Coalescence, interferometry and flow
NA44 has measured proton and deuteron distributions from SS and SPb collisions at 200 GeV/ c and PbPb collisions at 158 GeV/ c. The mean p T of both protons and deuterons grows with system size but the deuterons are somewhat slower than the protons. The phase space density of protons falls with m T...
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| Veröffentlicht in: | Nuclear physics. A 1999, Vol.661 (1), p.456-459 |
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| creator | Murray, Michael Bearden, I.G. Bøggild, H. Conin, L. Dodd, J. Erazmus, B. Esumi, S. Fabjan, C.W. Franz, A. Gaardhøje, J. Hansen, A. Hansen, O. Hardtke, D. van Hecke, H. Holzer, E.B. Humanic, T.J. Hummel, P. Jacak, B.V. Jayanti, R. Kaimi, K. Kaneta, M. Kohama, T. Kopytine, M.L. Leltchouk, M. Ljubicic, L. Lörstad, B. Maeda, N. Martin, L Medvedev, A. Ohnishi, H. Paic, G. Pandey, S.U. Piuz, F. Pluta, J. Polychronakos, V. Potekhin, M. Poulard, G. Reichhold, D. Sakaguchi, A. Schmidt-Sørensen, J. Simon-Gillo, J. Sondheim, W. Sugitate, T. Sullivan, J.P. Sumi, Y. Willis, W.J. Wolf, K. Xu, N. Zachary, D.S. |
| description | NA44 has measured proton and deuteron distributions from
SS and
SPb collisions at 200 GeV/
c and
PbPb collisions at 158 GeV/
c. The mean
p
T
of both protons and deuterons grows with system size but the deuterons are somewhat slower than the protons. The phase space density of protons falls with
m
T
but increases for larger systems. The phase space density of
p̄s is much lower than of protons while their average freeze-out radii are similar. The proton source size increases with system size but not as rapidly as the pion source. For
PbPb collisions, all radii lie on a single curve. |
| doi_str_mv | 10.1016/S0375-9474(99)85064-7 |
| format | Article |
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SS and
SPb collisions at 200 GeV/
c and
PbPb collisions at 158 GeV/
c. The mean
p
T
of both protons and deuterons grows with system size but the deuterons are somewhat slower than the protons. The phase space density of protons falls with
m
T
but increases for larger systems. The phase space density of
p̄s is much lower than of protons while their average freeze-out radii are similar. The proton source size increases with system size but not as rapidly as the pion source. For
PbPb collisions, all radii lie on a single curve.</description><identifier>ISSN: 0375-9474</identifier><identifier>EISSN: 1873-1554</identifier><identifier>DOI: 10.1016/S0375-9474(99)85064-7</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>Nuclear Theory ; Physics</subject><ispartof>Nuclear physics. A, 1999, Vol.661 (1), p.456-459</ispartof><rights>1999</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c293t-be1d530285c9942b70652c0b2d19e4aec6cbd3c4835a80bd30b35f53e70f43c13</citedby><cites>FETCH-LOGICAL-c293t-be1d530285c9942b70652c0b2d19e4aec6cbd3c4835a80bd30b35f53e70f43c13</cites><orcidid>0000-0002-9781-2632</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0375947499850647$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,309,310,314,776,780,785,786,881,3537,4010,4036,4037,23909,23910,25118,27900,27901,27902,65306</link.rule.ids><backlink>$$Uhttps://in2p3.hal.science/in2p3-00021434$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Murray, Michael</creatorcontrib><creatorcontrib>Bearden, I.G.</creatorcontrib><creatorcontrib>Bøggild, H.</creatorcontrib><creatorcontrib>Conin, L.</creatorcontrib><creatorcontrib>Dodd, J.</creatorcontrib><creatorcontrib>Erazmus, B.</creatorcontrib><creatorcontrib>Esumi, S.