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Article: Confirmation of the X(1835) and observation of the resonances X(2120) and X(2370) in J/ψ→γπ +π -η ′
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TitleConfirmation of the X(1835) and observation of the resonances X(2120) and X(2370) in J/ψ→γπ +π -η ′
 
AuthorsAblikim, M40
Achasov, MN13
An, L18
An, Q20
An, ZH40
Bai, JZ40
Baldini, R15
Ban, Y41
Becker, J1
Berger, N40
Bertani, M15
Bian, JM40
Boyko, I27
Briere, RA21
Bytev, V27
Cai, X40
Cao, GF40
Cao, XX40
Chang, JF40
Chelkov, G6 27
Chen, G40
Chen, HS40
Chen, JC40
Chen, ML40
Chen, SJ4
Chen, Y40
Chen, YB40
Cheng, HP31
Chu, YP40
CroninHennessy, D7
Dai, HL40
Dai, JP40
Dedovich, D27
Deng, ZY40
Denysenko, I27 45
Destefanis, M23
Ding, Y28
Dong, LY40
Dong, MY40
Du, SX14
Duan, MY44
Fan, RR40
Fang, J40
Fang, SS40
Feldbauer, F1
Feng, CQ20
Fu, CD40
Fu, JL4
Gao, Y36
Geng, C20
Goetzen, K34
Gong, WX40
Greco, M23
Grishin, S27
Gu, MH40
Gu, YT18
Guan, YH2
Guo, AQ24
Guo, LB26
Guo, YP24
Hao, XQ40
Harris, FA22
He, KL40
He, M40
He, ZY24
Heng, YK40
Hou, ZL40
Hu, HM40
Hu, JF2
Hu, T40
Huang, B40
Huang, GM16
Huang, JS35
Huang, XT5
Huang, YP40
Hussain, T32
Ji, CS20
Ji, Q40
Ji, XB40
Ji, XL40
Jia, LK40
Jiang, LL40
Jiang, XS40
Jiao, JB5
Jiao, Z31
Jin, DP40
Jin, S40
Jing, FF36
Kavatsyuk, M8
Komamiya, S33
Kuehn, W30
Lange, JS30
Leung, JKC10
Li, C20
Li, C20
Li, DM14
Li, F40
Li, G40
Li, HB40
Li, JC40
Li, L40
Li, NB26
Li, QJ40
Li, WD40
Li, WG40
Li, XL5
Li, XN40
Li, XQ24
Li, XR40
Li, ZB25
Liang, H20
Liang, YF42
Liang, YT30
Liao, GR38
Liao, XT40
Liu, BJ43
Liu, BJ10
Liu, CL21
Liu, CX40
Liu, CY40
Liu, FH44
Liu, F40
Liu, F16
Liu, GC40
Liu, H40
Liu, HB2
Liu, HM40
Liu, HW40
Liu, JP17
Liu, K41
Liu, KY28
Liu, Q22
Liu, SB20
Liu, X9
Liu, XH40
Liu, YB24
Liu, YW20
Liu, Y40
Liu, ZA40
Liu, ZQ40
Loehner, H8
Lu, GR35
Lu, HJ31
Lu, JG40
Lu, QW44
Lu, XR2
Lu, YP40
Luo, CL26
