Observation of the antimatter helium-4 nucleus


Autoria(s): AGAKISHIEV, H.; AGGARWAL, M. M.; AHAMMED, Z.; ALAKHVERDYANTS, A. V.; ALEKSEEV, I.; ALFORD, J.; ANDERSON, B. D.; ANSON, C. D.; ARKHIPKIN, D.; AVERICHEV, G. S.; BALEWSKI, J.; BEAVIS, D. R.; BEHERA, N. K.; BELLWIED, R.; BETANCOURT, M. J.; BETTS, R. R.; BHASIN, A.; BHATI, A. K.; BICHSEL, H.; BIELCIK, J.; BIELCIKOVA, J.; BIRITZ, B.; BLAND, L. C.; BORDYUZHIN, I. G.; BOROWSKI, W.; BOUCHET, J.; BRAIDOT, E.; BRANDIN, A. V.; BRIDGEMAN, A.; BROVKO, S. G.; BRUNA, E.; BUELTMANN, S.; BUNZAROV, I.; BURTON, T. P.; CAI, X. Z.; CAINES, H.; CALDERON, M.; CEBRA, D.; CENDEJAS, R.; CERVANTES, M. C.; CHAJECKI, Z.; CHALOUPKA, P.; CHATTOPADHYAY, S.; CHEN, H. F.; CHEN, J. H.; CHEN, J. Y.; CHEN, L.; CHENG, J.; CHERNEY, M.; CHIKANIAN, A.; CHOI, K. E.; CHRISTIE, W.; CHUNG, P.; CODRINGTON, M. J. M.; CORLISS, R.; CRAMER, J. G.; CRAWFORD, H. J.; LEYVA, A. Davila; SILVA, L. C. De; DEBBE, R. R.; DEDOVICH, T. G.; DEREVSCHIKOV, A. A.; SOUZA, R. Derradi de; DIDENKO, L.; DJAWOTHO, P.; DOGRA, S. M.; DONG, X.; DRACHENBERG, J. L.; DRAPER, J. E.; DUNLOP, C.; EFIMOV, L. G.; ELNIMR, M.; ENGELAGE, J.; EPPLEY, G.; ESTIENNE, M.; EUN, L.; EVDOKIMOV, O.; FATEMI, R.; FEDORISIN, J.; FERSCH, R. G.; FILIP, P.; FINCH, E.; FINE, V.; FISYAK, Y.; GAGLIARDI, C. A.; GANGADHARAN, D. R.; GEURTS, F.; GHOSH, P.; GORBUNOV, Y. N.; GORDON, A.; GREBENYUK, O. G.; GROSNICK, D.; GUERTIN, S. M.; GUPTA, A.; GUPTA, S.; GURYN, W.; HAAG, B.; HAJKOVA, O.; HAMED, A.; HAN, L-X.; HARRIS, J. W.; HAYS-WEHLE, J. P.; HEINZ, M.; HEPPELMANN, S.; HIRSCH, A.; HJORT, E.; HOFFMANN, G. W.; HOFMAN, D. J.; HUANG, B.; HUANG, H. Z.; HUMANIC, T. J.; HUO, L.; IGO, G.; JACOBS, P.; JACOBS, W.; JENA, C.; JIN, F.; JOSEPH, J.; JUDD, E. G.; KABANA, S.; KANG, K.; KAPITAN, J.; KAUDER, K.; KE, H. W.; KEANE, D.; KECHECHYAN, A.; KETTLER, D.; KIKOLA, D. P.; KIRYLUK, J.; KISIEL, A.; KIZKA, V.; KLEIN, S. R.; KNOSPE, A. G.; KOETKE, D. D.; KOLLEGGER, T.; KONZER, J.; KORALT, I.; KOROLEVA, L.; KORSCH, W.; KOTCHENDA, L.; KOUCHPIL, V.; KRAVTSOV, P.; KRUEGER, K.; KRUS, M.; KUMAR, L.; KURNADI, P.; LAMONT, M. A. C.; LANDGRAF, J. M.; LAPOINTE, S.; LAURET, J.; LEBEDEV, A.; LEDNICKY, R.; LEE, J. H.; LEIGHT, W.; LEVINE, M. J.; LI, C.; LI, L.; LI, N.; LI, W.; LI, X.; LI, X.; LI, Y.; LI, Z. M.; LISA, M. A.; LIU, F.; LIU, H.; LIU, J.; LJUBICIC, T.; LLOPE, W. J.; LONGACRE, R. S.; LOVE, W. A.; LU, Y.; LUKASHOV, E. V.; LUO, X.; MA, G. L.; MA, Y. G.; MAHAPATRA, D. P.; MAJKA, R.; MALL, O. I.; MANWEILER, R.; MARGETIS, S.; MARKERT, C.; MASUI, H.; MATIS, H. S.; MATULENKO, Yu