Published for SISSA by Springer
Received: February 7, 2017
Accepted: February 8, 2017 Published: February 16, 2017
A. Vinokurova,d A. Kuzmin,d S. Eidelman,d A. Abdesselam,bc I. Adachi,n;jH. Aihara,bh K. Arinstein,d D.M. Asner,au T. Aushev,ak;v R. Ayad,bc A.M. Bakich,bbV. Bansal,au V. Bhardwaj,an B. Bhuyan,p A. Bobrov,d A. Bondar,d A. Bozek,aqM. Bra cko,ag;w T.E. Browder,m V. Chekelian,ah B.G. Cheon,l K. Chilikin,vR. Chistov,v K. Cho,aa S.-K. Choi,k Y. Choi,ba D. Cinabro,bm J. Dingfelder,cZ. Dole zal,e Z. Dr asal,e A. Drutskoy,v;aj D. Dutta,p D. Epifanov,bh H. Farhat,bm J.E. Fast,au T. Ferber,g V. Gaur,bd N. Gabyshev,d A. Garmash,d R. Gillard,bm Y.M. Goh,l B. Golob,ae;w J. Haba,n;j K. Hayasaka,am H. Hayashii,an X.H. He,avW.-S. Hou,ap K. Inami,al A. Ishikawa,bg R. Itoh,n;j Y. Iwasaki,n D. Jo e,z T. Julius,ai K.H. Kang,ac E. Kato,bg C. Kiesling,ah D.Y. Kim,az H.J. Kim,ac J.H. Kim,aaK.T. Kim,ab M.J. Kim,ac S.H. Kim,l Y.J. Kim,aa K. Kinoshita,f B.R. Ko,ab P. Kody s,eS. Korpar,ag;w P. Kri zan,ae;w P. Krokovny,d T. Kuhr,y T. Kumita,bj Y.-J. Kwon,bo J.S. Lange,h L. Li Gioi,ah J. Libby,q D. Liventsev,n P. Lukin,d D. Matvienko,dK. Miyabayashi,an H. Miyake,n;j H. Miyata,ar G.B. Mohanty,bd A. Moll,ah;be T. Mori,alR. Mussa,u E. Nakano,at M. Nakao,n;j Z. Natkaniec,aq C. Ng,bh N.K. Nisar,bdS. Nishida,n;j S. Ogawa,bf S. Okuno,x S.L. Olsen,ay P. Pakhlov,v;aj G. Pakhlova,v C.W. Park,ba H. Park,ac T.K. Pedlar,af R. Pestotnik,w M. Petri c,w L.E. Piilonen,blE. Ribe zl,w M. Ritter,ah A. Rostomyan,g Y. Sakai,n;j S. Sandilya,bd D. Santel,fL. Santelj,n T. Sanuki,bg Y. Sato,al V. Savinov,aw O. Schneider,ad G. Schnell,a;oC. Schwanda,t D. Semmler,h K. Senyo,bn O. Seon,al M.E. Sevior,ai V. Shebalin,d C.P. Shen,b T.-A. Shibata,bi J.-G. Shiu,ap B. Shwartz,d A. Sibidanov,bb F. Simon,ah;beY.-S. Sohn,bo A. Sokolov,s E. Solovieva,v S. Stani c,as M. Stari c,w M. Steder,gM. Sumihama,i T. Sumiyoshi,bj U. Tamponi,u;bk G. Tatishvili,au Y. Teramoto,atM. Uchida,bi T. Uglov,v;ak Y. Unno,l S. Uno,n;j C. Van Hulse,a P. Vanhoefer,ahG. Varner,m V. Vorobyev,d M.N. Wagner,h C.H. Wang,ao M.-Z. Wang,ap P. Wang,rY. Watanabe,x K.M. Williams,bl E. Won,ab J. Yamaoka,au S. Yashchenko,g Y. Yook,bo
Z.P. Zhang,ax V. Zhulanovd and A. Zupancw
Open Access, c
[circlecopyrt] The Authors.
Article funded by SCOAP3. doi:http://dx.doi.org/10.1007/JHEP02(2017)088
Web End =10.1007/JHEP02(2017)088
Erratum: Search for B decays to nal states with the c meson
JHEP02(2017)088
BELLE
The BELLE collaboration
aUniversity of the Basque Country UPV/EHU, 48080 Bilbao, Spain
bBeihang University, Beijing 100191, P.R. China
cUniversity of Bonn, 53115 Bonn, Germany
dBudker Institute of Nuclear Physics SB RAS and Novosibirsk State University, Novosibirsk 630090, Russian Federation
eFaculty of Mathematics and Physics, Charles University, 121 16 Prague, The Czech Republic
f University of Cincinnati, Cincinnati, OH 45221, U.S.A.
gDeutsches Elektronen{Synchrotron, 22607 Hamburg, Germany
hJustus-Liebig-Universitat Gieen, 35392 Gieen, Germany
iGifu University, Gifu 501-1193, Japan
jThe Graduate University for Advanced Studies, Hayama 240-0193, Japan
kGyeongsang National University, Chinju 660-701, South Korea
lHanyang University, Seoul 133-791, South Korea
mUniversity of Hawaii, Honolulu, HI 96822, U.S.A.
