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Observation of an antimatter hypernucleus.

Authors :
Abelev BI
Aggarwal MM
Ahammed Z
Alakhverdyants AV
Alekseev I
Anderson BD
Arkhipkin D
Averichev GS
Balewski J
Barnby LS
Baumgart S
Beavis DR
Bellwied R
Betancourt MJ
Betts RR
Bhasin A
Bhati AK
Bichsel H
Bielcik J
Bielcikova J
Biritz B
Bland LC
Bonner BE
Bouchet J
Braidot E
Brandin AV
Bridgeman A
Bruna E
Bueltmann S
Bunzarov I
Burton TP
Cai XZ
Caines H
Calderon M
Catu O
Cebra D
Cendejas R
Cervantes MC
Chajecki Z
Chaloupka P
Chattopadhyay S
Chen HF
Chen JH
Chen JY
Cheng J
Cherney M
Chikanian A
Choi KE
Christie W
Chung P
Clarke RF
Codrington MJ
Corliss R
Cramer JG
Crawford HJ
Das D
Dash S
Davila Leyva A
De Silva LC
Debbe RR
Dedovich TG
DePhillips M
Derevschikov AA
Derradi de Souza R
Didenko L
Djawotho P
Dogra SM
Dong X
Drachenberg JL
Draper JE
Dunlop JC
Dutta Mazumdar MR
Efimov LG
Elhalhuli E
Elnimr M
Engelage J
Eppley G
Erazmus B
Estienne M
Eun L
Evdokimov O
Fachini P
Fatemi R
Fedorisin J
Fersch RG
Filip P
Finch E
Fine V
Fisyak Y
Gagliardi CA
Gangadharan DR
Ganti MS
Garcia-Solis EJ
Geromitsos A
Geurts F
Ghazikhanian V
Ghosh P
Gorbunov YN
Gordon A
Grebenyuk O
Grosnick D
Grube B
Guertin SM
Gupta A
Gupta N
Guryn W
Haag B
Hamed A
Han LX
Harris JW
Hays-Wehle JP
Heinz M
Heppelmann S
Hirsch A
Hjort E
Hoffman AM
Hoffmann GW
Hofman DJ
Hollis RS
Huang B
Huang HZ
Humanic TJ
Huo L
Igo G
Iordanova A
Jacobs P
Jacobs WW
Jakl P
Jena C
Jin F
Jones CL
Jones PG
Joseph J
Judd EG
Kabana S
Kajimoto K
Kang K
Kapitan J
Kauder K
Keane D
Kechechyan A
Kettler D
Kikola DP
Kiryluk J
Kisiel A
Klein SR
Knospe AG
Kocoloski A
Koetke DD
Kollegger T
Konzer J
Kopytine M
Koralt I
Koroleva L
Korsch W
Kotchenda L
Kouchpil V
Kravtsov P
Krueger K
Krus M
Kumar L
Kurnadi P
Lamont MA
Landgraf JM
LaPointe S
Lauret J
Lebedev A
Lednicky R
Lee CH
Lee JH
Leight W
Levine MJ
Li C
Li L
Li N
Li W
Li X
Li Y
Li Z
Lin G
Lindenbaum SJ
Lisa MA
Liu F
Liu H
Liu J
Ljubicic T
Llope WJ
Longacre RS
Love WA
Lu Y
Luo X
Ma GL
Ma YG
Mahapatra DP
Majka R
Mal OI
Mangotra LK
Manweiler R
Margetis S
Markert C
Masui H
Matis HS
Matulenko YA
McDonald D
McShane TS
Meschanin A
Milner R
Minaev NG
Mioduszewski S
Mischke A
Mitrovski MK
Mohanty B
Mondal MM
Morozov B
Morozov DA
Munhoz MG
Nandi BK
Nattrass C
Nayak TK
Nelson JM
Netrakanti PK
Ng MJ
Nogach LV
Nurushev SB
Odyniec G
Ogawa A
Okada H
Okorokov V
Olson D
Pachr M
Page BS
Pal SK
Pandit Y
Panebratsev Y
Pawlak T
Peitzmann T
Perevoztchikov V
Perkins C
Peryt W
Phatak SC
Pile P
Planinic M
Ploskon MA
Pluta J
Plyku D
Poljak N
Poskanzer AM
Potukuchi BV
Powell CB
Prindle D
Pruneau C
