The DarkSide-50 experiment, using a liquid argon time projection chamber, searched for annual modulation in dark matter signals but found no significant evidence, despite reaching unprecedented low-energy thresholds.
The presence of dark matter in neutron stars could lead to biased interpretations of their equation of state from gravitational wave observations, but the Einstein Telescope likely won't be sensitive enough to definitively detect dark matter through this method.
This paper presents a novel unitary evolution solution for calculating particle conversion probabilities, particularly relevant for scenarios where the widely used WKB approximation fails, such as dark photon dark matter conversion into gravitational waves in the solar magnetic field.
The SABRE South experiment, with its ultra-pure NaI(Tl) crystals and active background rejection system, aims to definitively test the DAMA/LIBRA dark matter signal by achieving unprecedentedly low background levels and operating in the Southern Hemisphere.
This paper presents a comprehensive summary of the ATLAS Collaboration's searches for fermionic dark matter candidates using simplified models with an s-channel mediator, utilizing up to 140 fb−1 of proton-proton collision data at √s = 13 TeV from the LHC Run 2.
This paper proposes a novel mechanism involving a first-order phase transition (FOPT) to generate the correct relic abundance of light thermal dark matter (DM) while enhancing its direct detection prospects.
Researchers have developed an innovative tuning method using auxetic materials to effectively utilize higher-order resonant modes in cavity haloscopes, significantly improving the sensitivity of dark matter axion searches in high-frequency ranges.
While often overlooked, heavy, strongly interacting dark matter could pose a radiation hazard to humans, particularly in space, and existing and future experiments could be used to constrain or detect this type of dark matter.
This paper proposes that a significant portion of dark matter could be composed of low-scale mirror Standard Model particles, detectable through gravitational waves generated by their phase transition and by analyzing the bow shock of the Guitar Nebula.
This chapter explores the use of Imaging Atmospheric Cherenkov Telescopes (IACTs) in searching for Weakly Interacting Massive Particles (WIMPs), a leading candidate for dark matter, through their gamma-ray signatures from annihilation or decay in various astrophysical targets.