activity
20222026
most citedA proposal for a low-frequency axion search in the 1-2 eV range and below with the BabyIAXO magnet

28 citations · 74 across the 11 of their papers we have counts for

collaborators

11 papers

hep-ex2026

Resonant heterodyne conversion applied to a low-frequency haloscope for dark matter axion searches in the 1-35 MHz range

Jose R. Navarro-Madrid, José Reina-Valero, Alejandro Díaz-Morcillo +1

We study resonant heterodyne up-conversion in the RADES-BabyIAXO haloscope as a method to search for low-mass dark matter axions using microwave cavities. Starting from axion elect…

astro-ph.IM2026

Global detector network to search for high-frequency gravitational waves (GravNet): conceptual design

Dorian Amaral, Diego Blas, Yuliia Borysenkova +30

We propose GravNet (Global detector network to search for high-frequency gravitational waves), a novel experimental scheme enabling the search for gravitational waves in the MHz to…

hep-ph2026

The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles

Ariel Arza, Deniz Aybas, Shyam Balaji +124

Axions and other very weakly interacting slim particles (WISPs), with masses below 1 GeV, arise naturally in many extensions of the Standard Model of particle physics. In particula…

hep-ph2025

Enhancement of dark-photon haloscope sensitivity with degenerate modes: toward axion-level form factor and polarization determination

Jose R. Navarro-Madrid, José Reina-Valero, Alejandro Díaz-Morcillo +1

The dark photon has been postulated as a potential constituent of dark matter, exhibiting notable similarities to the axion. The primary distinction between the two particles lies…

hep-ex2025

Multiple-cavities interferometric analysis for dark matter axions directional-sensitive search based on signal cross-correlation processing

José Reina-Valero, Alejandro Díaz-Morcillo, Benito Gimeno +5

Current axion detection limits neglect the relevance of the relative velocity between the axion field and the detectors. However, this aspect can lead to a daily modulation of the…

hep-ex2024

Dark Matter Axion Detection with Neural Networks at Ultra-Low Signal-to-Noise Ratio

José Reina-Valero, Alejandro Díaz-Morcillo, José Gadea-Rodríguez +5

We present the first analysis of Dark Matter axion detection applying neural networks for the improvement of sensitivity. The main sources of thermal noise from a typical read-out…

hep-ex2024

High-frequency gravitational waves detection with the BabyIAXO haloscopes

José Reina Valero, Jose R. Navarro Madrid, Diego Blas +4

We present the first analysis using RADES-BabyIAXO cavities as detectors of high-frequency gravitational waves (HFGWs). In particular, we discuss two configurations for distinct fr…

hep-ex2024★ 22 cited

RADES axion search results with a High-Temperature Superconducting cavity in an 11.7 T magnet

S. Ahyoune, A. Álvarez Melcón, S. Arguedas Cuendis +23

We describe the results of a haloscope axion search performed with an 11.7 T dipole magnet at CERN. The search used a custom-made radio-frequency cavity coated with high-temperatur…

hep-ph2023

Study of a cubic cavity resonator for gravitational waves detection in the microwave frequency range

Pablo Navarro, Benito Gimeno, Juan Monzó-Cabrera +2

The direct detection of gravitational waves (GWs) of frequencies above MHz has recently received considerable attention. In this work we present a precise study of the reach of a c…

physics.ins-det2023★ 28 cited

A proposal for a low-frequency axion search in the 1-2 eV range and below with the BabyIAXO magnet

S. Ahyoune, A. Álvarez Melcón, S. Arguedas Cuendis +27

In the near future BabyIAXO will be the most powerful axion helioscope, relying on a custom-made magnet of two bores of 70 cm diameter and 10 m long, with a total available magneti…

hep-ex2022★ 24 cited

Axion Dark Matter

C. B. Adams, N. Aggarwal, A. Agrawal +152

Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a…