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Volumn 77, Issue 6, 2008, Pages

Optomechanical coupling in a one-dimensional optical lattice

Author keywords

[No Author keywords available]

Indexed keywords

CRYSTAL LATTICES; LATTICE VIBRATIONS; OPTICAL MATERIALS; OPTICAL PUMPING; PRESSURE; PUMPS; STANDARDS;

EID: 46349091460     PISSN: 10502947     EISSN: 10941622     Source Type: Journal    
DOI: 10.1103/PhysRevA.77.063424     Document Type: Article
Times cited : (50)

References (45)
  • 1
    • 69149095392 scopus 로고    scopus 로고
    • For a review of the optical lattices, see AAMPE9 1049-250X
    • For a review of the optical lattices, see P. Jessen and I. Deutsch, Adv. At., Mol., Opt. Phys. AAMPE9 1049-250X 37, 95 (1996).
    • (1996) Adv. At., Mol., Opt. Phys. , vol.37 , pp. 95
    • Jessen, P.1    Deutsch, I.2
  • 2
    • 33644958906 scopus 로고    scopus 로고
    • ZZZZZZ 1745-2473
    • I. Bloch, Nat. Phys. ZZZZZZ 1745-2473 1, 23 (2005).
    • (2005) Nat. Phys. , vol.1 , pp. 23
    • Bloch, I.1
  • 3
    • 33746890865 scopus 로고    scopus 로고
    • SCIEAS 0036-8075 10.1126/science.1130365
    • G. Campbell, Science SCIEAS 0036-8075 10.1126/science.1130365 313, 649 (2006).
    • (2006) Science , vol.313 , pp. 649
    • Campbell, G.1
  • 7
    • 0037835924 scopus 로고    scopus 로고
    • JOBPDE 0740-3224 10.1364/JOSAB.20.001098
    • P. Domokos and H. Ritsch, J. Opt. Soc. Am. B JOBPDE 0740-3224 10.1364/JOSAB.20.001098 20, 1098 (2003).
    • (2003) J. Opt. Soc. Am. B , vol.20 , pp. 1098
    • Domokos, P.1    Ritsch, H.2
  • 8
    • 1542724862 scopus 로고    scopus 로고
    • NATUAS 0028-0836 10.1038/nature02387
    • P. Maunz, Nature (London) NATUAS 0028-0836 10.1038/nature02387 428, 50 (2004).
    • (2004) Nature (London) , vol.428 , pp. 50
    • Maunz, P.1
  • 9
    • 33750584661 scopus 로고    scopus 로고
    • NATUAS 0028-0836 10.1038/nature05273
    • S. Gigan, Nature (London) NATUAS 0028-0836 10.1038/nature05273 444, 67 (2006).
    • (2006) Nature (London) , vol.444 , pp. 67
    • Gigan, S.1
  • 10
    • 33750602437 scopus 로고    scopus 로고
    • NATUAS 0028-0836 10.1038/nature05244
    • O. Arcizet, Nature (London) NATUAS 0028-0836 10.1038/nature05244 444, 71 (2006).
    • (2006) Nature (London) , vol.444 , pp. 71
    • Arcizet, O.1
  • 11
    • 33750595448 scopus 로고    scopus 로고
    • NATUAS 0028-0836 10.1038/nature05231
    • D. Kleckner and D. Bouwmeester, Nature (London) NATUAS 0028-0836 10.1038/nature05231 444, 75 (2006).
    • (2006) Nature (London) , vol.444 , pp. 75
    • Kleckner, D.1    Bouwmeester, D.2
  • 15
    • 2542495140 scopus 로고    scopus 로고
    • PLRAAN 1050-2947 10.1103/PhysRevA.69.033403
    • T. Elsasser, B. Nagorny, and A. Hemmerich, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.69.033403 69, 033403 (2004).
    • (2004) Phys. Rev. A , vol.69 , pp. 033403
    • Elsasser, T.1    Nagorny, B.2    Hemmerich, A.3
  • 17
    • 69649108475 scopus 로고    scopus 로고
    • PLRAAN 1050-2947 10.1103/PhysRevA.70.013414
    • J. K. Asboth, P. Domokos, and H. Ritsch, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.70.013414 70, 013414 (2004).
    • (2004) Phys. Rev. A , vol.70 , pp. 013414
    • Asboth, J.K.1    Domokos, P.2    Ritsch, H.3
  • 18
    • 0037122317 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.89.253003
    • P. Domokos and H. Ritsch, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.89.253003 89, 253003 (2002).
    • (2002) Phys. Rev. Lett. , vol.89 , pp. 253003
    • Domokos, P.1    Ritsch, H.2
  • 20
    • 0346885951 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.91.203001
    • A. T. Black, H. W. Chan, and V. Vuletić, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.91.203001 91, 203001 (2003).
    • (2003) Phys. Rev. Lett. , vol.91 , pp. 203001
    • Black, A.T.1    Chan, H.W.2    Vuletić, V.3
  • 24
    • 37249040510 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.99.253601
    • G. R. M. Robb and W. J. Firth, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.253601 99, 253601 (2007).
    • (2007) Phys. Rev. Lett. , vol.99 , pp. 253601
    • Robb, G.R.M.1    Firth, W.J.2
  • 28
    • 33644955584 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.72.085130
    • J. Ng, Z. F. Lin, C. T. Chan, and P. Sheng, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.72.085130 72, 085130 (2005).
    • (2005) Phys. Rev. B , vol.72 , pp. 085130
    • Ng, J.1    Lin, Z.F.2    Chan, C.T.3    Sheng, P.4
  • 29
    • 33846881156 scopus 로고    scopus 로고
    • JOAOF8 1464-4258 10.1088/1464-4258/8/12/005
    • D. Maystre and P. Vincent, J. Opt. A, Pure Appl. Opt. JOAOF8 1464-4258 10.1088/1464-4258/8/12/005 8, 1059 (2006).
    • (2006) J. Opt. A, Pure Appl. Opt. , vol.8 , pp. 1059
    • Maystre, D.1    Vincent, P.2
  • 30
    • 33645139028 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.96.113903
    • T. M. Grzegorczyk, B. A. Kemp, and J. A. Kong, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.96.113903 96, 113903 (2006).
    • (2006) Phys. Rev. Lett. , vol.96 , pp. 113903
    • Grzegorczyk, T.M.1    Kemp, B.A.2    Kong, J.A.3
  • 33
    • 46349088777 scopus 로고    scopus 로고
