Machine Learning Predictions Successfully Model Atomic Masses of Nuclide Chart

A Los Alamos simulation of an accretion disk after the collision of two neutron stars.

The origin of heavy elements in our universe is theorized to be the result of neutron star collisions, which produce conditions hot and dense enough for free neutrons to merge with atomic nuclei and form new elements in a split-second window of time. Testing this theory and answering other astrophysical questions requires predictions for a vast range of masses of atomic nuclei. Los Alamos National Laboratory scientists are front and center in using machine learning algorithms (an application of artificial intelligence) to successfully model the atomic masses of the entire nuclide chart — the combination of all possible protons and neutrons that defines elements and their isotopes.

The post Machine Learning Predictions Successfully Model Atomic Masses of Nuclide Chart appeared first on HPCwire.

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