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  4. Observation of Two-Source Interference in the Photoproduction Reaction AuAu-->AuAu rho

Observation of Two-Source Interference in the Photoproduction Reaction AuAu-->AuAu rho

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Author(s)
Surrow, Bernd
•
Sakuma, Tai
•
Leight, William Axel
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Kocoloski, Adam Philip
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Jones, Christopher LaDon
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Corliss, Ross Cameron
•
Betancourt, Michael Joseph
•
Balewski, Jan T.
•
Surrow, Bernd
•
Walker, Matthew H
more
Date Issued
March 2009
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
STAR Collaboration et al. “Observation of Two-Source Interference in the Photoproduction Reaction AuAu-->AuAu rho.” Physical Review Letters 102.11 (2009): 112301. © 2009 The American Physical Society.
Version
Final published version
Abstract
In ultraperipheral relativistic heavy-ion collisions, a photon from the electromagnetic field of one nucleus can fluctuate to a quark-antiquark pair and scatter from the other nucleus, emerging as a ρ[superscript 0]. The ρ[superscript 0] production occurs in two well-separated (median impact parameters of 20 and 40 F for the cases considered here) nuclei, so the system forms a two-source interferometer. At low transverse momenta, the two amplitudes interfere destructively, suppressing ρ[superscript 0] production. Since the ρ[superscript 0] decays before the production amplitudes from the two sources can overlap, the two-pion system can only be described with an entangled nonlocal wave function, and is thus an example of the Einstein-Podolsky-Rosen paradox. We observe this suppression in 200 GeV per nucleon-pair gold-gold collisions. The interference is 87%±5%(stat.)±8%(syst.) of the expected level. This translates into a limit on decoherence due to wave function collapse or other factors of 23% at the 90% confidence level.
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
http://hdl.handle.net/1721.1/51784
DOI of Published Version
http://dx.doi.org/10.1103/PhysRevLett.102.112301
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