Loading…

Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR

Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the reson...

Full description

Saved in:
Bibliographic Details
Published in:Nuclear physics. A 2019-02, Vol.982 (C), p.535-538
Main Author: Zhao, Jie
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823
cites cdi_FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823
container_end_page 538
container_issue C
container_start_page 535
container_title Nuclear physics. A
container_volume 982
creator Zhao, Jie
description Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv>1.5GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv
doi_str_mv 10.1016/j.nuclphysa.2018.08.035
format article
fullrecord <record><control><sourceid>elsevier_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1580374</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0375947418301799</els_id><sourcerecordid>S0375947418301799</sourcerecordid><originalsourceid>FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823</originalsourceid><addsrcrecordid>eNqFUF1LwzAU7YOCc_obDL5Ka9I2a_tYhl8wEXT6Gu7SmzWzS0aSKvv3Zkx89XLgPtzzwT1JcsVoxiib3W4yM8ph1-89ZDlldUYjCn6STGhR8bQpq_IsOfd-Q-PMKJ0k_TOCHx1u0QRPrCKhRyJ77WAgW1gbDFoSVAplIN869GQF8nPt7Gg6or0dIGhriDYkp5Q84Adpx5t2JNIOg_bx5AkE8rZsXy-SUwWDx8vfPU3e7--W88d08fLwNG8XqSwLHtK8rpuyA4momKoaBpRzwDxXDTDelLyCqu5gVq06uWpquYIyLzlXoGRBq1mdF9Pk-uhrfdDCSx1Q9tIaEz8QjNexiDKSqiNJOuu9QyV2Tm_B7QWj4tCk2Ii_JsWhSUEjCh6V7VGJ8Ycvje4QgUZip90hobP6X48fJtGDjA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR</title><source>ScienceDirect Journals</source><creator>Zhao, Jie</creator><creatorcontrib>Zhao, Jie ; STAR collaboration ; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><description>Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv&gt;1.5GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv&lt;1.5GeV/c2), resonance peaks are observed in Δγ(minv). An event shape engineering (ESE) method is used to model the background shape in minv to extract the potential CME signal at low minv. In the comparative method, the ΨRP is assessed by spectator neutrons measured by the ZDCs, and the ΨPP by the 2nd-harmonic event plane measured by the TPC. The ν2 is stronger along ΨPP and weaker along ΨRP; in contrast, the magnetic field, mainly from spectator protons, is weaker along ΨPP and stronger along ΨRP. As a result, the Δγ measured with respect to ΨRP and ΨPP contain different amounts of CME and background, and can thus determine these two contributions. It is found that the possible CME signals with background isolation by these two novel methods are small, on the order of a few percent of the inclusive Δγ measurements.</description><identifier>ISSN: 0375-9474</identifier><identifier>DOI: 10.1016/j.nuclphysa.2018.08.035</identifier><language>eng</language><publisher>United States: Elsevier B.V</publisher><subject>chiral magnetic effect ; heavy-ion collisions ; invariant mass ; NUCLEAR PHYSICS AND RADIATION PHYSICS ; participant plane ; QCD ; reaction plane</subject><ispartof>Nuclear physics. A, 2019-02, Vol.982 (C), p.535-538</ispartof><rights>2018 The Authors</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823</citedby><cites>FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823</cites><orcidid>0000-0001-6408-2314 ; 0000000164082314</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27903,27904</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1580374$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Zhao, Jie</creatorcontrib><creatorcontrib>STAR collaboration</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><title>Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR</title><title>Nuclear physics. A</title><description>Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv&gt;1.5GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv&lt;1.5GeV/c2), resonance peaks are observed in Δγ(minv). An event shape engineering (ESE) method is used to model the background shape in minv to extract the potential CME signal at low minv. In the comparative method, the ΨRP is assessed by spectator neutrons measured by the ZDCs, and the ΨPP by the 2nd-harmonic event plane measured by the TPC. The ν2 is stronger along ΨPP and weaker along ΨRP; in contrast, the magnetic field, mainly from spectator protons, is weaker along ΨPP and stronger along ΨRP. As a result, the Δγ measured with respect to ΨRP and ΨPP contain different amounts of CME and background, and can thus determine these two contributions. It is found that the possible CME signals with background isolation by these two novel methods are small, on the order of a few percent of the inclusive Δγ measurements.