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Volumn 69, Issue 12, 2004, Pages

CERN Axion Solar Telescope as a probe of large extra dimensions

Author keywords

[No Author keywords available]

Indexed keywords


EID: 10944263273     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.125011     Document Type: Article
Times cited : (13)

References (42)
  • 6
  • 17
    • 85039594684 scopus 로고    scopus 로고
    • CAST Collaboration, J.I. Collar, hep-ex/0304024
    • Collar, J.I.1
  • 30
    • 85039597067 scopus 로고    scopus 로고
    • See, e.g., G. G. Raffelt, Stars as Laboratories for Fundamental Physics (The University of Chicago Press, Chicago, 1996).
    • See, e.g., G. G. Raffelt, Stars as Laboratories for Fundamental Physics (The University of Chicago Press, Chicago, 1996).
  • 40
    • 85039599127 scopus 로고    scopus 로고
    • By simply scaling the solar age limit of QCD axions (Formula presented) 16 with (Formula presented) due to the multiplicity of KK modes and observing that an allowed maximum mass is (Formula presented) before the solar flux gets suppressed by the kinematic threshold, one obtains for two extra dimensions: (i) for (Formula presented) (Formula presented) if (Formula presented) and (Formula presented) if (Formula presented) and (ii) for (Formula presented) nm: (Formula presented) if (Formula presented) and (Formula presented) if (Formula presented)
    • By simply scaling the solar age limit of QCD axions (Formula presented) 16 with (Formula presented) due to the multiplicity of KK modes and observing that an allowed maximum mass is (Formula presented) before the solar flux gets suppressed by the kinematic threshold, one obtains for two extra dimensions: (i) for (Formula presented) (Formula presented) if (Formula presented) and (Formula presented) if (Formula presented) and (ii) for (Formula presented) nm: (Formula presented) if (Formula presented) and (Formula presented) if (Formula presented)
  • 41
    • 17644448246 scopus 로고    scopus 로고
    • Particle Data Group, K. Hagiwara, Phys. Rev. D 66, 010001 (2002).
    • (2002) Phys. Rev. D , vol.66 , pp. 10001
    • Hagiwara, K.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.