Physics of hollow Bose-Einstein condensates

Karmela Padavić, Kuei Sun, Courtney Lannert, Smitha Vishveshwara

Research output: Contribution to journalArticle

Abstract

Bose-Einstein condensate shells, while occurring in ultracold systems of coexisting phases and potentially within neutron stars, have yet to be realized in isolation on Earth due to the experimental challenge of overcoming gravitational sag. Motivated by the expected realization of hollow condensates by the space-based Cold Atomic Laboratory in microgravity conditions, we study a spherical condensate undergoing a topological change from a filled sphere to a hollow shell. We argue that the collective modes of the system show marked and robust signatures of this hollowing transition accompanied by the appearance of a new boundary. In particular, we demonstrate that the frequency spectrum of the breathing modes shows a pronounced depression as it evolves from the filled-sphere limit to the hollowing transition. Furthermore, when the center of the system becomes hollow surface modes show a global restructuring of their spectrum due to the availability of a new, inner, surface for supporting density distortions. We pinpoint universal features of this topological transition as well as analyse the spectral evolution of collective modes in the experimentally relevant case of a bubble-trap.

Original languageEnglish (US)
Article number20004
JournalEPL
Volume120
Issue number2
DOIs
StatePublished - Oct 2017

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Bose-Einstein condensates
hollow
physics
condensates
breathing
microgravity
neutron stars
availability
isolation
bubbles
signatures
traps

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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Physics of hollow Bose-Einstein condensates. / Padavić, Karmela; Sun, Kuei; Lannert, Courtney; Vishveshwara, Smitha.

In: EPL, Vol. 120, No. 2, 20004, 10.2017.

Research output: Contribution to journalArticle

Padavić, Karmela ; Sun, Kuei ; Lannert, Courtney ; Vishveshwara, Smitha. / Physics of hollow Bose-Einstein condensates. In: EPL. 2017 ; Vol. 120, No. 2.
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