimetric liquid
2533:
2407:
2175:
681:
1982:
2211:
2448:
2553:
2483:
2422:
2140:
175:) to another, and this is the principle under which the experiment operates. The goal of Double Chooz is to more tightly constrain the value for the
2644:
653:{\displaystyle P=1-\sin ^{2}(2\theta _{13})\,\sin ^{2}\left({\frac {1.27\Delta m_{31}^{2}L}{E_{\nu }}}\right)\quad \mathrm {(in\;natural\;units).} }
1889:
Abe, Y.; et al. (Double Chooz
Collaboration) (December 2012). "First test of Lorentz violation with a reactor-based antineutrino experiment".
2797:
2558:
2005:
1563:
2583:
2432:
2412:
2201:
122:
For several years Double Chooz had operated with only the far detector and had used models such as Bugey4 to calculate the expected flux.
872:
significance. The central values of both Double Chooz and Daya Bay experiments were in excellent agreement and has remained so (within ≤2
2761:
2684:
2125:
1134:
2720:
2639:
1379:
300:
which was the best experimental upper limit for over a decade. The goal of the Double Chooz experiment is to continue to explore the
2715:
2674:
1649:
Abe, Y.; et al. (Double Chooz
Collaboration) (18 September 2012). "Reactor ν¯e disappearance in the Double Chooz experiment".
746:
particle. From this the value of the mixing angle can be measured from the oscillation amplitude in reactor neutrino oscillations.
2649:
2578:
2293:
2032:
1975:
1247:
1245:
Apollonio, M.; et al. (2003). "Search for neutrino oscillations on a long base-line at the CHOOZ nuclear power station".
880:
Neutron capture on hydrogen was used to produce independent data, which was analysed to yield a separate measurement in 2013:
2593:
2303:
2185:
1834:
1506:
1318:
1124:
333:
1122:
An improved measurement with reduced background and systematic uncertainties after 467.90 days of data was published in the
2792:
2659:
2613:
2771:
2603:
2513:
2463:
2160:
1991:
2135:
2751:
2155:
2150:
1968:
842:
In
November 2011, first results of the experiment, using 228 days of data, were presented at the LowNu conference in
764:
245:
1316:
Huber, P.; et al. (2006). "From Double Chooz to Triple Chooz — Neutrino
Physics at the Chooz Reactor Complex".
2634:
2488:
2679:
81:
50:
2503:
1500:
Abe, Y.; et al. (Double Chooz
Collaboration) (2014). "Improved measurements of the neutrino mixing angle θ
853:, followed by an article submitted to arXiv in December 2011. In the PRL article (published in 2012), the zero
2689:
2654:
2165:
2336:
1112:{\displaystyle \sin ^{2}(2\theta _{13})=0.102\pm 0.028\,\mathrm {(stat)} \pm 0.033\,\mathrm {(syst)} .}
988:{\displaystyle \sin ^{2}(2\theta _{13})=0.097\pm 0.034\,\mathrm {(stat)} \pm 0.034\,\mathrm {(syst)} .}
713:
437:
397:
2518:
2392:
2086:
1910:
1853:
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1732:
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1607:
1558:
1525:
1412:
1337:
1266:
475:
236:
140:
28:
2756:
2543:
2523:
2130:
1960:
303:
212:
178:
146:
2669:
2458:
2397:
2117:
1934:
1900:
1843:
1810:
1784:
1766:
Abe, Y.; et al. (Double Chooz
Collaboration) (2014). "Background-independent measurement of
1748:
1722:
1686:
1660:
1631:
1597:
1567:
1541:
1515:
1463:
1428:
1402:
1353:
1327:
1302:
1282:
1256:
755:
206:
55:
2237:
2216:
2009:
1891:
1775:
1713:
1651:
1623:
1000:
686:
46:
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2588:
2417:
2372:
2316:
2288:
2180:
1926:
1918:
1871:
1861:
1802:
1740:
1678:
1615:
1533:
1420:
1345:
1274:
2311:
2528:
2453:
2257:
431:
95:
32:
1455:
Ardellier, F.; et al. (2006). "Double Chooz: A Search for the
Neutrino Mixing Angle
1294:
Ardellier, F.; et al. (2006). "Double Chooz: A Search for the
Neutrino Mixing Angle
1914:
1857:
1798:
1736:
1674:
1611:
1529:
1416:
1349:
1341:
1270:
998:
Using reactor-off data, a background-independent measurement was published July 2014 in
478:. In the two-flavor model the survival probability of any given neutrino is modelled by
2725:
2705:
2538:
2272:
666:
2786:
2036:
474:
is much smaller than the other, the Double Chooz experiment only needs to consider a
1814:
1752:
1690:
1635:
1545:
1432:
1357:
1286:
868:. Shortly after, the Daya Bay experiment provided its confirming measurement with ≥5
2063:
1938:
1806:
1744:
1619:
1393:
Mikaelyan, L; Sinev, V (2000). "Neutrino Oscillations at Reactors: What Is Next?".
