arXiv · 1310.4059
Collective excitations in neutron-star crusts
Abstract
We explore the spectrum of low-energy collective excitations in the crust of a neutron star, especially in the inner region where neutron-proton clusters are immersed in a sea of superfluid neutrons. The speeds of the different modes are calculated systematically from the nuclear energy density functional theory using a Skyrme functional fitted to essentially all experimental atomic mass data.
Explore related subjects
Keep this discovery
N. Chamel, D. Page, S. Reddy. 2013-10-15. Collective excitations in neutron-star crusts. https://arxiv.org/abs/1310.4059
Cite the original work for its findings. Save a collection to share your selection of sources.