How Large Are Neutron Stars?
Data from the first observation of a neutron-star collision combined with input from modern nuclear theory narrow the range of neutron star radii.
Data from the first observation of a neutron-star collision combined with input from modern nuclear theory narrow the range of neutron star radii.
Observation of impulsive stimulated X-ray Raman scattering with attosecond soft X-ray pulses.
Crystals grown from layers of atoms arrange themselves on semiconductor surfaces to add new capabilities.
A new analysis provides a clearer picture of the universe by considering the yield of fast particles in grazing versus head-on nuclear collisions.
Transport effects raise the density in the plasma core
Swarms of synchronized active spinning particles exhibit complex collective behavior, ranging from liquid-like states to dynamic crystals.
New approaches shed light on arctic soil microbes and their potential to release greenhouse gases when permafrost thaws.
New measurements offer insights into binding interactions that glue fundamental building blocks of matter together.
Measurements of the electromagnetic properties of radioactive antimony-129 provide unique insight into the nature of the proton-neutron interaction and nuclear shapes.
New research and newly implemented techniques expand scientific understanding of isotopes whose nuclei have the “magic numbers” of less than 82 protons and more than 126 neutrons.
SEER, a new method to rapidly search for proteins involved in rearranging DNA molecules, increases genome editing efficiency.
Environmental factors can change interactions among microorganism communities.