69:
1278:
1955:
1866:
1829:
1704:
Abe, Y.; et al. (Double Chooz Collaboration) (2012). "First Measurement of
1537:
1216:
36:
1922:
1682:
2498:
2402:
2247:
2242:
2252:
135:
116:
1627:
1711:
from Delayed Neutron Capture on Hydrogen in the Double Chooz Experiment".
115:
Signals from the inner detector and the inner veto were recorded by 8-bit
2735:
2730:
2608:
2598:
2331:
2145:
2091:
1220:
471:
1930:
1875:
16:
2573:
1468:
1407:
1332:
1307:
1261:
1380:"Inauguration of second neutrino detector for Double Chooz experiment"
2766:
2548:
2508:
2493:
2427:
2367:
2341:
1424:
2346:
394:
Observations of the mixing angle are accomplished by observing the
2629:
2568:
2473:
2468:
2351:
2321:
2170:
2059:
1905:
1848:
1828:
Abe, Y.; et al. (Double Chooz Collaboration) (October 2014).
1789:
1727:
1665:
1602:
1520:
843:
1559:
Herve de Kerret, "First results from the Double Chooz experiment"
1200:{\displaystyle \sin ^{2}(2\theta _{13})=0.090_{-0.029}^{+0.032}.}
2267:
2262:
470:
flux from the reactors is about 50 per day. Because one of the
1964:
1830:"Ortho-positronium observation in the Double Chooz experiment"
45:, a neutrino oscillation parameter responsible for changing
1561:, Talk at the LowNu conference, Seoul, November 2011, via:
35:, France. Its goal was to measure or set a limit on the
683:
is the length in meters the neutrino has travelled and
384:{\displaystyle 0.03<\sin ^{2}(2\theta _{13})<0.2}
1235:
Limits on Lorentz violation parameters were also set.
1232:
was measured, compatible with other dedicated setups.
1137:
1013:
889:
767:
716:
689:
669:
487:
440:
400:
336:
306:
248:
215:
181:
149:
754:
The neutrinos from the reactor are observed via the
2744:
2698:
2622:
2441:
2385:
2360:
2302:
2281:
2225:
2194:
2116:
2101:
1998:
72:consisting of four concentric cylindrical vessels.
1199:
1111:
987:
817:
738:
702:
675:
652:
462:
422:
383:
319:
289:
228:
194:
167:
430:flux that comes off of the reactors during their
1992:Neutrino detectors, experiments, and facilities
818:{\displaystyle {\bar {\nu }}_{e}+p\to e^{+}+n.}
290:{\displaystyle \sin ^{2}(2\theta _{13})<0.2}
49:into other neutrinos. The experiment used the
1976:
8:
59:stopped taking data in late December 2017.
2752:BNO (Baksan or Baxan Neutrino Observatory)
2113:
1983:
1969:
1961:
1219:formation in their detector, which delays
627:
605:
1904:
1865:
1847:
1788:
1726:
1664:
1601:
1519:
1467:
1406:
1331:
1306:
1260:
1185:
1177:
1161:
1142:
1136:
1086:
1085:
1059:
1058:
1037:
1018:
1012:
962:
961:
935:
934:
913:
894:
888:
800:
781:
770:
769:
766:
730:
719:
718:
715:
694:
688:
668:
595:
582:
568:
563:
550:
537:
532:
523:
504:
486:
454:
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439:
414:
403:
402:
399:
366:
347:
335:
311:
305:
272:
253:
247:
220:
214:
209:, performed in the 1990s, found that the
186:
180:
148:
1495:
1493:
1491:
1489:
1487:
1485:
1483:
1481:
1479:
1450:
1448:
1446:
1444:
1442:
327:angle by probing an even smaller region
15:
1371:
7:
1215:Double Chooz was able to identify
1099:
1096:
1093:
1090:
1072:
1069:
1066:
1063:
975:
972:
969:
966:
948:
945:
942:
939:
640:
637:
634:
631:
628:
624:
621:
618:
615:
612:
609:
606:
602:
599:
556:
14:
2716:Long Baseline Neutrino Experiment
1564:"First Results from Double Chooz"
1504:with the Double Chooz detector".
