Author:
Aja Beatriz,Arguedas Cuendis Sergio,Arregui Ivan,Artal Eduardo,Barreiro R. Belén,Casas Francisco J.,de Ory Marina C.,Díaz-Morcillo Alejandro,de la Fuente Luisa,Gallego Juan Daniel,García-Barceló Jose María,Gimeno Benito,Gomez Alicia,Granados Daniel,Kavanagh Bradley J.,Laso Miguel A.G.,Lopetegi Txema,Lozano-Guerrero Antonio José,Magaz Maria T.,Martín-Pintado Jesús,Martínez-González Enrique,Miralda-Escudé Jordi,Monzó-Cabrera Juan,Najarro de la Parra Francisco,Navarro-Madrid Jose R.,Nuñez Chico Ana B.,Pascual Juan Pablo,Pelegrin Jorge,Peña Garay Carlos,Rodriguez David,Socuéllamos Juan M.,Teberio Fernando,Teniente Jorge,Vielva Patricio,Vila Iván,Vilar Rocío,Villa Enrique
Abstract
AbstractWe propose a novel experiment, the Canfranc Axion Detection Experiment (CADEx), to probe dark matter axions with masses in the range 330–460μeV, within the W-band (80–110 GHz), an unexplored parameter space in the well-motivated dark matter window of Quantum ChromoDynamics (QCD) axions. The experimental design consists of a microwave resonant cavity haloscope in a high static magnetic field coupled to a highly sensitive detecting system based on Kinetic Inductance Detectors via optimized quasi-optics (horns and mirrors). The experiment is in preparation and will be installed in the dilution refrigerator of the Canfranc Underground Laboratory. Sensitivity forecasts for axion detection with CADEx, together with the potential of the experiment to search for dark photons, are presented.
Subject
Astronomy and Astrophysics
Cited by
18 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献