Cargando…
Standard Cosmic Ray Energetics and Light Element Production
The recent observations of Be and B in metal poor stars has led to a reassessment of the origin of the light elements in the early Galaxy. At low it is metallicity ([O/H] < -1.75), it is necessary to introduce a production mechanism which is independent of the interstellar metallicity (primary)....
Autores principales: | Fields, Brian D., Olive, Keith A., Casse, Michel, Vangioni-Flam, Elisabeth |
---|---|
Lenguaje: | eng |
Publicado: |
2000
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1051/0004-6361:20010251 http://cds.cern.ch/record/467662 |
Ejemplares similares
-
Conference on LiBeB, Cosmic Rays, and Related X- and Gamma-Rays
por: Ramaty, Reuven, et al.
Publicado: (1999) -
Effects of Unstable Particles on Light-Element Abundances: Lithium versus Deuterium and He3
por: Ellis, John R., et al.
Publicado: (2005) -
2nd IAP Astrophysics Meeting
por: Audouze, Jean, et al.
Publicado: (1986) -
Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics
por: Cyburt, Richard H., et al.
Publicado: (2001) -
Bound-State Effects on Light-Element Abundances in Gravitino Dark Matter Scenarios
por: Cyburt, Richard H., et al.
Publicado: (2006)