Secondary cosmic-ray nuclei from supernova remnants and constraints on the propagation parameters

Astronomy and Astrophysics

Volumn 544, Issue , 2012, Pages

  Tomassetti, N ^a   Donato, F ^b  

^a INFN SEZIONE DI PERUGIA   (Italy)

^b UNIVERSITY OF TURIN   (Italy)

Author keywords

Acceleration of particles; Cosmic rays; ISM: supernova remnants; Nuclear reactions, nucleosynthesis, abundances

Indexed keywords

ACCELERATION OF PARTICLES; ANALYTICAL CALCULATION; COSMIC-RAY NUCLEUS; DIFFUSION PARAMETERS; DIFFUSIVE SHOCK ACCELERATIONS; HADRONIC INTERACTIONS; INTERSTELLAR MEDIUMS; ISM: SUPERNOVA REMNANTS; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; PROPAGATION PARAMETERS; PROPAGATION PROCESS; RE-ACCELERATION; SECONDARY NUCLEI; SECONDARY PRODUCTION; SIMULATED DATA; SUPERNOVA REMNANTS; TRANSPORT PARAMETERS; UNCERTAINTY BOUNDS;

BORON; CHEMICAL ELEMENTS; EXPERIMENTS; STARS;

COSMIC RAYS;

EID: 84864066671     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201218967     Document Type: Article

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