activity
20172020
most citedNonlocal effective actions in semiclassical gravity: thermal effects in stationary geometries

5 citations · 5 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2020

Scalar-tensor cosmologies without screening

Johannes Noller, Luca Santoni, Enrico Trincherini +1

Scalar-tensor theories are frequently only consistent with fifth force constraints in the presence of a screening mechanism, namely in order to suppress an otherwise unacceptably l…

hep-th2020

Hairy Black-holes in Shift-symmetric Theories

Paolo Creminelli, Nicolás Loayza, Francesco Serra +2

Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem of Hui and Nicolis, assuming spherical symmetry, time-independence of the scalar…

hep-th2019

To the sphere and back again: de Sitter infrared correlators at NTLO in 1/N

Diana López Nacir, Francisco D. Mazzitelli, Leonardo G. Trombetta

We analyze the infrared behavior of the two and four-point functions for the massless model in Lorentzian de Sitter spacetime, using the expansion. Our approach is bas…

hep-th2018

Long distance behavior of -model correlators in de Sitter space and the resummation of secular terms

Diana López Nacir, Francisco D. Mazzitelli, Leonardo G. Trombetta

We analyze the long distance behavior of the two-point functions for an interacting scalar model in de Sitter spacetime. Following our previous work, this behavior is analyz…

hep-th2018

Behind Horndeski: Structurally Robust Higher Derivative EFTs

Luca Santoni, Enrico Trincherini, Leonardo G. Trombetta

Higher derivative scalar interactions can give rise to interesting cosmological scenarios. We present a complete classification of such operators that can yield sizeable effects wi…

hep-th20175 cited

Nonlocal effective actions in semiclassical gravity: thermal effects in stationary geometries

M. Elías, F. D. Mazzitelli, L. G. Trombetta

We compute the gravitational effective action by integrating out quantum matter fields in a weak gravitational field, using the Schwinger-Keldysh (in-in) formalism. We pay particul…