A Constraint on Planck-scale Modifications to Electrodynamics with CMB polarization data
arXiv:0904.3201 · doi:10.1088/1475-7516/2009/08/021
Abstract
We show that the Cosmic Microwave Background (CMB) polarization data gathered by the BOOMERanG 2003 flight and WMAP provide an opportunity to investigate {\it in-vacuo} birefringence, of a type expected in some quantum pictures of space-time, with a sensitivity that extends even beyond the desired Planck-scale energy. In order to render this constraint more transparent we rely on a well studied phenomenological model of quantum-gravity-induced birefringence, in which one easily establishes that effects introduced at the Planck scale would amount to values of a dimensionless parameter, denoted by , with respect to the Planck energy which are roughly of order 1. By combining BOOMERanG and WMAP data we estimate at the 68% c.l. Moreover, we forecast on the sensitivity to achievable by future CMB polarization experiments (PLANCK, Spider, EPIC), which, in the absence of systematics, will be at the 1- confidence of (PLANCK), (Spider), and (EPIC) respectively. The cosmic variance-limited sensitivity from CMB is .
16 pages
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