activity
20162020
most citedChiral Anomaly, Schwinger Effect, Euler-Heisenberg Lagrangian, and application to axion inflation

82 citations · 82 across the 1 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2020

Deformation of the gravitational wave spectrum by density perturbations

Valerie Domcke, Ryusuke Jinno, Henrique Rubira

We study the effect of primordial scalar curvature perturbations on the propagation of gravitational waves over cosmic distances. We point out that such curvature perturbations def…

astro-ph.CO2020

Resonant backreaction in axion inflation

Valerie Domcke, Veronica Guidetti, Yvette Welling +1

Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which back…

astro-ph.CO2019

Measuring the net circular polarization of the stochastic gravitational wave background with interferometers

Valerie Domcke, Juan Garcia-Bellido, Marco Peloso +4

Parity violating interactions in the early Universe can source a stochastic gravitational wave background (SGWB) with a net circular polarization. In this paper, we study possible…

hep-ph201982 cited

Chiral Anomaly, Schwinger Effect, Euler-Heisenberg Lagrangian, and application to axion inflation

Valerie Domcke, Yohei Ema, Kyohei Mukaida

Particle production in strong electromagnetic fields is a recurring theme in solid state physics, heavy ion collisions, early universe cosmology and formal quantum field theory. In…

hep-ph2019

Baryogenesis from axion inflation

Valerie Domcke, Benedict von Harling, Enrico Morgante +1

The coupling of an axion-like particle driving inflation to the Standard Model particle content through a Chern-Simons term generically sources a dual production of massless helica…

astro-ph.CO2019

The Different Regimes of Axion Gauge Field Inflation

Valerie Domcke, Stefan Sandner

In axion gauge field inflation an axion-like particle driving cosmic inflation is coupled to the Chern-Simons density of an Abelian or non-Abelian gauge group. In the case of a non…