Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt sNN=200 GeV

S S Adler; S Afanasiev; C Aidala; N N Ajitanand; Y Akiba; J Alexander; R Amirikas; L Aphecetche; S H Aronson; R Averbeck; T C Awes; R Azmoun; V Babintsev; A Baldisseri; K N Barish; P D Barnes; B Bassalleck; S Bathe; S Batsouli; V Baublis; A Bazilevsky; S Belikov; Y Berdnikov; S Bhagavatula; J G Boissevain; H Borel; S Borenstein; M L Brooks; D S Brown; N Bruner; D Bucher; H Buesching; V Bumazhnov; G Bunce; J M Burward-Hoy; S Butsyk; X Camard; J-S Chai; P Chand; W C Chang; S Chernichenko; C Y Chi; J Chiba; M Chiu; I J Choi; J Choi; R K Choudhury; T Chujo; P Chung; V Cianciolo; Y Cobigo; B A Cole; P Constantin; M Csanád; T Csörgo; D d'Enterria; G David; H Delagrange; A Denisov; A Deshpande; E J Desmond; A Devismes; O Dietzsch; O Drapier; A Drees; R du Rietz; A Durum; D Dutta; Y V Efremenko; K El Chenawi; A Enokizono; H En'yo; S Esumi; L Ewell; D E Fields; F Fleuret; S L Fokin; B D Fox; Z Fraenkel; J E Frantz; A Franz; A D Frawley; S-Y Fung; S Garpman; T K Ghosh; A Glenn; G Gogiberidze; M Gonin; J Gosset; Y Goto; R Granier de Cassagnac; N Grau; S V Greene; M Grosse Perdekamp; W Guryn; H-A Gustafsson; T Hachiya; J S Haggerty; H Hamagaki; A G Hansen; E P Hartouni; M Harvey; R Hayano; N Hayashi; X He; M Heffner; T K Hemmick; J M Heuser; M Hibino; J C Hill; W Holzmann; K Homma; B Hong; A Hoover; T Ichihara; V V Ikonnikov; K Imai; D Isenhower; M Ishihara; M Issah; A Isupov; B V Jacak; W Y Jang; Y Jeong; J Jia; O Jinnouchi; B M Johnson; S C Johnson; K S Joo; D Jouan; S Kametani; N Kamihara; J H Kang; S S Kapoor; K Katou; S Kelly; B Khachaturov; A Khanzadeev; J Kikuchi; D H Kim; D J Kim; D W Kim; E Kim; G-B Kim; H J Kim; E Kistenev; A Kiyomichi; K Kiyoyama; C Klein-Boesing; H Kobayashi; L Kochenda; V Kochetkov; D Koehler; T Kohama; M Kopytine; D Kotchetkov; A Kozlov; P J Kroon; C H Kuberg; K Kurita; Y Kuroki; M J Kweon; Y Kwon; G S Kyle; R Lacey; V Ladygin; J G Lajoie; A Lebedev; S Leckey; D M Lee; S Lee; M J Leitch; X H Li; H Lim; A Litvinenko; M X Liu; Y Liu; C F Maguire; Y I Makdisi; A Malakhov; V I Manko; Y Mao; G Martinez; M D Marx; H Masui; F Matathias; T Matsumoto; P L McGaughey; E Melnikov; F Messer; Y Miake; J Milan; T E Miller; A Milov; S Mioduszewski; R E Mischke; G C Mishra; J T Mitchell; A K Mohanty; D P Morrison; J M Moss; F Mühlbacher; D Mukhopadhyay; M Muniruzzaman; J Murata; S Nagamiya; J L Nagle; M Nagy; T Nakamura; B K Nandi; M Nara; J Newby; P Nilsson; A S Nyanin; J Nystrand; E O'Brien; C A Ogilvie; H Ohnishi; I D Ojha; K Okada; M Ono; V Onuchin; A Oskarsson; I Otterlund; K Oyama; K Ozawa; D Pal; A P T Palounek; V Pantuev; V Papavassiliou; J Park; A Parmar; S F Pate; T Peitzmann; J-C Peng; V Peresedov; C Pinkenburg; R P Pisani; F Plasil; M L Purschke; A K Purwar; J Rak; I Ravinovich; K F Read; M Reuter; K Reygers; V Riabov; Y Riabov; G Roche; A Romana; M Rosati; P Rosnet; S S Ryu; M E Sadler; N Saito; T Sakaguchi; M Sakai; S Sakai; V Samsonov; L Sanfratello; R Santo; H D Sato; S Sato; S Sawada; Y Schutz; V Semenov; R Seto; M R Shaw; T K Shea; T-A Shibata; K Shigaki; T Shiina; C L Silva; D Silvermyr; K S Sim; C P Singh; V Singh; M Sivertz; A Soldatov; R A Soltz; W E Sondheim; S P Sorensen; I V Sourikova; F Staley; P W Stankus; E Stenlund; M Stepanov; A Ster; S P Stoll; T Sugitate; J P Sullivan; E M Takagui; A Taketani; M Tamai; K H Tanaka; Y Tanaka; K Tanida; M J Tannenbaum; A Taranenko; P Tarján; J D Tepe; T L Thomas; J Tojo; H Torii; R S Towell; I Tserruya; H Tsuruoka; S K Tuli; H Tydesjö; N Tyurin; H W van Hecke; J Velkovska; M Velkovsky; V Veszprémi; L Villatte; A A Vinogradov; M A Volkov; E Vznuzdaev; X R Wang; Y Watanabe; S N White; F K Wohn; C L Woody; W Xie; Y Yang; A Yanovich; S Yokkaichi; G R Young; I E Yushmanov; W A Zajc; C Zhang; S Zhou; S J Zhou; L Zolin

