skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Azimuthal anisotropy in U+U collisions at STAR

Journal Article · · Nuclear Physics. A

The azimuthal anisotropy of particle production is commonly used in high-energy nuclear collisions to study the early evolution of the expanding system. The prolate shape of uranium nuclei makes it possible to study how the geometry of the colliding nuclei affects final state anisotropies. It also provides a unique opportunity to understand how entropy is produced in heavy ion collisions. In this paper, the two- and four- particle cumulant v2 (v2{2} and v2{4}) from U+U collisions at √sNN = 193 GeV and Au+Au collisions at √sNN = 200 GeV for inclusive charged hadrons will be presented. The STAR Zero Degree Calorimeters are used to select very central collisions. Differences were observed between the multiplicity dependence of v2{2} for most central Au+Au and U+U collisions. The multiplicity dependence of v2{2} in central collisions were compared to Monte Carlo Glauber model predictions and it was seen that this model cannot explain the present results. (auth)

Research Organization:
Brookhaven National Lab. (BNL), Upton, NY (United States). Relativistic Heavy Ion Collider (RHIC)
Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP)
Contributing Organization:
STAR Collaboration
Grant/Contract Number:
SC00112704
OSTI ID:
1174122
Report Number(s):
BNL-107560-2015-JA; R&D Project: PO 004; KB0202012
Journal Information:
Nuclear Physics. A, Vol. 932, Issue 1-2; ISSN 0375-9474
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 8 works
Citation information provided by
Web of Science

References (8)

Experimental and theoretical challenges in the search for the quark–gluon plasma: The STAR Collaboration's critical assessment of the evidence from RHIC collisions journal August 2005
Multiplicity distribution and source deformation in full-overlap U + U collisions journal September 2005
Flow analysis with cumulants: Direct calculations journal April 2011
Energy and system-size dependence of two- and four-particle v 2 measurements in heavy-ion collisions at s N N = 62.4 and 200 GeV and their implications on flow fluctuations and nonflow journal July 2012
Testing the Chiral Magnetic Effect with Central U + U Collisions journal October 2010
Influence of initial fluctuations on geometry measures in relativistic U+U and Cu+Au collisions journal April 2013
Predictions of Elliptic flow and nuclear modification factor from 200 GeV <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mi mathvariant="normal">U</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:math> collisions at RHIC journal September 2009
Anisotropic Flow and Jet Quenching in Ultrarelativistic U + U Collisions journal April 2005

Cited By (2)


Similar Records

Azimuthal anisotophy in U + U and Au + Au collisions at RHIC
Journal Article · Tue Nov 24 00:00:00 EST 2015 · Physical Review Letters · OSTI ID:1174122

Systematic study of azimuthal anisotropy in Cu + Cu and Au + Au collisions at √sNN = 62.4 and 200 GeV
Journal Article · Wed Sep 23 00:00:00 EDT 2015 · Physical Review. C. Nuclear Physics · OSTI ID:1174122

Particle-type dependence of azimuthal anisotropy and nuclearmodification of particle production in Au+Au collisions at sNN = 200GeV
Journal Article · Wed Jun 18 00:00:00 EDT 2003 · Physical Review Letters · OSTI ID:1174122