Luo, MX11
Luo, T40
Luo, XL40
Ma, CL2
Ma, FC28
Ma, HL40
Ma, QM40
Ma, T40
Ma, X40
Ma, XY40
Maggiora, M23
Malik, QA32
Mao, H40
Mao, YJ41
Mao, ZP40
Messchendorp, JG8
Min, J40
Mitchell, RE37
Mo, XH40
Motzko, C1
Muchnoi, NYu13
Nefedov, Y27
Ning, Z40
Olsen, SL29
Ouyang, Q40
Pacetti, S15
Pelizaeus, M22
Peters, K34
Ping, JL26
Ping, RG40
Poling, R7
Pun, CSJ10
Qi, M4
Qian, S40
Qiao, CF2
Qin, XS40
Qiu, JF40
Rashid, KH32
Rong, G40
Ruan, XD18
Sarantsev, A27 3
Schulze, J1
Shao, M20
Shen, CP22
Shen, XY40
Sheng, HY40
Shepherd, MR37
Song, XY40
Sonoda, S33
Spataro, S23
Spruck, B30
Sun, DH40
Sun, GX40
Sun, JF35
Sun, SS40
Sun, XD40
Sun, YJ20
Sun, YZ40
Sun, ZJ40
Sun, ZT20
Tang, CJ42
Tang, X40
Tang, XF38
Tian, HL40
Toth, D7
Varner, GS22
Wan, X40
Wang, BQ41
Wang, K40
Wang, LL19
Wang, LS40
Wang, M5
Wang, P40
Wang, PL40
Wang, Q40
Wang, SG41
Wang, XL20
Wang, YD20
Wang, YF40
Wang, YQ5
Wang, Z40
Wang, ZG40
Wang, ZY40
Wei, DH38
Wen, SP40
Wiedner, U1
Wu, LH40
Wu, N40
Wu, W28
Wu, Z40
Xiao, ZJ26
Xie, YG40
Xu, GF40
Xu, GM41
Xu, H40
Xu, Y24
Xu, ZR20
Xu, ZZ20
Xue, Z40
Yan, L20
Yan, WB20
Yan, YH12
Yang, HX40
Yang, M40
Yang, T18
Yang, Y16
Yang, YX38
Ye, M40
Ye, MH19
Yu, BX40
Yu, CX24
Yu, L16
Yuan, CZ40
Yuan, WL26
Yuan, Y40
Zafar, AA32
Zallo, A15
Zeng, Y12
Zhang, BX40
Zhang, BY40
Zhang, CC40
Zhang, DH40
Zhang, HH25
Zhang, HY40
Zhang, J26
Zhang, JW40
Zhang, JY40
Zhang, JZ40
Zhang, L4
Zhang, SH40
Zhang, TR26
Zhang, XJ40
Zhang, XY5
Zhang, Y40
Zhang, YH40
Zhang, ZP20
Zhang, ZY17
Zhao, G40
Zhao, HS40
Zhao, J20
Zhao, J40
Zhao, L20
Zhao, L40
Zhao, MG24
Zhao, Q40
Zhao, SJ14
Zhao, TC39
Zhao, XH4
Zhao, YB40
Zhao, ZG20
Zhao, ZL18
Zhemchugov, A6 27
Zheng, B40
Zheng, JP40
Zheng, YH2
Zheng, ZP40
Zhong, B40
Zhong, J1
Zhong, L36
Zhou, L40
Zhou, XK2
Zhou, XR20
Zhu, C40
Zhu, K40
Zhu, KJ40
Zhu, SH40
Zhu, XL36
Zhu, XW40
Zhu, YS40
Zhu, ZA40
Zhuang, J40
Zou, BS40
Zou, JH40
Zuo, JX40
Zweber, P7
 
