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Volumn 1223, Issue , 2010, Pages 43-49

Astroparticle physiscs with AMS02

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Astroparticle

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EID: 77952004442     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.3395995     Document Type: Conference Paper
Times cited : (51)

References (7)
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    • Adriani1
  • 2
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    • Measurement of the Cosmic Ray e+e- Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
    • Abdo et al, Measurement of the Cosmic Ray e+e- Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope, Phys. Rev. Lett. - 102, 181101 (2009)
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    • Abdo1
  • 3
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    • New Measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic Radiation
    • Adriani et al, New Measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic Radiation, PRL 102 (2009) 051101
    • (2009) PRL , vol.102 , pp. 051101
    • Adriani1
  • 4
    • 37649011308 scopus 로고    scopus 로고
    • Mature gamma-ray pulsars as possible sources of Galactic positrons
    • B.Z.Dai et al., Mature gamma-ray pulsars as possible sources of Galactic positrons Nucl. Phys. B Volumes 175-176 (2008) Pages 517-520
    • (2008) Nucl. Phys. B , vol.175-176 , pp. 517-520
    • Dai, B.Z.1
  • 5
    • 68749096065 scopus 로고    scopus 로고
    • Origin of the Positron Excess in Cosmic Rays
    • P.Blasi,Origin of the Positron Excess in Cosmic Rays PRL 103, 051104 (2009)
    • (2009) PRL , vol.103 , pp. 051104
    • Blasi, P.1
  • 6
    • 56749143755 scopus 로고    scopus 로고
    • An excess of cosmic ray electrons at energies of 300âà Ş800 GeV
    • J. Chang et al., An excess of cosmic ray electrons at energies of 300âÃŞ800 GeV, Nature (London) 456, 362 (2008)
    • (2008) Nature (London) , vol.456 , pp. 362
    • Chang, J.1
  • 7
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    • Antideuteron ïňĆuxes from dark matter annihilation in diïňǍusion models
    • F. Donato, N. Fornengo and D.Maurin Antideuteron ïňĆ uxes from dark matter annihilation in diïňǍusion models, Phys. Rev. D 78, 043506 (2008)
    • (2008) Phys. Rev. D , vol.78 , pp. 043506
    • Donato, F.1    Fornengo, N.2    Maurin, D.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.