activity
20242026
collaborators

5 papers

hep-ph2026

Stochastic galactic supernova flux of semi-relativistic particles

David Alonso-González, David Cerdeño, Marina Cermeño +1

New exotic particles with MeV masses, such as axion-like particles or light dark matter, can be emitted from core-collapse supernovae (SNe) with semi-relativistic velocities. Due t…

hep-ph2025

Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors

David Alonso-González, David Cerdeño, Marina Cermeño +1

In this article, we claim that axion-like particles (ALPs) with MeV masses can be produced with semi-relativistic velocities in core-collapse supernovae (SNe), generating a diffuse…

hep-ph2025

Bayesian technique to combine independently-trained Machine-Learning models applied to direct dark matter detection

David Cerdeno, Martin de los Rios, Andres D. Perez

We carry out a Bayesian analysis of dark matter (DM) direct detection data to determine particle model parameters using the Truncated Marginal Neural Ratio Estimation (TMNRE) machi…

astro-ph.IM2025

Insights into Dark Matter Direct Detection Experiments: Decision Trees versus Deep Learning

Daniel E. Lopez-Fogliani, Andres D. Perez, Roberto Ruiz de Austri

The detection of Dark Matter (DM) remains a significant challenge in particle physics. This study exploits advanced machine learning models to improve detection capabilities of liq…

hep-ph2024

Disentangling axion-like particle couplings to nucleons via a delayed signal in Super-Kamiokande from a future supernova

David Alonso-González, David Cerdeño, Marina Cermeño +1

In this work, we show that, if axion-like particles (ALPs) from core-collapse supernovae (SNe) couple to protons, they would produce very characteristic signatures in neutrino wate…