Entanglement Growth via Splitting of a Few Thermal Quanta.

Phys Rev Lett

Department of Optics, Palacký University, 17. listopadu 1192/12, 771 46 Olomouc, Czech Republic.

Published: May 2024

AI Article Synopsis

  • - Quanta splitting is a key method for creating Gaussian entanglement, often seen in Einstein-Podolsky-Rosen states and requiring strong pumping from a low-noise external source.
  • - Recent experiments with trapped ions and superconducting circuits have explored the coupling of thermal quanta, leading to significant nonclassicality and measurable entanglement levels exceeding 3 dB of distillable quadrature squeezing.
  • - This new entanglement, which is not confined to Gaussian approximations, increases with the number of thermal quanta split, offering insights into non-linear bosonic systems and their potential for generating substantial entanglement.

Article Abstract

Quanta splitting is an essential generator of Gaussian entanglement, exemplified by Einstein-Podolsky-Rosen states and apparently the most commonly occurring form of entanglement. In general, it results from the strong pumping of a nonlinear process with a highly coherent and low-noise external drive. In contrast, recent experiments involving efficient trilinear processes in trapped ions and superconducting circuits have opened the complementary possibility to test the splitting of a few thermal quanta. Stimulated by such small thermal energy, a strong degenerate trilinear coupling generates large amounts of nonclassicality, detectable by more than 3 dB of distillable quadrature squeezing. Substantial entanglement can be generated via frequent passive linear coupling to a third mode present in parallel with the trilinear coupling. This new form of entanglement, outside any Gaussian approximation, surprisingly grows with the mean number of split thermal quanta; a quality absent from Gaussian entanglement. Using distillable squeezing we shed light on this new entanglement mechanism for nonlinear bosonic systems.

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Source
http://dx.doi.org/10.1103/PhysRevLett.132.210201DOI Listing

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