Pion-Kaon Correlations in Central Au + Au Collisions at √SNN= 130 GeV

STAR Collaboration

Pion-Kaon Correlations in Central Au + Au Collisions at √S_NN= 130 GeV

STAR Collaboration

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

56 Citas (Scopus)

Resumen

Pion-kaon correlation functions are constructed from central Au + Au STAR data taken at √s_NN = 130 GeV by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The results suggest that pions and kaons are not emitted at the same average space-time point. Space-momentum correlations, i.e., transverse flow, lead to a space-time emission asymmetry of pions and kaons that is consistent with the data. This result provides new independent evidence that the system created at RHIC undergoes a collective transverse expansion.

Idioma original	Inglés
Número de artículo	262302
Páginas (desde-hasta)	2623021-2623026
Número de páginas	6
Publicación	Physical Review Letters
Volumen	91
N.º	26 I
Estado	Publicada - 31 dic. 2003
Publicado de forma externa	Sí

Otros archivos y enlaces

Enlace a la publicación en Scopus

Citar esto

@article{cb391d0d57bf48a4b5fe3d159a96b654,

title = "Pion-Kaon Correlations in Central Au + Au Collisions at √SNN= 130 GeV",

abstract = "Pion-kaon correlation functions are constructed from central Au + Au STAR data taken at √sNN = 130 GeV by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The results suggest that pions and kaons are not emitted at the same average space-time point. Space-momentum correlations, i.e., transverse flow, lead to a space-time emission asymmetry of pions and kaons that is consistent with the data. This result provides new independent evidence that the system created at RHIC undergoes a collective transverse expansion.",

author = "J. Adams and C. Adler and Aggarwal, \{M. M.\} and Z. Ahammed and S. Kabana and \{STAR Collaboration\}",

note = "Publisher Copyright: {\textcopyright} 2003 The American Physical Society.",

year = "2003",

month = dec,

day = "31",

language = "English",

volume = "91",

pages = "2623021--2623026",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "26 I",

}

TY - JOUR

T1 - Pion-Kaon Correlations in Central Au + Au Collisions at √SNN= 130 GeV

AU - Adams, J.

AU - Adler, C.

AU - Aggarwal, M. M.

AU - Ahammed, Z.

AU - Kabana, S.

AU - STAR Collaboration

PY - 2003/12/31

Y1 - 2003/12/31

N2 - Pion-kaon correlation functions are constructed from central Au + Au STAR data taken at √sNN = 130 GeV by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The results suggest that pions and kaons are not emitted at the same average space-time point. Space-momentum correlations, i.e., transverse flow, lead to a space-time emission asymmetry of pions and kaons that is consistent with the data. This result provides new independent evidence that the system created at RHIC undergoes a collective transverse expansion.

AB - Pion-kaon correlation functions are constructed from central Au + Au STAR data taken at √sNN = 130 GeV by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The results suggest that pions and kaons are not emitted at the same average space-time point. Space-momentum correlations, i.e., transverse flow, lead to a space-time emission asymmetry of pions and kaons that is consistent with the data. This result provides new independent evidence that the system created at RHIC undergoes a collective transverse expansion.

UR - https://www.scopus.com/pages/publications/1842553443

M3 - Article

AN - SCOPUS:1842553443

SN - 0031-9007

VL - 91

SP - 2623021

EP - 2623026

JO - Physical Review Letters

JF - Physical Review Letters

IS - 26 I

M1 - 262302

ER -

Pion-Kaon Correlations in Central Au + Au Collisions at √SNN= 130 GeV

Resumen

Otros archivos y enlaces

Huella

Citar esto

Pion-Kaon Correlations in Central Au + Au Collisions at √S_NN= 130 GeV