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Peter Christiansen Profile

Peter Christiansen

Professor

Peter Christiansen Profile

Azimuthal-Angle Dependence of Charged-Pion-Interferometry Measurements with Respect to Second- and Third-Order Event Planes in Au+Au Collisions at sqrt[s_{NN}]=200 GeV.

Author

  • A Adare
  • S Afanasiev
  • C Aidala
  • N N Ajitanand
  • Y Akiba
  • H Al-Bataineh
  • J Alexander
  • K Aoki
  • Y Aramaki
  • E T Atomssa
  • R Averbeck
  • T C Awes
  • B Azmoun
  • V Babintsev
  • M Bai
  • G Baksay
  • L Baksay
  • K N Barish
  • B Bassalleck
  • A T Basye
  • S Bathe
  • V Baublis
  • C Baumann
  • A Bazilevsky
  • S Belikov
  • R Belmont
  • R Bennett
  • A Berdnikov
  • Y Berdnikov
  • A A Bickley
  • J S Bok
  • K Boyle
  • M L Brooks
  • H Buesching
  • V Bumazhnov
  • G Bunce
  • S Butsyk
  • C M Camacho
  • S Campbell
  • C-H Chen
  • C Y Chi
  • M Chiu
  • I J Choi
  • R K Choudhury
  • Peter Christiansen
  • T Chujo
  • P Chung
  • O Chvala
  • V Cianciolo
  • Z Citron
  • B A Cole
  • M Connors
  • P Constantin
  • M Csanád
  • T Csörgő
  • T Dahms
  • S Dairaku
  • I Danchev
  • K Das
  • A Datta
  • G David
  • A Denisov
  • A Deshpande
  • E J Desmond
  • O Dietzsch
  • A Dion
  • M Donadelli
  • O Drapier
  • A Drees
  • K A Drees
  • J M Durham
  • A Durum
  • D Dutta
  • S Edwards
  • Y V Efremenko
  • F Ellinghaus
  • T Engelmore
  • A Enokizono
  • H En'yo
  • S Esumi
  • B Fadem
  • D E Fields
  • M Finger
  • M Finger
  • F Fleuret
  • S L Fokin
  • Z Fraenkel
  • J E Frantz
  • A Franz
  • A D Frawley
  • K Fujiwara
  • Y Fukao
  • T Fusayasu
  • I Garishvili
  • A Glenn
  • H Gong
  • M Gonin
  • Y Goto
  • R Granier de Cassagnac
  • N Grau
  • S V Greene
  • M Grosse Perdekamp
  • T Gunji
  • Hans-Åke Gustafsson
  • J S Haggerty
  • K I Hahn
  • H Hamagaki
  • J Hamblen
  • R Han
  • J Hanks
  • E P Hartouni
  • Eva Haslum
  • R Hayano
  • X He
  • M Heffner
  • T K Hemmick
  • T Hester
  • J C Hill
  • M Hohlmann
  • W Holzmann
  • K Homma
  • B Hong
  • T Horaguchi
  • D Hornback
  • S Huang
  • T Ichihara
  • R Ichimiya
  • J Ide
  • Y Ikeda
  • K Imai
  • M Inaba
  • D Isenhower
  • M Ishihara
  • T Isobe
  • M Issah
  • A Isupov
  • D Ivanischev
  • B V Jacak
  • J Jia
  • J Jin
  • B M Johnson
  • K S Joo
  • D Jouan
  • D S Jumper
  • F Kajihara
  • S Kametani
  • N Kamihara
  • J Kamin
  • J H Kang
  • J Kapustinsky
  • K Karatsu
  • D Kawall
  • M Kawashima
  • A V Kazantsev
  • T Kempel
  • A Khanzadeev
  • K M Kijima
  • B I Kim
  • D H Kim
  • D J Kim
  • E Kim
  • E-J Kim
  • S H Kim
  • Y-J Kim
  • E Kinney
  • K Kiriluk
  • A Kiss
  • E Kistenev
  • L Kochenda
  • B Komkov
  • M Konno
  • J Koster
  • D Kotchetkov
  • A Kozlov
  • A Král
  • A Kravitz
  • G J Kunde
  • K Kurita
  • M Kurosawa
  • Y Kwon
  • G S Kyle
  • R Lacey
  • Y S Lai
  • J G Lajoie
  • A Lebedev
  • D M Lee
  • J Lee
  • K Lee
  • K B Lee
  • K S Lee
  • M J Leitch
  • M A L Leite
  • E Leitner
  • B Lenzi
  • X Li
  • P Liebing
  • L A Linden Levy
  • T Liška
  • A Litvinenko
  • H Liu
  • M X Liu
  • B Love
  • R Luechtenborg
  • D Lynch
  • C F Maguire
  • Y I Makdisi
  • A Malakhov
  • M D Malik
  • V I Manko
  • E Mannel
  • Y Mao
  • H Masui
  • F Matathias
  • M McCumber
  • P L McGaughey
  • N Means
  • B Meredith
  • Y Miake
  • A C Mignerey
  • P Mikeš
  • K Miki
  • A Milov
  • M Mishra
