Multiplicity distributions in {bar p}p interactions at √s = 1800 GeV [electronic resource]

Preliminary results on multiplicity distributions at √s = 1800 GeV in the η intervals {vert_bar} η {vert_bar} ≤ 2.5, 2.0, 1.5, 1.0, 0.5 are presented. The data were collected with a minimum bias trigger by the Collider Detector at Fermilab in two different runs. A small sample of data at √s = 630 Ge...

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Bibliographic Details
Online Access: Online Access
Corporate Authors: Fermi National Accelerator Laboratory (Researcher), Federal Energy Technology Center (U.S.) (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : United States. Dept. of Energy ; distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy, 1993.
Subjects:

MARC

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500 |a 23. international symposium on multiparticle dynamics,Aspen, CO (United States),13-17 Sep 1993. 
500 |a CDF Collaboration; Rimondi, F. 
520 3 |a Preliminary results on multiplicity distributions at √s = 1800 GeV in the η intervals {vert_bar} η {vert_bar} ≤ 2.5, 2.0, 1.5, 1.0, 0.5 are presented. The data were collected with a minimum bias trigger by the Collider Detector at Fermilab in two different runs. A small sample of data at √s = 630 GeV was used for comparison with lower energy results and for checking on systematic effects. The multiplicity distributions at √s = 1800 GeV deviate from the negative binomial distribution in rapidity intervals larger than {vert_bar} η {vert_bar} ≥ 0.5. This confirms the trend already observed at √s = 900 GeV where the deviation from the negative binomial starts at {vert_bar} η {vert_bar} > 2.5. 
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