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    Astronomy

    3,185 courses
    GW Detection with Haloscopes
    Galileo Galilei Institute

    GW Detection with Haloscopes

    Axion Quark Nugget Dark Matter Model
    Galileo Galilei Institute

    Axion Quark Nugget Dark Matter Model

    Axions as Solar Thermometers
    Galileo Galilei Institute

    Axions as Solar Thermometers

    Gravitational Instantons, Strong CP Problem and Its Companion Axion Solution
    Galileo Galilei Institute

    Gravitational Instantons, Strong CP Problem and Its Companion Axion Solution

    Axion Bose-Einstein Condensation
    Galileo Galilei Institute

    Axion Bose-Einstein Condensation

    Axion Astrophysical Bounds
    Galileo Galilei Institute

    Axion Astrophysical Bounds

    Gravitational Instantons, Strong CP Problem and Its Companion Axion Solution
    Galileo Galilei Institute

    Gravitational Instantons, Strong CP Problem and Its Companion Axion Solution

    The Piezoaxionic Effect - Dark Matter Detection in Piezoelectric Crystals
    Galileo Galilei Institute

    The Piezoaxionic Effect - Dark Matter Detection in Piezoelectric Crystals

    Data Taking and Analysis with the IAXO Pathfinder System
    Galileo Galilei Institute

    Data Taking and Analysis with the IAXO Pathfinder System

    Axion Mass from Magnetic Monopole Loops
    Galileo Galilei Institute

    Axion Mass from Magnetic Monopole Loops

    Detector Development for Solar Axion Searches
    Galileo Galilei Institute

    Detector Development for Solar Axion Searches

    Experimental Searches for Axion Dark Matter - Overview
    Galileo Galilei Institute

    Experimental Searches for Axion Dark Matter - Overview

    Wire Metamaterials for Axion Search - ALPHA
    Galileo Galilei Institute

    Wire Metamaterials for Axion Search - ALPHA

    Topological Defects of Light Bosons
    Galileo Galilei Institute

    Topological Defects of Light Bosons

    Nuclear Decay Anomalies as a Signature of Axion Dark Matter
    Galileo Galilei Institute

    Nuclear Decay Anomalies as a Signature of Axion Dark Matter

    How Observations May Tell Axions and WIMPs Apart
    Galileo Galilei Institute

    How Observations May Tell Axions and WIMPs Apart

    Wave Dark Matter
    Galileo Galilei Institute

    Wave Dark Matter

    Axions and Where to Find Them - New Elements for the Identikit
    Galileo Galilei Institute

    Axions and Where to Find Them - New Elements for the Identikit

    The Echo Method for Axion Dark Matter Detection
    Galileo Galilei Institute

    The Echo Method for Axion Dark Matter Detection

    Axion Kinetic Misalignment - What Is It, What Does It Do, and How Do You Get It?
    Galileo Galilei Institute

    Axion Kinetic Misalignment - What Is It, What Does It Do, and How Do You Get It?

    The Axion Background
    Galileo Galilei Institute

    The Axion Background