2021
DOI: 10.1088/1367-2630/ac136c
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Observation of blackbody radiation enhanced superradiance in ultracold Rydberg gases

Abstract: An ensemble of excited atoms can synchronize emission of light collectively in a process known as superradiance when its characteristic size is smaller than the wavelength of emitted photons. The underlying superradiance depends strongly on electromagnetic (photon) fields surrounding the atomic ensemble. High mode densities of microwave photons from 300 K blackbody radiation (BBR) significantly enhance decay rates of Rydberg states to neighbouring states, enabling superradiance that is not possible with bare v… Show more

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Cited by 13 publications
(21 citation statements)
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“…It is noted that the superradiation effect has a negligible effect on the lifetime measurement in this work. When the Rydberg density is larger than ∼10 10 cm −3 , the superradiation will strongly accelerate the decay rate and modify the lifetime of Rydberg state [4,25]. The high precision measurement of the lifetime provides a powerful tool for investigating the cross section for the quenching collision and also has a significant correction to quantum defects.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…It is noted that the superradiation effect has a negligible effect on the lifetime measurement in this work. When the Rydberg density is larger than ∼10 10 cm −3 , the superradiation will strongly accelerate the decay rate and modify the lifetime of Rydberg state [4,25]. The high precision measurement of the lifetime provides a powerful tool for investigating the cross section for the quenching collision and also has a significant correction to quantum defects.…”
Section: Discussionmentioning
confidence: 99%
“…In this section, we consider the effect of the BBR on the decay rate of Rydberg state. As we know that the room temperature BBR has a negligible effect for the ground atom, but has a strong effect for electronically high-lying Rydberg states and enhance the decay rate of Rydberg states [22][23][24][25]. Taking into account the BBR effect, the effective radiation decay rate of Rydberg atoms Γ e f f (T) can be written as…”
Section: Blackbody Radiation Induced Decaymentioning
confidence: 99%
“…the Dicke limit R jk λ [2], decay becomes collective such that its rate depends on the number of atoms in the ensemble, and hence can be much larger than the individual decay rate [3]. Since predicted by Dicke, superradiance has been confirmed in a variety experimental settings including Rydberg atoms [4][5][6][7][8], cavities [9][10][11], Bose-Einstein condensates [12][13][14], and quantum dots [15]. On the other hand, insights gained from the study of superradiance allow us to develop applications in quantum metrology [16,17], narrow linewidth lasers [18][19][20] and atomic clocks [21], etc.…”
Section: Introductionmentioning
confidence: 99%
“…Radiative decay is therefore here not expected to acquire a collective character and is typically modelled as a singleatom process. Note, that super-and subradiance can nevertheless occur -and have been investigated -in Rydberg gases [35][36][37][38]. However, in these studies the considered radiative transitions take place among Rydberg states and the associated wavelengths are on the order of millimetres to centimetres [39].…”
mentioning
confidence: 99%