-
1
-
-
1842581806
-
-
SCIEAS 0036-8075 10.1126/science.1094419
-
M. D. LaHaye, O. Buu, B. Camarota, and K. C. Schwab, Science SCIEAS 0036-8075 10.1126/science.1094419 304, 74 (2004).
-
(2004)
Science
, vol.304
, pp. 74
-
-
Lahaye, M.D.1
Buu, O.2
Camarota, B.3
Schwab, K.C.4
-
3
-
-
33750584661
-
-
NATUAS 0028-0836 10.1038/nature05273
-
S. Gigan, H. R. Böhm, M. Paternostro, F. Blaser, G. Langer, J. B. Hertzberg, K. C. Schwab, D. Bäuerle, M. Aspelmeyer, and A. Zeilinger, Nature (London) NATUAS 0028-0836 10.1038/nature05273 444, 67 (2006).
-
(2006)
Nature (London)
, vol.444
, pp. 67
-
-
Gigan, S.1
Böhm, H.R.2
Paternostro, M.3
Blaser, F.4
Langer, G.5
Hertzberg, J.B.6
Schwab, K.C.7
Bäuerle, D.8
Aspelmeyer, M.9
Zeilinger, A.10
-
4
-
-
33845517100
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.97.243905
-
A. Schliesser, P. Del'Haye, N. Nooshi, K. J. Vahala, and T. J. Kippenberg, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.97.243905 97, 243905 (2006).
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 243905
-
-
Schliesser, A.1
Del'Haye, P.2
Nooshi, N.3
Vahala, K.J.4
Kippenberg, T.J.5
-
5
-
-
34848819421
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.99.137205
-
K. R. Brown, J. Britton, R. J. Epstein, J. Chiaverini, D. Leibfried, and D. J. Wineland, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.137205 99, 137205 (2007).
-
(2007)
Phys. Rev. Lett.
, vol.99
, pp. 137205
-
-
Brown, K.R.1
Britton, J.2
Epstein, R.J.3
Chiaverini, J.4
Leibfried, D.5
Wineland, D.J.6
-
7
-
-
35848936082
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.76.205302
-
F. Xue, Y. D. Wang, Y. X. Liu, and F. Nori, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.76.205302 76, 205302 (2007).
-
(2007)
Phys. Rev. B
, vol.76
, pp. 205302
-
-
Xue, F.1
Wang, Y.D.2
Liu, Y.X.3
Nori, F.4
-
8
-
-
34548269961
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.99.093902
-
F. Marquardt, J. P. Chen, A. A. Clerk, and S. M. Girvin, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.093902 99, 093902 (2007).
-
(2007)
Phys. Rev. Lett.
, vol.99
, pp. 093902
-
-
Marquardt, F.1
Chen, J.P.2
Clerk, A.A.3
Girvin, S.M.4
-
9
-
-
34548209883
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.99.093901
-
I. Wilson-Rae, N. Nooshi, W. Zwerger, and T. J. Kippenberg, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.093901 99, 093901 (2007).
-
(2007)
Phys. Rev. Lett.
, vol.99
, pp. 093901
-
-
Wilson-Rae, I.1
Nooshi, N.2
Zwerger, W.3
Kippenberg, T.J.4
-
10
-
-
2342430947
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.69.125339
-
I. Martin, A. Shnirman, L. Tian, and P. Zoller, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.69.125339 69, 125339 (2004).
-
(2004)
Phys. Rev. B
, vol.69
, pp. 125339
-
-
Martin, I.1
Shnirman, A.2
Tian, L.3
Zoller, P.4
-
11
-
-
28844481503
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.72.041405
-
W. K. Hensinger, D. W. Utami, H.-S. Goan, K. Schwab, C. Monroe, and G. J. Milburn, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.72.041405 72, 041405 (R) (2005).
-
(2005)
Phys. Rev. a
, vol.72
, pp. 041405
-
-
Hensinger, W.K.1
Utami, D.W.2
Goan, H.-S.3
Schwab, K.4
Monroe, C.5
Milburn, G.J.6
-
12
-
-
46749149974
-
-
arXiv:0708.0665 ZZZZZZ 1745-2473 (to be published).
-
M. Grajcar, S. H. W. van der Ploeg, A. Izmalkov, E. Il'ichev, H. G. Meyer, A. Fedorov, A. Shnirman, and G. Schön, arXiv:0708.0665, Nat. Phys. ZZZZZZ 1745-2473 (to be published).