Pruthi NK
Pujahari PR
Putschke J
Qiu H
Raniwala R
Raniwala S
Ray RL
Redwine R
Reed R
Ritter HG
Roberts JB
Rogachevskiy OV
Romero JL
Rose A
Roy C
Ruan L
Sahoo R
Sakai S
Sakrejda I
Sakuma T
Salur S
Sandweiss J
Sangaline E
Schambach J
Scharenberg RP
Schmitz N
Schuster TR
Seele J
Seger J
Selyuzhenkov I
Seyboth P
Shahaliev E
Shao M
Sharma M
Shi SS
Sichtermann EP
Simon F
Singaraju RN
Skoby MJ
Smirnov N
Sorensen P
Sowinski J
Spinka HM
Srivastava B
Stanislaus TD
Staszak D
Stevens JR
Stock R
Strikhanov M
Stringfellow B
Suaide AA
Suarez MC
Subba NL
Sumbera M
Sun XM
Sun Y
Sun Z
Surrow B
Svirida DN
Symons TJ
Szanto de Toledo A
Takahashi J
Tang AH
Tang Z
Tarini LH
Tarnowsky T
Thein D
Thomas JH
Tian J
Timmins AR
Timoshenko S
Tlusty D
Tokarev M
Trainor TA
Tram VN
Trentalange S
Tribble RE
Tsai OD
Ulery J
Ullrich T
Underwood DG
Van Buren G
van Leeuwen M
van Nieuwenhuizen G
Vanfossen JA Jr
Varma R
Vasconcelos GM
Vasiliev AN
Videbaek F
Viyogi YP
Vokal S
Voloshin SA
Wada M
Walker M
Wang F
Wang G
Wang H
Wang JS
Wang Q
Wang XL
Wang Y
Webb G
Webb JC
Westfall GD
Whitten C Jr
Wieman H
Wingfield E
Wissink SW
Witt R
Wu Y
Xie W
Xu H
Xu N
Xu QH
Xu W
Xu Y
Xu Z
Xue L
Yang Y
Yepes P
Yip K
Yoo IK
Yue Q
Zawisza M
Zbroszczyk H
Zhan W
Zhang J
Zhang S
Zhang WM
Zhang XP
Zhang Y
Zhang ZP
Zhao J
Zhong C
Zhou J
Zhou W
Zhu X
Zhu YH
Zoulkarneev R
Zoulkarneeva Y
Source :
Science (New York, N.Y.) [Science] 2010 Apr 02; Vol. 328 (5974), pp. 58-62. Date of Electronic Publication: 2010 Mar 04.
Publication Year :
2010

Abstract

Nuclear collisions recreate conditions in the universe microseconds after the Big Bang. Only a very small fraction of the emitted fragments are light nuclei, but these states are of fundamental interest. We report the observation of antihypertritons--comprising an antiproton, an antineutron, and an antilambda hyperon--produced by colliding gold nuclei at high energy. Our analysis yields 70 +/- 17 antihypertritons ((Lambda)(3)-H) and 157 +/- 30 hypertritons (Lambda3H). The measured yields of Lambda3H ((Lambda)(3)-H) and 3He (3He) are similar, suggesting an equilibrium in coordinate and momentum space populations of up, down, and strange quarks and antiquarks, unlike the pattern observed at lower collision energies. The production and properties of antinuclei, and of nuclei containing strange quarks, have implications spanning nuclear and particle physics, astrophysics, and cosmology.

Details

Language :
English
ISSN :
1095-9203
Volume :
328
Issue :
5974
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
20203011
Full Text :
https://doi.org/10.1126/science.1183980