New Clues on Twin Neutron Stars and the Extreme Physics Inside
Scientists have new insights into factors that determine how twin neutron stars—stars with the same mass but different sizes and compositions—can coexist.
Scientists have new insights into factors that determine how twin neutron stars—stars with the same mass but different sizes and compositions—can coexist.
Theoretical calculations enable more accurate determination of reaction rates for modelling primordial lithium-6 abundance and massive stars’ lifecycle.
Remarkably, the rate of proton-proton fusion in the sun is not precisely understood, but it can be better predicted using the process of triton decay.
Researchers imaged individual barium ions in dense xenon gas, offering a new path toward ultra-low-background searches for neutrinoless double beta decay.
Calculations of charge distribution in mesons provide a benchmark for experimental measurements and validate widely used 'factorization' method.
Precise measurement of beryllium-7 nuclear decay recoils directly probes the quantum properties of the neutrino for the first time.
Theorists show gluon fields characterizing gluon saturation can describe a universal pattern of particle emissions—a manifestation of asymptotic symmetry.
Successfully modeling chromium-62 hints at an interesting structure for neutron-laden calcium-60.
Data show the distribution of gluon “glue” in protons and neutrons changes when they are bound together in nuclei.
Scientists use high-energy heavy ion collisions in a new way to reveal subtleties of nuclear structure with implications for many areas of physics.
A Subatomic Challenge Resolved: Supercomputer Calculations Produce the First Accurate Theoretical View of the Sigma Meson
Theorists identify new effects needed to compute the nuclear beta decay rate with a precision of a few parts in ten thousand.