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arXiv:cond-mat/0303063 · Physical Review A

“Cosmological” quasiparticle production in harmonically trapped superfluid gases

Peter O. Fedichev, Uwe R. Fischer

Published Mar 8, 2004• 153 citations
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Abstract

We show that a variety of cosmologically motivated effective quasiparticle space-times can be produced in harmonically trapped superfluid Bose and Fermi gases. We study the analog of cosmological particle production in these effective space-times, induced by trapping potentials and coupling constants possessing an arbitrary time dependence. The WKB probabilities for phonon creation from the superfluid vacuum are calculated, and an experimental procedure to detect quasiparticle production by measuring density-density correlation functions is proposed.

DOI
10.1103/physreva.69.033602

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Publisher's Note: “Cosmological” quasiparticle production in harmonically trapped superfluid gases [Phys. Rev. A69, 033602 (2004)]

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We show that a variety of cosmologically motivated effective quasiparticle space-times can be produced in harmonically trapped superfluid Bose and Fermi gases. We study the analog of cosmological particle production in these effective space-times, induced by trapping potentials and coupling constants possessing an arbitrary time dependence. The WKB probabilities for phonon creation from the superfluid vacuum are calculated, and an experimental procedure to detect quasiparticle production by measuring density-density correlation functions is proposed.
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We present a theoretical study of the dynamics of a Bose-Einstein condensate (BEC) trapped inside an expanding toroid that can realize an analog inflationary universe. As the system expands, we find that phonons in the BEC undergo redshift and damping due to quantum pressure effects, owing to the thinness of the ring. We predict that rapidly expanding toroidal BEC's can exhibit spontaneous particle creation, and study this phenomenon in the context of an initial coherent state wave function. We show how particle creation would be revealed in the atom density and density correlations, and discuss connections to the cosmological theory of inflation.
In standard cosmological models, inflation is driven by a quantum field, the inflaton, whos constant energy density drove the superluminal expansion of the universe [1]. When inflation stops, the universe has an extremely low density btu the inflaton field starts to oscillate arround its minimum of energy and decays into entengled pairs of particles [2], known as the pre-heating phase. Created pairs of particles then start to interact leading to decoherence and thermalization : the re-heating stage. If in situ observation of inflaton particle creation process is impossible, this pair production through parametric amplification is analogous to the creation of phonon pairs in a Bose-Einstein (BEC) condensate whose interaction strenght is time modulated. Modulating the stiffness of a dipole trap of a cigar-shape BEC being equivalent to modulate the effective one-dimensionnal interaction strenght in a BEC, we are able to probe the correlation of entengled metastable helium atoms by the use of a micro-channel plate detector (MCP). Our experimental procedure is the following [3] : we modulate in time the trap stiffness of the dipole trap laser and then release the trap (see figure 1). During expansion, the phonon kinetic energy is adiabatically transferred to one atom that is detected by the MCP after a 300 ms time of flight. The amount of created phonon pairs is expected to depend on the duration of the excitation, its amplitude and the excitation frequency. However, the region in which the entenglement of the phonon pairs can be observed is expected to be quite narrow [4]. We propose to investigate the entenglement and correlations of those pairs of particles. [1] L. Kofman, A. Linde, and A. Starobinsky, Phys. Rev. D 56, 3258 (1997). [2] D. Campo and R. Parentani, Phys. Rev. D 74, 025001 (2006). [3] S. Robertson, F. Michel, and R. Parentani, Phys. Rev. D 95, 065020 (2017). [4] J.-C. Jaskula et al., Phys. Rev. Lett. 109, 220401 (2012).
We experimentally study cosmological particle production in a two-dimensional Bose-Einstein condensate, whose density excitations map to an analog cosmology. The expansion of spacetime is realized with tunable interactions. The particle spectrum can be understood through an analogy to quantum mechanical scattering, in which the dynamics of the spacetime metric determine the shape of the scattering potential. Hallmark scattering phenomena such as resonant forward scattering and Bragg reflection are connected to their cosmological counterparts, namely linearly expanding space and bouncing universes. We compare our findings to a theoretical description that extends beyond the acoustic approximation, which enables us to apply the model to high-momentum excitations.