846:, hinting at a non-zero value of
739:{\displaystyle {\bar {\nu }}_{e}}
472:neutrino mass-squared differences
463:{\displaystyle {\bar {\nu }}_{e}}
423:{\displaystyle {\bar {\nu }}_{e}}
80:The innermost vessel was made of
1248:The European Physical Journal C
594:
94:buffer vessel were 390 10-inch
1835:Journal of High Energy Physics
1807:10.1016/j.physletb.2014.04.045
1745:10.1016/j.physletb.2013.04.050
1620:10.1103/PhysRevLett.108.131801
1507:Journal of High Energy Physics
1319:Journal of High Energy Physics
1167:
1151:
1125:Journal of High Energy Physics
1102:
1087:
1075:
1060:
1043:
1027:
978:
963:
951:
936:
919:
903:
793:
775:
724:
643:
596:
529:
513:
448:
408:
372:
356:
278:
262:
1:
2033:Lederman–Schwartz–Steinberger
1350:10.1088/1126-6708/2006/05/072
76:Neutrino target and γ-catcher
2798:Reactor neutrino experiments
2772:List of neutrino experiments
320:{\displaystyle \theta _{13}}
229:{\displaystyle \theta _{13}}
195:{\displaystyle \theta _{13}}
168:{\displaystyle e,\mu ,\tau }
2814:
1923:10.1103/PhysRevD.86.112009
1683:10.1103/PhysRevD.86.052008
1279:10.1140/epjc/s2002-01127-9
51:Chooz Nuclear Power Plant
1395:Physics of Atomic Nuclei
703:{\displaystyle E_{\nu }}
1867:10.1007/JHEP10(2014)032
1590:Physical Review Letters
1538:10.1007/JHEP10(2014)086
126:Experimental techniques
1201:
1113:
989:
819:
740:
704:
677:
654:
476:two-flavor oscillation
464:
424:
385:
321:
291:
230:
196:
169:
89:Buffer vessel and PMTs
21:
1202:
1114:
990:
820:
741:
710:is the energy of the
705:
678:
655:
465:
425:
386:
322:
292:
231:
197:
170:
102:Inner and outer vetos
96:photomultiplier tubes
27:was a short-baseline
20:The Double Chooz logo
19:
2793:Neutrino experiments
2087:Neutrino oscillation
1382:. 25 September 2014.
1135:
1011:
887:
765:
714:
687:
667:
485:
438:
398:
334:
304:
246:
213:
179:
147:
29:neutrino oscillation
2757:Kamioka Observatory
1915:2012PhRvD..86k2009A
1858:2014JHEP...10..032A
1799:2014PhLB..735...51A
1737:2013PhLB..723...66A
1675:2012PhRvD..86e2008A
1612:2012PhRvL.108m1801A
1530:2014JHEP...10..086A
1417:2000PAN....63.1002M
1342:2006JHEP...05..072H
1271:2003EPJC...27..331A
1193:
573:
1773:in Double Chooz".
