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4
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33646637674
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V. Braginsky, M. Gorodetsky, F. Khalili, A. Matsko, K. Thorne, and S. Vyatchanin, gr-qc/0109003
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In V. Braginsky, M. Gorodetsky, F. Khalili, A. Matsko, K. Thorne, and S. Vyatchanin, gr-qc/0109003, it was shown that the quantization of the test masses (mirrors of the interferometer) does not affect the interferometric gravitational-wave measurement.
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6
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0037054143
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K. McKenzie, D.A. Shaddock, D.E. McClelland, B.C. Buchler, and P.K. Lam, Phys. Rev. Lett. 88, 231102 (2002).
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(2002)
Phys. Rev. Lett.
, vol.88
, pp. 231102
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McKenzie, K.1
Shaddock, D.A.2
McClelland, D.E.3
Buchler, B.C.4
Lam, P.K.5
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7
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0003029071
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edited by P. Meystre and M. O. Scully (Plenum, New York)
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W. G. Unruh, in Quantum Optics, Experimental Gravitation, and Measurement Theory, edited by P. Meystre and M. O. Scully (Plenum, New York, 1982), p. 647.
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(1982)
Quantum Optics, Experimental Gravitation, and Measurement Theory
, pp. 647
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Unruh, W.G.1
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8
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0037080790
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H.J. Kimble, Yu. Levin, A.B. Matsko, K.S. Thorne, and S.P. Vyatchanin, Phys. Rev. D 65, 022002 (2002).
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(2002)
Phys. Rev. D
, vol.65
, pp. 022002
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Kimble, H.J.1
Levin, Yu.2
Matsko, A.B.3
Thorne, K.S.4
Vyatchanin, S.P.5
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9
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0141768409
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J. Harms, Y. Chen, S. Chelkowski, A. Franzen, H. Vahlbruch, K. Danzmann, and R. Schnabel, Phys. Rev. D 68, 042001 (2003).
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(2003)
Phys. Rev. D
, vol.68
, pp. 042001
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Harms, J.1
Chen, Y.2
Chelkowski, S.3
Franzen, A.4
Vahlbruch, H.5
Danzmann, K.6
Schnabel, R.7
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14
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33646646025
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note
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Since the vacuum fluctuations entering the cavity due to losses and those due to finite transmissivity are uncorrelated, we add them in quadrature.
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15
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33646654022
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note
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A "pure" squeezed state refers to the case where the variance of the noise in one quadrature increases by exactly the same amount as that in the orthogonal quadrature is reduced, i.e., the area of the noise ellipse is unity. When excess noise is present in one quadrature, this condition is not satisfied.
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16
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33646647567
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note
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"Conventional" refers to a power-recycled Michelson interferometer with Fabry-Pérot cavities in the arms, after Ref. [8].
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17
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33646640110
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note
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1,2 and |sqz〉→|0〉.
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18
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33646668233
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note
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The critical frequency was first pointed out by Yanbei Chen.
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20
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0037516817
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P. Fritschel, Proc. SPIE 4856-39, 282 (2002).
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(2002)
Proc. SPIE
, vol.4856
, Issue.39
, pp. 282
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Fritschel, P.1
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21
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33646654758
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note
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We recall that γ=2π×100 Hz for the conventional interferometer considered here.
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22
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33646638649
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edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge)
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K. S. Thorne, in 300 Years of Gravitation, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, 1987), pp. 369 and 380.
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(1987)
300 Years of Gravitation
, pp. 369
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Thorne, K.S.1
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23
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33646643730
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note
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-7/3 dependence. This upper cutoff frequency does not affect the estimate of the SNR here.
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