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Volumn 674, Issue 2, 2009, Pages 83-86

Probing a possible vacuum refractive index with γ-ray telescopes

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EID: 62849124509     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2009.02.030     Document Type: Article
Times cited : (63)

References (46)
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    • See, for instance:. GLAST Collaboration and references therein
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    • 4-8 January 2009, Long Beach, California (USA) See also:
    • Dermer C., McEnery J., and Ritz S. 213th American Astronomical Society Meeting. 4-8 January 2009, Long Beach, California (USA). http://www.sciencenews.org/view/generic/id/39228/title/New_window_on_the_high-energy_universe See also:
    • 213th American Astronomical Society Meeting
    • Dermer, C.1    McEnery, J.2    Ritz, S.3
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    • We differ on this point from. arXiv:0901.2932 [astro-ph.HE]
    • We differ on this point from. Wagner R. arXiv:0901.2932 [astro-ph.HE]
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    • This range is also compatible with the weaker limits found previously by the Whipple Collaboration, who found no significant time-lag in emissions during a flare of AGN Mkn 421:. Whipple Collaboration. gr-qc/9810044
    • This range is also compatible with the weaker limits found previously by the Whipple Collaboration, who found no significant time-lag in emissions during a flare of AGN Mkn 421:. Biller S.D., et al., Whipple Collaboration. Phys. Rev. Lett. 83 (1999) 2108. gr-qc/9810044
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    • This model of refractive index is based on the noncritical string approach:
    • This model of refractive index is based on the noncritical string approach:. Ellis J.R., Mavromatos N.E., and Nanopoulos D.V. Phys. Lett. B 293 (1992) 37
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    • Ellis, J.R.1    Mavromatos, N.E.2    Nanopoulos, D.V.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.