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

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. T...

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Veröffentlicht in:Physical review letters 2007-03, Vol.98 (13), p.132301-132301
Hauptverfasser: Adler, S S, Afanasiev, S, Aidala, C, Ajitanand, N N, Akiba, Y, Alexander, J, Amirikas, R, Aphecetche, L, Aronson, S H, Averbeck, R, Awes, T C, Azmoun, R, Babintsev, V, Baldisseri, A, Barish, K N, Barnes, P D, Bassalleck, B, Bathe, S, Batsouli, S, Baublis, V, Bazilevsky, A, Belikov, S, Berdnikov, Y, Bhagavatula, S, Boissevain, J G, Borel, H, Borenstein, S, Brooks, M L, Brown, D S, Bruner, N, Bucher, D, Buesching, H, Bumazhnov, V, Bunce, G, Burward-Hoy, J M, Butsyk, S, Camard, X, Chai, J-S, Chand, P, Chang, W C, Chernichenko, S, Chi, C Y, Chiba, J, Chiu, M, Choi, I J, Choi, J, Choudhury, R K, Chujo, T, Chung, P, Cianciolo, V, Cobigo, Y, Cole, B A, Constantin, P, Csanád, M, Csörgo, T, d'Enterria, D, David, G, Delagrange, H, Denisov, A, Deshpande, A, Desmond, E J, Devismes, A, Dietzsch, O, Drapier, O, Drees, A, du Rietz, R, Durum, A, Dutta, D, Efremenko, Y V, Chenawi, K El, Enokizono, A, En'yo, H, Esumi, S, Ewell, L, Fields, D E, Fleuret, F, Fokin, S L, Fox, B D, Fraenkel, Z, Frantz, J E, Franz, A, Frawley, A D, Fung, S-Y, Garpman, S, Ghosh, T K, Glenn, A, Gogiberidze, G, Gonin, M, Gosset, J, Goto, Y, Granier de Cassagnac, R, Grau, N, Greene, S V, Perdekamp, M Grosse, Guryn, W, Gustafsson, H-A, Hachiya, T, Haggerty, J S, Hamagaki, H, Hansen, A G
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container_title Physical review letters
container_volume 98
creator Adler, S S
Afanasiev, S
Aidala, C
Ajitanand, N N
Akiba, Y
Alexander, J
Amirikas, R
Aphecetche, L
Aronson, S H
Averbeck, R
Awes, T C
Azmoun, R
Babintsev, V
Baldisseri, A
Barish, K N
Barnes, P D
Bassalleck, B
Bathe, S
Batsouli, S
Baublis, V
Bazilevsky, A
Belikov, S
Berdnikov, Y
Bhagavatula, S
Boissevain, J G
Borel, H
Borenstein, S
Brooks, M L
Brown, D S
Bruner, N
Bucher, D
Buesching, H
Bumazhnov, V
Bunce, G
Burward-Hoy, J M
Butsyk, S
Camard, X
Chai, J-S
Chand, P
Chang, W C
Chernichenko, S
Chi, C Y
Chiba, J
Chiu, M
Choi, I J
Choi, J
Choudhury, R K
Chujo, T
Chung, P
Cianciolo, V
Cobigo, Y
Cole, B A
Constantin, P
Csanád, M
Csörgo, T
d'Enterria, D
David, G
Delagrange, H
Denisov, A
Deshpande, A
Desmond, E J
Devismes, A
Dietzsch, O
Drapier, O
Drees, A
du Rietz, R
Durum, A
Dutta, D
Efremenko, Y V
Chenawi, K El
Enokizono, A
En'yo, H
Esumi, S
Ewell, L
Fields, D E
Fleuret, F
Fokin, S L
Fox, B D
Fraenkel, Z
Frantz, J E
Franz, A
Frawley, A D
Fung, S-Y
Garpman, S
Ghosh, T K
Glenn, A
Gogiberidze, G
Gonin, M
Gosset, J
Goto, Y
Granier de Cassagnac, R
Grau, N
Greene, S V
Perdekamp, M Grosse
Guryn, W
Gustafsson, H-A
Hachiya, T
Haggerty, J S
Hamagaki, H
Hansen, A G
description 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.
