Dark Matter, Neutrino Physics, and Compact Object Astrophysics
This research community investigates the fundamental constituents of the universe, focusing on the detection of dark matter, the properties of neutrinos, and the behavior of compact objects like neutron stars and black holes.
The work centers on direct detection experiments using liquid xenon, liquid argon, and liquid scintillator detectors to search for dark matter particles and neutrinoless double beta decay. It also encompasses the study of neutron star mergers, white dwarf evolution, and gravitational wave sources. Recurring methodologies include time projection chambers, cross-section measurements, and the application of machine learning to large-scale astronomical datasets. The research frequently addresses the Standard Model of particle physics, cosmic ray interactions, and the formation of massive stars within the Milky Way and globular clusters.
The community is most prominent in research tracked for Helium, representing 8.9% of all Helium-related papers, and Xenon, accounting for 7.8% of Xenon research. It also holds a significant share of Argon research at 5.1%.
The community comprises 50,289 papers, published primarily in The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society, and Astronomy and Astrophysics.
Recent work includes the Atacama Cosmology Telescope’s constraints on cosmological models, updates to the Standard Model’s description of the muon’s magnetic moment, and dark matter searches using the XENONnT and LZ experiments.