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Phys. Rev. D 65, 083001 (2002) [5 pages]

Quintessence and variation of the fine structure constant in the cosmic microwave background radiation

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Greg Huey
Astronomy Unit, School of Mathematical Sciences, Queen Mary College, London E1 4NS, United Kingdom

Stephon Alexander and Levon Pogosian
Theoretical Physics, The Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom

Received 25 October 2001; published 8 March 2002

We study the dependence of the CMB temperature anisotropy spectrum on the value of the fine structure constant α and the equation of state of the dark energy component of the total density of the universe. We find that bounds imposed on the variation of α from the analysis of currently available CMB data sets can be significantly relaxed if one also allows for a change in the equation of state.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.65.083001
DOI:
10.1103/PhysRevD.65.083001
PACS:
98.70.Vc