REPORTS greatly eases the requirements on the sign<strong>al</strong>-beamcavity d<strong>et</strong>uning due to both param<strong>et</strong>ric instabilities at positive d<strong>et</strong>uning and the contamination of cross-correlation by therm<strong>al</strong> motion (12, 15, 26), but it does not change the sensitivity of the resonator to RPSN relative to therm<strong>al</strong> forces. The effect of the optomechanic<strong>al</strong> coupling on the resonator from a single laser (25, 27) or multiple beams (15) has been well studied. The resonator’s mechanic<strong>al</strong> susceptibility is modified to include optomechanic<strong>al</strong> damping and frequency shifts from each laser. Addition<strong>al</strong>ly, the effective phonon occupation, nm, is modified. The optomechanic<strong>al</strong> damping cools the resonator; RPSN increases the amplitude of motion. In equilibrium, a simple rate equation gives nm = (nthG0 + nSGS + nMGM)/Gm. Here, nth is the therm<strong>al</strong> phonon occupation; nS and GS (or nM and GM) are the effective bath temperature and optomechanic<strong>al</strong> damping rate of the sign<strong>al</strong> (or m<strong>et</strong>er) laser. The tot<strong>al</strong> mechanic<strong>al</strong> damping rate is Gm = G0 + GS + GM. In our experiments GM >> G0 and GS, whereas ∆S ~0andNS >> NM,where∆Sand NS (or ∆M and NM) are the laser-cavity d<strong>et</strong>uning and intracavity photon occupation of the sign<strong>al</strong> (or m<strong>et</strong>er) beam. RPSN dominates over therm<strong>al</strong> noise when the ratio of radiation to therm<strong>al</strong> forces RS =(CS/nth)[1 + (2wm/k) 2 ] −1 > 1, where CS =4NSg 2 /kG0 is the multiphoton cooperativity. We are able to reach this highcooperativity regime (CS ~10 6 The increase in phonon occupation resulting from RPSN is shown in Fig. 2. The m<strong>et</strong>er beam transmission spectrum, SIMðwÞ (Fig. 2, ins<strong>et</strong>), shows a marked increase in spectr<strong>al</strong> area, or equiv<strong>al</strong>ently, nm as the measurement strength is increased to where RS ~ 1. Here, the employed NS =3.6×10 ) due to the sm<strong>al</strong>l mass, weak intrinsic damping, and cryogenic environment of our resonator. 8 serve a large response from this mode, which indicates that the absorbed laser light causes a
REPORTS 804 themembranewithawhitenoise–driven piezoelectric actuator (purple trace exceeds dashed curve in Fig. 3B), which <strong>al</strong>so drives mechanic<strong>al</strong> modes of the mirrors and supports, leading to extra modulation. However, the cross-correlation spectrum (blue trace) remains unchanged, equ<strong>al</strong> to the unperturbed spectrum (dashed curve), implying that very little of the ambient motion is transduced. The cross-correlation can <strong>al</strong>so be viewed as evidence that we have made a quantum nondemolition (QND) measurement of the intracavity photon fluctuations of the sign<strong>al</strong> beam (14, 28). Here, the membrane acts as the measurement device, with its state of motion recording the photon fluctuations over the band of the mechanic<strong>al</strong> resonance. The correlation C is equiv<strong>al</strong>ent to a state preparation fidelity for a nonide<strong>al</strong> QND measurement (29). Further, it has been shown that frequency-dependent ponderomotive squeezing of the sign<strong>al</strong> beam quantum noise is possible (30) and has recently been demonstrated in an atomic gas cavity optomechanic<strong>al</strong> system (31). For our current laser configuration (∆S = 0), we do not expect to see squeezing in the d<strong>et</strong>ected amplitude quadrature. However, our device param<strong>et</strong>ers are sufficient to re<strong>al</strong>ize much stronger squeezing than has previously been demonstrated, limited mainly by optic<strong>al</strong> loss. Our observations open the door to re<strong>al</strong>izing position measurement near the SQL if residu<strong>al</strong> therm<strong>al</strong> noise and excess cavity-laser phase noise can be eliminated with improved devices or a colder base temperature. References and Notes 1. G. M. Harry, Class. Quantum Gravity 27, 084006 (2010). 