paper

Chirality oscillation of primordial gravitational waves during inflation

arXiv:1608.06508 · doi:10.1007/JHEP03(2017)024

Abstract

We show that if the gravitational Chern-Simons term couples to a massive scalar field (), the primordial gravitational waves (GWs) will show itself the chirality oscillation, i.e., the amplitudes of the left- and right-handed GWs modes will convert into each other and oscillate in their propagations. This oscillation will eventually develop a permanent difference of the amplitudes of both modes, which leads to nearly opposite oscillating shapes in the power spectra of the left- and right-handed primordial GWs. We discuss its implication to the CMB B-mode polarization.

14 pages, 11 figures; published version in JHEP; one figure added; references and comments added

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