Baym–Pines model of neutron stars

E1937663 UNEXPLORED

The Baym–Pines model of neutron stars is a theoretical framework that describes how the elastic crust and internal structure of neutron stars respond to stresses, rotation, and deformations.

Try in SPARQL Jump to: Surface forms Referenced by

All labels observed (1)

Label Occurrences
Baym–Pines model of neutron stars canonical 1

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Gordon Baym notableWork Baym–Pines model of neutron stars