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Parametric amplification of vacuum fluctuations in a spinor condensate

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arxiv 0907.3413 v1 pith:3WDBOWCV submitted 2009-07-20 cond-mat.quant-gas

Parametric amplification of vacuum fluctuations in a spinor condensate

classification cond-mat.quant-gas
keywords vacuumfluctuationscondensatecreationamplificationpairparametricspinor
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Parametric amplification of vacuum fluctuations is crucial in modern quantum optics, enabling the creation of squeezing and entanglement. We demonstrate the parametric amplification of vacuum fluctuations for matter waves using a spinor F=2 Rb-87 condensate. Interatomic interactions lead to correlated pair creation in the m_F= +/- 1 states from an initial unstable m_F=0 condensate, which acts as a vacuum for m_F unequal 0. Although this pair creation from a pure m_F=0 condensate is ideally triggered by vacuum fluctuations, unavoidable spurious initial m_F= +/- 1 atoms induce a classical seed which may become the dominant triggering mechanism. We show that pair creation is insensitive to a classical seed for sufficiently large magnetic fields, demonstrating the dominant role of vacuum fluctuations. The presented system thus provides a direct path towards the generation of non-classical states of matter on the basis of spinor condensates.

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