28:
127:. It was prototyped in 2004 and had a 47.9 kg-day commissioning run in 2007 and operated 2009 to 2011. CRESST-II Phase 1 experiment observed excess events above known background that could be understood to constitute a dark matter signal. However, later analysis showed that these excess events were due to a previously uncounted for excess of background from the detector itself and not a true signal from dark matter. The source of the excess background in the detector was removed for Phase 2.
1210:
618:
1222:
313:
Angloher, G; Bauer, M; Bavykina, I; Bento, A; Bucci, C; Ciemniak, C; Deuter, G; von
Feilitzsch, F; Hauff, D; Huff, P; Isaila, C; Jochum, J; Kiefer, M; Kimmerle, M; Lanfranchi, J. -C; Petricca, F; Pfister, S; Potzel, W; Pröbst, F; Reindl, F; Roth, S; Rottler, K; Sailer, C; Schäffner, K; Schmaler, J;
134:
crystal with better radiopurity, improved detectors, and significantly reduced background. It began July 2013 to explore excess signals in the prior run. The results of Phase 2 showed no signal above expected background, proving that the result of Phase 1 had indeed been due to excess background by
146:. CRESST-II phase 1 full results were published in 2012. New phase 2 results have been presented in July 2014 with a limit on spin-independent WIMP-nucleon scattering for WIMP masses below 3 GeV/c.
160:
detector with a lowered energy threshold of 30.1 eV, about 1/10 that of CRESST-II. This allows the detection of WIMPs as light as 0.16 GeV/c, slightly heavier than a
917:
897:
887:
149:
In 2015 the CRESST detectors were upgraded by a sensitivity factor of 100 allowing dark-matter particles with a mass around that of a proton to be detected.
1248:
812:
1070:
1075:
1050:
468:
314:
Scholl, S; Seidel, W; Sivers, M. v; Stodolsky, L; et al. (Apr 12, 2012). "Results from 730 kg days of the CRESST-II Dark Matter search".
667:
542:
72:
1025:
755:
882:
672:
907:
43:) is a collaboration of European experimental particle physics groups involved in the construction of cryogenic detectors for direct
862:
647:
48:
1055:
1045:
1030:
967:
1175:
83:
56:
1040:
1060:
977:
927:
807:
802:
787:
597:
79:
31:
The building housing the CRESST cryostat, located in Hall A of the LNGS deep underground laboratory, Gran Sasso, Italy.
27:
1015:
902:
842:
822:
745:
106:, the excellent discrimination and energy resolution of the detectors allows identification of rare particle events.
1035:
740:
535:
60:
760:
602:
725:
677:
1226:
383:
710:
607:
515:
1214:
982:
730:
652:
567:
528:
434:
333:
285:
228:
87:
64:
415:(CRESST Collab.) (31 March 2019). "First results from the CRESST-III low-mass dark matter program".
1020:
68:
735:
695:
450:
424:
349:
323:
275:
244:
218:
1180:
1065:
587:
582:
99:
972:
1139:
937:
932:
877:
867:
715:
662:
592:
572:
442:
341:
293:
236:
165:
922:
857:
17:
1195:
1080:
577:
298:
263:
438:
337:
289:
232:
1134:
720:
1242:
1190:
1170:
912:
750:
353:
345:
248:
209:
Davis, Jonathan (2015). "The Past and Future of Light Dark Matter Direct
Detection".
454:
169:
143:
121:
192:
1165:
1129:
1121:
705:
642:
551:
446:
139:
124:
103:
44:
1160:
997:
962:
847:
700:
657:
240:
172:, there was an unexplained excess of events imparting less than 200 eV.
1144:
1101:
892:
505:
175:
The experiment is planning an upgrade to accommodate 100 detector modules.
852:
411:
1185:
1085:
957:
112:
took data in 2000 using sapphire detectors with tungsten thermometers.
