activity
20232026
most citedRadiation-dominated bouncing model with slow contraction and inflation

3 citations · 3 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2026

Optimising ultra-light dark matter searches with ground-based interferometers

Paola C. M. Delgado, Ornella J. Piccinni, Federico R. Urban

Ultra-light dark matter fields induce nearly monochromatic signals in gravitational-wave detectors through their coupling to the Standard Model. Their spectral morphology exhibits…

hep-ph2026

Dark graviton sensing with magnetically levitated superconductors

Valentina Danieli, Paola C. M. Delgado, Federico R. Urban

Levitated sensors have emerged as a new frontier to detect ultra-light dark matter such as axion-like particles and dark photons. In this work we study how a magnetically levitated…

astro-ph.CO2026

Testing gravitational wave polarizations with LISA

Shingo Akama, Maxence Corman, Paola C. M. Delgado +16

In this paper we quantify the ability of the Laser Interferometer Space Antenna (LISA) to test the presence of non-tensorial polarizations as well as modifications to the tensor on…

gr-qc2025

Constraining the Gravitational Wave Speed in the Early Universe via Gravitational Cherenkov Radiation

Paola C. M. Delgado, Alexander Ganz, Chunshan Lin +1

Scalar particles traveling faster than a subluminal gravitational wave generate gravitons via gravitational Cherenkov radiation. In this paper, we investigate graviton production b…

astro-ph.CO2024

Towards testing the general bounce cosmology with the CMB B-mode auto-bispectrum

Shingo Akama, Giorgio Orlando, Paola C. M. Delgado

It has been shown that a three-point correlation function of tensor perturbations from a bounce model in general relativity with a minimally-coupled scalar field is highly suppress…

gr-qc2023★ 3 cited

Radiation-dominated bouncing model with slow contraction and inflation

Piero A. P. Molinari, Paola C. M. Delgado, Rodrigo F. Pinheiro +1

A very simple non-singular inflationary model is presented where the unique matter content is a radiation fluid. The model slowly contracts from a very large, almost empty and flat…