KeywordsDecay mode
Invariant-mass spectra
Radiative photons
Statistical significance
Mass spectrometry
 
Issue Date2011
 
PublisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org
 
CitationPhysical Review Letters, 2011, v. 106 n. 7 [How to Cite?]
DOI: http://dx.doi.org/10.1103/PhysRevLett.106.072002
 
AbstractWith a sample of (225.2±2.8)×106 J/ψ events registered in the BESIII detector, J/ψ→γπ +π -η ′ is studied using two η ′ decay modes: η ′→π +π -η and η ′→γρ0. The X(1835), which was previously observed by BESII, is confirmed with a statistical significance that is larger than 20σ. In addition, in the π +π -η ′ invariant-mass spectrum, the X(2120) and the X(2370), are observed with statistical significances larger than 7.2σ and 6.4σ, respectively. For the X(1835), the angular distribution of the radiative photon is consistent with expectations for a pseudoscalar. © 2011 American Physical Society.
 
ISSN0031-9007
2013 Impact Factor: 7.728
 
DOIhttp://dx.doi.org/10.1103/PhysRevLett.106.072002
 
ISI Accession Number IDWOS:000287392300004
Funding AgencyGrant Number
Ministry of Science and Technology of China
National Natural Science Foundation of China
Chinese Academy of Sciences
Istituto Nazionale di Fisica Nucleare
Russian Foundation for Basic Research
Russian Academy of Science (Siberian branch)
U.S. Department of Energy
National Research Foundation of Korea
Funding Information:

We thank the accelerator group and computer staff of IHEP for their effort in producing beams and processing data. We are grateful for support from our institutes and universities and from these agencies: Ministry of Science and Technology of China, National Natural Science Foundation of China, Chinese Academy of Sciences, Istituto Nazionale di Fisica Nucleare, Russian Foundation for Basic Research, Russian Academy of Science (Siberian branch), U.S. Department of Energy, and National Research Foundation of Korea.

 
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DC FieldValue
dc.contributor.authorAblikim, M
 
dc.contributor.authorAchasov, MN
 
dc.contributor.authorAn, L
 
dc.contributor.authorAn, Q
 
dc.contributor.authorAn, ZH
 
dc.contributor.authorBai, JZ
 
dc.contributor.authorBaldini, R
 
dc.contributor.authorBan, Y
 
dc.contributor.authorBecker, J
 
dc.contributor.authorBerger, N
 
dc.contributor.authorBertani, M
 
dc.contributor.authorBian, JM
 
dc.contributor.authorBoyko, I
 
dc.contributor.authorBriere, RA
 
dc.contributor.authorBytev, V
 
dc.contributor.authorCai, X
 
dc.contributor.authorCao, GF
 
dc.contributor.authorCao, XX
 
dc.contributor.authorChang, JF
 
dc.contributor.authorChelkov, G
 
dc.contributor.authorChen, G
 
dc.contributor.authorChen, HS
 
dc.contributor.authorChen, JC
 
dc.contributor.authorChen, ML
 
dc.contributor.authorChen, SJ
 
dc.contributor.authorChen, Y
 
dc.contributor.authorChen, YB
 
dc.contributor.authorCheng, HP
 
dc.contributor.authorChu, YP
 
dc.contributor.authorCroninHennessy, D
 
dc.contributor.authorDai, HL
 
dc.contributor.authorDai, JP
 
dc.contributor.authorDedovich, D
 
dc.contributor.authorDeng, ZY
 
dc.contributor.authorDenysenko, I
 
dc.contributor.authorDestefanis, M
 
dc.contributor.authorDing, Y
 
dc.contributor.authorDong, LY
 
dc.contributor.authorDong, MY
 
dc.contributor.authorDu, SX
 
dc.contributor.authorDuan, MY
 
dc.contributor.authorFan, RR
 
dc.contributor.authorFang, J
 
dc.contributor.authorFang, SS
 
dc.contributor.authorFeldbauer, F
 
dc.contributor.authorFeng, CQ
 
dc.contributor.authorFu, CD
 
dc.contributor.authorFu, JL
 
dc.contributor.authorGao, Y
 
dc.contributor.authorGeng, C
 
dc.contributor.authorGoetzen, K
 
dc.contributor.authorGong, WX
 
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dc.contributor.authorGrishin, S
 
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dc.contributor.authorJiao, Z
 
dc.contributor.authorJin, DP
 
dc.contributor.authorJin, S
 
dc.contributor.authorJing, FF
 
dc.contributor.authorKavatsyuk, M
 
dc.contributor.authorKomamiya, S
 
dc.contributor.authorKuehn, W
 
dc.contributor.authorLange, JS
 
dc.contributor.authorLeung, JKC
 
dc.contributor.authorLi, C
 
dc.contributor.authorLi, C
 
dc.contributor.authorLi, DM
 
dc.contributor.authorLi, F
 
dc.contributor.authorLi, G
 
dc.contributor.authorLi, HB
 
dc.contributor.authorLi, JC
 
dc.contributor.authorLi, L
 
dc.contributor.authorLi, NB
 
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dc.contributor.authorLiu, YB
 
