ρ[superscript 0] photoproduction in AuAu collisions at √sNN=62.4 GeV measured with the STAR detector
Name
Agakishiev-2012-ρ0 photoproduction in AuAu collisions at √sNN
Size
310.53 KB
Format
Adobe PDF
Checksum (MD5)
c3b22ffa7bb76aee3cc8cfa6f3289973
Author(s) • • • • • • • • •
Balewski, Jan T.
Betancourt, Michael Joseph
Corliss, Ross Cameron
Hays-Wehle, James Prewitt
Leight, William Axel
Surrow, Bernd
Walker, Margaret R.
Milner, Richard G
Redwine, Robert P
Seele, Joseph Patrick
Date Issued
January 2012
Journal
Physical Review C
Publisher
American Physical Society
Citation
©2012 American Physical Society
Version
Final published version
Abstract
Vector mesons may be photoproduced in relativistic heavy-ion collisions when a virtual photon emitted by one nucleus scatters from the other nucleus, emerging as a vector meson. The STAR Collaboration has previously presented measurements of coherent ρ[superscript 0] photoproduction at center of mass energies of 130 GeV and 200 GeV in AuAu collisions. Here, we present a measurement of the cross section at 62.4 GeV; we find that the cross section for coherent ρ[superscript 0] photoproduction with nuclear breakup is 10.5±1.5±1.6 mb at 62.4 GeV. The cross-section ratio between 200 GeV and 62.4 GeV is 4.4±0.6, less than is predicted by most theoretical models. It is, however, proportionally much larger than the previously observed 15%±55% increase between 130 GeV and 200 GeV.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1103/PhysRevC.85.014910