TY - JOUR
T1 - A falsely fat curvaton with an observable running of the spectral tilt
AU - Peloso, Marco
AU - Sorbo, Lorenzo
AU - Tasinato, Gianmassimo
N1 - Academic no longer at University to chase for post-print.
PY - 2014/6/17
Y1 - 2014/6/17
N2 - In slow roll inflation, the running of the spectral tilt is generically proportional to the square of the deviation from scale invariance, αs (ns-1)2, and is therefore currently undetectable. We present a mechanism able to generate a much larger running within slow roll. The mechanism is based on a curvaton field with a large mass term, and a time evolving normalization. This may happen for instance to the angular direction of a complex field in presence of an evolving radial direction. At the price of a single tuning between the mass term and the rate of change of the normalization, the curvaton can be made effectively light at the CMB scales, giving a spectral tilt in agreement with observations. The lightness is not preserved at later times, resulting in a detectable running of the spectral tilt. This mechanism shows that fields with a large mass term do not necessarily decouple from the inflationary physics, and provides a new tool for model building in inflation.
AB - In slow roll inflation, the running of the spectral tilt is generically proportional to the square of the deviation from scale invariance, αs (ns-1)2, and is therefore currently undetectable. We present a mechanism able to generate a much larger running within slow roll. The mechanism is based on a curvaton field with a large mass term, and a time evolving normalization. This may happen for instance to the angular direction of a complex field in presence of an evolving radial direction. At the price of a single tuning between the mass term and the rate of change of the normalization, the curvaton can be made effectively light at the CMB scales, giving a spectral tilt in agreement with observations. The lightness is not preserved at later times, resulting in a detectable running of the spectral tilt. This mechanism shows that fields with a large mass term do not necessarily decouple from the inflationary physics, and provides a new tool for model building in inflation.
KW - cosmological perturbation theory
KW - inflation
KW - RCUK
KW - STFC
KW - ST/H005498/1
UR - http://www.scopus.com/inward/record.url?scp=84902584947&partnerID=8YFLogxK
U2 - 10.1088/1475-7516/2014/06/040
DO - 10.1088/1475-7516/2014/06/040
M3 - Article
AN - SCOPUS:84902584947
SN - 1475-7516
VL - 2014
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 6
M1 - 040
ER -