dc.contributor.authorLiu, YW
 
dc.contributor.authorLiu, Y
 
dc.contributor.authorLiu, ZA
 
dc.contributor.authorLiu, ZQ
 
dc.contributor.authorLoehner, H
 
dc.contributor.authorLu, GR
 
dc.contributor.authorLu, HJ
 
dc.contributor.authorLu, JG
 
dc.contributor.authorLu, QW
 
dc.contributor.authorLu, XR
 
dc.contributor.authorLu, YP
 
dc.contributor.authorLuo, CL
 
dc.contributor.authorLuo, MX
 
dc.contributor.authorLuo, T
 
dc.contributor.authorLuo, XL
 
dc.contributor.authorMa, CL
 
dc.contributor.authorMa, FC
 
dc.contributor.authorMa, HL
 
dc.contributor.authorMa, QM
 
dc.contributor.authorMa, T
 
dc.contributor.authorMa, X
 
dc.contributor.authorMa, XY
 
dc.contributor.authorMaggiora, M
 
dc.contributor.authorMalik, QA
 
dc.contributor.authorMao, H
 
dc.contributor.authorMao, YJ
 
dc.contributor.authorMao, ZP
 
dc.contributor.authorMesschendorp, JG
 
dc.contributor.authorMin, J
 
dc.contributor.authorMitchell, RE
 
dc.contributor.authorMo, XH
 
dc.contributor.authorMotzko, C
 
dc.contributor.authorMuchnoi, NYu
 
dc.contributor.authorNefedov, Y
 
dc.contributor.authorNing, Z
 
dc.contributor.authorOlsen, SL
 
dc.contributor.authorOuyang, Q
 
dc.contributor.authorPacetti, S
 
dc.contributor.authorPelizaeus, M
 
dc.contributor.authorPeters, K
 
dc.contributor.authorPing, JL
 
dc.contributor.authorPing, RG
 
dc.contributor.authorPoling, R
 
dc.contributor.authorPun, CSJ
 
dc.contributor.authorQi, M
 
dc.contributor.authorQian, S
 
dc.contributor.authorQiao, CF
 
dc.contributor.authorQin, XS
 
dc.contributor.authorQiu, JF
 
dc.contributor.authorRashid, KH
 
dc.contributor.authorRong, G
 
dc.contributor.authorRuan, XD
 
dc.contributor.authorSarantsev, A
 
dc.contributor.authorSchulze, J
 
dc.contributor.authorShao, M
 
dc.contributor.authorShen, CP
 
dc.contributor.authorShen, XY
 
dc.contributor.authorSheng, HY
 
dc.contributor.authorShepherd, MR
 
dc.contributor.authorSong, XY
 
dc.contributor.authorSonoda, S
 
dc.contributor.authorSpataro, S
 
dc.contributor.authorSpruck, B
 
dc.contributor.authorSun, DH
 
dc.contributor.authorSun, GX
 
dc.contributor.authorSun, JF
 
dc.contributor.authorSun, SS
 
dc.contributor.authorSun, XD
 
dc.contributor.authorSun, YJ
 
dc.contributor.authorSun, YZ
 
dc.contributor.authorSun, ZJ
 
dc.contributor.authorSun, ZT
 
dc.contributor.authorTang, CJ
 
dc.contributor.authorTang, X
 
dc.contributor.authorTang, XF
 
dc.contributor.authorTian, HL
 
dc.contributor.authorToth, D
 
dc.contributor.authorVarner, GS
 
dc.contributor.authorWan, X
 
dc.contributor.authorWang, BQ
 
dc.contributor.authorWang, K
 
dc.contributor.authorWang, LL
 
dc.contributor.authorWang, LS
 
dc.contributor.authorWang, M
 
dc.contributor.authorWang, P
 
dc.contributor.authorWang, PL
 
dc.contributor.authorWang, Q
 
dc.contributor.authorWang, SG
 
dc.contributor.authorWang, XL
 
dc.contributor.authorWang, YD
 
dc.contributor.authorWang, YF
 