</creatorcontrib><creatorcontrib>Fabjan, C.W.</creatorcontrib><creatorcontrib>Franz, A.</creatorcontrib><creatorcontrib>Gaardhøje, J.</creatorcontrib><creatorcontrib>Hansen, A.</creatorcontrib><creatorcontrib>Hansen, O.</creatorcontrib><creatorcontrib>Hardtke, D.</creatorcontrib><creatorcontrib>van Hecke, H.</creatorcontrib><creatorcontrib>Holzer, E.B.</creatorcontrib><creatorcontrib>Humanic, T.J.</creatorcontrib><creatorcontrib>Hummel, P.</creatorcontrib><creatorcontrib>Jacak, B.V.</creatorcontrib><creatorcontrib>Jayanti, R.</creatorcontrib><creatorcontrib>Kaimi, K.</creatorcontrib><creatorcontrib>Kaneta, M.</creatorcontrib><creatorcontrib>Kohama, T.</creatorcontrib><creatorcontrib>Kopytine, M.L.</creatorcontrib><creatorcontrib>Leltchouk, M.</creatorcontrib><creatorcontrib>Ljubicic, L.</creatorcontrib><creatorcontrib>Lörstad, B.</creatorcontrib><creatorcontrib>Maeda, N.</creatorcontrib><creatorcontrib>Martin, L</creatorcontrib><creatorcontrib>Medvedev, A.</creatorcontrib><creatorcontrib>Ohnishi, H.</creatorcontrib><creatorcontrib>Paic, G.</creatorcontrib><creatorcontrib>Pandey, S.U.</creatorcontrib><creatorcontrib>Piuz, F.</creatorcontrib><creatorcontrib>Pluta, J.</creatorcontrib><creatorcontrib>Polychronakos, V.</creatorcontrib><creatorcontrib>Potekhin, M.</creatorcontrib><creatorcontrib>Poulard, G.</creatorcontrib><creatorcontrib>Reichhold, D.</creatorcontrib><creatorcontrib>Sakaguchi, A.</creatorcontrib><creatorcontrib>Schmidt-Sørensen, J.</creatorcontrib><creatorcontrib>Simon-Gillo, J.</creatorcontrib><creatorcontrib>Sondheim, W.</creatorcontrib><creatorcontrib>Sugitate, T.</creatorcontrib><creatorcontrib>Sullivan, J.P.</creatorcontrib><creatorcontrib>Sumi, Y.</creatorcontrib><creatorcontrib>Willis, W.J.</creatorcontrib><creatorcontrib>Wolf, K.</creatorcontrib><creatorcontrib>Xu, N.</creatorcontrib><creatorcontrib>Zachary, D.S.</creatorcontrib><creatorcontrib>NA44 Collaboration</creatorcontrib><title>Coalescence, interferometry and flow</title><title>Nuclear physics. A</title><description>NA44 has measured proton and deuteron distributions from
SS and
SPb collisions at 200 GeV/
c and
PbPb collisions at 158 GeV/
c. The mean
p
T
of both protons and deuterons grows with system size but the deuterons are somewhat slower than the protons. The phase space density of protons falls with
m
T
but increases for larger systems. The phase space density of
p̄s is much lower than of protons while their average freeze-out radii are similar. The proton source size increases with system size but not as rapidly as the pion source. For
PbPb collisions, all radii lie on a single curve.</description><subject>Nuclear Theory</subject><subject>Physics</subject><issn>0375-9474</issn><issn>1873-1554</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1999</creationdate><recordtype>article</recordtype><recordid>eNqFkE9Lw0AQxRdRMFY_gtCDB0Wjs_-y2ZOUoFYoeFDPy2YzwZU0Kbuh0m9v0kivzmXm8HuPeY-QSwr3FGj28A5cyVQLJa61vsklZCJVRyShueIplVIck-SAnJKzGL9hmAwgIVdFZxuMDluHd3Pf9hhqDN0a-7Cb27aa1033c05OattEvPjbM_L5_PRRLNPV28trsViljmnepyXSSnJguXRaC1YqyCRzULKKahQWXebKijuRc2lzGE4ouawlRwW14I7yGbmdfL9sYzbBr23Ymc56s1ysjG_Zhpvhb0YFF9uRlhPtQhdjwPogoWDGYsy-GDOmNlqbfTFGDbrHSYdDlK3HYKLzY_7KB3S9qTr_j8MvIAhobQ</recordid><startdate>1999</startdate><enddate>1999</enddate><creator>Murray, Michael</creator><creator>Bearden, I.G.</creator><creator>Bøggild, H.</creator><creator>Conin, L.</creator><creator>Dodd, J.</creator><creator>Erazmus, B.</creator><creator>Esumi, S.</creator><creator>Fabjan, C.W.</creator><creator>Franz, A.</creator><creator>Gaardhøje, J.</creator><creator>Hansen, A.