1197:
1173:
1109:
985:
815:
756:inverse beta decay
736:
700:
673:
650:
559:
460:
420:
381:
317:
287:
239:is constrained by
226:
192:
165:
47:electron neutrinos
22:
2780:
2779:
2514:Heidelberg-Moscow
2381:
2380:
2238:ICARUS (Fermilab)
1892:Physical Review D
1776:Physics Letters B
1714:Physics Letters B
1652:Physical Review D
1001:Physics Letters B
861:the amplitude of
778:
727:
676:{\displaystyle L}
588:
451:
432:fission reactions
411:
143:from one flavor (
2805:
2665:Neutrino Factory
2418:Hyper-Kamiokande
2181:Super-Kamiokande
2114:
2081:
2080:
2079:
2071:
2070:
2054:
2053:
2052:
2044:
2043:
2027:
2026:
2025:
2017:
2016:
1985:
1978:
1971:
1962:
1956:Project Homepage
1943:
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1757:
1756:
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1701:
1695:
1694:
1668:
1646:
1640:
1639:
1605:
1585:
1579:
1578:
1576:
1575:
1566:. Archived from
1556:
1550:
1549:
1523:
1497:
1474:
1473:
1471:
1452:
1437:
1436:
1425:10.1134/1.855739
1410:
1390:
1384:
1383:
1376:
1361:
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1310:
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1231:
1229:
1206:
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1203:
1198:
1192:
1184:
1166:
1165:
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1118:
1116:
1115:
1110:
1105:
1078:
1042:
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1023:
1022:
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991:
986:
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918:
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899:
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824:
822:
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771:
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659:
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429:
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207:Chooz experiment
201:
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2190:
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2064:
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2046:
2042:
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2038:
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2024:
2021:
2020:
2019:
2015:
2013:
2012:
2011:
2010:
1994:
1989:
1952:
1947:
1946:
1888:
1887:
1883:
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1826:
1822:
1772:
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1710:
1703:
1702:
1698:
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1440:
1392:
1391:
1387:
1378:
1377:
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1315:
1300:
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1241:
1227:
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1213:
1157:
1138:
1133:
1132:
1033:
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1009:
1008:
909:
890:
885:
884:
879:
867:
859:
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840:
835:
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768:
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762:
752:
717:
712:
711:
690:
685:
684:
665:
664:
578:
552:
546:
533:
519:
500:
483:
482:
441:
436:
435:
434:. The expected
401:
396:
395:
362:
343:
332:
331:
307:
302:
301:
268:
249:
244:
243:
216:
211:
210:
182:
177:
176:
145:
144:
133:
131:Neutrino mixing
128:
113:
111:Data collection
104:
91:
82:acrylic plastic
78:
65:
63:Detector design
42:
12:
11:
5:
2811:
2809:
2801:
2800:
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2785:
2784:
2778:
2777:
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2774:
2769:
2764:
2759:
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2748:
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2742:
2741:
2739:
2738:
2733:
2728:
2726:NESTOR Project
2723:
2718:
2713:
2708:
2706:DUMAND Project
2702:
2700:
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2695:
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2692:
2687:
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2677:
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2611:
2606:
2601:
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2586:
