Phonon Superradiance in Dilute Gas Bose-Einstein Condensates
Abstract
The analogy between the propagation of a massless scalar field in curved spacetime
and the propagation of sound waves in a Bose-Einstein Condensate (BEC) gives rise
to the possibility of observing the analogues of black hole radiance effects, such as
Hawking Radiation and superradiance, in the laboratory. In order to provide a solid
foundation for realising such analogue gravity models in an experimental setting,
we have conducted a numerical investigation of phonon scattering from a BEC
vortex by solving the time-dependent Gross-Pitaevskii (GP) equation, describing
the dynamics of dilute gas BECs. The consideration of phonon superradiance in
BECs in advance of Hawking Radiation is motivated by the fact superradiance may
be easier to detect.
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We first present the results of one-dimensional simulations of sound waves propagating
in a BEC and reflecting from a vortex-like density profile. Using these results as
a guide, two-dimensional simulations of sound propagation in a BEC, and reflection
from a BEC vortex, are performed. The technique of propagating the wavefunction
in imaginary time was employed to find the vortex ground state. The accuracy of
the simulations and the convergence of the solution to the vortex ground state was
verified using a range of numerical diagnostics. Finally, preliminary simulations were
performed within the superradiant frequency regime for the purposes of determining
whether the amplification of incoming waves occurs given an appropriate choice of
parameters. Overall, the two-dimensional modelling of reflection of cylindrical waves
from a BEC vortex provides a basis for a systematic study of phonon superradiance
in BECs.
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