“…In 1954, Dicke predicted that the radiation emitted by a dense ensemble of atoms should be dramatically different than the emission from independent atoms [1]. According to Dicke, the decay of a fully inverted cloud of N emitters confined in a region smaller than their transition wavelength is characterized by a burst of radiation with peak intensity scaling ∝ N 2 , rather than the expected ∝ N. This behavior, known as superradiance (or superfluorescence), has been investigated in many experimental platforms including low density clouds of atoms or molecules [2][3][4][5][6][7][8], semiconductors [9,10], nuclei [11], superconducting qubits [12] and Rydberg gases [13][14][15][16]. Recently, interest in superradiance has grown, following theoretical proposals [17,18] and experiments [19][20][21][22][23][24] that describe how superradiance could help realize a novel class of ultra-stable lasers.…”