format Article
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L</creatorcontrib><creatorcontrib>Fields, D E</creatorcontrib><creatorcontrib>Fleuret, F</creatorcontrib><creatorcontrib>Fokin, S L</creatorcontrib><creatorcontrib>Fox, B D</creatorcontrib><creatorcontrib>Fraenkel, Z</creatorcontrib><creatorcontrib>Frantz, J E</creatorcontrib><creatorcontrib>Franz, A</creatorcontrib><creatorcontrib>Frawley, A D</creatorcontrib><creatorcontrib>Fung, S-Y</creatorcontrib><creatorcontrib>Garpman, S</creatorcontrib><creatorcontrib>Ghosh, T K</creatorcontrib><creatorcontrib>Glenn, A</creatorcontrib><creatorcontrib>Gogiberidze, G</creatorcontrib><creatorcontrib>Gonin, M</creatorcontrib><creatorcontrib>Gosset, J</creatorcontrib><creatorcontrib>Goto, Y</creatorcontrib><creatorcontrib>Granier de Cassagnac, R</creatorcontrib><creatorcontrib>Grau, N</creatorcontrib><creatorcontrib>Greene, S V</creatorcontrib><creatorcontrib>Perdekamp, M Grosse</creatorcontrib><creatorcontrib>Guryn, W</creatorcontrib><creatorcontrib>Gustafsson, 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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. 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S-Y ; Garpman, S ; Ghosh, T K ; Glenn, A ; Gogiberidze, G ; Gonin, M ; Gosset, J ; Goto, Y ; Granier de Cassagnac, R ; Grau, N ; Greene, S V ; Perdekamp, M Grosse ; Guryn, W ; Gustafsson, H-A ; Hachiya, T ; Haggerty, J S ; Hamagaki, H ; Hansen, A G</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p543-bf9dd9e49a6391c1f66bab0e73b2f7957a9ac8db91e7bc40b82ae75eaa0880d73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Adler, S S</creatorcontrib><creatorcontrib>Afanasiev, S</creatorcontrib><creatorcontrib>Aidala, C</creatorcontrib><creatorcontrib>Ajitanand, N N</creatorcontrib><creatorcontrib>Akiba, Y</creatorcontrib><creatorcontrib>Alexander, J</creatorcontrib><creatorcontrib>Amirikas, R</creatorcontrib><creatorcontrib>Aphecetche, L</creatorcontrib><creatorcontrib>Aronson, S 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D</creatorcontrib><creatorcontrib>Buesching, H</creatorcontrib><creatorcontrib>Bumazhnov, V</creatorcontrib><creatorcontrib>Bunce, G</creatorcontrib><creatorcontrib>Burward-Hoy, J M</creatorcontrib><creatorcontrib>Butsyk, S</creatorcontrib><creatorcontrib>Camard, X</creatorcontrib><creatorcontrib>Chai, J-S</creatorcontrib><creatorcontrib>Chand, P</creatorcontrib><creatorcontrib>Chang, W C</creatorcontrib><creatorcontrib>Chernichenko, S</creatorcontrib><creatorcontrib>Chi, C Y</creatorcontrib><creatorcontrib>Chiba, J</creatorcontrib><creatorcontrib>Chiu, M</creatorcontrib><creatorcontrib>Choi, I J</creatorcontrib><creatorcontrib>Choi, J</creatorcontrib><creatorcontrib>Choudhury, R K</creatorcontrib><creatorcontrib>Chujo, T</creatorcontrib><creatorcontrib>Chung, P</creatorcontrib><creatorcontrib>Cianciolo, V</creatorcontrib><creatorcontrib>Cobigo, Y</creatorcontrib><creatorcontrib>Cole, B A</creatorcontrib><creatorcontrib>Constantin, P</creatorcontrib><creatorcontrib>Csanád, M</creatorcontrib><creatorcontrib>Csörgo, T</creatorcontrib><creatorcontrib>d'Enterria, D</creatorcontrib><creatorcontrib>David, G</creatorcontrib><creatorcontrib>Delagrange, H</creatorcontrib><creatorcontrib>Denisov, A</creatorcontrib><creatorcontrib>Deshpande, A</creatorcontrib><creatorcontrib>Desmond, E J</creatorcontrib><creatorcontrib>Devismes, A</creatorcontrib><creatorcontrib>Dietzsch, O</creatorcontrib><creatorcontrib>Drapier, O</creatorcontrib><creatorcontrib>Drees, A</creatorcontrib><creatorcontrib>du Rietz, R</creatorcontrib><creatorcontrib>Durum, A</creatorcontrib><creatorcontrib>Dutta, D</creatorcontrib><creatorcontrib>Efremenko, Y V</creatorcontrib><creatorcontrib>Chenawi, K El</creatorcontrib><creatorcontrib>Enokizono, A</creatorcontrib><creatorcontrib>En'yo, H</creatorcontrib><creatorcontrib>Esumi, S</creatorcontrib><creatorcontrib>Ewell, L</creatorcontrib><creatorcontrib>Fields, D