942:
817:
95:
91:
52:
510:
86:. The modular detectors used by CRESST facilitate discrimination of
429:
223:
156:, which ran from 2016 to 2018. CRESST-III used a single 23.6-g CaWO
1106:
992:
987:
837:
792:
637:
632:
384:"New detectors allow search for lightweight dark matter particles"
371:
328:
280:
26:
500:
952:
947:
872:
827:
797:
161:
524:
520:
368:
Results on low mass WIMPs using an upgraded CRESST-II detector
37:
102:
crystals. By cooling the detectors to temperatures of a few
469:"Searches for Dark Matter with the CRESST-III Experiment"
152:
In 2019, the team reported results of the first phase of
78:
The CRESST collaboration currently runs an array of
1153:
1119:
1094:
1006:
778:
769:
686:
625:
558:
47:searches. The participating institutes are the
536:
8:
775:
543:
529:
521:
90:events by the simultaneous measurement of
428:
327:
297:
279:
222:
262:Lang, Rafael; Seidel, Wolfgang (2009).
184:
82:in the underground laboratory of the
73:Istituto Nazionale di Fisica Nucleare
7:
1221:
264:"Search for dark matter with CRESST"
204:
202:
1249:Experiments for dark matter search
25:
1220:
1209:
1208:
616:
49:Max Planck Institute for Physics
372:https://arxiv.org/abs/1407.3146
164:. Despite many events from the
1176:Galaxy formation and evolution
516:Gran Sasso National Laboratory
346:10.1140/epjc/s10052-012-1971-8
299:10.1088/1367-2630/11/10/105017
84:Gran Sasso National Laboratory
69:Comenius University Bratislava
57:Technical University of Munich
1:
138:CRESST-II first detected the
598:Self-interacting dark matter
135:components of the detector.
756:Navarro–Frenk–White profile
746:Massive compact halo object
741:Mass dimension one fermions
447:10.1103/PhysRevD.100.102002
316:European Physical Journal C
98:signals from scintillating
18:CRESST (Dark Matter Search)
1265:
366:The CRESST Collaboration,
1204:
614:
241:10.1142/S0217751X15300380
761:Scalar field dark matter
603:Scalar field dark matter
511:CRESST Publication 2011
506:CRESST Publication 2004
501:CRESST Official Website
626:Hypothetical particles
608:Primordial black holes
268:New Journal of Physics
130:Phase 2 has a new CaWO
61:University of TĂĽbingen
32:
711:Dark globular cluster
67:(Great Britain), the
30:
731:Dwarf galaxy problem
653:Minicharged particle
568:Baryonic dark matter
211:Int. J. Mod. Phys. A
88:background radiation
65:University of Oxford
439:2019PhRvD.100j2002A
338:2012EPJC...72.1971A
290:2009NJPh...11j5017L
233:2015IJMPA..3030038D
80:cryogenic detectors
71:(Slovakia) and the
736:Halo mass function
696:Cuspy halo problem
409:A. H. Abdelhameed
33:
1236:
1235:
1181:Illustris project
1115:
1114:
588:Mixed dark matter
583:Light dark matter
417:Physical Review D
100:calcium tungstate
16:(Redirected from
1256:
1224:
1223:
1212:
1211:
776:
716:Dark matter halo
663:Sterile neutrino
620:
619:
593:Warm dark matter
573:Cold dark matter
545:
538:
531:
522:
488:
487:
485:
483:
473:
465:
459:
458:
432:
406:
400:
399:
397:
395:
390:. September 2015
380:
374:
364:
358:
357:
331:
310:
304:
303:
301:
283:
259:
253:
252:
226:
206:
197:
196:
189:
166:electron capture
144:tungsten-180 (W)
21:
1264:
1263:
1259:
1258:
1257:
1255:
1254:
1253:
1239:
1238:
1237:
1232:
1200:
1196:UniverseMachine
1149:
1111:
1090:
1008:
1002:
780:
771:
765:
688:
682:
621:
617:
612:
578:Hot dark matter
560:
554:
549:
497:
492:
491:
481:
479:
471:
467:
466:
462:
408:
407:
403:
393:
391:
382:
381:
377:
365:
361:
312:
311:
307:
261:
260:
256:
217:(15): 1530038.
208:
207:
200:
191:
190:
186:
181:
159:
133:
119:
75:(INFN, Italy).
