- Access by Xinjiang University
Pion production by protons and He on a Au target at beam energies of 2.8, 5, 10, and 16.587 GeV/nucleon
Phys. Rev. C 85, 024911 – Published 29 February, 2012
DOI: https://doi.org/10.1103/PhysRevC.85.024911
Abstract
Based on a relativistic Boltzmann-Uehling-Uhlenbeck transport model, proton- and He-induced reactions on a Au target at beam energies of 2.8, 5, 10, and 16.587 GeV/nucleon are studied. It is found that compared with proton-induced reactions, He-induced reactions give larger cross sections of pion production, about 5 times those of the proton-induced reactions. And more importantly, pion production from He-induced reaction is more inclined to low-angle emission. Neutrino production via positively charged pion is also discussed accordingly.
Article Text
References (33)
- L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
- L. Wolfenstein, Phys. Rev. D 20, 2634 (1979).
- R. N. Mohapatra and G. Senjanović, Phys. Rev. Lett. 44, 912 (1980).
- Y. Ashie et al. (Super-Kamiokande Collaboration), Phys. Rev. Lett. 93, 101801 (2004).
- M. Ambrosio et al. (MACRO Collaboration), Phys. Lett. B 566, 35 (2003).
- M. Sanchez et al. (Soudan2 Collaboration), Phys. Rev. D 68, 113004 (2003).
- T. Araki et al. (KamLAND Collaboration), Phys. Rev. Lett. 94, 081801 (2005).
- M. B. Smy et al. (Super-Kamiokande Collaboration), Phys. Rev. D 69, 011104 (2004).
- S. N. Ahmed et al. (SNO Collaboration), Phys. Rev. Lett. 92, 181301 (2004).
- E. Aliu et al. (K2K Collaboration), Phys. Rev. Lett. 94, 081802 (2005).
- S. Abe et al. (KamLAND Collaboration), Phys. Rev. Lett. 100, 221803 (2008).
- A. Strumia and F. Vissani, arXiv:hep-ph/0606054.
- J. Collot, H. G. Kirk, and N. V. Mokhov, Nucl. Instrum. Methods Phys. Res., Sect. A 451, 327 (2000).
- I. Chemakin et al., Phys. Rev. C 65, 024904 (2002).
- I. Chemakin et al., Phys. Rev. C 77, 015209 (2008).
- M. Apollonio et al. (HARP Collaboration), Phys. Rev. C 80, 065204 (2009) and Refs. [12–21] therein.
- S. Agostinelli (GEANT4 Collaboration), Nucl. Instrum. Meth. A 506, 250 (2003).
- N. V. Mokhov and S. I. Striganov, MARS Overview, FERMILAB-CONF-07-008-AD, 2007.
- K. Gallmeister and U. Mosel, Nucl. Phys. A 826, 151 (2009) arXiv:0901.1770.
- D. H. Wright et al., AIP Conf. Proc. 896, 11 (2007).
- A. Heikkinen et al., eConf C0303241, MOMT008 (2003).
- H. W. Bertini and P. Guthrie, Nucl. Phys. A 169, 670 (1971).
- G. Folger and H. P. Wellisch, eConf C0303241, MOMT007 (2003).
- S. G. Mashnik et al., LANL Report LA-UR-05-7321, 2005.
- K. Long, Nucl. Phys. B, Proc. Suppl. 154, 111 (2006).
- G. F. Bertsch and S. Das Gupta, Phys. Rep. 160, 189 (1988).
- B. A. Li and C. M. Ko, Phys. Rev. C 52, 2037 (1995).
- Z.-W. Lin, C. M. Ko, B.-A. Li, B. Zhang, and S. Pal, Phys. Rev. C 72, 064901 (2005).
- K. Kubodera and S. Nozawa, Int. J. Mod. Phys. E 3, 101 (1995).
- E. Kolbe, K. Langanke, G. Martínez-Pinedo, and P. Vogel, J. Phys. G 29, 2569 (2003).
- T. Leitner and U. Mosel, Phys. Rev. C 82, 035503 (2010); T. Leitner, L. Alvarez-Ruso, and U. Mosel, ibid. 73, 065502 (2006).
- A. Y. Illarionov, B. A. Kniehl, and A. V. Kotikov, Phys. Rev. Lett. 106, 231802 (2011).
- A. A. Aguilar-Arevalo et al., Phys. Rev. D 79, 072002 (2009).