Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Lettere al nuovo cimento della societa italiana di fisica/Lettere al nuovo cimento

Superfluid ground state of neutron matter and other strongly interacting many-fermion systems

J. W. Clark, C.-H. Yang

Published Feb 1, 1970• 18 citations
Publisher
DOI
10.1007/bf02755910

Related papers

Superfluidity in Strongly Interacting Fermi Systems with Applications to Neutron Stars

V.V. Khodel

•Jan 1, 1997•0 citations

Pairing in strongly correlated Fermi gases: Superfluidity in cold gases and neutron matter

Heng Fan, E. Krotscheck

•Jan 1, 2017•0 citations

On the superfluid state of strongly-interacting fermions

P. Szépfalusy

Il Nuovo Cimento•Oct 1, 1963•1 citation

Vortex line in the unitary Fermi gas

Lucas Madeira, S. A. Vitiello, Stefano Gandolfi +1 more

We report diffusion Monte Carlo results for the ground state of unpolarized spin-1/2 fermions in a cylindrical container and properties of the system with a vortex-line excitation. The density profile of the system with a vortex line presents a nonzero density at the core. We calculate the ground-state energy per particle, the superfluid pairing gap, and the excitation energy per particle. These simulations can be extended to calculate the properties of vortex excitations in other strongly interacting systems such as superfluid neutron matter using realistic nuclear Hamiltonians.

arXiv:1510.07952•Physical Review A•Apr 6, 2016•11 citations

SUPERFLUIDITY IN A GAS OF STRONGLY INTERACTING FERMIONS

Wolfgang Ketterle, Yong-il Shin, André Schirotzek +1 more

WORLD SCIENTIFIC eBooks•Nov 1, 2010•0 citations

Vortices in low-density neutron matter and cold Fermi gases

Lucas Madeira, Stefano Gandolfi, Kevin E. Schmidt +1 more

Cold gas experiments can be tuned to achieve strongly-interacting regimes such as that of low-density neutron matter found in neutron-stars' crusts. We report $T=0$ diffusion Monte Carlo results (i) for the ground state of both spin-1/2 fermions with short-range interactions and low-density neutron matter in a cylindrical container, and (ii) properties of these systems with a vortex line excitation. We calculate the equation of state for cold atoms and low-density neutron matter in the bulk systems, and we contrast it to our results in the cylindrical container. We compute the vortex line excitation energy for different interaction strengths, and we find agreement between cold gases and neutron matter for very low densities. We also calculate density profiles, which allow us to determine the density depletion at the vortex core, which depends strongly on the short-ranged interaction in cold atomic gases, but it is of $\ensuremath{\approx}25%$ for neutron matter in the density regimes studied in this work. Our results can be used to constrain neutron matter properties by using measurements from cold Fermi gases experiments.

arXiv:1903.06724•Physical Review C•Jul 8, 2019•9 citations
We report diffusion Monte Carlo results for the ground state of unpolarized spin-1/2 fermions in a cylindrical container and properties of the system with a vortex-line excitation. The density profile of the system with a vortex line presents a nonzero density at the core. We calculate the ground-state energy per particle, the superfluid pairing gap, and the excitation energy per particle. These simulations can be extended to calculate the properties of vortex excitations in other strongly interacting systems such as superfluid neutron matter using realistic nuclear Hamiltonians.
Cold gas experiments can be tuned to achieve strongly-interacting regimes such as that of low-density neutron matter found in neutron-stars' crusts. We report T=0T=0T=0 diffusion Monte Carlo results (i) for the ground state of both spin-1/2 fermions with short-range interactions and low-density neutron matter in a cylindrical container, and (ii) properties of these systems with a vortex line excitation. We calculate the equation of state for cold atoms and low-density neutron matter in the bulk systems, and we contrast it to our results in the cylindrical container. We compute the vortex line excitation energy for different interaction strengths, and we find agreement between cold gases and neutron matter for very low densities. We also calculate density profiles, which allow us to determine the density depletion at the vortex core, which depends strongly on the short-ranged interaction in cold atomic gases, but it is of $\ensuremath{\approx}25%$ for neutron matter in the density regimes studied in this work. Our results can be used to constrain neutron matter properties by using measurements from cold Fermi gases experiments.