23:
22:
15:
12:
11:
5:
1262:
1260:
1252:
1251:
1241:
1240:
1234:
1233:
1231:
1230:
1218:
1205:
1202:
1201:
1199:
1198:
1193:
1188:
1186:Imaginary mass
1183:
1178:
1173:
1168:
1163:
1157:
1155:
1151:
1150:
1148:
1147:
1142:
1137:
1135:HVC 127-41-330
1132:
1126:
1124:
1117:
1116:
1113:
1112:
1110:
1109:
1104:
1098:
1096:
1095:Other projects
1092:
1091:
1089:
1088:
1083:
1078:
1073:
1068:
1063:
1058:
1053:
1048:
1043:
1038:
1033:
1028:
1023:
1018:
1012:
1010:
1004:
1003:
1001:
1000:
995:
990:
985:
980:
975:
970:
965:
960:
955:
950:
945:
940:
935:
930:
925:
920:
915:
910:
905:
900:
895:
890:
885:
880:
875:
870:
865:
860:
855:
850:
845:
840:
835:
830:
825:
820:
815:
810:
805:
800:
795:
790:
784:
782:
773:
767:
766:
764:
763:
758:
753:
748:
743:
738:
733:
728:
723:
721:Dark radiation
718:
713:
708:
703:
698:
692:
690:
684:
683:
681:
680:
675:
670:
665:
660:
655:
650:
645:
640:
635:
629:
627:
623:
622:
615:
613:
611:
610:
605:
600:
595:
590:
585:
580:
575:
570:
564:
562:
556:
555:
550:
548:
547:
540:
533:
525:
519:
518:
513:
508:
503:
496:
495:External links
493:
490:
489:
478:. 28 July 2020
460:
423:(10): 102002.
401:
375:
359:
305:
274:(10): 105017.
254:
198:
193:"CRESST: Home"
183:
182:
180:
177:
157:
131:
117:
24:
14:
13:
10:
9:
6:
4:
3:
2:
1261:
1250:
1247:
1246:
1244:
1229:
1228:
1219:
1217:
1216:
1207:
1206:
1203:
1197:
1194:
1192:
1191:Negative mass
1189:
1187:
1184:
1182:
1179:
1177:
1174:
1172:
1171:Exotic matter
1169:
1167:
1164:
1162:
1159:
1158:
1156:
1152:
1146:
1143:
1141:
1140:Smith's Cloud
1138:
1136:
1133:
1131:
1128:
1127:
1125:
1123:
1122:dark galaxies
1118:
1108:
1105:
1103:
1100:
1099:
1097:
1093:
1087:
1084:
1082:
1079:
1077:
1074:
1072:
1069:
1067:
1064:
1062:
1059:
1057:
1054:
1052:
1049:
1047:
1044:
1042:
1039:
1037:
1034:
1032:
1029:
1027:
1024:
1022:
1019:
1017:
1014:
1013:
1011:
1005:
999:
996:
994:
991:
989:
986:
984:
981:
979:
976:
974:
971:
969:
966:
964:
961:
959:
956:
954:
951:
949:
946:
944:
941:
939:
936:
934:
931:
929:
926:
924:
921:
919:
916:
914:
911:
909:
906:
904:
901:
899:
896:
894:
891:
889:
886:
884:
881:
879:
876:
874:
871:
869:
866:
864:
861:
859:
856:
854:
851:
849:
846:
844:
841:
839:
836:
834:
831:
829:
826:
824:
821:
819:
816:
814:
811:
809:
806:
804:
801:
799:
796:
794:
791:
789:
786:
785:
783:
777:
774:
768:
762:
759:
757:
754:
752:
751:Mirror matter
749:
747:
744:
742:
739:
737:
734:
732:
729:
727:
724:
722:
719:
717:
714:
712:
709:
707:
704:
702:
699:
697:
694:
693:
691:
685:
679:
676:
674:
671:
669:
666:
664:
661:
659:
656:
654:
651:
649:
646:
644:
641:
639:
636:
634:
631:
630:
628:
624:
609:
606:
604:
601:
599:
596:
594:
591:
589:
586:
584:
581:
579:
576:
574:
571:
569:
566:
565:
563:
557:
553:
546:
541:
539:
534:
532:
527:
526:
523:
517:
514:
512:
509:
507:
504:
502:
499:
498:
494:
477:
470:
464:
461:
456:
452:
448:
444:
440:
436:
431:
426:
422:
418:
414:
413:
405:
402:
389:
385:
379:
376:
373:
369:
363:
360:
355:
351:
347:
343:
339:
335:
330:
325:
321:
317:
309:
306:
300:
295:
291:
287:
282:
277:
273:
269:
265:
258:
255:
250:
246:
242:
238:
234:
230:
225:
220:
216:
212:
205:
203:
199:
194:
188:
185:
178:
176:
173:
171:
167:
163:
155:
150:
147:
145:
141:
136:
128:
126:
123:
122:scintillating
115:
111:
107:
105:
101:
97:
93:
89:
85:
81:
76:
74:
70:
66:
62:
58:
54:
50:
46:
42:
38:
29:
19:
1225:
1213:
832:
480:. Retrieved
475:
463:
420:
416:
410:
404:
394:14 September
392:. Retrieved
387:
378:
367:
362:
319:
315:
308:
271:
267:
257:
214:
210:
187:
174:
153:
151:
148:
137:
129:
125:calorimeters
113:
109:
108:
77:
40:
36:
34:
1166:Dark energy
1130:HE0450-2958
772:experiments
706:Dark galaxy
689:and objects
643:Dark photon
561:dark matter
552:Dark matter
476:Indico.cern
322:(4): 1971.