2. V. Braginsky, S. Vyatchanin, Sov. Phys. JETP 47, 433 (1978). 3. C. M. Caves, Phys. Rev. D Part. Fields 23, 1693 (1981). 4. K. Somiya, Class. Quantum Gravity 29, 124007 (2012). 5. H. J. Kimble, Y. Levin, A. B. Matsko, K. S. Thorne, S. P. Vyatchanin, Phys.Rev.DPart.Fields65, 022002 (2001). 6. V. B. Braginsky, Y. I. Vorontsov, K. S. Thorne, Science 209, 547 (1980). 7. J. D. Teufel, T. Donner, M. A. Castellanos-Beltran, J.W.Harlow,K.W.Lehnert,Nat. Nanotechnol. 4, 820 (2009). 8. G. An<strong>et</strong>sberger <strong>et</strong> <strong>al</strong>., Phys. Rev. A 82, 061804 (2010). 9. D. M. Stamper-Kurn, in Cavity Optomechanics, M.Aspelmeyer, T. Kippenberg, F. Marquardt, Eds. (Springer, New York); preprint available at http://arxiv.org/abs/1204.4351. 10. K. W. Murch, K. L. Moore, S. Gupta, D. M. Stamper-Kurn, Nat. Phys. 4, 561 (2008). 11. I. Tittonen <strong>et</strong> <strong>al</strong>., Phys. Rev. A 59, 1038 (1999). 12. P. Verlot <strong>et</strong> <strong>al</strong>., C. R. Phys. 12, 826 (2011). 13. P. Verlot, A. Tavernarakis, T. Briant, P.-F. Cohadon, A. Heidmann, Phys. Rev. L<strong>et</strong>t. 102, 103601 (2009). 14. A. Heidmann, Y. Hadjar, M. Pinard, Appl. Phys. B 64, 173 (1997). 15. K. Børkje <strong>et</strong> <strong>al</strong>., Phys. Rev. A 82, 013818 (2010). 16. K. Yamamoto <strong>et</strong> <strong>al</strong>., Phys. Rev. A 81, 033849 (2010). 17. A. Naik <strong>et</strong> <strong>al</strong>., Nature 443, 193 (2006). 18. J. D. Teufel <strong>et</strong> <strong>al</strong>., Nature 475, 359 (2011). 19. J. Chan <strong>et</strong> <strong>al</strong>., Nature 478, 89 (2011). 20. E. Verhagen, S. Deléglise, S. Weis, A. Schliesser, T. J. Kippenberg, Nature 482, 63 (2012). Similarity of Scattering Rates in M<strong>et</strong><strong>al</strong>s Showing T-Linear Resistivity J. A. N. Bruin, 1 H. Sakai, 1 R. S. Perry, 2 A. P. Mackenzie 1 Many exotic compounds, such as cuprate superconductors and heavy fermion materi<strong>al</strong>s, exhibit a linear in temperature (T) resistivity, the origin of which is not well understood. We found that the resistivity of the quantum critic<strong>al</strong> m<strong>et</strong><strong>al</strong> Sr3Ru2O7 is <strong>al</strong>so T-linear at the critic<strong>al</strong> magn<strong>et</strong>ic field of 7.9 T. Using the precise existing data for the Fermi surface topography and quasiparticle velocities of Sr3Ru2O7, we show that in the region of the T-linear resistivity, the scattering rate per kelvin is well approximated by the ratio of the Boltzmann constant to the Planck constant divided by 2p. Extending the an<strong>al</strong>ysis to a number of other materi<strong>al</strong>s reve<strong>al</strong>s similar results in the T-linear region, in spite of large differences in the microscopic origins of the scattering. When the high-temperature cuprate superconductors were discovered, it quickly became clear that the highest superconducting transition temperatures were seen in materi<strong>al</strong>s whose electric<strong>al</strong> resistivity varied linearly with temperature (T) in certain regions of the temperature-doping phase diagram. Since then, T-linear resistivity has been seen in the pnictide and organic superconductors, as well as in many heavy fermion compounds, both