doi:10.1103/PhysRevLett.98.132301

Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt sNN=200 GeV

Phys Rev Lett. 2007 Mar 30;98(13):132301. doi: 10.1103/PhysRevLett.98.132301. Epub 2007 Mar 26.

Authors

S S Adler¹, S Afanasiev, C Aidala, N N Ajitanand, Y Akiba, J Alexander, R Amirikas, L Aphecetche, S H Aronson, R Averbeck, T C Awes, R Azmoun, V Babintsev, A Baldisseri, K N Barish, P D Barnes, B Bassalleck, S Bathe, S Batsouli, V Baublis, A Bazilevsky, S Belikov, Y Berdnikov, S Bhagavatula, J G Boissevain, H Borel, S Borenstein, M L Brooks, D S Brown, N Bruner, D Bucher, H Buesching, V Bumazhnov, G Bunce, J M Burward-Hoy, S Butsyk, X Camard, J-S Chai, P Chand, W C Chang, S Chernichenko, C Y Chi, J Chiba, M Chiu, I J Choi, J Choi, R K Choudhury, T Chujo, P Chung, V Cianciolo, Y Cobigo, B A Cole, P Constantin, M Csanád, T Csörgo, D d'Enterria, G David, H Delagrange, A Denisov, A Deshpande, E J Desmond, A Devismes, O Dietzsch, O Drapier, A Drees, R du Rietz, A Durum, D Dutta, Y V Efremenko, K El Chenawi, A Enokizono, H En'yo, S Esumi, L Ewell, D E Fields, F Fleuret, S L Fokin, B D Fox, Z Fraenkel, J E Frantz, A Franz, A D Frawley, S-Y Fung, S Garpman, T K Ghosh, A Glenn, G Gogiberidze, M Gonin, J Gosset, Y Goto, R Granier de Cassagnac, N Grau, S V Greene, M Grosse Perdekamp, W Guryn, H-A Gustafsson, T Hachiya, J S Haggerty, H Hamagaki, A G Hansen, E P Hartouni, M Harvey, R Hayano, N Hayashi, X He, M Heffner, T K Hemmick, J M Heuser, M Hibino, J C Hill, W Holzmann, K Homma, B Hong, A Hoover, T Ichihara, V V Ikonnikov, K Imai, D Isenhower, M Ishihara, M Issah, A Isupov, B V Jacak, W Y Jang, Y Jeong, J Jia, O Jinnouchi, B M Johnson, S C Johnson, K S Joo, D Jouan, S Kametani, N Kamihara, J H Kang, S S Kapoor, K Katou, S Kelly, B Khachaturov, A Khanzadeev, J Kikuchi, D H Kim, D J Kim, D W Kim, E Kim, G-B Kim, H J Kim, E Kistenev, A Kiyomichi, K Kiyoyama, C Klein-Boesing, H Kobayashi, L Kochenda, V Kochetkov, D Koehler, T Kohama, M Kopytine, D Kotchetkov, A Kozlov, P J Kroon, C H Kuberg, K Kurita, Y Kuroki, M J Kweon, Y Kwon, G S Kyle, R Lacey, V Ladygin, J G Lajoie, A Lebedev, S Leckey, D M Lee, S Lee, M J Leitch, X H Li, H Lim, A Litvinenko, M X Liu, Y Liu, C F Maguire, Y I Makdisi, A Malakhov, V I Manko, Y Mao, G Martinez, M D Marx, H Masui, F