140:alpha decay
104:millikelvin
63:(Germany),
45:dark matter
1161:Antimatter
1120:Potential
848:DAMA/LIBRA
701:Dark fluid
658:Neutralino
482:20 January
430:1904.00498
224:1506.03924
179:References
154:CRESST-III
1145:VIRGOHI21
1102:MultiDark
1009:detection
893:EDELWEISS
781:detection
726:Dark star
354:119283621
329:1109.0702
281:0906.3290
249:119269304
168:decay of
116:uses CaWO
114:CRESST-II
1243:Category
1215:Category
1007:Indirect
863:DarkSide
853:DAMA/NaI
687:Theories
559:Forms of
455:90261775
120:crystal
110:CRESST-I
1227:Commons
1154:Related
1086:VERITAS
1061:IceCube
1021:ANTARES
973:TREX-DM
958:ROSEBUD
948:PICASSO
435:Bibcode
334:Bibcode
286:Bibcode
229:Bibcode
1081:PAMELA
1016:AMS-02
998:ZEPLIN
968:SIMPLE
943:PandaX
938:NEWS-G
933:NEWAGE
898:EURECA
878:DM-Ice
868:DARWIN
833:CRESST
823:COSINE
818:CoGeNT
779:Direct
770:Search
453:
412:et al.
388:PhyOrg
352:
247:
96:photon
92:phonon
53:Munich
41:CRESST
1107:PVLAS
1066:MAGIC
1046:Fermi
1041:DAMPE
1031:CALET
993:XMASS
988:XENON
978:UKDMC
963:SABRE
928:NAIAD
923:MIMAC
918:MACRO
888:DRIFT
883:DMTPC
858:DAMIC
838:CUORE
828:COUPP
813:CLEAN
793:ANAIS
638:Axion
633:Axino
472:(PDF)
451:S2CID
425:arXiv
350:S2CID
324:arXiv
276:arXiv
245:S2CID
219:arXiv
1076:OGLE
1056:HESS
1051:HAWC
1036:CAST
1026:ATIC
983:WARP
953:PICO
903:KIMS
873:DEAP
808:CDMS
803:CDEX
798:ArDM
788:ADMX
678:WISP
673:WIMP
668:SIMP
484:2022
396:2015
162:pion
94:and
35:The
1071:MOA
908:LUX
648:LSP
443:doi
421:100
342:doi
294:doi
237:doi
142:of
55:),
1245::
913:LZ
843:D3
474:.
449:.
441:.
433:.
419:.
386:.
370:,
348:.
340:.
332:.
320:72
318:.
292:.
284:.
272:11
270:.
266:.
243:.
235:.
227:.
215:30
213:.
201:^
170:Ta
59:,
544:e
537:t
530:v
486:.
457:.
445::
437::
427::
398:.
356:.
344::
336::
326::
302:.
296::
288::
278::
251:.
239::
231::
221::
195:.
158:4
132:4
118:4
51:(
39:(
20:)
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