E</creatorcontrib><creatorcontrib>Fleuret, F</creatorcontrib><creatorcontrib>Fokin, S L</creatorcontrib><creatorcontrib>Fox, B D</creatorcontrib><creatorcontrib>Fraenkel, Z</creatorcontrib><creatorcontrib>Frantz, J E</creatorcontrib><creatorcontrib>Franz, A</creatorcontrib><creatorcontrib>Frawley, A D</creatorcontrib><creatorcontrib>Fung, S-Y</creatorcontrib><creatorcontrib>Garpman, S</creatorcontrib><creatorcontrib>Ghosh, T K</creatorcontrib><creatorcontrib>Glenn, A</creatorcontrib><creatorcontrib>Gogiberidze, G</creatorcontrib><creatorcontrib>Gonin, M</creatorcontrib><creatorcontrib>Gosset, J</creatorcontrib><creatorcontrib>Goto, Y</creatorcontrib><creatorcontrib>Granier de Cassagnac, R</creatorcontrib><creatorcontrib>Grau, N</creatorcontrib><creatorcontrib>Greene, S V</creatorcontrib><creatorcontrib>Perdekamp, M Grosse</creatorcontrib><creatorcontrib>Guryn, W</creatorcontrib><creatorcontrib>Gustafsson, H-A</creatorcontrib><creatorcontrib>Hachiya, T</creatorcontrib><creatorcontrib>Haggerty, J S</creatorcontrib><creatorcontrib>Hamagaki, H</creatorcontrib><creatorcontrib>Hansen, A G</creatorcontrib><collection>PubMed</collection><collection>MEDLINE - Academic</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adler, S S</au><au>Afanasiev, S</au><au>Aidala, C</au><au>Ajitanand, N N</au><au>Akiba, Y</au><au>Alexander, J</au><au>Amirikas, R</au><au>Aphecetche, L</au><au>Aronson, S H</au><au>Averbeck, R</au><au>Awes, T C</au><au>Azmoun, R</au><au>Babintsev, V</au><au>Baldisseri, A</au><au>Barish, K N</au><au>Barnes, P D</au><au>Bassalleck, B</au><au>Bathe, S</au><au>Batsouli, S</au><au>Baublis, V</au><au>Bazilevsky, A</au><au>Belikov, S</au><au>Berdnikov, Y</au><au>Bhagavatula, S</au><au>Boissevain, J G</au><au>Borel, H</au><au>Borenstein, S</au><au>Brooks, M L</au><au>Brown, D S</au><au>Bruner, N</au><au>Bucher, D</au><au>Buesching, H</au><au>Bumazhnov, V</au><au>Bunce, G</au><au>Burward-Hoy, J M</au><au>Butsyk, S</au><au>Camard, X</au><au>Chai, J-S</au><au>Chand, P</au><au>Chang, W C</au><au>Chernichenko, S</au><au>Chi, C Y</au><au>Chiba, J</au><au>Chiu, M</au><au>Choi, I J</au><au>Choi, J</au><au>Choudhury, R K</au><au>Chujo, T</au><au>Chung, P</au><au>Cianciolo, V</au><au>Cobigo, Y</au><au>Cole, B A</au><au>Constantin, P</au><au>Csanád, M</au><au>Csörgo, T</au><au>d'Enterria, D</au><au>David, G</au><au>Delagrange, H</au><au>Denisov, A</au><au>Deshpande, A</au><au>Desmond, E J</au><au>Devismes, A</au><au>Dietzsch, O</au><au>Drapier, O</au><au>Drees, A</au><au>du Rietz, R</au><au>Durum, A</au><au>Dutta, D</au><au>Efremenko, Y V</au><au>Chenawi, K El</au><au>Enokizono, A</au><au>En'yo, H</au><au>Esumi, S</au><au>Ewell, L</au><au>Fields, D E</au><au>Fleuret, F</au><au>Fokin, S L</au><au>Fox, B D</au><au>Fraenkel, Z</au><au>Frantz, J E</au><au>Franz, A</au><au>Frawley, A D</au><au>Fung, S-Y</au><au>Garpman, S</au><au>Ghosh, T K</au><au>Glenn, A</au><au>Gogiberidze, G</au><au>Gonin, M</au><au>Gosset, J</au><au>Goto, Y</au><au>Granier de Cassagnac, R</au><au>Grau, N</au><au>Greene, S V</au><au>Perdekamp, M Grosse</au><au>Guryn, W</au><au>Gustafsson, H-A</au><au>Hachiya, T</au><au>Haggerty, J S</au><au>Hamagaki, H</au><au>Hansen, A G</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt sNN=200 GeV</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2007-03-30</date><risdate>2007</risdate><volume>98</volume><issue>13</issue><spage>132301</spage><epage>132301</epage><pages>132301-132301</pages><issn>0031-9007</issn><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.</abstract><cop>United States</cop><pmid>17501193</pmid><tpages>1</tpages></addata></record>
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title Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt sNN=200 GeV
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