superconducting and non-superconducting. In most of the heavy fermion materi<strong>al</strong>s, the T-linear resistivity is seen when they have been tuned by some extern<strong>al</strong> 1 Scottish Universities Physics Alliance, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK. 2 Scottish Universities Physics Alliance, School of Physics and Astronomy, University of Edinburgh, Mayfield Road, Edinburgh EH9 3JZ, UK. param<strong>et</strong>er to create a low-temperature continuous phase transition known as a quantum critic<strong>al</strong> point (QCP). T-linear resistivity is therefore often associated with quantum critic<strong>al</strong>ity. However, other power laws—for example, T 1.5 —are <strong>al</strong>so seen in the resistivity in quantum critic<strong>al</strong> systems (1), and the origin of the T-linear term remains the subject of active research and debate. Here, we present an an<strong>al</strong>ysis of electric<strong>al</strong> transport data from 1.5 to 400 K in Sr3Ru2O7 and compare our findings to those in a wide vari<strong>et</strong>y of other materi<strong>al</strong>s, including element<strong>al</strong> m<strong>et</strong><strong>al</strong>s, that exhibit T-linear resistivity. Sr3Ru2O7 is a magn<strong>et</strong>ic-field–tuned quantum critic<strong>al</strong> system (2) that can be prepared in singlecryst<strong>al</strong> form with very low levels of disorder (3, 4). For an applied field oriented par<strong>al</strong>lel to the cryst<strong>al</strong>lographic c axis, the approach to the quantum 15 FEBRUARY 2013 VOL 339 SCIENCE www.sciencemag.org 21. F. Y. Kh<strong>al</strong>ili <strong>et</strong> <strong>al</strong>., Phys. Rev. A 86, 033840 (2012). 22. A. H. Safavi-Naeini <strong>et</strong> <strong>al</strong>., Phys. Rev. L<strong>et</strong>t. 108, 033602 (2012). 23. T. P. Purdy, R. W. P<strong>et</strong>erson, P.-L. Yu, C. A. Reg<strong>al</strong>, New J. Phys. 14, 115021 (2012). 24. J. D. Thompson <strong>et</strong> <strong>al</strong>., Nature 452, 72 (2008). 25. F. Marquardt, J. P. Chen, A. A. Clerk, S. M. Girvin, Phys. Rev. L<strong>et</strong>t. 99, 093902 (2007). 26. Materi<strong>al</strong>s and m<strong>et</strong>hods are available as supplementary materi<strong>al</strong>s on Science Online. 27. I. Wilson-Rae, N. Nooshi, W. Zwerger, T. J. Kippenberg, Phys. Rev. L<strong>et</strong>t. 99, 093901 (2007). 28. K. Jacobs, P. Tombesi, M. J. Coll<strong>et</strong>t, D. F. W<strong>al</strong>ls, Phys. Rev. A 49, 1961 (1994). 29. M. J. Holland, M. J. Coll<strong>et</strong>t, D. F. W<strong>al</strong>ls, M. D. Levenson, Phys. Rev. A 42, 2995 (1990). 30. C. Fabre <strong>et</strong> <strong>al</strong>., Phys. Rev. A 49, 1337 (1994). 31. D. W. C. Brooks <strong>et</strong> <strong>al</strong>., Nature 488, 476 (2012). Acknowledgments: We thank P.-L. Yu for technic<strong>al</strong> assistance and K. Lehnert’s group for helpful discussions. This work is supported by: the Defense Advanced Research Projects Agency Quantum-Assisted Sensing and Readout program, the Office of Nav<strong>al</strong> Research Young Investigator Program, and the JILA NSF Physics Frontier Center. T.P.P. thanks the Nation<strong>al</strong> Research Council for support. C.A.R. thanks the Clare Boothe Luce foundation for support. Supplementary Materi<strong>al</strong>s www.sciencemag.org/cgi/content/full/339/6121/801/DC1 Materi<strong>al</strong>s and M<strong>et</strong>hods Figs. S1 to S5 References (32, 33) 9 October 2012; accepted 18 December 2012 10.1126/science.1231282 critic<strong>al</strong> point at the critic<strong>al</strong> field moHc =7.9Tis cut off by the formation of a purity-sensitive nematic phase for 7.8 T < moH
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