Charged pions from Ni on Ni collisions between 1 and 2 AGeV

被引:43
作者
Pelte, D
Eskef, M
Goebels, G
Hafele, E
Herrmann, N
Korolija, M
Merlitz, H
Mohren, S
Trzaska, M
Alard, JP
Amouroux, V
Andronic, A
Basrak, Z
Bastid, N
Belyaev, I
Best, D
Biegansky, J
Buta, A
Claplar, R
Cindro, N
Coffin, JP
Crochet, P
Dupieux, P
Dzelalija, M
Ero, J
Fintz, P
Fodor, Z
GenouxLubain, A
Gobbi, A
Guillaume, G
Hildenbrand, KD
Hong, B
Jundt, F
Kecskemeti, J
Kirejczyk, M
Koncz, P
Korchagin, Y
Kotte, R
Kuhn, C
Lambrecht, D
Lebedev, A
Legrand, I
Leifels, Y
Manko, V
Mosner, J
Moisa, D
Neubert, W
Petrovici, M
Pinkenburg, C
Pras, P
机构
[1] FORSCHUNGSZENTRUM ROSSENDORF EV,DRESDEN,GERMANY
[2] GESELL SCHWERIONENFORSCH MBH,D-6100 DARMSTADT,GERMANY
[3] UNIV CLERMONT FERRAND,CLERMONT FERRAN,FRANCE
[4] CNRS,IN2P3,PHYS CORPUSCULAIRE LAB,CLERMONT FERRAN,FRANCE
[5] CENT RES INST PHYS,H-1525 BUDAPEST,HUNGARY
[6] INST PHYS & NUCL ENGN,BUCHAREST,ROMANIA
[7] INST THEORET & EXPT PHYS,MOSCOW 117259,RUSSIA
[8] KURCHATOV INST,MOSCOW,RUSSIA
[9] UNIV LOUIS PASTEUR STRASBOURG 1,STRASBOURG,FRANCE
[10] CTR RECH NUCL,STRASBOURG,FRANCE
[11] UNIV WARSAW,INST EXPT PHYS,WARSAW,POLAND
[12] RUDJER BOSKOVIC INST,ZAGREB,CROATIA
来源
ZEITSCHRIFT FUR PHYSIK A-HADRONS AND NUCLEI | 1997年 / 359卷 / 01期
关键词
D O I
10.1007/s002180050367
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
Charged pions from Ni + Ni reactions at 1.05, 1.45 and 1.93 AGeV are measured with the FOPI detector. The pi(+/-) multiplicities per mean number of participants increase crease with beam energy, in accordance with earlier studies of the Ar + KCl and La + La systems. The pion kinetic energy spectra have concave shape and are fitted by the superposition of two Boltzmann distributions with different temperatures. These apparent temperatures depend only weakly on bombarding energy. The pion angular distributions show a forward/backward enhancement at all energies, but not the Theta = 90 degrees enhancement which was observed in case of the Au + Au system. These features also determine the rapidity distributions which are therefore in disagreement with the hypothesis of one thermal source. The importance of the Coulomb interaction and of the pion rescattering by spectator matter in producing these phenomena is discussed.
引用
收藏
页码:55 / 64
页数:10
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