Cargando…
High energy rise of the cosmic ray positron fraction: Possible causes
In the last year, the PAMELA satellite has suggested an “anomalous” rise with energy of the cosmic ray positron fraction. Several explanations have been proposed: here I recapitulate the basic physics behind astrophysical explanations and summarize the existing issues in interpreting the data via da...
Autor principal: | Serpico, Pasquale D |
---|---|
Lenguaje: | eng |
Publicado: |
2009
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.nuclphysbps.2009.07.014 http://cds.cern.ch/record/1264082 |
Ejemplares similares
-
Pulsars as the Sources of High Energy Cosmic Ray Positrons
por: Hooper, Dan, et al.
Publicado: (2008) -
Possible causes of a rise with energy of the cosmic ray positron fraction
por: Serpico, Pasquale Dario
Publicado: (2008) -
Ultra-high energy cosmic ray autocorrelation function after Auger
por: Dario Serpico, Pasquale
Publicado: (2009) -
Precision Measurement of the Positron Fraction in Primary Cosmic Rays with AMS on the Space Station
por: Vagelli, Valerio, et al.
Publicado: (2017) -
High energy cosmic rays
por: Stanev, Todor
Publicado: (2004)