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Looking For Disoriented Chiral Condensates From Pion Distributions

Nuclear Theory 2009-10-31 v1 High Energy Physics - Phenomenology Nuclear Experiment

Abstract

We suggest two methods for the detection of the formation of disoriented chiral condensates in heavy ion collisions. We show that the variance in the number of charged pions (in a suitable range of momentum space) provides a signature for the observation of a disoriented chiral condensate. The signal should be observable even if multiple domains of Dχ\chiC form provided the average number of pions per domain is significantly larger than unity. The variance of the number charged pions alone provides a signal which can be used even if the number of neutral pions cannot be measured in a given detector. On the other hand, the probability distribution in RR, the proportion of neutral pions to all pions emitted in heavy ion collisions in certain kinematic regions, has been suggested as a signal of a disoriented chiral condensate. Here we note that the signature can be greatly enhanced by making suitable cuts in the data. In particular, we consider reducing the data set such that the kk pions with lowest pTp_T are all neutral. We find that, given such cuts, <R><R> can be substantially different from 1/3. For example, for a single Dχ\chiC domain without contamination due to incoherently emitted pions, <R><R> is 3/5 given the pion with lowest pTp_T is neutral, and 5/7 given the two pions with lowest pTp_T are both neutral, {\it etc.}. The effects of multi-domain Dχ\chiC formation and noise due to incoherent pion emission can be systematically incorporated. Potential applications to experiments and their limitations are briefly discussed.

Keywords

Cite

@article{arxiv.nucl-th/9908013,
  title  = {Looking For Disoriented Chiral Condensates From Pion Distributions},
  author = {Chi-Keung Chow and Thomas D. Cohen},
  journal= {arXiv preprint arXiv:nucl-th/9908013},
  year   = {2009}
}

Comments

16 pages in REVTeX, 7 figures. Combined and updated version of nucl-th/9903029 and nucl-th/9904074. Accepted by Phys. Rev. C

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