Azimuthal Dependence of Collective Expansion for Symmetric Heavy-Ion Collisions

Physical Review Letters

Volumn 92, Issue 7, 2004, Pages

  Stoicea, G ^a   Petrovici, M ^a,d   Andronic, A ^a,d   Herrmann, N ^f   Alard, J P ^c   Basrak, Z ^k   Barret, V ^c   Bastid, N ^c   Caplar R ^k   Crochet, P ^c   Dupieux, P ^c   Dzelalija M ^k   Fodor, Z ^b   Hartmann, O ^d   Hildenbrand, K D ^d   Hong, B ⁱ   Kecskemeti, J ^b   Kim, Y J ⁱ   Kirejczyk, M ^l   Korolija, M ^k   Kotte, R ^e   Kress, T ^d   Lebedev, A ^g   Leifels, Y ^d   Lopez, X ^c   Merschmeier, M ^f   Neubert, W ^e   Pelte, D ^f   Rami, F ^j   Reisdorf, W ^d   Schull D ^d   Seres, Z ^b   Sikora, B ^l   Sim, K S ⁱ   Simion, V ^a   Siwek Wilczynska K ^l   Smolyankin, V ^g   Stockmeier, M ^f   Wisniewski K ^d   Wohlfarth, D ^e   Yushmanov, I ^h   Zhilin, A ^g   Danielewicz, P ^d,m   more..

^a HORIA HULUBEI NATIONAL INSTITUTE OF PHYSICS AND NUCLEAR ENGINEERING   (Romania)

^b WIGNER RESEARCH CENTRE FOR PHYSICS   (Hungary)

^c UNIVERSITÉ BLAISE PASCAL   (France)

^d GSI HELMHOLTZZENTRUM FÜR SCHWERIONENFORSCHUNG GMBH   (Germany)

^e INSTITUTE OF ION BEAM PHYSICS AND MATERIALS RESEARCH   (Germany)

^f UNIVERSITY OF HEIDELBERG   (Germany)

^g INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

^h KURCHATOV INSTITUTE   (Russian Federation)

ⁱ Korea University   (South Korea)

^j UNIVERSITÉ DE STRASBOURG   (France)

^k RUDER BO KOVI INSTITUTE   (Croatia)

^l UNIVERSITY OF WARSAW   (Poland)

^m MICHIGAN STATE UNIVERSITY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; EQUATIONS OF STATE; HIGH ENERGY PHYSICS; KINETIC ENERGY; MATHEMATICAL MODELS; NUCLEAR PHYSICS; PARTICLE SIZE ANALYSIS;

AZIMUTHAL ANGLE; EXCITATION ENERGY;

HEAVY IONS;

EID: 12144290278     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.92.072303     Document Type: Article

References (29)

1. G.F. Chapline et al, Phys. Rev. D 8, 4302 (1973).10.1103/PhysRevD.8.4302
2. W. Scheid et al, Phys. Rev. Lett. 32, 741 (1974).10.1103/PhysRevLett.32.741
3. H.W. Barz et al, Nucl. Phys. A531, 453 (1991).
4. W. Bauer et al, Phys. Rev. C 47, R1838 (1994).10.1103/PhysRevC.47.R1838
5. S.C. Jeong et al, Phys. Rev. Lett. 72, 3468 (1994).10.1103/PhysRevLett.72.3468
6. W.C. Hsi et al, Phys. Rev. Lett. 73, 3367 (1994.10.1103/PhysRevLett.73.3367
7. M. Petrovici et al, Phys. Rev. Lett. 74, 5001 (1995).10.1103/PhysRevLett.74.5001
8. G. Poggi et al, Nucl. Phys. A586, 755 (1995).
9. M.A. Lisa et al, Phys. Rev. Lett. 75, 2662 (1995).10.1103/PhysRevLett.75.2662
10. P. Braun-Munzinger et al, Phys. Lett. B 344, 43 (1995).10.1016/0370-2693(94)01534-J
11. W. Reisdorf et al, Nucl. Phys. A612, 493 (1997).
12. H. Stöcker et al, Phys. Rev. C 25, 1873 (1982).10.1103/PhysRevC.25.1873
13. H.H. Gutbrod et al, Phys. Lett. B 216, 267 (1989). 10.1016/0370-2693(89)91113-1
14. M. Demoulins et al, Phys. Lett. B 241, 476 (1990).10.1016/0370-2693(90)91855-6
15. D. Brill et al, Phys. Rev. Lett. 71, 336 (1993).10.1103/PhysRevLett.71.336
16. L.B. Venema et al, Phys. Rev. Lett. 71, 835 (1993).10.1103/PhysRevLett.71.835
17. Y. Leifels et al, Phys. Rev. Lett. 71, 963 (1993).10.1103/PhysRevLett.71.963
18. D. Lambrecht et al, Z. Phys. A 350, 115 (1994).
19. S. Wang et al, Phys. Rev. Lett. 76, 3911 (1996).10.1103/PhysRevLett.76.3911
20. N. Bastid et al, Nucl. Phys. A622, 573 (1997).
21. Y. Shin et al, Phys. Rev. Lett. 81, 1576 (1998).10.1103/PhysRevLett.81.1576
22. M. Petrovici et al, Heavy Ion Physics Using (Formula presented) Detectors (World Scientific, Singapore, 1997), p.�216.
23. W.K. Wilson et al, Phys. Rev. C 51, 3136 (1995).10.1103/PhysRevC.51.3136
24. A. Andronic et al, Nucl. Phys. A679, 765 (2001).
25. J. Ritman et al, Nucl. Phys. B44, 708 (1995)
26. A. Gobbi et al, Nucl. Instrum. Methods Phys. Res., Sect. A 324, 156 (1993).10.1016/0168-9002(93)90974-M
27. P. Danielewicz et al, Phys. Lett. B 157, 146 (1985).
28. P. Danielewicz and Q. Pan, Phys. Rev. C 46, 2002 (1992); 10.1103/PhysRevC.46.2002
29. P. Danielewicz, Nucl. Phys. A673, 375 (2000).