Static Response of Neutron Matter

Mateusz Buraczynski and Alexandros Gezerlis
Phys. Rev. Lett. 116, 152501 – Published 11 April 2016

Abstract

We generalize the problem of strongly interacting neutron matter by adding a periodic external modulation. This allows us to study from first principles a neutron system that is extended and inhomogeneous, with connections to the physics of both neutron-star crusts and neutron-rich nuclei. We carry out fully nonperturbative microscopic quantum Monte Carlo calculations of the energy of neutron matter at different densities, as well as different strengths and periodicities of the external potential. In order to remove systematic errors, we examine finite-size effects and the impact of the wave function ansatz. We also make contact with energy-density functional theories of nuclei and disentangle isovector gradient contributions from bulk properties. Finally, we calculate the static density-density linear response function of neutron matter and compare it with the response of other physical systems.

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  • Received 5 November 2015

DOI:https://doi.org/10.1103/PhysRevLett.116.152501

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Mateusz Buraczynski and Alexandros Gezerlis

  • Department of Physics, University of Guelph, Guelph, ON N1G 2W1, Canada

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Issue

Vol. 116, Iss. 15 — 15 April 2016

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