  • J T Mitchell
  • A K Mohanty
  • Y Morino
  • A Morreale
  • D P Morrison
  • T V Moukhanova
  • J Murata
  • S Nagamiya
  • J L Nagle
  • M Naglis
  • M I Nagy
  • I Nakagawa
  • Y Nakamiya
  • T Nakamura
  • K Nakano
  • J Newby
  • M Nguyen
  • T Niida
  • R Nouicer
  • A S Nyanin
  • E O'Brien
  • S X Oda
  • C A Ogilvie
  • M Oka
  • K Okada
  • Y Onuki
  • Anders Oskarsson
  • M Ouchida
  • K Ozawa
  • R Pak
  • V Pantuev
  • V Papavassiliou
  • I H Park
  • J Park
  • S K Park
  • W J Park
  • S F Pate
  • H Pei
  • J-C Peng
  • H Pereira
  • V Peresedov
  • D Yu Peressounko
  • C Pinkenburg
  • R P Pisani
  • M Proissl
  • M L Purschke
  • A K Purwar
  • H Qu
  • J Rak
  • A Rakotozafindrabe
  • I Ravinovich
  • K F Read
  • K Reygers
  • V Riabov
  • Y Riabov
  • E Richardson
  • D Roach
  • G Roche
  • S D Rolnick
  • M Rosati
  • C A Rosen
  • Sarah Rosendahl
  • P Rosnet
  • P Rukoyatkin
  • P Ružička
  • B Sahlmueller
  • N Saito
  • T Sakaguchi
  • K Sakashita
  • V Samsonov
  • S Sano
  • T Sato
  • S Sawada
  • K Sedgwick
  • J Seele
  • R Seidl
  • A Yu Semenov
  • R Seto
  • D Sharma
  • I Shein
  • T-A Shibata
  • K Shigaki
  • M Shimomura
  • K Shoji
  • P Shukla
  • A Sickles
  • C L Silva
  • D Silvermyr
  • C Silvestre
  • K S Sim
  • B K Singh
  • C P Singh
  • V Singh
  • M Slunečka
  • R A Soltz
  • W E Sondheim
  • S P Sorensen
  • I V Sourikova
  • N A Sparks
  • P W Stankus
  • Evert Stenlund
  • S P Stoll
  • T Sugitate
  • A Sukhanov
  • J Sziklai
  • E M Takagui
  • A Taketani
  • R Tanabe
  • Y Tanaka
  • K Tanida
  • M J Tannenbaum
  • S Tarafdar
  • A Taranenko
  • P Tarján
  • H Themann
  • T L Thomas
  • T Todoroki
  • M Togawa
  • A Toia
  • L Tomášek
  • H Torii
  • R S Towell
  • I Tserruya
  • Y Tsuchimoto
  • C Vale
  • H Valle
  • H W van Hecke
  • E Vazquez-Zambrano
  • A Veicht
  • J Velkovska
  • R Vértesi
  • A A Vinogradov
  • M Virius
  • V Vrba
  • E Vznuzdaev
  • X R Wang
  • D Watanabe
  • K Watanabe
  • Y Watanabe
  • F Wei
  • R Wei
  • J Wessels
  • S N White
  • D Winter
  • J P Wood
  • C L Woody
  • R M Wright
  • M Wysocki
  • W Xie
  • Y L Yamaguchi
  • K Yamaura
  • R Yang
  • A Yanovich
  • J Ying
  • S Yokkaichi
  • Z You
  • G R Young
  • I Younus
  • I E Yushmanov
  • W A Zajc
  • C Zhang
  • S Zhou
  • L Zolin

Summary, in English

Charged-pion-interferometry measurements were made with respect to the second- and third-order event plane for Au+Au collisions at sqrt[s_{NN}]=200 GeV. A strong azimuthal-angle dependence of the extracted Gaussian-source radii was observed with respect to both the second- and third-order event planes. The results for the second-order dependence indicate that the initial eccentricity is reduced during the medium evolution, which is consistent with previous results. In contrast, the results for the third-order dependence indicate that the initial triangular shape is significantly reduced and potentially reversed by the end of the medium evolution, and that the third-order oscillations are largely dominated by the dynamical effects from triangular flow.

Department/s

  • Particle and nuclear physics

Publishing year

2014

Language

English

Publication/Series

Physical Review Letters

Volume

112

Issue

22

Document type

Journal article

Publisher

American Physical Society

Topic

  • Subatomic Physics

Status

Published

ISBN/ISSN/Other

  • ISSN: 1079-7114