Higgs-Dilaton Cosmology: an effective field theory approach - INSPIRE

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Higgs-Dilaton Cosmology: an effective field theory approach

Fedor Bezrukov
(
- Connecticut U. and
- RIKEN BNL
)
,
Georgios K. Karananas
(
- Natl. Tech. U., Athens and
- IPT, Lausanne
)
,
Javier Rubio
(
- IPT, Lausanne
)
,
Mikhail Shaposhnikov
(
- IPT, Lausanne
)

Dec, 2012

17 pages

Published in:

Phys.Rev.D 87 (2013) 9, 096001

Published: May 1, 2013

e-Print:

1212.4148 [hep-ph]

DOI:

10.1103/PhysRevD.87.096001

Report number:

RBRC-1007

View in:

ADS Abstract Service

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Abstract: (APS)

The Higgs-dilaton cosmological model is able to describe simultaneously an inflationary expansion in the early Universe and a dark energy dominated stage responsible for the present day acceleration. It also leads to a nontrivial relation between the spectral tilt of scalar perturbations ns and the dark energy equation of state ω. We study the self-consistency of this model from an effective field theory point of view. Taking into account the influence of the dynamical background fields, we determine the effective cutoff of the theory, which turns out to be parametrically larger than all the relevant energy scales from inflation to the present epoch. We finally formulate the set of assumptions needed to estimate the amplitude of the quantum corrections in a systematic way and show that the connection between ns and ω remains unaltered if these assumptions are satisfied.

Note:

typos corrected, references and appendix added, published version

95.36.+x
11.30.-j
11.10.Gh
98.80.Cq
dark energy: equation of state
perturbation: scalar
correction: quantum
effective field theory
cosmological model
inflation

References(64)

Figures(11)

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