</creator><creator>Hansen, O.</creator><creator>Hardtke, D.</creator><creator>van Hecke, H.</creator><creator>Holzer, E.B.</creator><creator>Humanic, T.J.</creator><creator>Hummel, P.</creator><creator>Jacak, B.V.</creator><creator>Jayanti, R.</creator><creator>Kaimi, K.</creator><creator>Kaneta, M.</creator><creator>Kohama, T.</creator><creator>Kopytine, M.L.</creator><creator>Leltchouk, M.</creator><creator>Ljubicic, L.</creator><creator>Lörstad, B.</creator><creator>Maeda, N.</creator><creator>Martin, L</creator><creator>Medvedev, A.</creator><creator>Ohnishi, H.</creator><creator>Paic, G.</creator><creator>Pandey, S.U.</creator><creator>Piuz, F.</creator><creator>Pluta, J.</creator><creator>Polychronakos, V.</creator><creator>Potekhin, M.</creator><creator>Poulard, G.</creator><creator>Reichhold, D.</creator><creator>Sakaguchi, A.</creator><creator>Schmidt-Sørensen, J.</creator><creator>Simon-Gillo, J.</creator><creator>Sondheim, W.</creator><creator>Sugitate, T.</creator><creator>Sullivan, J.P.</creator><creator>Sumi, Y.</creator><creator>Willis, W.J.</creator><creator>Wolf, K.</creator><creator>Xu, N.</creator><creator>Zachary, D.S.</creator><general>Elsevier B.V</general><general>North-Holland ; Elsevier [1967-....]</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-9781-2632</orcidid></search><sort><creationdate>1999</creationdate><title>Coalescence, interferometry and flow</title><author>Murray, Michael ; Bearden, I.G. ; Bøggild, H. ; Conin, L. ; Dodd, J. ; Erazmus, B. ; Esumi, S. ; Fabjan, C.W. ; Franz, A. ; Gaardhøje, J. ; Hansen, A. ; Hansen, O. ; Hardtke, D. ; van Hecke, H. ; Holzer, E.B. ; Humanic, T.J. ; Hummel, P. ; Jacak, B.V. ; Jayanti, R. ; Kaimi, K. ; Kaneta, M. ; Kohama, T. ; Kopytine, M.L. ; Leltchouk, M. ; Ljubicic, L. ; Lörstad, B. ; Maeda, N. ; Martin, L ; Medvedev, A. ; Ohnishi, H. ; Paic, G. ; Pandey, S.U. ; Piuz, F. ; Pluta, J. ; Polychronakos, V. ; Potekhin, M. ; Poulard, G. ; Reichhold, D. ; Sakaguchi, A. ; Schmidt-Sørensen, J. ; Simon-Gillo, J. ; Sondheim, W. ; Sugitate, T. ; Sullivan, J.P. ; Sumi, Y. ; Willis, W.J. ; Wolf, K. ; Xu, N. ; Zachary, D.S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c293t-be1d530285c9942b70652c0b2d19e4aec6cbd3c4835a80bd30b35f53e70f43c13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1999</creationdate><topic>Nuclear Theory</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Murray, Michael</creatorcontrib><creatorcontrib>Bearden, I.G.</creatorcontrib><creatorcontrib>Bøggild, H.</creatorcontrib><creatorcontrib>Conin, L.</creatorcontrib><creatorcontrib>Dodd, J.</creatorcontrib><creatorcontrib>Erazmus, B.</creatorcontrib><creatorcontrib>Esumi, S.</creatorcontrib><creatorcontrib>Fabjan, C.W.</creatorcontrib><creatorcontrib>Franz, A.</creatorcontrib><creatorcontrib>Gaardhøje, J.</creatorcontrib><creatorcontrib>Hansen, A.</creatorcontrib><creatorcontrib>Hansen, O.</creatorcontrib><creatorcontrib>Hardtke, D.</creatorcontrib><creatorcontrib>van Hecke, H.</creatorcontrib><creatorcontrib>Holzer, E.B.</creatorcontrib><creatorcontrib>Humanic, T.J.</creatorcontrib><creatorcontrib>Hummel, P.</creatorcontrib><creatorcontrib>Jacak, B.V.</creatorcontrib><creatorcontrib>Jayanti, R.</creatorcontrib><creatorcontrib>Kaimi, K.</creatorcontrib><creatorcontrib>Kaneta, M.</creatorcontrib><creatorcontrib>Kohama, T.</creatorcontrib><creatorcontrib>Kopytine, M.L.</creatorcontrib><creatorcontrib>Leltchouk, M.</creatorcontrib><creatorcontrib>Ljubicic, L.</creatorcontrib><creatorcontrib>Lörstad, B.</creatorcontrib><creatorcontrib>Maeda, N.