A.; MCDONALD, D.; MCSHANE, T. S.; MESCHANIN, A.; MILNER, R.; MINAEV, N. G.; MIODUSZEWSKI, S.; MITROVSKI, M. K.; MOHAMMED, Y.; MOHANTY, B.; MONDAL, M. M.; MOROZOV, B.; MOROZOV, D. A.; Munhoz, Marcelo Gameiro; MUSTAFA, M. K.; NAGLIS, M.; NANDI, B. K.; NAYAK, T. K.; NETRAKANTI, P. K.; NOGACH, L. V.; NURUSHEV, S. B.; ODYNIEC, G.; OGAWA, A.; OH, K.; OHLSON, A.; OKOROKOV, V.; OLDAG, E. W.; OLSON, D.; PACHR, M.; PAGE, B. S.; PAL, S. K.; PANDIT, Y.; PANEBRATSEV, Y.; PAWLAK, T.; PEI, H.; PEITZMANN, T.; PERKINS, C.; PERYT, W.; PILE, P.; PLANINIC, M.; PLOSKON, M. A.; PLUTA, J.; PLYKU, D.; POLJAK, N.; PORTER, J.; POSKANZER, A. M.; POTUKUCHI, B. V. K. S.; POWELL, C. B.; PRINDLE, D.; PRUNEAU, C.; PRUTHI, N. K.; PUJAHARI, P. R.; PUTSCHKE, J.; QIU, H.; RANIWALA, R.; RANIWALA, S.; RAY, R. L.; REDWINE, R.; REED, R.; RITTER, H. G.; ROBERTS, J. B.; ROGACHEVSKIY, O. V.; ROMERO, J. L.; RUAN, L.; RUSNAK, J.; SAHOO, N. R.; SAKREJDA, I.; SALUR, S.; SANDWEISS, J.; SANGALINE, E.; SARKAR, A.; SCHAMBACH, J.; SCHARENBERG, R. P.; SCHMAH, A. M.; SCHMITZ, N.; SCHUSTER, T. R.; SEELE, J.; SEGER, J.; SELYUZHENKOV, I.; SEYBOTH, P.; SHAH, N.; SHAHALIEV, E.; SHAO, M.; SHARMA, M.; SHI, S. S.; SHOU, Q. Y.; SICHTERMANN, E. P.; SIMON, F.; SINGARAJU, R. N.; SKOBY, M. J.; SMIRNOV, N.; SOLANKI, D.; SORENSEN, P.; SPINKA, H. M.; SRIVASTAVA, B.; STANISLAUS, T. D. S.; STASZAK, D.; STEADMAN, S. G.; STEVENS, J. R.; STOCK, R.; STRIKHANOV, M.; STRINGFELLOW, B.; Suaide, Alexandre Alarcon do Passo; SUAREZ, M. C.; SUBBA, N. L.; SUMBERA, M.; SUN, X. M.; SUN, Y.; SUN, Z.; SURROW, B.; SVIRIDA, D. N.; SYMONS, T. J. M.; Szanto de Toledo, Alejandro; TAKAHASHI, J.; TANG, A. H.; TANG, Z.; TARINI, L. H.; TARNOWSKY, T.; THEIN, D.; THOMAS, J. H.; TIAN, J.; TIMMINS, A. R.; TLUSTY, D.; TOKAREV, M.; TRAINOR, T. A.; TRENTALANGE, S.; TRIBBLE, R. E.; TRIBEDY, P.; TSAI, O. D.; ULLRICH, T.; UNDERWOOD, D. G.; BUREN, G. Van; NIEUWENHUIZEN, G. van; VANFOSSEN JR., J. A.; VARMA, R.; VASCONCELOS, G. M. S.; VASILIEV, A. N.; VIDEBAEK, F.; VIYOGI, Y. P.; VOKAL, S.; VOLOSHIN, S. A.; WADA, M.; WALKER, M.; WANG, F.; WANG, G.; WANG, H.; WANG, J. S.; WANG, Q.; WANG, X. L.; WANG, Y.; WEBB, G.; WEBB, J. C.; WESTFALL, G. D.; WHITTEN JR., C.; WIEMAN, H.; WISSINK, S. W.; WITT, R.; WITZKE, W.; WU, Y. F.; XIAO, Z.; XIE, W.; XU, H.; XU, N.; XU, Q. H.; XU, W.; XU, Y.; XU, Z.; XUE, L.; YANG, Y.; YANG, Y.; YEPES, P.; YIP, K.; YOO, I-K.; ZAWISZA, M.; ZBROSZCZYK, H.; ZHAN, W.; ZHANG, J. B.; ZHANG, S.; ZHANG, W. M.; ZHANG, X. P.; ZHANG, Y.; ZHANG, Z. P.; ZHAO, F.; ZHAO, J.; ZHONG, C.; ZHOU, W.; ZHU, X.; ZHU, Y. H.; ZOULKARNEEV, R.; ZOULKARNEEVA, Y.; STAR Collaboration
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2011

