Abstract
We construct dark soliton solutions in a holographic model of a relativistic superfluid. We study the length scales associated with the condensate and the charge density depletion, and find that the two scales differ by a nontrivial function of the chemical potential. By adjusting the chemical potential, we study the variation of the depletion of charge density at the interface.
- Received 23 July 2009
DOI:https://doi.org/10.1103/PhysRevD.80.121901
©2009 American Physical Society