Matathias, T Matsumoto, P L McGaughey, E Melnikov, F Messer, Y Miake, J Milan, T E Miller, A Milov, S Mioduszewski, R E Mischke, G C Mishra, J T Mitchell, A K Mohanty, D P Morrison, J M Moss, F Mühlbacher, D Mukhopadhyay, M Muniruzzaman, J Murata, S Nagamiya, J L Nagle, M Nagy, T Nakamura, B K Nandi, M Nara, J Newby, P Nilsson, A S Nyanin, J Nystrand, E O'Brien, C A Ogilvie, H Ohnishi, I D Ojha, K Okada, M Ono, V Onuchin, A Oskarsson, I Otterlund, K Oyama, K Ozawa, D Pal, A P T Palounek, V Pantuev, V Papavassiliou, J Park, A Parmar, S F Pate, T Peitzmann, J-C Peng, V Peresedov, C Pinkenburg, R P Pisani, F Plasil, M L Purschke, A K Purwar, J Rak, I Ravinovich, K F Read, M Reuter, K Reygers, V Riabov, Y Riabov, G Roche, A Romana, M Rosati, P Rosnet, S S Ryu, M E Sadler, N Saito, T Sakaguchi, M Sakai, S Sakai, V Samsonov, L Sanfratello, R Santo, H D Sato, S Sato, S Sawada, Y Schutz, V Semenov, R Seto, M R Shaw, T K Shea, T-A Shibata, K Shigaki, T Shiina, C L Silva, D Silvermyr, K S Sim, C P Singh, V Singh, M Sivertz, A Soldatov, R A Soltz, W E Sondheim, S P Sorensen, I V Sourikova, F Staley, P W Stankus, E Stenlund, M Stepanov, A Ster, S P Stoll, T Sugitate, J P Sullivan, E M Takagui, A Taketani, M Tamai, K H Tanaka, Y Tanaka, K Tanida, M J Tannenbaum, A Taranenko, P Tarján, J D Tepe, T L Thomas, J Tojo, H Torii, R S Towell, I Tserruya, H Tsuruoka, S K Tuli, H Tydesjö, N Tyurin, H W van Hecke, J Velkovska, M Velkovsky, V Veszprémi, L Villatte, A A Vinogradov, M A Volkov, E Vznuzdaev, X R Wang, Y Watanabe, S N White, F K Wohn, C L Woody, W Xie, Y Yang, A Yanovich, S Yokkaichi, G R Young, I E Yushmanov, W A Zajc, C Zhang, S Zhou, S J Zhou, L Zolin

Affiliation

¹ Brookhaven National Laboratory, Upton, New York 11973-5000, USA.

PMID: 17501193
DOI: 10.1103/PhysRevLett.98.132301

Abstract

Emission source functions are extracted from correlation functions constructed from charged pions produced at midrapidity in Au+Au collisions at sqrt[s(NN)]=200 GeV. The source parameters extracted from these functions at low k(T) give first indications of a long tail for the pion emission source. The source extension cannot be explained solely by simple kinematic considerations. The possible role of a halo of secondary pions from resonance emissions is explored.