Inclusive (KSKS0)-K-0 resonance production in ep collisions at HERA

ZEUS Collaboration; S. Chekanov; M Derrick; S Magill; B. Musgrave; D Nicholass; J. Repond; R Yoshida; M. C. K. Mattingly; P. Antonioli; G. Bari; L. Bellagamba; D. Boscherini; A. Bruni; G. Bruni; F. Cindolo

doi:10.1103/PhysRevLett.101.112003

Back

Inclusive (KSKS0)-K-0 resonance production in ep collisions at HERA

Journal article

Peer reviewed

Inclusive (KSKS0)-K-0 resonance production in ep collisions at HERA

ZEUS Collaboration, S. Chekanov, M Derrick, S Magill, B. Musgrave, D Nicholass, J. Repond, R Yoshida, M. C. K. Mattingly, P. Antonioli, …

Physical review letters, Vol.101(11), 112003

09/12/2008

DOI: 10.1103/PhysRevLett.101.112003

PMID: 18851276

View Online

Abstract

Inclusive (KSKS0)-K-0 production in ep collisions at the DESY ep collider HERA was studied with the ZEUS detector using an integrated luminosity of 0.5 fb(-1). Enhancements in the mass spectrum were observed and are attributed to the production of f(2)(1270)/a(2)(0)(1320), f(2)(')(1525) and f(0)(1710). Masses and widths were obtained using a fit which takes into account theoretical predictions based on SU(3) symmetry arguments, and are consistent with the Particle Data Group values. The f(0)(1710) state, which has a mass consistent with a glueball candidate, was observed with a statistical significance of 5 standard deviations. However, if this state is the same as that seen in gamma gamma -> (KSKS0)-K-0, it is unlikely to be a pure glueball state.

Physical Sciences

Physics

Physics, Multidisciplinary

Science & Technology

Details

Title: Subtitle: Inclusive (KSKS0)-K-0 resonance production in ep collisions at HERA
Creators: ZEUS Collaboration
S. Chekanov (Contributor) - Argonne National Laboratory
M Derrick (Contributor) - Argonne National Laboratory
S Magill (Contributor) - Argonne National Laboratory
B. Musgrave (Contributor) - Argonne National Laboratory
D Nicholass (Contributor) - Argonne National Laboratory
J. Repond (Contributor) - Argonne National Laboratory
R Yoshida (Contributor) - Argonne National Laboratory
M. C. K. Mattingly (Contributor) - Andrews University
P. Antonioli (Contributor) - Argonne National Laboratory
G. Bari (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
L. Bellagamba (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
D. Boscherini (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
A. Bruni (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
G. Bruni (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
F. Cindolo (Contributor) - Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
Resource Type: Journal article
Publication Details: Physical review letters, Vol.101(11), 112003
DOI: 10.1103/PhysRevLett.101.112003
PMID: 18851276
NLM abbreviation: Phys Rev Lett
ISSN: 0031-9007
eISSN: 1079-7114
Publisher: Amer Physical Soc
Number of pages: 6
Grant note: PP/E000452/1 / Science and Technology Facilities Council; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) PP/E000452/1 / STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC)
Language: English
Date published: 09/12/2008
Academic Unit: Physics and Astronomy
Record Identifier: 9984627211202771

Metrics

12 Record Views

11 Times Cited - Web of Science