nHigh Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan
oIKERBASQUE, Basque Foundation for Science, 48013 Bilbao, Spain
pIndian Institute of Technology Guwahati, Assam 781039, India
qIndian Institute of Technology Madras, Chennai 600036, India
rInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, P.R. China
sInstitute for High Energy Physics, Protvino 142281, Russian Federation
tInstitute of High Energy Physics, Vienna 1050, Austria
uINFN - Sezione di Torino, 10125 Torino, Italy
vInstitute for Theoretical and Experimental Physics, Moscow 117218, Russian Federation
wJ. Stefan Institute, 1000 Ljubljana, Slovenia
xKanagawa University, Yokohama 221-8686, Japan
yInstitut fur Experimentelle Kernphysik, Karlsruher Institut fur Technologie, 76131 Karlsruhe, Germany
zKennesaw State University, Kennesaw GA 30144, U.S.A.
aaKorea Institute of Science and Technology Information, Daejeon 305-806, South Korea
abKorea University, Seoul 136-713, South Korea
acKyungpook National University, Daegu 702-701, South Korea
ad
Ecole Polytechnique F ed erale de Lausanne (EPFL), Lausanne 1015, Switzerland
aeFaculty of Mathematics and Physics, University of Ljubljana, 1000 Ljubljana, Slovenia
af Luther College, Decorah, IA 52101, U.S.A.
agUniversity of Maribor, 2000 Maribor, Slovenia
ahMax-Planck-Institut fur Physik, 80805 Munchen, Germany
aiSchool of Physics, University of Melbourne, Victoria 3010, Australia
ajMoscow Physical Engineering Institute, Moscow 115409, Russian Federation
akMoscow Institute of Physics and Technology, Moscow Region 141700, Russian Federation
alGraduate School of Science, Nagoya University, Nagoya 464-8602, Japan
amKobayashi-Maskawa Institute, Nagoya University, Nagoya 464-8602, Japan
anNara Womens University, Nara 630-8506, Japan
aoNational United University, Miao Li 36003, Taiwan
apDepartment of Physics, National Taiwan University, Taipei 10617, Taiwan
JHEP02(2017)088
aqH. Niewodniczanski Institute of Nuclear Physics, Krakow 31-342, Poland
arNiigata University, Niigata 950-2181, Japan
asUniversity of Nova Gorica, 5000 Nova Gorica, Slovenia
atOsaka City University, Osaka 558-8585, Japan
auPaci c Northwest National Laboratory, Richland, WA 99352, U.S.A.
avPeking University, Beijing 100871, P.R. China
awUniversity of Pittsburgh, Pittsburgh, PA 15260, U.S.A.
axUniversity of Science and Technology of China, Hefei 230026, P.R. China
aySeoul National University, Seoul 151-742, South Korea
azSoongsil University, Seoul 156-743, South Korea
baSungkyunkwan University, Suwon 440-746, South Korea
bbSchool of Physics, University of Sydney, NSW 2006, Australia
bcDepartment of Physics, Faculty of Science, University of Tabuk, Tabuk 71451, Saudi Arabia
bdTata Institute of Fundamental Research, Mumbai 400005, India
beExcellence Cluster Universe, Technische Universitat Munchen, 85748 Garching, Germany
bf Toho University, Funabashi 274-8510, Japan
bgTohoku University, Sendai 980-8578, Japan
bhDepartment of Physics, University of Tokyo, Tokyo 113-0033, Japan
biTokyo Institute of Technology, Tokyo 152-8550, Japan
bjTokyo Metropolitan University, Tokyo 192-0397, Japan
bkUniversity of Torino, 10124 Torino, Italy
blCNP, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, U.S.A.
bmWayne State University, Detroit, MI 48202, U.S.A.
bnYamagata University, Yamagata 990-8560, Japan
boYonsei University, Seoul 120-749, South Korea
E-mail: mailto:[email protected]
Web End [email protected]
Erratum to: http://dx.doi.org/10.1007/JHEP06(2015)132
Web End =JHEP06(2015)132
ArXiv ePrint: 1501.06351
JHEP02(2017)088
{ 1 {
Events/5 MeV/c2
Events/5 MeV/c2
20
4
15
3
10
2
5
1
JHEP02(2017)088
0 3.8 3.9 4 4.1
0 3.8 3.9 4 4.1
M(hch), GeV/c2
M(hch), GeV/c2
Figure 1. Corrected gure 10. The combined t projections of the c invariant mass distributions in case of the ! (left) and ! +0 (right) modes corresponding to the search for the
X(3915) resonance.
Events/5 MeV/c2
20
15
10
5
0 3.8 3.9 4 4.1
M(hcp0), GeV/c2
Figure 2. Corrected gure 11. The c0 invariant mass distribution corresponding to the search for the X(3915) resonance.
We have found an error in the t of the c and c0 invariant masses that is used to search for the X(3915) state. The corrected ts are shown in gures 1 and 2. The resonance parameters are xed to the world average values (3918 MeV/c2 and 20 MeV/c2 for mass and width correspondingly).
The t results are summarized in table 1.
Changes in the ts of the X(3915) resonance lead to changes of the corresponding upper limits. The corrected upper limits on the X(3915) production and decay branching fraction products are summarized in table 2. All other results of the paper are correct.
{ 2 {
Decay mode Fitting function E ciency, % Yield
X(3915) ! c , ! (3.12) 6.60 0.02 7.1 14.5
! +0 1.64 0.01 1.0 2.1
X(3915) ! c0 (3.11) 6.88 0.02 6.9 17.3 Table 1. Corrected table 3. Fit results for the X(3915) resonance.
Resonance Decay mode Upper limit (90% C.L.)
X(3915) c 4.7 105 c0 1.7 105
Table 2. Corrected entry of table 8. Results of branching fraction measurements for the B decays containing intermediate X(3915).
Open Access. This article is distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/
Web End =CC-BY 4.0 ), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
JHEP02(2017)088
{ 3 {
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