0000000000286750

AUTHOR

Hector Masia-roig

showing 5 related works from this author

Intensity interferometry for ultralight bosonic dark matter detection

2023

Ultralight bosonic dark matter (UBDM) can be described by a classical wave-like field oscillating near the Compton frequency of the bosons. If a measurement scheme for the direct detection of UBDM interactions is sensitive to a signature quadratic in the field, then there is a near-zero-frequency (dc) component of the signal. Thus, a detector with a given finite bandwidth can be used to search for bosons with Compton frequencies many orders of magnitude larger than its bandwidth. This opens the possibility of a detection scheme analogous to Hanbury Brown and Twiss intensity interferometry. Assuming that the UBDM is virialized in the galactic gravitational potential, the random velocities pr…

High Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)FOS: Physical sciencesAstrophysics - Cosmology and Nongalactic AstrophysicsHigh Energy Physics - ExperimentPhysics - Atomic PhysicsPhysical Review
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Analysis method for detecting topological defect dark matter with a global magnetometer network

2019

Abstract The Global Network of Optical Magnetometers for Exotic physics searches (GNOME) is a network of time-synchronized, geographically separated, optically pumped atomic magnetometers that is being used to search for correlated transient signals heralding exotic physics. GNOME is sensitive to exotic couplings of atomic spins to certain classes of dark matter candidates, such as axions. This work presents a data analysis procedure to search for axion dark matter in the form of topological defects: specifically, walls separating domains of discrete degenerate vacua in the axion field. An axion domain wall crossing the Earth creates a distinctive signal pattern in the network that can be d…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)Spins010308 nuclear & particles physicsMagnetometerDark matterFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesTopological defectlaw.inventionDomain wall (string theory)Space and Planetary Sciencelaw0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)GnomeAstrophysics - Cosmology and Nongalactic Astrophysics
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Characterization of the global network of optical magnetometers to search for exotic physics (GNOME)

2018

The Global Network of Optical Magnetometers to search for Exotic physics (GNOME) is a network of geographically separated, time-synchronized, optically pumped atomic magnetometers that is being used to search for correlated transient signals heralding exotic physics. The GNOME is sensitive to nuclear- and electron-spin couplings to exotic fields from astrophysical sources such as compact dark-matter objects (for example, axion stars and domain walls). Properties of the GNOME sensors such as sensitivity, bandwidth, and noise characteristics are studied in the present work, and features of the network's operation (e.g., data acquisition, format, storage, and diagnostics) are described. Charac…

PhysicsQuantum PhysicsPhysics - Instrumentation and DetectorsAtomic Physics (physics.atom-ph)010308 nuclear & particles physicsMagnetometerBandwidth (signal processing)FOS: Physical sciencesAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)01 natural sciencesPhysics - Atomic Physicslaw.inventionStarsData acquisitionSpace and Planetary Sciencelaw0103 physical sciencesGlobal networkQuantum Physics (quant-ph)010306 general physicsAxionTransient signalGnomeRemote sensingPhysics of the Dark Universe
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A machine learning algorithm for direct detection of axion-like particle domain walls

2021

The Global Network of Optical Magnetometers for Exotic physics searches (GNOME) conducts an experimental search for certain forms of dark matter based on their spatiotemporal signatures imprinted on a global array of synchronized atomic magnetometers. The experiment described here looks for a gradient coupling of axion-like particles (ALPs) with proton spins as a signature of locally dense dark matter objects such as domain walls. In this work, stochastic optimization with machine learning is proposed for use in a search for ALP domain walls based on GNOME data. The validity and reliability of this method were verified using binary classification. The projected sensitivity of this new analy…

Space and Planetary SciencePhysics - Data Analysis Statistics and ProbabilityFOS: Physical sciencesddc:530Astronomy and AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Data Analysis Statistics and Probability (physics.data-an)Physics::Geophysics
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Search for topological defect dark matter with a global network of optical magnetometers

2021

Ultralight bosons such as axion-like particles are viable candidates for dark matter. They can form stable, macroscopic field configurations in the form of topological defects that could concentrate the dark matter density into many distinct, compact spatial regions that are small compared with the Galaxy but much larger than the Earth. Here we report the results of the search for transient signals from the domain walls of axion-like particles by using the global network of optical magnetometers for exotic (GNOME) physics searches. We search the data, consisting of correlated measurements from optical atomic magnetometers located in laboratories all over the world, for patterns of signals p…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsAtomic Physics (physics.atom-ph)Particle physicsGeneral Physics and AstronomyFOS: Physical sciences53001 natural sciencesArticleHigh Energy Physics - ExperimentPhysics - Atomic PhysicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesDark energy and dark matterddc:530Atomic and molecular physics010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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