We propose a new broadband search strategy for ultralight axion dark matter covering fifteen orders of magnitude in mass, including astrophysically long-ranged fuzzy dark matter.
We propose an approach to search for axion dark matter with a superconducting radio frequency cavity, using axion-induced transitions between nearly degenerate resonant modes of frequency $\sim \text{GHz}$.
We introduce new IRC-safe counting observables whose discrimination performance exceeds that of jet mass and approaches that of track multiplicity.
We introduce a broad class of fractal jet observables that recursively probe the collective properties of hadrons produced in jet fragmentation.
We use the stochastic thermodynamics of Markov jump processes to compute the minimum rate at which energy must be supplied and dissipated to maintain an arbitrary nonequilibrium distribution in a given energy landscape.