dc.contributor.authorWang, YQ
 
dc.contributor.authorWang, Z
 
dc.contributor.authorWang, ZG
 
dc.contributor.authorWang, ZY
 
dc.contributor.authorWei, DH
 
dc.contributor.authorWen, SP
 
dc.contributor.authorWiedner, U
 
dc.contributor.authorWu, LH
 
dc.contributor.authorWu, N
 
dc.contributor.authorWu, W
 
dc.contributor.authorWu, Z
 
dc.contributor.authorXiao, ZJ
 
dc.contributor.authorXie, YG
 
dc.contributor.authorXu, GF
 
dc.contributor.authorXu, GM
 
dc.contributor.authorXu, H
 
dc.contributor.authorXu, Y
 
dc.contributor.authorXu, ZR
 
dc.contributor.authorXu, ZZ
 
dc.contributor.authorXue, Z
 
dc.contributor.authorYan, L
 
dc.contributor.authorYan, WB
 
dc.contributor.authorYan, YH
 
dc.contributor.authorYang, HX
 
dc.contributor.authorYang, M
 
dc.contributor.authorYang, T
 
dc.contributor.authorYang, Y
 
dc.contributor.authorYang, YX
 
dc.contributor.authorYe, M
 
dc.contributor.authorYe, MH
 
dc.contributor.authorYu, BX
 
dc.contributor.authorYu, CX
 
dc.contributor.authorYu, L
 
dc.contributor.authorYuan, CZ
 
dc.contributor.authorYuan, WL
 
dc.contributor.authorYuan, Y
 
dc.contributor.authorZafar, AA
 
dc.contributor.authorZallo, A
 
dc.contributor.authorZeng, Y
 
dc.contributor.authorZhang, BX
 
dc.contributor.authorZhang, BY
 
dc.contributor.authorZhang, CC
 
dc.contributor.authorZhang, DH
 
dc.contributor.authorZhang, HH
 
dc.contributor.authorZhang, HY
 
dc.contributor.authorZhang, J
 
dc.contributor.authorZhang, JW
 
dc.contributor.authorZhang, JY
 
dc.contributor.authorZhang, JZ
 
dc.contributor.authorZhang, L
 
dc.contributor.authorZhang, SH
 
dc.contributor.authorZhang, TR
 
dc.contributor.authorZhang, XJ
 
dc.contributor.authorZhang, XY
 
dc.contributor.authorZhang, Y
 
dc.contributor.authorZhang, YH
 
dc.contributor.authorZhang, ZP
 
dc.contributor.authorZhang, ZY
 
dc.contributor.authorZhao, G
 
dc.contributor.authorZhao, HS
 
dc.contributor.authorZhao, J
 
dc.contributor.authorZhao, J
 
dc.contributor.authorZhao, L
 
dc.contributor.authorZhao, L
 
dc.contributor.authorZhao, MG
 
dc.contributor.authorZhao, Q
 
dc.contributor.authorZhao, SJ
 
dc.contributor.authorZhao, TC
 
dc.contributor.authorZhao, XH
 
dc.contributor.authorZhao, YB
 
dc.contributor.authorZhao, ZG
 
dc.contributor.authorZhao, ZL
 
dc.contributor.authorZhemchugov, A
 
dc.contributor.authorZheng, B
 
dc.contributor.authorZheng, JP
 
dc.contributor.authorZheng, YH
 
dc.contributor.authorZheng, ZP
 
dc.contributor.authorZhong, B
 
dc.contributor.authorZhong, J
 
dc.contributor.authorZhong, L
 
dc.contributor.authorZhou, L
 
dc.contributor.authorZhou, XK
 
dc.contributor.authorZhou, XR
 
dc.contributor.authorZhu, C
 
dc.contributor.authorZhu, K
 
dc.contributor.authorZhu, KJ
 
dc.contributor.authorZhu, SH
 
dc.contributor.authorZhu, XL
 
dc.contributor.authorZhu, XW
 
dc.contributor.authorZhu, YS
 
dc.contributor.authorZhu, ZA
 
dc.contributor.authorZhuang, J
 
dc.contributor.authorZou, BS
 
