TY - JOUR
T1 - Resilience of the standard predictions for primordial tensor modes
AU - Creminelli, Paolo
AU - Gleyzes, Jérôme
AU - Noreña, Jorge
AU - Vernizzi, Filippo
N1 - Publisher Copyright:
© 2014 American Physical Society.
PY - 2014/12/3
Y1 - 2014/12/3
N2 - We show that the prediction for the primordial tensor power spectrum cannot be modified at leading order in derivatives. Indeed, one can always set to unity the speed of propagation of gravitational waves during inflation by a suitable disformal transformation of the metric, while a conformal one can make the Planck mass time independent. Therefore, the tensor amplitude unambiguously fixes the energy scale of inflation. Using the effective field theory of inflation, we check that predictions are independent of the choice of frame, as expected. The first corrections to the standard prediction come from two parity violating operators with three derivatives. Also the correlator 〈γγγ〉 is standard and only receives higher derivative corrections. These results hold also in multifield models of inflation and in alternatives to inflation and make the connection between a (quasi-)scale-invariant tensor spectrum and inflation completely robust.
AB - We show that the prediction for the primordial tensor power spectrum cannot be modified at leading order in derivatives. Indeed, one can always set to unity the speed of propagation of gravitational waves during inflation by a suitable disformal transformation of the metric, while a conformal one can make the Planck mass time independent. Therefore, the tensor amplitude unambiguously fixes the energy scale of inflation. Using the effective field theory of inflation, we check that predictions are independent of the choice of frame, as expected. The first corrections to the standard prediction come from two parity violating operators with three derivatives. Also the correlator 〈γγγ〉 is standard and only receives higher derivative corrections. These results hold also in multifield models of inflation and in alternatives to inflation and make the connection between a (quasi-)scale-invariant tensor spectrum and inflation completely robust.
UR - http://www.scopus.com/inward/record.url?scp=84918504707&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.113.231301
DO - 10.1103/PhysRevLett.113.231301
M3 - Article
AN - SCOPUS:84918504707
SN - 0031-9007
VL - 113
JO - Physical Review Letters
JF - Physical Review Letters
IS - 23
M1 - 231301
ER -