Matter inside neutron stars can have different forms: a dense liquid of nucleons or a dense liquid of quarks.
Matter inside neutron stars can have different forms: a dense liquid of nucleons or a dense liquid of quarks.
Researchers examine the structure of the low-energy nuclear states of carbon-12 using nuclear lattice effective field theory.
Scientists translate predictions of hydrodynamics into experimentally observable particle patterns.
UC Irvine Earth system scientists and data scientists led the development of the high-fidelity tool
G.P. Li and David Reinkensmeyer recognized for beneficial innovations
Simulations of binary neutron star mergers suggest that future detectors will distinguish between different models of hot nuclear matter.
Jets of particles in quark-gluon plasma from heavy-ion collisions lose energy via radiation, but how they radiate energy depends on the jet’s structure.
Theorists predict differential distribution of 'up' and 'down' quarks within protons—and differential contributions to the proton's properties.
The campus began exploring artificial intelligence in the mid-1960s
Novel techniques allow the first direct observation of a predicted effect that results in the suppression of gluon radiation emitted by a heavy quark.