2581:
2576:
2571:
2566:
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2111:
2099:
2098:
2096:
2095:
2094:neutrino burst
2089:
2084:
2076:
2068:
2057:
2049:
2041:
2030:
2022:
2014:
2002:
2000:
1996:
1995:
1990:
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1965:
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1950:External links
1948:
1945:
1944:
1899:(11): 112009.
1881:
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1721:(1–3): 66–70.
1708:
1696:
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1596:(19): 131801.
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1469:hep-ex/0606025
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1408:hep-ex/9908047
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1333:hep-ph/0601266
1313:
1308:hep-ex/0606025
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1262:hep-ex/0301017
1255:(3): 331–374.
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31:experiment in
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2100:
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2028:
2007:
2004:
2003:
2001:
1997:
1993:
1986:
1981:
1979:
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1972:
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1966:
1963:
1957:
1954:
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1676:
1672:
1667:
1662:
1659:(5): 052008.
1658:
1654:
1653:
1645:
1642:
1637:
1633:
1629:
1625:
1621:
1617:
1613:
1609:
1604:
1599:
1595:
1591:
1584:
1581:
1570:on 2011-11-12
1569:
1565:
1560:
1555:
1552:
1547:
1543:
1539:
1535:
1531:
1527:
1522:
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1404:
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1396:
1389:
1386:
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1339:
1334:
1329:
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1321:
1320:
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1297:
1292:
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1263:
1258:
1254:
1250:
1249:
1243:
1242:
1238:
1236:
1233:
1222:
1218:
1211:Other results
1210:
1194:
1189:
1186:
1181:
1178:
1174:
1170:
1162:
1158:
1154:
1148:
1143:
1139:
1131:
1130:
1129:
1127:
1126:
1106:
1082:
1079:
1055:
1052:
1049:
1046:
1038:
1034:
1030:
1024:
1019:
1015:
1007:
1006:
1005:
1003:
1002:
982:
958:
955:
931:
928:
925:
922:
914:
910:
906:
900:
895:
891:
883:
882:
881:
877:
875:
871:
864:
856:
849:
845:
837:
832:
830:
812:
809:
806:
801:
797:
790:
787:
782:
772:
761:
760:
759:
757:
749:
747:
731:
721:
695:
691:
670:
646:
590:
583:
579:
574:
569:
564:
560:
553:
547:
543:
538:
534:
524:
520:
516:
510:
505:
501:
497:
494:
491:
488:
481:
480:
479:
477:
473:
455:
445:
433:
415:
405:
378:
375:
367:
363:
359:
353:
348:
344:
340:
337:
330:
329:
328:
312:
308:
284:
281:
273:
269:
265:
259:
254:
250:
242:
241:
240:
238:
221:
217:
208:
203:
187:
183:
162:
159:
156:
153:
150:
142:
137:
130:
125:
123:
120:
118:
110:
108:
101:
99:
97:
88:
86:
83:
75:
73:
71:
62:
60:
57:
52:
48:
44:
39:
34:
30:
26:
18:
2721:NEMO Project
2479:Double Chooz
2478:
2386:Construction
2118:Astronomical
2006:Cowan–Reines
1931:1721.1/76809
1896:
1890:
1884:
1876:1721.1/92880
1839:
1833:
1823:
1780:
1774:
1767:
1761:
1718:
1712:
1705:
1699:
1656:
1650:
1644:
1593:
1589:
1583:
1572:. Retrieved
1568:the original
1554:
1511:
1505:
1456:
1398:
1394:
1388:
1374:
1323:
1317:
1295:
1252:
1246:
1239:Bibliography
1234:
1230:0.15 ns
1214:
1123:
1121:
999:
997:
878:
873:
869:
862:
854:
847:
841:
838:Mixing angle
827:
753:
750:Observations
662:
393:
299:
237:mixing angle
204:
134:
121:
114:
105:
92:
79:
70:scintillator
66:
43:mixing angle
37:
25:Double Chooz
24:
23:
2327:KamLAND-Zen
2226:Accelerator
2104:(divided by
1999:Discoveries
1401:(6): 1002.
1326:(72): 072.
1217:positronium
2787:Categories
2544:Kamiokande
2499:Gargamelle
2403:Baikal-GVD
2258:NA61/SHINE
2243:MicroBooNE
1842:(10): 32.
1574:2011-11-10
1514:(10): 86.
1366:References
2699:Cancelled
2519:Homestake
2469:Cuoricino
2433:SuperNEMO
2253:MiniBooNE
2102:Operating
1906:1209.5810
1849:1407.6913
1790:1401.5981
1783:: 51–56.
1728:1301.2948
1666:1207.6632