</description><subject>chiral magnetic effect</subject><subject>heavy-ion collisions</subject><subject>invariant mass</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>participant plane</subject><subject>QCD</subject><subject>reaction plane</subject><issn>0375-9474</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNqFUF1LwzAU7YOCc_obDL5Ka9I2a_tYhl8wEXT6Gu7SmzWzS0aSKvv3Zkx89XLgPtzzwT1JcsVoxiib3W4yM8ph1-89ZDlldUYjCn6STGhR8bQpq_IsOfd-Q-PMKJ0k_TOCHx1u0QRPrCKhRyJ77WAgW1gbDFoSVAplIN869GQF8nPt7Gg6or0dIGhriDYkp5Q84Adpx5t2JNIOg_bx5AkE8rZsXy-SUwWDx8vfPU3e7--W88d08fLwNG8XqSwLHtK8rpuyA4momKoaBpRzwDxXDTDelLyCqu5gVq06uWpquYIyLzlXoGRBq1mdF9Pk-uhrfdDCSx1Q9tIaEz8QjNexiDKSqiNJOuu9QyV2Tm_B7QWj4tCk2Ii_JsWhSUEjCh6V7VGJ8Ycvje4QgUZip90hobP6X48fJtGDjA</recordid><startdate>20190201</startdate><enddate>20190201</enddate><creator>Zhao, Jie</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-6408-2314</orcidid><orcidid>https://orcid.org/0000000164082314</orcidid></search><sort><creationdate>20190201</creationdate><title>Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR</title><author>Zhao, Jie</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>chiral magnetic effect</topic><topic>heavy-ion collisions</topic><topic>invariant mass</topic><topic>NUCLEAR PHYSICS AND RADIATION PHYSICS</topic><topic>participant plane</topic><topic>QCD</topic><topic>reaction plane</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zhao, Jie</creatorcontrib><creatorcontrib>STAR collaboration</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Nuclear physics. A</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhao, Jie</au><aucorp>STAR collaboration</aucorp><aucorp>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR</atitle><jtitle>Nuclear physics. A</jtitle><date>2019-02-01</date><risdate>2019</risdate><volume>982</volume><issue>C</issue><spage>535</spage><epage>538</epage><pages>535-538</pages><issn>0375-9474</issn><abstract>Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv&gt;1.5GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv&lt;1.5GeV/c2), resonance peaks are observed in Δγ(minv). An event shape engineering (ESE) method is used to model the background shape in minv to extract the potential CME signal at low minv. In the comparative method, the ΨRP is assessed by spectator neutrons measured by the ZDCs, and the ΨPP by the 2nd-harmonic event plane measured by the TPC. The ν2 is stronger along ΨPP and weaker along ΨRP; in contrast, the magnetic field, mainly from spectator protons, is weaker along ΨPP and stronger along ΨRP. As a result, the Δγ measured with respect to ΨRP and ΨPP contain different amounts of CME and background, and can thus determine these two contributions. It is found that the possible CME signals with background isolation by these two novel methods are small, on the order of a few percent of the inclusive Δγ measurements.</abstract><cop>United States</cop><pub>Elsevier B.V</pub><doi>10.1016/j.nuclphysa.2018.08.035</doi><tpages>4</tpages><orcidid>https://orcid.org/0000-0001-6408-2314</orcidid><orcidid>https://orcid.org/0000000164082314</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0375-9474
ispartof Nuclear physics. A, 2019-02, Vol.982 (C), p.535-538
issn 0375-9474
language eng
recordid cdi_osti_scitechconnect_1580374
source ScienceDirect Journals
subjects chiral magnetic effect
heavy-ion collisions
invariant mass
NUCLEAR PHYSICS AND RADIATION PHYSICS
participant plane
QCD
reaction plane
title Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-23T11%3A57%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Measurements%20of%20the%20chiral%20magnetic%20effect%20with%20background%20isolation%20in%20200%20GeV%20Au+Au%20collisions%20at%20STAR&rft.jtitle=Nuclear%20physics.%20A&rft.au=Zhao,%20Jie&rft.aucorp=STAR%20collaboration&rft.date=2019-02-01&rft.volume=982&rft.issue=C&rft.spage=535&rft.epage=538&rft.pages=535-538&rft.issn=0375-9474&rft_id=info:doi/10.1016/j.nuclphysa.2018.08.035&rft_dat=%3Celsevier_osti_%3ES0375947418301799%3C/elsevier_osti_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c435t-28894daceef1f791a055ae22f9a159457a78da67bdcb98cba42455fafc3076823%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true