Measurements of W and Z/γ∗ cross sections and their ratios in p+p collisions at RHIC

We report on the W and Z/γ∗ differential and total cross sections as well as the W+/W− and (WW−)/(Z/γ∗) cross section ratios measured by the STAR experiment at RHIC in p+p collisions at √s=500 GeV and 510 GeV. The cross sections and their ratios are sensitive to quark and antiquark parton distributi...

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Bibliographic Details
Main Authors: Adam, Jaroslav (Author) , Deppner, Ingo Martin (Author) , Herrmann, Norbert (Author)
Corporate Author: STAR Collaboration (Author)
Format: Article (Journal)
Language:English
Published: 4 January 2021
In: Physical review
Year: 2021, Volume: 103, Issue: 1
ISSN:2470-0029
DOI:10.1103/PhysRevD.103.012001
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevD.103.012001
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.103.012001
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Author Notes:J. Adam, I.M. Deppner, N. Herrmann [und viele weitere] (STAR Collaboration)
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Summary:We report on the W and Z/γ∗ differential and total cross sections as well as the W+/W− and (WW−)/(Z/γ∗) cross section ratios measured by the STAR experiment at RHIC in p+p collisions at √s=500 GeV and 510 GeV. The cross sections and their ratios are sensitive to quark and antiquark parton distribution functions. In particular, at leading order, the W cross section ratio is sensitive to the ¯d/¯u ratio. These measurements were taken at high Q2∼M2W,M2Z and can serve as input into global analyses to provide constraints on the sea quark distributions. The results presented here combine three STAR datasets from 2011, 2012, and 2013, accumulating an integrated luminosity of 350 pb−1. We also assess the expected impact that our W+/W− cross section ratios will have on various quark distributions, and find sensitivity to the ¯u−¯d and ¯d/¯u distributions.
Item Description:Gesehen am 18.02.2021
Im Titel ist der griechische Buchstabe "ast" als Tropfensternchen (englisch: teardrop-spoked asterisk) dargestellt
Physical Description:Online Resource
ISSN:2470-0029
DOI:10.1103/PhysRevD.103.012001