-
Nat. Phys.
-
-
Grajcar, M.1
Van Der Ploeg, S.H.W.2
Izmalkov, A.3
Il'Ichev, E.4
Meyer, H.G.5
Fedorov, A.6
Shnirman, A.7
Schön, G.8
-
13
-
-
34548814780
-
-
PLEEE8 1063-651X 10.1103/PhysRevE.76.031105
-
H. T. Quan, Y. Liu, C. P. Sun, and F. Nori, Phys. Rev. E PLEEE8 1063-651X 10.1103/PhysRevE.76.031105 76, 031105 (2007).
-
(2007)
Phys. Rev. e
, vol.76
, pp. 031105
-
-
Quan, H.T.1
Liu, Y.2
Sun, C.P.3
Nori, F.4
-
14
-
-
33845446976
-
-
SCIEAS 0036-8075 10.1126/science.1134008
-
S. O. Valenzuela, W. D. Oliver, D. M. Berns, K. K. Berggren, L. S. Levitov, and T. P. Orlando, Science SCIEAS 0036-8075 10.1126/science.1134008 314, 1589 (2006);
-
(2006)
Science
, vol.314
, pp. 1589
-
-
Valenzuela, S.O.1
Oliver, W.D.2
Berns, D.M.3
Berggren, K.K.4
Levitov, L.S.5
Orlando, T.P.6
-
15
-
-
38849100210
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.100.047001
-
J. Q. You, Y. X. Liu, and F. Nori, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.100.047001 100, 047001 (2008).
-
(2008)
Phys. Rev. Lett.
, vol.100
, pp. 047001
-
-
You, J.Q.1
Liu, Y.X.2
Nori, F.3
-
16
-
-
0018000591
-
-
It is worth mentioning here that similar sideband cooling mechanisms have appeared in different contexts over the years. See, e.g., 1063-7834
-
It is worth mentioning here that similar sideband cooling mechanisms have appeared in different contexts over the years. See, e.g., M. I. Dykman, Sov. Phys. Solid State 20, 1306 (1978). 1063-7834
-
(1978)
Sov. Phys. Solid State
, vol.20
, pp. 1306
-
-
Dykman, M.I.1
-
17
-
-
0037472921
-
-
NATUAS 0028-0836 10.1038/421496a
-
X. Henry Huang, C. A. Zorman, M. Mehregany, and M. L. Roukes, Nature (London) NATUAS 0028-0836 10.1038/421496a 421, 496 (2003).
-
(2003)
Nature (London)
, vol.421
, pp. 496
-
-
Henry Huang, X.1
Zorman, C.A.2
Mehregany, M.3
Roukes, M.L.4
-
18
-
-
4644252328
-
-
0028-0836
-
V. Sazonova, Y. Yaish, T. A. A. H. Üstünel, D. Roundy, and P. L. McEuen, Nature (London) 431, 284 (2004). 0028-0836
-
(2004)
Nature (London)
, vol.431
, pp. 284
-
-
Sazonova, V.1
Yaish, Y.2
Üstünel, T.A.A.H.3
Roundy, D.4
McEuen, P.L.5
-
19
-
-
33747791245
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.97.087203
-
H. B. Peng, C. W. Chang, S. Aloni, T. D. Yuzvinsky, and A. Zettl, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.97.087203 97, 087203 (2006).
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 087203
-
-
Peng, H.B.1
Chang, C.W.2
Aloni, S.3
Yuzvinsky, T.D.4
Zettl, A.5
-
20
-
-
33845269357
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.97.237201
-
L. F. Wei, Y. X. Liu, C. P. Sun, and F. Nori, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.97.237201 97, 237201 (2006).
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 237201
-
-
Wei, L.F.1
Liu, Y.X.2
Sun, C.P.3
Nori, F.4
-
22
-
-
27544445288
-
-
PHTOAD 0031-9228
-
J. Q. You and F. Nori, Phys. Today PHTOAD 0031-9228 58 (11), 42 (2005).
-
(2005)
Phys. Today
, vol.58
, Issue.11
, pp. 42
-
-
You, J.Q.1
Nori, F.2
-
23
-
-
33745297751
-
-
NJOPFM 1367-2630 10.1088/1367-2630/8/6/105
-
S. Savel'ev, X. Hu, and F. Nori, New J. Phys. NJOPFM 1367-2630 10.1088/1367-2630/8/6/105 8, 105 (2006).
-
(2006)
New J. Phys.