    • For ImΘ0, we have | m- | <1< | m+ | or | m+ | <1< | m- |. Multiplication of many transfer matrices is therefore numerically ill conditioned: Important variables can take on different orders of magnitude and are then added together. In numerical calculations in mesoscopic physics it can therefore be advisable to fall back to the scattering matrix. For the transfer matrices in our case, usually | ImΘ | is of the order of Imζ, and as normally | NImζ | <1 (required so that absorption does not alter the asymmetry too much throughout the sample), these numerical issues do not concern us.
    • For ImΘ0, we have | m- | <1< | m+ | or | m+ | <1< | m- |. Multiplication of many transfer matrices is therefore numerically ill conditioned: Important variables can take on different orders of magnitude and are then added together. In numerical calculations in mesoscopic physics it can therefore be advisable to fall back to the scattering matrix. For the transfer matrices in our case, usually | ImΘ | is of the order of Imζ, and as normally | NImζ | <1 (required so that absorption does not alter the asymmetry too much throughout the sample), these numerical issues do not concern us.
  • 35
    • 33645077858 scopus 로고    scopus 로고
    • PLRAAN 1050-2947 10.1103/PhysRevA.73.033417
    • D. Meiser and P. Meystre, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.73.033417 73, 033417 (2006).
    • (2006) Phys. Rev. A , vol.73 , pp. 033417
    • Meiser, D.1    Meystre, P.2
  • 36
    • 33845242759 scopus 로고    scopus 로고
    • PLRAAN 1050-2947 10.1103/PhysRevA.74.065801
    • D. Meiser and P. Meystre, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.74.065801 74, 065801 (2006).
    • (2006) Phys. Rev. A , vol.74 , pp. 065801
    • Meiser, D.1    Meystre, P.2
  • 37
    • 36048951560 scopus 로고    scopus 로고
    • PLRAAN 1050-2947 10.1103/PhysRevA.76.057801
    • J. K. Asboth and P. Domokos, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.76.057801 76, 057801 (2007).
    • (2007) Phys. Rev. A , vol.76 , pp. 057801
    • Asboth, J.K.1    Domokos, P.2
  • 38
    • 0000788958 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.60.2363
    • M. I. Antonoyiannakis and J. B. Pendry, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.60.2363 60, 2363 (1999).
    • (1999) Phys. Rev. B , vol.60 , pp. 2363
    • Antonoyiannakis, M.I.1    Pendry, J.B.2
  • 39
    • 46349108105 scopus 로고    scopus 로고
    • Note that the fluctuations of this force, arising from the spontaneous emission accompanying absorption, lead to a heating of the cloud, which limits the time scale of experiments. We come back to this issue in Sec. 7.
    • Note that the fluctuations of this force, arising from the spontaneous emission accompanying absorption, lead to a heating of the cloud, which limits the time scale of experiments. We come back to this issue in Sec. 7.
  • 40
    • 4243504131 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.24.156
    • A. Ashkin, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.24.156 24, 156 (1970).
    • (1970) Phys. Rev. Lett. , vol.24 , pp. 156
    • Ashkin, A.1
  • 41
    • 46349107937 scopus 로고    scopus 로고
    • The color coding and slashed lines denoting the regimes of stability come in fact from the analytical calculations detailed in Sec. 5, and not directly from simulations themselves (the computational cost is only linear with N, but simulations with N= 106 are still impractical). Therefore they correspond to stability with respect to infinitesimal perturbations. As such, they have been checked via simulation and seen to be correct several times, as illustrated in the examples in Figs. 9 10.
    • The color coding and slashed lines denoting the regimes of stability come in fact from the analytical calculations detailed in Sec. 5, and not directly from simulations themselves (the computational cost is only linear with N, but simulations with N= 106 are still impractical). Therefore they correspond to stability with respect to infinitesimal perturbations. As such, they have been checked via simulation and seen to be correct several times, as illustrated in the examples in Figs. 9 10.
  • 42
    • 46349105146 scopus 로고    scopus 로고
    • In fact, the derivation of Eq. 62 is not valid for symmetric pumping, and therefore one must use a different approach. However, as we show in Eq. 9, a mathematically sound procedure also leads to Eq. 63.
    • In fact, the derivation of Eq. 62 is not valid for symmetric pumping, and therefore one must use a different approach. However, as we show in Eq. 9, a mathematically sound procedure also leads to Eq. 63.
  • 43
    • 0010746493 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.83.3285
    • R. A. Simha and S. Ramaswamy, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83.3285 83, 3285 (1999).
    • (1999) Phys. Rev. Lett. , vol.83 , pp. 3285
    • Simha, R.A.1    Ramaswamy, S.2
  • 45
    • 34648814071 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.99.124502
    • T. Beatus, R. Bar-Ziv, and T. Tlusty, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.124502 99, 124502 (2007).
    • (2007) Phys. Rev. Lett. , vol.99 , pp. 124502
    • Beatus, T.1    Bar-Ziv, R.2    Tlusty, T.3


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