Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas

被引:63
作者
Evoli, Carmelo [1 ,2 ]
Gaggero, Daniele [3 ]
Vittino, Andrea [4 ,5 ]
Di Mauro, Mattia [6 ,7 ]
Grasso, Dario [8 ]
Mazziotta, Mario Nicola [9 ]
机构
[1] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, Italy
[2] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Via G Acitelli 22, I-67100 Assergi, AQ, Italy
[3] Univ Amsterdam, Inst Phys, GRAPPA, NL-1098 XH Amsterdam, Netherlands
[4] Tech Univ Munich, Phys Dept T30d, James Franck Str 1, D-85748 Garching, Germany
[5] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany
[6] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Dept Phys, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA
[7] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA
[8] INFN Pisa, Largo B Pontecorvo 3, I-56127 Pisa, Italy
[9] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2018年 / 07期
基金
欧盟地平线“2020”;
关键词
cosmic ray theory; absorption and radiation processes; cosmic ray experiments; dark matter experiments; ISOTOPIC CROSS-SECTIONS; LIQUID-HYDROGEN TARGET; HIGH-ENERGY; ASTROPHYSICAL APPLICATIONS; DARK-MATTER; FLUKA CODE; GAMMA-RAYS; C-12; ANTIPROTONS; GALAXY;
D O I
10.1088/1475-7516/2018/07/006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Understanding the isotopic composition of cosmic rays (CRs) observed near Earth represents a milestone towards the identification of their origin. Local fluxes contain all the known stable and long-lived isotopes, reflecting the complex history of primaries and secondaries as they traverse the interstellar medium. For that reason, a numerical code which aims at describing the CR transport in the Galaxy must unavoidably rely on accurate modelling of the production of secondary particles. In this work we provide a detailed description of the nuclear cross sections and decay network as implemented in the forthcoming release of the galactic propagation code DRAGON2. We present the secondary production models implemented in the code and we apply the different prescriptions to compute quantities of interest to interpret local CR fluxes (e.g., nuclear fragmentation timescales, secondary and tertiary source terms). In particular, we develop a nuclear secondary production model aimed at accurately computing the light secondary fluxes (namely: Li, Be, B) above 1 GeV/n. This result is achieved by fitting existing empirical or semi-empirical formalisms to a large sample of measurements in the energy range 100 MeV/n to 100 GeV/n and by considering the contribution of the most relevant decaying isotopes up to iron. Concerning secondary antiparticles (positrons and antiprotons), we describe a collection of models taken from the literature, and provide a detailed quantitative comparison.
引用
收藏
页数:29
相关论文
共 90 条
[11]   Parametrizations of inclusive cross sections for pion production in proton-proton collisions [J].
Blattnig, SR ;
Swaminathan, SR ;
Kruger, AT ;
Ngom, M ;
Norbury, JW .
PHYSICAL REVIEW D, 2000, 62 (09) :1-12
[12]   The FLUKA Code: Developments and Challenges for High Energy and Medical Applications [J].
Boehlen, T. T. ;
Cerutti, F. ;
Chin, M. P. W. ;
Fosso, A. ;
Ferrari, A. ;
Ortega, P. G. ;
Mairani, A. ;
Sala, P. R. ;
Smirnov, G. ;
Vlachoudisl, V. .
NUCLEAR DATA SHEETS, 2014, 120 :211-214
[13]   The DArk Matter Particle Explorer mission [J].
Chang, J. ;
Ambrosi, G. ;
An, Q. ;
Asfandiyarov, R. ;
Azzarello, P. ;
Bernardini, P. ;
Bertucci, B. ;
Cai, M. S. ;
Caragiulo, M. ;
Chen, D. Y. ;
Chen, H. F. ;
Chen, J. L. ;
Chen, W. ;
Cui, M. Y. ;
Cui, T. S. ;
D'Amone, A. ;
De Benedittis, A. ;
De Mitri, I. ;
Di Santo, M. ;
Dong, J. N. ;
Dong, T. K. ;
Dong, Y. F. ;
Dong, Z. X. ;
Donvito, G. ;
Droz, D. ;
Duan, K. K. ;
Duan, J. L. ;
Duranti, M. ;
D'Urso, D. ;
Fan, R. R. ;
Fan, Y. Z. ;
Fang, F. ;
Feng, C. Q. ;
Feng, L. ;
Fusco, P. ;
Gallo, V. ;
Gan, F. J. ;
Gan, W. Q. ;
Gao, M. ;
Gao, S. S. ;
Gargano, F. ;
Gong, K. ;
Gong, Y. Z. ;
Guo, J. H. ;
Hu, Y. M. ;
Huang, G. S. ;
Huang, Y. Y. ;
Ionica, M. ;
Jiang, D. ;
Jiang, W. .
ASTROPARTICLE PHYSICS, 2017, 95 :6-24
[14]   Constraining Galactic cosmic-ray parameters with Z ≤ 2 nuclei [J].
Coste, B. ;
Derome, L. ;
Maurin, D. ;
Putze, A. .
ASTRONOMY & ASTROPHYSICS, 2012, 539
[15]  
DERMER CD, 1986, ASTRON ASTROPHYS, V157, P223
[16]   BINARY COLLISION RATES OF RELATIVISTIC THERMAL PLASMAS .2. SPECTRA [J].
DERMER, CD .
ASTROPHYSICAL JOURNAL, 1986, 307 (01) :47-59
[17]   New evaluation of the antiproton production cross section for cosmic ray studies [J].
Di Mauro, Mattia ;
Donato, Fiorenza ;
Goudelis, Andreas ;
Serpico, Pasquale Dario .
PHYSICAL REVIEW D, 2014, 90 (08)
[18]   On the annihilation of electrons and protons [J].
Dirac, PAM .
PROCEEDINGS OF THE CAMBRIDGE PHILOSOPHICAL SOCIETY, 1930, 26 :361-375
[19]   Prescriptions on antiproton cross section data for precise theoretical antiproton flux predictions [J].
Donato, Fiorenza ;
Korsmeier, Michael ;
Di Mauro, Mattia .
PHYSICAL REVIEW D, 2017, 96 (04)
[20]   Parametrization of the antiproton inclusive production cross section on nuclei -: art. no. 094017 [J].
Duperray, RP ;
Huang, CY ;
Protasov, KV ;
Buénerd, M .
PHYSICAL REVIEW D, 2003, 68 (09)