Low-energy theory for superfluid and solid matter and its application to the neutron star crust

Type: Article

Publication Date: 2011-10-27

Citations: 31

DOI: https://doi.org/10.1103/physrevc.84.045809

Abstract

We formulate a low-energy effective theory describing phases of matter that are both solid and superfluid. These systems simultaneously break translational symmetry and the phase symmetry associated with particle number. The symmetries restrict the combinations of terms that can appear in the effective action and the lowest order terms featuring equal number of derivatives and Goldstone fields are completely specified by the thermodynamic free energy or, equivalently, by the long-wavelength limit of static correlation functions in the ground state. We show that the underlying interaction between particles that constitute the lattice and the superfluid gives rise to entrainment, and mixing between the Goldstone modes. As a concrete example we discuss the low-energy theory for the inner crust of a neutron star, where a lattice of ionized nuclei coexists with a neutron superfluid.

Locations

  • Physical Review C - View - PDF
  • arXiv (Cornell University) - View - PDF
  • OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) - View
  • DataCite API - View

Similar Works

Action Title Year Authors
+ PDF Chat Generalized equation of state for cold superfluid neutron stars 2011 N. Chamel
John Pearson
S. Goriely
E. Göğüş
Ünal Ertan
T. Belloni
+ PDF Chat Long-wavelength phonons in the crystalline and pasta phases of neutron-star crusts 2018 David Durel
Mi­chael Urban
+ PDF Chat A minimal model for finite temperature superfluid dynamics 2013 Nils Andersson
C. Krüger
G. L. Comer
Lars Samuelsson
+ PDF Chat Time-dependent nuclear energy-density functional theory toolkit for neutron star crust: Dynamics of a nucleus in a neutron superfluid 2024 Daniel Pęcak
Agata Zdanowicz
N. Chamel
Piotr Magierski
Gabriel Wlazłowski
+ PDF Chat Superfluid Density of Neutrons in the Inner Crust of Neutron Stars: New Life for Pulsar Glitch Models 2017 Gentaro Watanabe
C. J. Pethick
+ Terrestrial and Astrophysical Superfluidity: Cold Atoms and Neutron Matter 2011 Alexandros Gezerlis
J. Carlson
+ PDF Chat Elementary excitations in homogeneous superfluid neutron star matter: Role of the neutron-proton coupling 2017 M. Baldo
C. Ducoin
+ PDF Chat The dynamics of neutron star crusts: Lagrangian perturbation theory for a relativistic superfluid-elastic system 2019 Nils Andersson
B. Haskell
G. L. Comer
Lars Samuelsson
+ PDF Chat Elementary excitations in homogeneous superfluid neutron star matter: Role of the proton component 2011 M. Baldo
C. Ducoin
+ PDF Chat Nucleus-nucleus interactions in the inner crust of neutron stars 2016 D. Kobyakov
C. J. Pethick
+ Neutron Matter from Low to High Density 2015 Stefano Gandolfi
Alexandros Gezerlis
J. Carlson
+ PDF Chat Superfluidity and neutron star crust matter 1996 Ø. Elgarøy
L. Engvik
E. Osnes
Fabio Vittorio De Blasio
M. Hjorth‐Jensen
G. Lazzari
+ PDF Chat Fermionic superfluidity: from cold atoms to neutron stars 2022 Annette Lopez
P.M. Kelly
Kaelyn Dauer
Ettore Vitali
+ NEWTONIAN MECHANICS OF NEUTRON SUPERFLUID IN ELASTIC STAR CRUST 2006 Brandon Carter
Elie Chachoua
+ PDF Chat Neutron matter: a superfluid gas 2004 Siyuan Chang
J. Morales
V. R. Pandharipande
D. G. Ravenhall
J. Carlson
Steven C. Pieper
R. B. Wiringa
K. E. Schmidt
+ PDF Chat Relativistic mechanics of neutron superfluid in (magneto)elastic star crust 2006 Brandon Carter
Lars Samuelsson
+ Goldstone modes in the neutron star core 2014 Paulo F. Bedaque
Sanjay Reddy
+ PDF Chat Towards real neutron star seismology: accounting for elasticity and superfluidity 2011 Andrea Passamonti
Nils Andersson
+ PDF Chat Superfluidity in neutron stars and cold atoms 2007 A. Schwenk
+ PDF Chat A realistic model of superfluidity in the neutron star inner crust 2007 M. Baldo
É. E. Saperstein
S. V. Tolokonnikov