dc.contributor.authorZou, JH
 
dc.contributor.authorZuo, JX
 
dc.contributor.authorZweber, P
 
dc.date.accessioned2011-10-28T02:48:31Z
 
dc.date.available2011-10-28T02:48:31Z
 
dc.date.issued2011
 
dc.description.abstractWith a sample of (225.2±2.8)×106 J/ψ events registered in the BESIII detector, J/ψ→γπ +π -η ′ is studied using two η ′ decay modes: η ′→π +π -η and η ′→γρ0. The X(1835), which was previously observed by BESII, is confirmed with a statistical significance that is larger than 20σ. In addition, in the π +π -η ′ invariant-mass spectrum, the X(2120) and the X(2370), are observed with statistical significances larger than 7.2σ and 6.4σ, respectively. For the X(1835), the angular distribution of the radiative photon is consistent with expectations for a pseudoscalar. © 2011 American Physical Society.
 
dc.description.naturepublished_or_final_version
 
dc.identifier.citationPhysical Review Letters, 2011, v. 106 n. 7 [How to Cite?]
DOI: http://dx.doi.org/10.1103/PhysRevLett.106.072002
 
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevLett.106.072002
 
dc.identifier.hkuros196928
 
dc.identifier.isiWOS:000287392300004
Funding AgencyGrant Number
Ministry of Science and Technology of China
National Natural Science Foundation of China
Chinese Academy of Sciences
Istituto Nazionale di Fisica Nucleare
Russian Foundation for Basic Research
Russian Academy of Science (Siberian branch)
U.S. Department of Energy
National Research Foundation of Korea
Funding Information:

We thank the accelerator group and computer staff of IHEP for their effort in producing beams and processing data. We are grateful for support from our institutes and universities and from these agencies: Ministry of Science and Technology of China, National Natural Science Foundation of China, Chinese Academy of Sciences, Istituto Nazionale di Fisica Nucleare, Russian Foundation for Basic Research, Russian Academy of Science (Siberian branch), U.S. Department of Energy, and National Research Foundation of Korea.

 
dc.identifier.issn0031-9007
2013 Impact Factor: 7.728
 
dc.identifier.issue7
 
dc.identifier.openurl
 
dc.identifier.pmid21405509
 
dc.identifier.scopuseid_2-s2.0-79951634119
 
dc.identifier.urihttp://hdl.handle.net/10722/142496
 
dc.identifier.volume106
 
dc.languageeng
 
dc.publisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org
 
dc.publisher.placeUnited States
 
dc.relation.ispartofPhysical Review Letters
 
dc.relation.referencesReferences in Scopus
 
dc.rightsPhysical Review Letters. Copyright © American Physical Society.
 
dc.rightsCreative Commons: Attribution 3.0 Hong Kong License
 
dc.subjectDecay mode
 
dc.subjectInvariant-mass spectra
 
dc.subjectRadiative photons
 
dc.subjectStatistical significance
 
dc.subjectMass spectrometry
 
dc.titleConfirmation of the X(1835) and observation of the resonances X(2120) and X(2370) in J/ψ→γπ +π -η ′
 