Resumo

High-energy nuclear collisions create an energy density similar to that of the Universe microseconds after the Big Bang(1); in both cases, matter and antimatter are formed with comparable abundance. However, the relatively short-lived expansion in nuclear collisions allows antimatter to decouple quickly from matter, and avoid annihilation. Thus, a high-energy accelerator of heavy nuclei provides an efficient means of producing and studying antimatter. The antimatter helium-4 nucleus ((4)(He) over bar), also known as the anti-alpha ((alpha) over bar), consists of two antiprotons and two antineutrons (baryon number B = -4). It has not been observed previously, although the alpha-particle was identified a century ago by Rutherford and is present in cosmic radiation at the ten per cent level(2). Antimatter nuclei with B -1 have been observed only as rare products of interactions at particle accelerators, where the rate of antinucleus production in high-energy collisions decreases by a factor of about 1,000 with each additional antinucleon(3-5). Here we report the observation of (4)<(He) over bar, the heaviest observed antinucleus to date. In total, 18 (4)(He) over bar counts were detected at the STAR experiment at the Relativistic Heavy Ion Collider (RHIC; ref. 6) in 10(9) recorded gold-on-gold (Au+Au) collisions at centre-of-mass energies of 200 GeV and 62 GeV per nucleon-nucleon pair. The yield is consistent with expectations from thermodynamic(7) and coalescent nucleosynthesis(8) models, providing an indication of the production rate of even heavier antimatter nuclei and a benchmark for possible future observations of (4)(He) over bar in cosmic radiation.

RHIC Operations Group

RHIC Operations Group

RACF at BNL

RACF at BNL

NERSC Center at LBNL

NERSC Center at LBNL

Open Science Grid consortium

Open Science Grid consortium

U.S. Department of Energy (DOE)

Offices of NP and HEP within the US DOE Office of Science

U.S. National Science Foundation (NSF)

US NSF

Sloan Foundation

Sloan Foundation

DFG cluster of excellence `Origin and Structure of the Universe` of Germany

Deutsche Forschungsgemeinschaf (DFG)

CNRS/IN2P3

CNRS/IN2P3

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

FAPESP

CNPq of Brazil

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Ministry of Education and Science of the Russian Federation

Ministry of Education and Science of the Russian Federation

NNSFC Natural Science Foundation of China

Natural Science Foundation of China (NSFC)

CAS of China

Chinese Academy of Sciences (CAS)

MoST of China

MoST of China

MoE of China

MoE of China

GA and MSMT of the Czech Republic

GA and MSMT of the Czech Republic

Foundation for Fundamental Research on Matter (FOM)

Netherlands Organisation for Scientific Research (NWO)

FOM and NWO of the Netherlands

DAE, DST and CSIR of India

DST and CSIR of India

Department of Atomic Energy of India (DAE)

Polish Ministry of Science and Higher Education

Polish Ministry of Science and Higher Education

Korea Research Foundation

Korea Research Foundation

Ministry of Science, Education and Sports of Croatia

Ministry of Science, Education and Sports of Croatia

RosAtom of Russia

RosAtom of Russia

Identificador

NATURE, v.473, n.7347, p.353-356, 2011

0028-0836

http://producao.usp.br/handle/BDPI/29504

10.1038/nature10079

http://dx.doi.org/10.1038/nature10079

Idioma(s)

eng

Publicador

NATURE PUBLISHING GROUP

Relação

Nature

Direitos

restrictedAccess

Copyright NATURE PUBLISHING GROUP

Palavras-Chave #QUARK-GLUON PLASMA #ANTIPROTONS #COLLISIONS #ELECTRON #Multidisciplinary Sciences
Tipo

article

original article

publishedVersion