Systematic uncertainties on the cosmic-ray transport parameters: Is it possible to reconcile B/C data with δ = 1/3 or δ = 1/2?

Astronomy and Astrophysics

Volumn 516, Issue 19, 2010, Pages

  Maurin, D ^a,b,c   Putze, A ^d,e   Derome, L ^d  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^d UNIVERSITÉ JOSEPH FOURIER GRENOBLE 1   (France)

^e STOCKHOLM UNIVERSITY   (Sweden)

Author keywords

cosmic rays; methods: statistical

Indexed keywords

COSMIC RAYS; COSMOLOGY; STATISTICAL MECHANICS; STATISTICS; WIND POWER;

DIFFUSION COEFFICIENTS; GALACTIC DISC; GAS DENSITY; IN-LINE; LOW ENERGIES; METHODS:STATISTICAL; NUCLEAR FRAGMENTATION; RE-ACCELERATION; SPECTRAL SHAPES; STATISTICAL TOOLS; STATISTICAL UNCERTAINTY; SYSTEMATIC UNCERTAINTIES; THEORETICAL VALUES; TRANSPORT PARAMETERS; WIND STRENGTH;

DIFFUSION;

EID: 77957838098     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014011     Document Type: Article

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