Constraining the Skyrme energy density functional with quantum Monte Carlo calculations

Alessandro Roggero, Abhishek Mukherjee, and Francesco Pederiva
Phys. Rev. C 92, 054303 – Published 9 November 2015

Abstract

We study the problem of an impurity in fully polarized (spin-up) low-density neutron matter with the help of an accurate quantum Monte Carlo method in conjunction with a realistic nucleon-nucleon interaction derived from chiral effective field theory at next-to-next-to leading order. Our calculations show that the behavior of the proton spin-down impurity is very similar to that of a polaron in a fully polarized unitary Fermi gas. We show that our results can be used to put tight constraints on the time-odd parts of the Skyrme energy density functional, independent of the time-even parts, in the density regime relevant to neutron-rich nuclei and compact astrophysical objects such as neutron stars and supernovae.

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  • Received 4 July 2014
  • Revised 4 May 2015

DOI:https://doi.org/10.1103/PhysRevC.92.054303

©2015 American Physical Society

Authors & Affiliations

Alessandro Roggero1,*, Abhishek Mukherjee2,3, and Francesco Pederiva4,5

  • 1Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195, USA
  • 2ECT*, Villa Tambosi, I-38123 Villazzano (Trento), Italy
  • 3ClusterVision B.V., Nieuw-Zeelandweg 15B, 1045 AL, Amsterdam, Netherlands
  • 4Physics Department, University of Trento, via Sommarive 14, I-38123 Trento, Italy
  • 5INFN-TIFPA, Trento Institute for Fundamental Physics and Applications, Trento, Italy

  • *roggero@uw.edu

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Vol. 92, Iss. 5 — November 2015

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