activity
20242026
collaborators

11 papers

astro-ph.CO2026

Axion Inflation: Perturbative control in the strong backreaction regime

Valerie Domcke, Alexandros Papageorgiou, Marco Peloso +1

We study the strong backreaction regime in axion inflation, in which the friction from Abelian gauge fields generated via the pseudo-scalar interaction $\fracβ{4 M_p} ϕF {\tilde…

astro-ph.CO2026

Primordial black hole dark matter from axion inflation

Gabriele Franciolini, Nadir Ijaz, Marco Peloso

We revisit the production of primordial black holes (PBHs) by a U(1) gauge field with a pseudo-scalar coupling to the inflaton. We improve upon the existing literature by working i…

astro-ph.CO2026

Revisiting the Chern-Simons interaction during inflation with a non-canonical pseudo-scalar

Jun'ya Kume, Marco Peloso, Nicola Bartolo

A Chern-Simons interaction between a pseudo-scalar field and a U(1) gauge field results in the generation of a chiral gravitational wave background. The detection of this signal is…

gr-qc2026

Challenges and Opportunities of Gravitational Wave Searches above 10 kHz

Nancy Aggarwal, Odylio D. Aguiar, Diego Blas +34

The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges…

astro-ph.CO2025

Axion inflation in the regime of homogeneous backreaction

Matteo Barbon, Nadir Ijaz, Marco Peloso

We investigate the Stochastic Gravitational Wave Background (SGWB) produced in models of axion inflation coupled to gauge fields. Achieving a detectable signal at Pulsar Timing Arr…

astro-ph.CO2025

Strong scale-dependence does not enhance the kinematic boosting of gravitational wave backgrounds

Giorgio Mentasti, Carlo R. Contaldi, Marco Peloso

Existing expressions in the literature appear to indicate that Doppler boosting, due to our proper motion with respect to the isotropic frame of the universe, can amplify stochasti…