15,216 research outputs found
Parity violation in pre-inflationary bounce
The power suppression at largest scale in the CMB TT powerspectrum might
imply the occurrence of a pre-inflationary bounce. We calculate the circularly
polarized gravitational wave, leaded by the gravitational Chern-Simons term
which universally appears in particle physics and string theory, in an
inflationary background with the pre-inflationary bounce. The circularly
polarized gravitational wave will induce TB and EB correlations at CMB last
scatting surface. We find that although the BB powerspectrum at largest scale
is also suppressed, the TB and EB powerspectra at corresponding scales may be
enhanced.Comment: 15 pages, 4 figures,the final versio
Oscillation in power spectrum of primordial gravitational wave as a signature of higher-order stringy corrections
In low-energy effective string theory, corrections involve the
coupling of the dilaton field to Gauss-Bonnet term. We assume that the dilaton
potential is fine tuned so that the dilaton field may oscillate rapidly for a
while around the minimum of its potential but the inflation background is not
affected. By numerical method, we find that if the dilaton starts to oscillate
at the time of about e-folds before the end of inflation,
correction may bring unusual oscillations to the inflationary
gravitational wave spectrum, which might be measurably imprinted in the CMB
B-mode polarization.Comment: 19 pages, 7 figures; published version in JHEP, many details
supplemented, including 3 appendixes and 1 figure; references and comments
added, presentation improve
Chirality oscillation of primordial gravitational waves during inflation
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.Comment: 14 pages, 11 figures; published version in JHEP; one figure added;
references and comments adde
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