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CERN Accelerating science

CERN Document Server Pronađeno je 3 zapisa  Pretraživanje je potrajalo 0.60 sekundi 
1.
Theoretical Challenges in Acceleration and Transport of Ultra High Energy Cosmic Rays: A Review / Blasi, Pasquale (Arcetri Observ. ; Gran Sasso)
The wealth of data collected in the last few years thanks to the Pierre Auger Observatory and recently to the Telescope Array made the problem of the origin of ultra high energy cosmic rays a genuinely experimental/observational one. The apparently contradictory results provided by these experiments in terms of spectrum, chemical composition and anisotropies do not allow to reach any final conclusions as yet. [...]
arXiv:1208.1682.- 2012 - 14 p. - Published in : EPJ Web Conf. 53 (2013) 01002 External link: Preprint
In : International Symposium on future Directions in UHECR Physics
2.
High-energy antiprotons from old supernova remnants / Blasi, Pasquale (Arcetri Observ.) ; Serpico, Pasquale D. (CERN)
A recently proposed model (arXiv:0903.2794) explains the rise in energy of the positron fraction measured by the PAMELA satellite in terms of hadronic production of positrons in aged supernova remnants, and acceleration therein. Here we present a preliminary calculation of the anti-proton flux produced by the same mechanism. [...]
arXiv:0904.0871.- 2009 - 4 p. - Published in : Phys. Rev. Lett. 103 (2009) 081103 APS Published version, local copy : PDF; Fulltext: PDF; External link: Preprint
3.
Pulsars as the Sources of High Energy Cosmic Ray Positrons / Hooper, Dan (Chicago U., Astron. Astrophys. Ctr. ; Fermilab) ; Blasi, Pasquale (Arcetri Observ. ; Fermilab ; Gran Sasso) ; Serpico, Pasquale Dario (CERN ; Fermilab)
Recent preliminary results from the PAMELA satellite indicate the presence of a large flux of positrons (relative to electrons) in the cosmic ray spectrum between approximately 10 and 50 GeV. As annihilating dark matter particles in many models are predicted to contribute to the cosmic ray positron spectrum in this energy range, a great deal of interest has resulted from this observation. [...]
arXiv:0810.1527; FERMILAB-PUB-08-429-A; CERN-PH-TH-2008-228; FERMILAB-PUB-08-429-A.- 2009 - 10 p. - Published in : JCAP 01 (2009) 025 Fulltext: PDF; IOP Open Access article: PDF; External link: Fermilab Library Server (fulltext available)

Također vidi: slična imena autora
134 Blasi, P
1 Blasi, P.
1 Blasi, Paolo
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