Adding all-to-all atomic interactions to a parametrically driven, dissipative Tavis-Cummings model shifts and sculpts the superradiant phase boundary, with repulsive interactions suppressing and attractive interactions mostly enhancing superradiance.
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Parametrically Driven Superradiance of an Interacting Tavis-Cummings Model
Adding all-to-all atomic interactions to a parametrically driven, dissipative Tavis-Cummings model shifts and sculpts the superradiant phase boundary, with repulsive interactions suppressing and attractive interactions mostly enhancing superradiance.