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A limit on the detectability of the energy scale of inflation

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arxiv astro-ph/0202286 v1 pith:SWGA4FUZ submitted 2002-02-15 astro-ph hep-ph

classification astro-phhep-ph
keywords inflationcurldensitydetectabilityenergygravityperturbationspolarization
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We show that the polarization of the cosmic microwave background can be used to detect gravity waves from inflation if the energy scale of inflation is above 3.2 times 10^15 GeV. These gravity waves generate polarization patterns with a curl, whereas (to first order in perturbation theory) density perturbations do not. The limiting ``noise'' arises from the second--order generation of curl from density perturbations, or rather residuals from its subtraction. We calculate optimal sky coverage and detectability limits as a function of detector sensitivity and observing time.

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