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.
- Received 4 July 2014
- Revised 4 May 2015
DOI:https://doi.org/10.1103/PhysRevC.92.054303
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