Pion shadowing as a tool to study the topology of heavy-ion collisions at intermediate energies

Physical Review C - Nuclear Physics

Volumn 55, Issue 5, 1997, Pages 2506-2520

  Badala A ^a   Barbera, R ^a,b   Palmeri, A ^a   Pappalardo, G S ^a   Riggi, F ^a,b   Russo, A C ^a   Russo, G ^a,b   Turrisi, R ^a,b  

^a INFN SEZIONE DI CATANIA   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0031525485     PISSN: 05562813     EISSN: 1089490X     Source Type: Journal    
DOI: 10.1103/PhysRevC.55.2506     Document Type: Article

References (32)

1. W. Cassing, V. Metag, U. Mosel, and K. Niita, Phys. Rep.188, 365 (1990)
2. A. Bonasera, F. Gulminelli, and J. J. Molitoris, Phys. Rep.243, 1 (1993)
3. For a review, see D. Ashery and J. P. Schiffer, Annu. Rev. Nucl. Part. Sci.36, 207 (1986), and references therein
4. P. Hecking, Phys. Rev. B103, 401 (1981)
5. W. Cassing, Z. Phys. A329, 487 (1988)
6. R. S. Mayer et al., Phys. Rev. Lett.70, 904 (1993)
7. A. Badalà et al., Phys. Rev. C48, 2350 (1993)
8. E. Migneco et al., Nucl. Instrum. Methods Phys. Res. A314, 31 (1992)
9. T. Murakami, J. Kasagi, H. Tachibanaki, K. Yoshida, Y. Shibata, T. Nakagawa, M. Ogihara, S. M. Lee, T. Kubo, and T. Motobayashi, Nucl. Instrum. Methods Phys. Res. A253, 163 (1986)
10. A. Del Zoppo et al., Nucl. Instrum. Methods Phys. Res. A327, 363 (1993)
11. A. Badalà, R. Barbera, A. Palmeri, G. S. Pappalardo, F. Riggi, and A. C. Russo, Nucl. Instrum. Methods Phys. Res. A306, 283 (1991)
12. G. Bellia et al., Nucl. Instrum. Methods Phys. Res. A329, 173 (1994)
13. CERN Application Software Group, GEANT: Detector Description and Simulation Tool (CERN, Geneva, 1993); CERN Program Library Long Writeups W5013.
14. A. Badalà, R. Barbera, A. Palmeri, G. S. Pappalardo, F. Riggi, A. C. Russo, G. Russo, and R. Turrisi, Nucl. Instrum. Methods Phys. Res. A351, 387 (1994)
15. A. Badalà, R. Barbera, A. Palmeri, G. S. Pappalardo, F. Riggi, A. C. Russo, G. Russo, and R. Turrisi, Nucl. Instrum. Methods Phys. Res. A357, 443 (1995)
16. A. Badalà, R. Barbera, A. Palmeri, G. S. Pappalardo, F. Riggi, A. C. Russo, G. Russo, and R. Turrisi, Phys. Rev. C 55, 2521 (1997), the following paper
17. A. Badalà et al., Phys. Rev. C47, 231 (1993)
18. M. Gyulassy, K. A. Frankel, and H. Stöcker, Phys. Lett.110B, 185 (1982)
19. P. Danielewicz and G. Odyniec, Phys. Lett.157B, 146 (1985)
20. W. K. Wilson, R. Lacey, C. A. Ogilvie, and G. D. Westfall, Phys. Rev. C45, 738 (1992)
21. M. B. Tsang et al., Phys. Rev. Lett.57, 559 (1986)
22. R. P. Schmitt and B. K. Srivastava, Z. Phys. A335, 49 (1990)
23. A. Badalà, R. Barbera, A. Palmeri, G. S. Pappalardo, F. Riggi, and A. C. Russo, Z. Phys. A344, 455 (1993)
24. D. Brill et al., Phys. Rev. Lett.71, 336 (1993)
25. L. B. Venema et al., Phys. Rev. Lett.71, 835 (1993)
26. A. Schubert et al., Phys. Lett. B328, 10 (1994)
27. S. A. Bass, C. Hartnack, H. Stöcker, and W. Greiner, Phys. Rev. Lett.71, 1144 (1993)
28. B. A. Li, Phys. Lett. B319, 412 (1993)
29. A. Bonasera, G. Russo, and H. H. Wolter, Phys. Lett. B246, 337 (1990)
30. E. Migneco et al., Phys. Lett. B298, 46 (1993)
31. J. Hüfner and M. Thies, Phys. Rev. C20, 273 (1979)
32. W. Cassing, Z. Phys. A329, 487 (1988). ZAANEE