1603:1112.6353
1521:1406.7763
1179:−
1159:θ
1149:
1128:in 2014:
1080:±
1053:±
1035:θ
1025:
956:±
929:±
911:θ
901:
794:→
776:¯
773:ν
725:¯
722:ν
696:ν
584:ν
557:Δ
544:
521:θ
511:
498:−
449:¯
446:ν
409:¯
406:ν
364:θ
354:
309:θ
270:θ
260:
218:θ
184:θ
163:τ
157:μ
141:oscillate
136:Neutrinos
117:flash ADC
2745:See also
2690:WATCHMAN
2640:JEM-EUSO
2623:Proposed
2609:Soudan 2
2599:SciBooNE
2332:MAJORANA
2282:Collider
2202:Daya Bay
2146:Borexino
2108:neutrino
1815:27219821
1753:59462260
1691:30891902
1636:19008791
1628:22540693
1546:53849018
1433:15221390
1358:13576581
1287:14226312
1221:positron
2670:Nucifer
2489:EXO-200
2442:Retired
2398:ARIANNA
2294:SND@LHC
2248:MINERνA
2207:KamLAND
2195:Reactor
2161:IceCube
2131:ANTARES
2110:source)
2106:primary
2092:SN 1987
1939:3282231
1911:Bibcode
1854:Bibcode
1795:Bibcode
1733:Bibcode
1671:Bibcode
1608:Bibcode
1526:Bibcode
1413:Bibcode
1338:Bibcode
1267:Bibcode
833:Results
2767:SNOLAB
2711:LAGUNA
2655:LEGEND
2574:MINOS+
2549:KARMEN
2524:ICARUS
2494:GALLEX
2449:AMANDA
2428:KM3NeT
2368:KATRIN
2342:PandaX
2217:STEREO
2077:τ
2072:ν
2050:μ
2045:ν
2018:ν
1937:
1813:
1751:
1689:
1634:
1626:
1544:
1457:θ
1431:
1356:
1296:θ
1285:
2736:BOREX
2675:P-ONE
2645:GRAND
2630:CUPID
2589:OPERA
2569:MINOS
2564:MACRO
2504:GERDA
2474:DONUT
2459:Chooz
2373:WITCH
2361:Other
2352:XMASS
2322:CUORE
2317:COBRA
2312:AMoRE
2289:FASER
2233:ANNIE
2186:SNEWS
2171:NEVOD
2141:BDUNT
2126:ANITA
2060:DONUT
1935:S2CID
1901:arXiv
1844:arXiv
1811:S2CID
1785:arXiv
1749:S2CID
1723:arXiv
1687:S2CID
1661:arXiv
1632:S2CID
1598:arXiv
1542:S2CID
1516:arXiv
1464:arXiv
1429:S2CID
1403:arXiv
1354:S2CID
1328:arXiv
1303:arXiv
1283:S2CID
1257:arXiv
1190:0.032
1182:0.029
1175:0.090
1083:0.033
1056:0.028
1050:0.102
959:0.034
932:0.034
926:0.097
844:Seoul
663:Here
56:Chooz
33:Chooz
2762:LNGS
2680:SBND
2660:LENA
2635:nEXO
2614:Utah
2594:RICE
2584:NEMO
2579:NARC
2559:LSND
2529:IGEX
2484:ERPM
2464:CNGS
2454:CDHS
2423:JUNO
2413:DUNE
2408:BEST
2347:SNO+
2337:NEXT
2304:0νββ
2268:NuMI
2263:NOvA
2212:RENO
2176:SAGE
2156:HALO
2151:BUST
1840:2014
1624:PMID
1512:2014
1324:0605
1226:3.68
554:1.27
376:<
341:<
338:0.03
282:<
205:The
2731:SOX
2685:UNO
2650:INO
2604:SNO
2554:KGF
2539:K2K
2534:IMB
2509:GNO
2393:ARA
2273:T2K
2166:LVD
2136:ASD
1927:hdl
1919:doi
1872:hdl
1862:doi
1803:doi
1781:735
1741:doi
1719:723
1679:doi
1616:doi
1594:108
1534:doi
1462:".
1421:doi
1346:doi
1301:".
1275:doi
1140:sin
1016:sin
892:sin
535:sin
502:sin
379:0.2
345:sin
285:0.2
251:sin
2789::
1933:.
1925:.
1917:.
1909:.
1897:86
1895:.
1870:.
1860:.
1852:.
1838:.
1832:.
1809:.
1801:.
1793:.
1779:.
1771:13
1747:.
1739:.
1731:.
1717:.
1709:13
1685:.
1677:.
1669:.
1657:86
1655:.
1630:.
1622:.
1614:.
1606:.
1592:.
1540:.
1532:.
1524:.
1510:.
1502:13
1478:^
1460:13
1441:^
1427:.
1419:.
1411:.
1399:63
1397:.
1352:.
1344:.
1336:.
1322:.
1299:13
1281:.
1273:.
1265:.
1253:27
1251:.
1163:13
1039:13
1004::
915:13
866:13
858:13
851:13
565:31
525:13
368:13
313:13
274:13
222:13
188:13
41:13
2083:)
2062:(
2056:)
2035:(
2029:)
2023:e
2008:(
1984:e
1977:t
1970:v
1941:.
1929::
1921::
1913::
1903::
1878:.
1874::
1864::
1856::
1846::
1817:.
1805::
1797::
1787::
1768:θ
1755:.
1743::
1735::
1725::
1706:θ
1693:.
1681::
1673::
1663::
1638:.
1618::
1610::
1600::
1577:.
1548:.
1536::
1528::
1518::
1472:.
1466::
1435:.
1423::
1415::
1405::
1360:.
1348::
1340::
1330::
1311:.
1305::
1289:.
1277::
1269::
1259::
1228:±
1195:.
1187:+
1171:=
1168:)
1155:2
1152:(
1144:2
1107:.
1103:)
1100:t
1097:s
1094:y
1091:s
1088:(
1076:)
1073:t
1070:a
1067:t
1064:s
1061:(
1047:=
1044:)
1031:2
1028:(
1020:2
983:.
979:)
976:t
973:s
970:y
967:s
964:(
952:)
949:t
946:a
943:t
940:s
937:(
923:=
920:)
907:2
904:(
896:2
874:σ
870:σ
863:θ
855:θ
848:θ
813:.
810:n
807:+
802:+
798:e
791:p
788:+
783:e
732:e
692:E
671:L
647:.
644:)
641:s
638:t
635:i
632:n
629:u
625:l
622:a
619:r
616:u
613:t
610:a
607:n
603:n
600:i
597:(
591:)
580:E
575:L
570:2
561:m
548:(
539:2
530:)
517:2
514:(
506:2
495:1
492:=
489:P
456:e
416:e
373:)
360:2
357:(
349:2
279:)
266:2
263:(
255:2
160:,
154:,
151:e
38:θ
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