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Volumn 69, Issue 8, 2004, Pages 11-

Cosmological acceleration, varying couplings, and Lorentz breaking

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EID: 2442689088     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.083513     Document Type: Article
Times cited : (152)

References (114)
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    • See, e.g., Boomerang Collaboration, P. de Bernardis, Nature (London) 404, 955 (2000)
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    • There exist also parameter choices leading to a variation of α that approximately matches observations 16 29. In these cases, however, the resulting cosmological expansion is phenomenologically uninteresting
    • There exist also parameter choices leading to a variation of α that approximately matches observations 1629. In these cases, however, the resulting cosmological expansion is phenomenologically uninteresting.
  • 88
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    • R. Lehnert, in New Worlds in Astroparticle Physics, edited by A. Krasnitz, A.M. Mourão, M.Pimenta, and R. Potting (World Scientific, Singapore, 2003), hep-ph/0308208.
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    • For recent experimental progress and theoretical ideas in this subject, see CPT and Lorentz Symmetry II, edited by V. A. Kostelecký (World Scientific, Singapore, 2002)
    • For recent experimental progress and theoretical ideas in this subject, see CPT and Lorentz Symmetry II, edited by V. A. Kostelecký (World Scientific, Singapore, 2002).
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    • a local comoving inertial frame, the time coordinate (Formula presented) agrees to first order with comoving time t, so that we can take (Formula presented)
    • In a local comoving inertial frame, the time coordinate (Formula presented) agrees to first order with comoving time t, so that we can take (Formula presented)


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