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Volumn 78, Issue 3, 2008, Pages

Energy distribution and cooling of a single atom in an optical tweezer

Author keywords

[No Author keywords available]

Indexed keywords

ATOMIC PHYSICS; BOLTZMANN EQUATION; COOLING; ELECTRIC POWER DISTRIBUTION; ION BEAMS; RUBIDIUM;

EID: 53349146123     PISSN: 10502947     EISSN: 10941622     Source Type: Journal    
DOI: 10.1103/PhysRevA.78.033425     Document Type: Article
Times cited : (191)

References (32)
  • 1
    • 11944258314 scopus 로고
    • RMPHAT 0034-6861 10.1103/RevModPhys.62.525
    • H. Dehmelt, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.62.525 62, 525 (1990).
    • (1990) Rev. Mod. Phys. , vol.62 , pp. 525
    • Dehmelt, H.1
  • 8
    • 0028538773 scopus 로고
    • OPLEDP 0146-9592
    • Z. Hu and H. J. Kimble, Opt. Lett. OPLEDP 0146-9592 19, 1888 (1994).
    • (1994) Opt. Lett. , vol.19 , pp. 1888
    • Hu, Z.1    Kimble, H.J.2
  • 19
    • 0001017189 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.48.596
    • W. D. Phillips and H. Metcalf, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.48.596 48, 596 (1982).
    • (1982) Phys. Rev. Lett. , vol.48 , pp. 596
    • Phillips, W.D.1    Metcalf, H.2
  • 20
    • 0037042997 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.89.023005
    • N. Schlosser, G. Reymond, and P. Grangier, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.89.023005 89, 023005 (2002).
    • (2002) Phys. Rev. Lett. , vol.89 , pp. 023005
    • Schlosser, N.1    Reymond, G.2    Grangier, P.3
  • 30
    • 53349156053 scopus 로고    scopus 로고
    • We assume that an atom with an energy greater than the trap depth has sufficient time to exit the trap provided the following condition is fulfilled: 1/τ ν, where τ is the time the atom is in the trap and ν is the trap frequency in the axial direction. This condition is satisfied down to a final trap depth Uf / Ui ∼ 10-4, where τ× ν ∼10/1.
    • We assume that an atom with an energy greater than the trap depth has sufficient time to exit the trap provided the following condition is fulfilled: 1/τ ν, where τ is the time the atom is in the trap and ν is the trap frequency in the axial direction. This condition is satisfied down to a final trap depth Uf / Ui ∼ 10-4, where τ× ν ∼10/1.
  • 31
    • 53349119636 scopus 로고    scopus 로고
    • For the effective minimum trap depth Umin taking gravity into account turns out to be important for trap depths less than ∼10 μK because the gravity potential acts to tilt the trapping potential, thus lowering the potential barrier along the gravity axis.
    • For the effective minimum trap depth Umin taking gravity into account turns out to be important for trap depths less than ∼10 μK because the gravity potential acts to tilt the trapping potential, thus lowering the potential barrier along the gravity axis.
  • 32
    • 53349123563 scopus 로고    scopus 로고
    • After the release and recapture sequence we needed to bring the trap depth close to its initial value to measure if the atom is still present in the trap, otherwise the lasers sent on the atom would kick it out of the shallow trap too quickly to measure its presence.
    • After the release and recapture sequence we needed to bring the trap depth close to its initial value to measure if the atom is still present in the trap, otherwise the lasers sent on the atom would kick it out of the shallow trap too quickly to measure its presence.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.