, vol.8
, pp. 105
-
-
Savel'Ev, S.1
Hu, X.2
Nori, F.3
-
28
-
-
33748636436
-
-
NATUAS 0028-0836 10.1038/nature05027
-
A. Naik, O. Buu, M. D. LaHaye, A. D. Armour, A. A. Clerk, M. P. Blencowe, and K. C. Schwab, Nature (London) NATUAS 0028-0836 10.1038/nature05027 443, 193 (2006).
-
(2006)
Nature (London)
, vol.443
, pp. 193
-
-
Naik, A.1
Buu, O.2
Lahaye, M.D.3
Armour, A.D.4
Clerk, A.A.5
Blencowe, M.P.6
Schwab, K.C.7
-
29
-
-
34948814148
-
-
NATUAS 0028-0836 10.1038/nature06141
-
O. Astafiev, K. Inomata, A. O. Niskanen, T. Yamamoto, Y. A. Pashkin, Y. Nakamura, and J. S. Tsai, Nature (London) NATUAS 0028-0836 10.1038/nature06141 449, 588 (2007).
-
(2007)
Nature (London)
, vol.449
, pp. 588
-
-
Astafiev, O.1
Inomata, K.2
Niskanen, A.O.3
Yamamoto, T.4
Pashkin, Y.A.5
Nakamura, Y.6
Tsai, J.S.7
-
30
-
-
46749109111
-
-
It should be emphasized here that the presence of a nonlinearity in the Hamiltonian is crucial for the cooling mechanism. In other words, a completely linear system [i.e., a system composed of two linear oscillators that are coupled linearly to each other, to the environment, and to the driving force (Ref.)] will not experience any thermal change in the presence or absence of an ideal driving force. The nonlinearity can therefore be seen as a mixer between the resonator frequency and the driving frequency that allows the "upconversion" of vibrational quanta and therefore cooling.
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It should be emphasized here that the presence of a nonlinearity in the Hamiltonian is crucial for the cooling mechanism. In other words, a completely linear system [i.e., a system composed of two linear oscillators that are coupled linearly to each other, to the environment, and to the driving force (Ref.)] will not experience any thermal change in the presence or absence of an ideal driving force. The nonlinearity can therefore be seen as a mixer between the resonator frequency and the driving frequency that allows the "upconversion" of vibrational quanta and therefore cooling.
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46749098888
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In this paper we use the convention where linear coupling between two harmonic oscillators means a coupling term of the form g (α ar + α ar†) (β am + β am†) and linear coupling to the driving force means a term of the form (ζ ar + ζ ar† +η am + η am†) cos (ωp t+θ), where α, β, ζ, η, ωp, and θ are constants. Under this convention parametric driving, i.e., when the coupling strength g in Eq. 24 is modulated by an externally applied signal, corresponds to a nonlinear driving term. Although such parametric driving can be used to implement the sideband cooling mechanism, in this paper we are only considering the case where the externally applied driving signal couples to the charge on the resonator, i.e., a linear driving term according to the convention that we follow
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In this paper we use the convention where linear coupling between two harmonic oscillators means a coupling term of the form g (α ar + α ar†) (β am + β am†) and linear coupling to the driving force means a term of the form (ζ ar + ζ ar† +η am + η am†) cos (ωp t+θ), where α, β, ζ, η, ωp, and θ are constants. Under this convention parametric driving, i.e., when the coupling strength g in Eq. 24 is modulated by an externally applied signal, corresponds to a nonlinear driving term. Although such parametric driving can be used to implement the sideband cooling mechanism, in this paper we are only considering the case where the externally applied driving signal couples to the charge on the resonator, i.e., a linear driving term according to the convention that we follow. Since we further assume a linear mechanical oscillator and linear coupling to the environment (in the case of linear oscillators), a nonlinearity is needed either in the coolant Hamiltonian or the coupling term.
-
-
-
-
35
-
-
46749093246
-
-
arXiv:0806.1298v1 (unpublished).
-
J. Hauss, A. Fedorov, S. André, V. Brosco, C. Hutter, R. Kothari, S. Yeshwant, A. Shnirman, and G. Schön, arXiv:0806.1298v1 (unpublished).
-
-
-
Hauss, J.1
Fedorov, A.2
André, S.3
Brosco, V.4
Hutter, C.5
Kothari, R.6
Yeshwant, S.7
Shnirman, A.8
Schön, G.9
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