English

Zero Sound and First Sound in a Disk-Shaped Normal Fermi gas

Other Condensed Matter 2009-11-13 v1

Abstract

We study the zero sound and the first sound in a dilute and ultracold disk-shaped normal Fermi gas with a strong harmonic confinement along the axial direction and uniform in the two planar directions. Working at zero temperature we calculate the chemical potential μ\mu of the fermionic fluid as a function of the uniform planar density ρ\rho and find that μ\mu changes its slope in correspondence to the filling of harmonic axial modes (shell effects). Within the linear response theory, and under the random phase approximation, we calculate the velocity cs0c^{0}_s of the zero sound. We find that also cs0c^0_s changes its slope in correspondence of the filling of the harmonic axial modes and that this effect depends on the Fermi-Fermi scattering length aFa_F. In the collisional regime, we calculate the velocity csc_s of first sound showing that csc_s displays jumps at critical densities fixed by the scattering length aFa_F. Finally, we discuss the experimental achievability of these zero sound and first sound waves with ultracold alkali-metal atoms.

Keywords

Cite

@article{arxiv.0901.3438,
  title  = {Zero Sound and First Sound in a Disk-Shaped Normal Fermi gas},
  author = {Giovanni Mazzarella and Luca Salasnich and Flavio Toigo},
  journal= {arXiv preprint arXiv:0901.3438},
  year   = {2009}
}

Comments

9 pages, 5 figures, editorially approved for publication on Phys. Rev. A

R2 v1 2026-06-21T12:03:33.098Z