</creatorcontrib><creatorcontrib>Martin, L</creatorcontrib><creatorcontrib>Medvedev, A.</creatorcontrib><creatorcontrib>Ohnishi, H.</creatorcontrib><creatorcontrib>Paic, G.</creatorcontrib><creatorcontrib>Pandey, S.U.</creatorcontrib><creatorcontrib>Piuz, F.</creatorcontrib><creatorcontrib>Pluta, J.</creatorcontrib><creatorcontrib>Polychronakos, V.</creatorcontrib><creatorcontrib>Potekhin, M.</creatorcontrib><creatorcontrib>Poulard, G.</creatorcontrib><creatorcontrib>Reichhold, D.</creatorcontrib><creatorcontrib>Sakaguchi, A.</creatorcontrib><creatorcontrib>Schmidt-Sørensen, J.</creatorcontrib><creatorcontrib>Simon-Gillo, J.</creatorcontrib><creatorcontrib>Sondheim, W.</creatorcontrib><creatorcontrib>Sugitate, T.</creatorcontrib><creatorcontrib>Sullivan, J.P.</creatorcontrib><creatorcontrib>Sumi, Y.</creatorcontrib><creatorcontrib>Willis, W.J.</creatorcontrib><creatorcontrib>Wolf, K.</creatorcontrib><creatorcontrib>Xu, N.</creatorcontrib><creatorcontrib>Zachary, D.S.</creatorcontrib><creatorcontrib>NA44 Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Nuclear physics. A</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Murray, Michael</au><au>Bearden, I.G.</au><au>Bøggild, H.</au><au>Conin, L.</au><au>Dodd, J.</au><au>Erazmus, B.</au><au>Esumi, S.</au><au>Fabjan, C.W.</au><au>Franz, A.</au><au>Gaardhøje, J.</au><au>Hansen, A.</au><au>Hansen, O.</au><au>Hardtke, D.</au><au>van Hecke, H.</au><au>Holzer, E.B.</au><au>Humanic, T.J.</au><au>Hummel, P.</au><au>Jacak, B.V.</au><au>Jayanti, R.</au><au>Kaimi, K.</au><au>Kaneta, M.</au><au>Kohama, T.</au><au>Kopytine, M.L.</au><au>Leltchouk, M.</au><au>Ljubicic, L.</au><au>Lörstad, B.</au><au>Maeda, N.</au><au>Martin, L</au><au>Medvedev, A.</au><au>Ohnishi, H.</au><au>Paic, G.</au><au>Pandey, S.U.</au><au>Piuz, F.</au><au>Pluta, J.</au><au>Polychronakos, V.</au><au>Potekhin, M.</au><au>Poulard, G.</au><au>Reichhold, D.</au><au>Sakaguchi, A.</au><au>Schmidt-Sørensen, J.</au><au>Simon-Gillo, J.</au><au>Sondheim, W.</au><au>Sugitate, T.</au><au>Sullivan, J.P.</au><au>Sumi, Y.</au><au>Willis, W.J.</au><au>Wolf, K.</au><au>Xu, N.</au><au>Zachary, D.S.</au><aucorp>NA44 Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Coalescence, interferometry and flow</atitle><jtitle>Nuclear physics. A</jtitle><date>1999</date><risdate>1999</risdate><volume>661</volume><issue>1</issue><spage>456</spage><epage>459</epage><pages>456-459</pages><issn>0375-9474</issn><eissn>1873-1554</eissn><abstract>NA44 has measured proton and deuteron distributions from
SS and
SPb collisions at 200 GeV/
c and
PbPb collisions at 158 GeV/
c. The mean
p
T
of both protons and deuterons grows with system size but the deuterons are somewhat slower than the protons. The phase space density of protons falls with
m
T
but increases for larger systems. The phase space density of
p̄s is much lower than of protons while their average freeze-out radii are similar. The proton source size increases with system size but not as rapidly as the pion source. For
PbPb collisions, all radii lie on a single curve.</abstract><pub>Elsevier B.V</pub><doi>10.1016/S0375-9474(99)85064-7</doi><tpages>4</tpages><orcidid>https://orcid.org/0000-0002-9781-2632</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0375-9474 |
| ispartof | Nuclear physics. A, 1999, Vol.661 (1), p.456-459 |
| issn | 0375-9474 1873-1554 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_in2p3_00021434v1 |
| source | Elsevier ScienceDirect Journals |
| subjects | Nuclear Theory Physics |
| title | Coalescence, interferometry and flow |
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