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Highlights

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False color plot showing the density of the mass in the equatorial (bottom) and meridional, or “southern” (top) planes of a neutron star merger remnant about 100 milliseconds after the merger.

What Happens to the Remains of Neutron Star Mergers?

Simulations of massive neutron star merger remnants reveal their structure and early evolution as they cool down by emitting neutrinos.

Top: protons striking a nucleus deflect from their original path depending on velocity, location of impact, and force from the protons inside the nucleus. Bottom: elastic proton scattering cross sections from oxygen-16 at different orders of magnitude.

Ab Initio Methods Help Scientists Make Sense of Complex Particle Collisions

Research finds ab initio effective field theories are useful for calculating how nucleons scatter from collisions of atomic nuclei.

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