Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. Identified Hadron Compositions in p+p and Au+Au Collisions at High Transverse Momenta at √sNN=200  GeV

Identified Hadron Compositions in p+p and Au+Au Collisions at High Transverse Momenta at √sNN=200  GeV

Thumbnail Image
Download
Name

Agakishiev-2012-Identified Hadron Compositions in p+p and Au+Au Collisions at High Transverse Momenta at √sNN

Size

314.88 KB

Format

Adobe PDF

Checksum (MD5)

66e8e6571399c2a6e4b6d47fe03b54eb

Author(s)
Balewski, Jan T.
•
Betancourt, Michael Joseph
•
Corliss, Ross
•
Hays-Wehle, James Prewitt
•
Leight, William Axel
•
Milner, Richard G.
•
Redwine, Robert P
•
Seele, J.
•
Steadman, Stephen G.
•
Surrow, Bernd
more
Date Issued
February 2012
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Agakishiev, G., M. M. Aggarwal, Z. Ahammed, et al. Identified Hadron Compositions in P+p and Au+Au Collisions at High Transverse Momenta at sqrt[s_{NN}]=200 GeV. Physical Review Letters 108(7). 2012. © 2012 American Physical Society
Version
Final published version
Abstract
We report transverse momentum (pT≤15  GeV/c) spectra of π[superscript ±], K[superscript ±], p, p̅ , K[subscript S][superscript 0], and ρ[superscript 0] at midrapidity in p+p and Au+Au collisions at √sNN=200  GeV. Perturbative QCD calculations are consistent with π[superscript ±] spectra in p+p collisions but do not reproduce K and p(p̅ ) spectra. The observed decreasing antiparticle-to-particle ratios with increasing p[subscript T] provide experimental evidence for varying quark and gluon jet contributions to high-p[subscript T] hadron yields. The relative hadron abundances in Au+Au at p[subscript T]≳8  GeV/c are measured to be similar to the p+p results, despite the expected Casimir effect for parton energy loss.
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/1721.1/78678
DOI of Published Version
https://doi.org/10.1103/PhysRevLett.108.072302
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.