publication . Article . Other literature type . Preprint . 2018

Search for muoproduction of X (3872) at COMPASS and indication of a new state $\widetilde{X}$(3872)

COMPASS Collaboration; Aghasyan, M.; Augsten, K.; Kondo, K.; Königsmann, K.; Konorov, I.; Konstantinov, V. F.; Kotzinian, A. M.; Kouznetsov, O. M.; Kral, Z.; ...
View all 200 authors
Open Access English
  • Published: 01 Jan 2018
  • Publisher: HAL CCSD
Abstract
Comment: 12 pages, 6 figures
doi: 10.1016/j.physletb.2018.07.008 , 10.18154/rwth-2018-228935
handle: 10400.26/27381
Subjects
arXiv: High Energy Physics::Experiment
free text keywords: muon, statistical, branching ratio, photoproduction, charmonium, tetraquark: model, pi+ pi-: mass spectrum, * Automatic Keywords *, Exotic charmonia, Tetraquark, X(3872), COMPASS, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Subatomic Physics, Subatomär fysik, CERN SPS, X(3872) --> J/psi(3100) 2pi, hadronic decay [X(3872)], leptoproduction [X(3872)], branching ratio: measured [channel cross section], exclusive production, experimental results, hadron, two-pion [mass spectrum], exclusive reaction [muon nucleus], scattering [muon+ nucleus], beam [muon+], X (3872), фотопродукция, тетракварки, чармоний, hep-ex, Particle Physics - Experiment, COMPASS; X(3872); Photoproduction; Tetraquark; Exotic charmonia, High Energy Physics - Experiment, Nuclear and High Energy Physics, ddc:530, Branching fraction, Particle physics, Physics
Related Organizations
View more
Funded by
EC| HADRONPHYSICS3
Project
HADRONPHYSICS3
Study of Strongly Interacting Matter
  • Funder: European Commission (EC)
  • Project Code: 283286
  • Funding stream: FP7 | SP4 | INFRA
, NSF| A Program of Medium Energy Nuclear Physics
Project
A Program of Medium Energy Nuclear Physics
  • Funder: National Science Foundation (NSF)
  • Project Code: 1506416
Download fromView all 17 versions
HAL-CEA
Article . 2018
Provider: HAL-CEA
Electronic archive of Tomsk Polytechnic University
Article . 2018
Provider: Electronic archive of Tomsk Polytechnic University
HAL-Inserm
Article . 2018
Provider: HAL-Inserm
CERN Document Server
Other literature type . 2018
Provider: CERN Document Server
View more
45 references, page 1 of 3

[1] S.K. Choi, et al., Belle Collaboration, Phys. Rev. Lett. 91 (2003) 262001.

[2] G. Gokhroo, et al., Belle Collaboration, Phys. Rev. Lett. 97 (2006) 162002.

[3] T. Aushev, et al., Belle Collaboration, Phys. Rev. D 81 (2010) 031103.

[4] V. Bhardwaj, et al., Belle Collaboration, Phys. Rev. Lett. 107 (2011) 091803.

[5] S.K. Choi, et al., Belle Collaboration, Phys. Rev. D 84 (2011) 052004.

[6] B. Aubert, et al., BaBar Collaboration, Phys. Rev. D 71 (2005) 071103.

[7] B. Aubert, et al., BaBar Collaboration, Phys. Rev. D 73 (2006) 011101.

[8] B. Aubert, et al., BaBar Collaboration, Phys. Rev. D 74 (2006) 071101.

[9] B. Aubert, et al., BaBar Collaboration, Phys. Rev. D 77 (2008) 011102.

[10] B. Aubert, et al., BaBar Collaboration, Phys. Rev. D 77 (2008) 111101.

[11] B. Aubert, et al., BaBar Collaboration, Phys. Rev. Lett. 102 (2009) 132001.

[12] P. del Amo Sanchez, et al., BaBar Collaboration, Phys. Rev. D 82 (2010) 011101.

[13] M. Ablikim, et al., BESIII Collaboration, Phys. Rev. Lett. 112 (2014) 092001.

[14] D. Acosta, et al., CDF Collaboration, Phys. Rev. Lett. 93 (2004) 072001.

[15] A. Abulencia, et al., CDF Collaboration, Phys. Rev. Lett. 96 (2006) 102002.

45 references, page 1 of 3
Powered by OpenAIRE Research Graph
Any information missing or wrong?Report an Issue