Published July 2009 | Version v1
Journal article

Induced interaction and crystallization of self-localized impurity fields in a Bose-Einstein condensate

  • 1. Facultad de Ingenieria y Ciencias, Universidad Adolfo Ibanez, Avda. Diagonal las Torres 2640, Penalolen, Santiago (Chile)
  • 2. Laboratoire de Physique Statistique, Ecole Normale Superieure, UPMC Paris 06, CNRS, Universite Paris Diderot, 24 rue Lhomond, 75005 Paris (France)
  • 3. Theoretical Division and Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

Description

We model the behavior of N classical impurity fields immersed in a larger Bose-Einstein condensate by N+1 coupled nonlinear Schroedinger equations in one, two, and three space dimensions. We discuss the stability of the uniform miscible system and show the importance of surface tension for self-localization of the impurity fields. We derive analytically the attractive tail of the impurity-impurity interaction due to mediation by the underlying condensate. Assuming all impurity fields interact with the same strength, we explore numerically the resulting phase diagram, which contains four phases: (I) all fields are miscible; (II) the impurity fields are miscible with each other but phase separate from the condensate as a single bubble; (III) the localized impurity fields stay miscible with the condensate, but not with each other; and (IV) the impurity fields phase separate from the condensate and each other, forming a crystalline structure within a bubble. Thus, we show that a crystal can be constructed solely from superfluid components. Finally, we argue that the crystalline phases maintain their superfluid behavior, i.e., they possess a nonclassical rotational inertia, which - combined with lattice order - is a characteristic of supersolidity.

Additional details

Publishing Information

Journal Title
Physical Review. A
Journal Volume
80
Journal Issue
1
Journal Page Range
p. 013609-013609.13
ISSN
1050-2947
CODEN
PLRAAN

Optional Information

Notes
(c) 2009 The American Physical Society