dc.typeArticle
 
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<contributor.author>An, ZH</contributor.author>
<contributor.author>Bai, JZ</contributor.author>
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<date.accessioned>2011-10-28T02:48:31Z</date.accessioned>
<date.available>2011-10-28T02:48:31Z</date.available>
<date.issued>2011</date.issued>
<identifier.citation>Physical Review Letters, 2011, v. 106 n. 7</identifier.citation>
<identifier.issn>0031-9007</identifier.issn>
<identifier.uri>http://hdl.handle.net/10722/142496</identifier.uri>
<description.abstract>With a sample of (225.2&#177;2.8)&#215;106 J/&#968; events registered in the BESIII detector, J/&#968;&#8594;&#947;&#960; +&#960; -&#951; &#8242; is studied using two &#951; &#8242; decay modes: &#951; &#8242;&#8594;&#960; +&#960; -&#951; and &#951; &#8242;&#8594;&#947;&#961;0. The X(1835), which was previously observed by BESII, is confirmed with a statistical significance that is larger than 20&#963;. In addition, in the &#960; +&#960; -&#951; &#8242; invariant-mass spectrum, the X(2120) and the X(2370), are observed with statistical significances larger than 7.2&#963; and 6.4&#963;, respectively. For the X(1835), the angular distribution of the radiative photon is consistent with expectations for a pseudoscalar. &#169; 2011 American Physical Society.</description.abstract>
<language>eng</language>
<publisher>American Physical Society. The Journal&apos;s web site is located at http://prl.aps.org</publisher>
<relation.ispartof>Physical Review Letters</relation.ispartof>
<rights>Physical Review Letters. Copyright &#169; American Physical Society.</rights>
<rights>Creative Commons: Attribution 3.0 Hong Kong License</rights>
<subject>Decay mode</subject>
<subject>Invariant-mass spectra</subject>
<subject>Radiative photons</subject>
<subject>Statistical significance</subject>
<subject>Mass spectrometry</subject>
<title>Confirmation of the X(1835) and observation of the resonances X(2120) and X(2370) in J/&#968;&#8594;&#947;&#960; +&#960; -&#951; &#8242;</title>
<type>Article</type>
<identifier.openurl>http://library.hku.hk:4550/resserv?sid=HKU:IR&amp;issn=0031-9007&amp;volume=106&amp;issue=7, article no. 072002&amp;spage=&amp;epage=&amp;date=2011&amp;atitle=Confirmation+of+the+X(1835)+and+observation+of+the+resonances+X(2120)+and+X(2370)+in+J/&#968;&#8594;&#947;&#960;+&#960;-&#951;&#8242;</identifier.openurl>
<description.nature>published_or_final_version</description.nature>
<identifier.doi>10.1103/PhysRevLett.106.072002</identifier.doi>
<identifier.pmid>21405509</identifier.pmid>
<identifier.scopus>eid_2-s2.0-79951634119</identifier.scopus>
<identifier.hkuros>196928</identifier.hkuros>
<relation.references>http://www.scopus.com/mlt/select.url?eid=2-s2.0-79951634119&amp;selection=ref&amp;src=s&amp;origin=recordpage</relation.references>
<identifier.volume>106</identifier.volume>
<identifier.issue>7</identifier.issue>
<identifier.isi>WOS:000287392300004</identifier.isi>
<publisher.place>United States</publisher.place>
<bitstream.url>http://hub.hku.hk/bitstream/10722/142496/1/content.pdf</bitstream.url>
</item>
Author Affiliations
  1. Universität Bochum
  2. Graduate University of Chinese Academy of Sciences
  3. Saint Petersburg Nuclear Physics Institute, Russian Academy of Sciences
  4. Nanjing University
  5. Shandong University
  6. Moskovskij Fiziko-Tehniceskij Institut - Gosudarstvennyj Universitet
  7. University of Minnesota Twin Cities
  8. Rijksuniversiteit Groningen
  9. Lanzhou University
  10. The University of Hong Kong
  11. Zhejiang University
  12. Hunan University
  13. Budker Institute of Nuclear Physics of the Siberian Branch of the RAS
  14. Zhengzhou University
  15. Laboratori Nazionali di Frascati di INFN
  16. Huazhong Normal University
  17. Wuhan University
  18. Guangxi University
  19. China Center of Advanced Science and Technology World Laboratory
  20. University of Science and Technology of China
  21. Carnegie Mellon University
  22. University of Hawaii at Manoa
  23. Università degli Studi di Torino
  24. Nankai University
  25. Sun Yat-Sen University
  26. Nanjing Normal University
  27. Joint Institute for Nuclear Research, Dubna
  28. Liaoning University
  29. Seoul National University
  30. null
  31. Huangshan University
  32. University of the Punjab Lahore
  33. University of Tokyo
  34. GSI Helmholtz Centre for Heavy Ion Research GmbH
  35. Henan Normal University
  36. Tsinghua University
  37. Indiana University
  38. Guangxi Normal University
  39. University of Washington Seattle
  40. Institute of High Energy Physics Chinese Academy of Science
  41. Peking University
  42. Sichuan University
  43. Chinese University of Hong Kong
  44. Shanxi University
  45. Bogolyubov Institute for Theoretical Physics Nasu