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Volumn 921, Issue , 2007, Pages 181-183

WIMP gamma rays from the Galactic Center with GLAST and accelerator comparison

Author keywords

Dark matter; Gamma rays; Supersymmetry

Indexed keywords


EID: 48249158624     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.2757298     Document Type: Conference Paper
Times cited : (2)

References (10)
  • 3
    • 78649799167 scopus 로고    scopus 로고
    • hep-ph/0001086. The source code is available at
    • H. Baer, F. E. Paige, S. D. Protopopescu and X. Tata, (2000) hep-ph/0001086. The source code is available at ftp://ftp.phy.bnl.gov/pub/isajet
    • (2000)
    • Baer, H.1    Paige, F.E.2    Protopopescu, S.D.3    Tata, X.4
  • 5
    • 70450175333 scopus 로고    scopus 로고
    • H. Baer, et al., JCAP 0408 (2004) 005
    • (2004) JCAP , vol.408 , pp. 005
    • Baer, H.1
  • 8
    • 78649779082 scopus 로고    scopus 로고
    • D. N. Spergel, et al, the WMAP Collaboration, astro-ph/0603449
    • D. N. Spergel, et al., the WMAP Collaboration, astro-ph/0603449
  • 10
    • 78649789697 scopus 로고    scopus 로고
    • http://www-glast.slac.stanford.edu/software/IS/glast-lat-performance.htm


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.