On the space-time difference of proton and composite particle emission in central heavy-ion reactions at 400 A • MeV

被引:29
作者
Kotte, R
Barz, HW
Neubert, W
Plettner, C
Wohlfarth, D
Alard, JP
Andronic, A
Averbeck, R
Basrak, Z
Bastid, N
Bendarag, N
Berek, G
Caplar, R
Cindro, N
Crochet, P
Devismes, A
Dupieux, P
Dzelalija, M
Eskef, M
Fodor, Z
Gobbi, A
Grishkin, Y
Herrmann, N
Hildenbrand, KD
Hong, B
Kecskemeti, J
Kim, YJ
Kirejczyk, M
Korolija, M
Kowalczyk, M
Kress, T
Kutsche, R
Lebedev, A
Lee, KS
Leifels, Y
Manko, V
Merlitz, H
Moisa, D
Nianine, A
Pelte, D
Petrovici, M
Rami, F
Reisdorf, W
de Schauenburg, B
Schüll, D
Seres, Z
Sikora, B
Sim, KS
Simion, V
Siwek-Wilczynska, K
机构
[1] Rossendorf Inc, Forschungszentrum Rossendorf EV, D-01314 Dresden, Germany
[2] Inst Nucl Phys & Engn, Bucharest, Romania
[3] Cent Res Inst Phys, H-1525 Budapest, Hungary
[4] Univ Blaise Pascal, Phys Corpusculaire Lab, Clermont Ferrand, France
[5] Gesell Schwerionenforsch GmbH, D-6100 Darmstadt, Germany
[6] Univ Heidelberg, Inst Phys, D-6900 Heidelberg, Germany
[7] Inst Theoret & Expt Phys, Moscow 117259, Russia
[8] IV Kurchatov Atom Energy Inst, Moscow 123182, Russia
[9] Korea Univ, Seoul 136701, South Korea
[10] ULP, CNRS, IN2P3, Inst Rech Subatom, Strasbourg, France
[11] Univ Warsaw, Inst Expt Phys, Warsaw, Poland
[12] Rudjer Boskovic Inst, Zagreb, Croatia
关键词
D O I
10.1007/s100500050333
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Small-angle correlations of pairs of nonidentical light charged particles produced in central collisions of heavy ions in the A = 100 mass region at a beam energy of 400 A.MeV are investigated with the FOPI detector system at GSI Darmstadt. The difference of longitudinal correlation functions with the relative velocity parallel and anti-parallel to the center-of-mass velocity of the pair in the central source frame is studied. This method allows extracting the apparent space-time differences of the emission of the charged particles. Comparing the correlations with results of a final-state interaction model delivers quantitative estimates of these asymmetries. Time delays as short as 1 fm/c or - alternatively - source radius differences of a few tenth fm are resolved. The strong collective expansion of the participant zone introduces not only an apparent reduction of the source radius but also a modification of the emission times. After correcting for both effects a complete sequence of the space-time emission of p, d, t, He-3, alpha particles is presented for the first time.
引用
收藏
页码:185 / 195
页数:11
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