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Wei Xie

Researcher at Purdue University

Publications -  1527
Citations -  87958

Wei Xie is an academic researcher from Purdue University. The author has contributed to research in topics: Large Hadron Collider & Lepton. The author has an hindex of 128, co-authored 1281 publications receiving 77097 citations. Previous affiliations of Wei Xie include University of Trento & Purdue University Calumet.

Papers
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Dielectron Mass Spectra from Au+Au Collisions at $\sqrt{s_{\rm NN}}$ = 200 GeV

Leszek Adamczyk, +349 more
TL;DR: In this paper, the STAR measurements of dielectron production at midrapidity ( | y e e | 1 ) in Au + Au collisions at s N N = 200 GeV are evaluated in different invariant mass regions with a focus on 0.30-0.76 ( ρ -like), 0.76 −0.80 ( ω-like), and 0.98 −1.05 ( ϕ -like) GeV / c 2.
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Measurement of differential cross sections for the production of a pair of isolated photons in pp collisions at √s=7TeV

S. Chatrchyan, +2212 more
TL;DR: In this article, a measurement of differential cross sections for the production of a pair of isolated photons in proton-proton collisions at squarert(s) = 7 TeV is presented.
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A search for the standard model Higgs boson decaying to charm quarks

Albert M. Sirunyan, +2363 more
TL;DR: In this article, a direct search for the standard model Higgs boson produced in association with a vector boson, V (W or Z), and decaying to a charm quark pair is presented.
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Measurement of the Higgs boson production rate in association with top quarks in final states with electrons, muons, and hadronically decaying tau leptons at √s=13Te

Albert M. Sirunyan, +2410 more
TL;DR: The most sensitive measurement of the Higgs boson coupling to the tau lepton was obtained in this paper, where the authors used machine learning techniques and matrix-element methods.
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Jet-hadron correlations in sNN =200GeV p+p and central Au+Au collisions

Leszek Adamczyk, +352 more
TL;DR: Azimuthal angular correlations of charged hadrons with respect to the axis of a reconstructed (trigger) jet in Au+Au and p+p collisions at √[s(NN)]=200 GeV in STAR are presented in this article.