1999
DOI: 10.1103/physreva.60.r29
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Quantum-diffractive background gas collisions in atom-trap heating and loss

Abstract: We derive a simple formula for the heating rate that arises from quantum-diffractive background gas collisions in atom traps. This result appears to explain the residual heating rates reported for recent experiments with a Cs vapor-loaded, far-detuned optical trap at Ӎ10 Ϫ9 Torr ͓Phys. Rev. Lett. 81, 5768 ͑1998͔͒. Diffractive collisions may determine the minimum heating rates achievable in shallow all-optical or magnetic atom traps operating at low temperature and high density. ͓S1050-2947͑99͒50307-7͔PACS numb… Show more

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Cited by 63 publications
(65 citation statements)
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“…Using σ Rb−Rb = 2.5 × 10 −13 cm 2 [36] we find τ c = 55 s at a pressure of 1 × 10 −10 mbar. Even without resorting to cryogenic vacuum systems pressures as low as 10 −11 mbar are achievable, which would imply collisional lifetimes of order 10 minutes.…”
Section: B Background Gas Collisionsmentioning
confidence: 99%
See 1 more Smart Citation
“…Using σ Rb−Rb = 2.5 × 10 −13 cm 2 [36] we find τ c = 55 s at a pressure of 1 × 10 −10 mbar. Even without resorting to cryogenic vacuum systems pressures as low as 10 −11 mbar are achievable, which would imply collisional lifetimes of order 10 minutes.…”
Section: B Background Gas Collisionsmentioning
confidence: 99%
“…The characteristic energy change for which diffractive collisions must be accounted for is ∼ 2.8 mK for Rb [36]. As we are considering a shallow FORT of depth |U m | = 1 mK we will neglect diffractive and heating effects and approximate the FORT lifetime due to background collisions mediated by a van der Waals interaction as [36] …”
Section: B Background Gas Collisionsmentioning
confidence: 99%
“…In Figure 5(b), we scan the off time from 2 s to 20 s to get the probabilities of atoms still in, and then fit the curve with an exponential decay function. Under our experimental conditions, the 1/e lifetime of single atoms is about 11.4 s due to collisions with untrapped background atoms in the ultrahigh vacuum chamber and heating mechanisms caused by intensity fluctuations and photon scattering of the FORT light [24][25][26].…”
Section: The Lifetime Of Single Atomsmentioning
confidence: 99%
“…The temperature of the cloud given by a time of flight measurement is 21 µK, in good agreement with the in situ measurement. As one does not expect a thermodynamic equilibrium to be reached when considering the conservative dynamics of independent particles in a trap, the good agreement between these two methods to estimate the temperature , where e is the electron charge, a0 is the Bohr radius and 0 the vacuum permittivity (data taken from [29]). Trap loss rate γi computed from Eq.…”
Section: Quasi-steady Regimementioning
confidence: 99%