activity
20012022
most citedFeatures of heavy physics in the CMB power spectrum

383 citations · 3k across the 62 of their papers we have counts for

collaborators

62 papers

hep-ph2022★ 2 cited

Snowmass Theory Frontier: Astrophysics and Cosmology

Daniel Green, Joshua T. Ruderman, Benjamin R. Safdi +84

We summarize progress made in theoretical astrophysics and cosmology over the past decade and areas of interest for the coming decade. This Report is prepared as the TF09 "Astrophy…

astro-ph.CO2022★ 79 cited

Inflation: Theory and Observations

Ana Achúcarro, Matteo Biagetti, Matteo Braglia +19

Cosmic inflation provides a window to the highest energy densities accessible in nature, far beyond those achievable in any realistic terrestrial experiment. Theoretical insights i…

hep-th2021★ 1 cited

The hand-made tail: Non-perturbative tails from multifield inflation

Ana Achucarro, Sebastian Cespedes, Anne-Christine Davis +1

It is becoming increasingly clear that large but rare fluctuations of the primordial curvature field, controlled by the tail of its probability distribution, could have dramatic ef…

astro-ph.CO2021

Primordial gravitational waves from excited states

Jacopo Fumagalli, Gonzalo A. Palma, Sébastien Renaux-Petel +3

We show that a scalar excited state with large occupation numbers during inflation leads to an enhancement of tensor modes and a characteristic pattern of order-one oscillations in…

astro-ph.IM2021★ 42 cited

Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency Bands

Sumit Dahal, John W. Appel, Rahul Datta +37

The Cosmology Large Angular Scale Surveyor (CLASS) observes the polarized cosmic microwave background (CMB) over the angular scales of 1 90 with the…

hep-th2020★ 10 cited

Unifying attractor and non-attractor models of inflation under a single soft theorem

Rafael Bravo, Gonzalo A. Palma

We study the generation of local non-Gaussianity in models of canonical single field inflation when their backgrounds are either attractor or non-attractor. We show that the invari…