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This work was supported by the National Natural Science Foundation of China (Grant Nos. 11774286, 11604258, 11534008, 11374238, and 11574247), and the China Postdoctoral Science Foundation (Grant No. 2016M592771).
[1] Fang N.. Science, 2005, 308: 534-537 CrossRef PubMed ADS Google Scholar
[2] Berggren K., Bard A., Wilbur J., Gillaspy J., Helg A., McClelland J., Rolston S., Phillips W., Prentiss M., Whitesides G.. Science, 1995, 269: 1255-1257 CrossRef ADS Google Scholar
[3] Firstenberg O., London P., Shuker M., Ron A., Davidson N.. Nat. Phys, 2009, 5: 665-668 CrossRef ADS arXiv Google Scholar
[4] Yavuz D. D., Proite N. A.. Phys. Rev. A, 2007, 76: 041802 CrossRef ADS Google Scholar
[5] Gorshkov A. V., Jiang L., Greiner M., Zoller P., Lukin M. D.. Phys. Rev. Lett., 2008, 100: 093005 CrossRef PubMed ADS arXiv Google Scholar
[6] Kapale K. T., Agarwal G. S.. Opt. Lett., 2010, 35: 2792 CrossRef ADS Google Scholar
[7] Dey T. N., Evers J.. Phys. Rev. A, 2011, 84: 043842 CrossRef ADS arXiv Google Scholar
[8] Verma O. N., Zhang L., Evers J., Dey T. N.. Phys. Rev. A, 2013, 88: 013810 CrossRef ADS arXiv Google Scholar
[9]
J. Zhou, B. J. Liu, Z. P. Hong, and Z. Y. Xue, Sci. China-Phys. Mech. Astron.
[10] Ding D. S., Zhou Z. Y., Shi B. S.. Opt. Lett., 2014, 39: 240 CrossRef ADS arXiv Google Scholar
[11] Cao M., Zhang L., Yu Y., Ye F., Wei D., Guo W., Zhang S., Gao H., Li F.. Opt. Lett., 2014, 39: 2723 CrossRef ADS Google Scholar
[12] Zhang L., Evers J.. Phys. Rev. A, 2014, 89: 013817 CrossRef ADS arXiv Google Scholar
[13] Verma O. N., Dey T. N.. Phys. Rev. A, 2015, 91: 013820 CrossRef ADS arXiv Google Scholar
[14] Cho Y. W., Oh J. E., Kim Y. H.. Opt. Express, 2012, 20: 5809 CrossRef ADS Google Scholar
[15] Cho Y. W., Oh J. E., Kim Y. H.. Phys. Rev. A, 2012, 86: 013844 CrossRef ADS Google Scholar
[16] Zhong M. L., Xu P., Lu L. L., Zhu S. N.. Sci. China-Phys. Mech. Astron., 2016, 59: 670311 CrossRef ADS Google Scholar
[17] Li J., Luo B., Yang D., Yin L., Wu G., Guo H.. Sci. Bull., 2017, 62: 717-723 CrossRef Google Scholar
[18] Yu Y., Wang C., Liu J., Wang J., Cao M., Wei D., Gao H., Li F.. Opt. Express, 2016, 24: 18290 CrossRef ADS Google Scholar
[19] Cao M., Yang X., Wang J., Qiu S., Wei D., Gao H., Li F.. Opt. Lett., 2016, 41: 5349 CrossRef ADS Google Scholar
[20] Cao M., Wang J., Yang X., Qiu S., Gao H., Li F.. Sci Rep, 2017, 7: 8015 CrossRef PubMed Google Scholar
[21] Wang Y., Wang F., Liu R., Chen D., Gao H., Zhang P., Li F.. Opt. Lett., 2015, 40: 5323 CrossRef ADS arXiv Google Scholar
[22]
G. F. Xu, Sci. China-Phys. Mech. Astron.
[23] Yang Z., Maga {n}a-Loaiza O. S., Mirhosseini M., Zhou Y., Gao B., Gao L., Rafsanjani S. M. H., Long G. L., Boyd R. W.. Light Sci Appl, 2017, 6: e17013 CrossRef Google Scholar
Figure 1
(Color online) (a) Theoretical model of the probe beam propagation through an atomic medium. (b) Three-level $~\Lambda~$ configuration. A three-level diagram of $D$$_{1}$ line of $^{87}$Rb. The energy level configuration is taken as the following: $|b\rangle~(5^{2}S_{1/2},F=2,M_{F}=2)$ and $|c\rangle~(5^{2}S_{1/2},F=2,M_{F}=0)$ are two Zeeman sublevels of the $^{87}$Rb atom, $|a\rangle~(5^{2}P_{1/2},F'=1)$ is the excited state. $\omega_{\text{c}}$ and $\omega_{\text{p}}$ correspond to the frequency of coupling and probe beams. $\Delta_{\text{p}}=\omega_{\text{p}}-\omega_{ac}$ is the single-photon detuning of the probe beam, $\Delta_{\text{c}}=\omega_{\text{c}}-\omega_{ab}$ is the single-photon detuning of the coupling beam.
Figure 2
(Color online) (a) Normalized intensity of the transmitted probe beam. The output is taken at exit plane of the 5-cm-long medium. We choose the parameters for numerical calculations as given by $N=10^{12}$ cm$^{-3}$, $g^{0}=0.1\gamma$, $G^{0}=0.7\gamma$ and $\lambda=795$ nm. (b) Variation of the full width at half maximum of the probe beam with different $\Delta_{\text{c}}$ for $\Delta_{\text{p}}=0$.
Figure 3
(Color online) The experimental setup. SMF, single mode optical fiber; L, lens; M, mirrors; HWP, half-wave plate; QWP, quarter-wave plate; PBS, polarization beam splitter; BS, beam splitter; CCD, charge coupled device camera; AOM, acoustic optical modulator.
Figure 4
(Color online) The first row of graphs are intensity distributions ((a), (c)) and the second order correlation ((b), (d)) of thermal light in free space and CPT condition; the second row (without atoms) ((e)-(h)) and third row (with atoms) ((i)-(l)) represent corresponding speckle in different color box. The frequency detuning of coupling beam is $\Delta_{\text{c}}$=74 MHz. The horizontal coordinates represent pixels and a pixel is 5.8 $\mu$m.
Figure 5
(Color online) The experimental results of GI. (a) Detection setup (see text for detail description). (b)-(d) The cases in free space , blue detuning and red detuning of coupling beam. The horizontal coordinates represent pixels and a pixel is 5.8 $\mu$m.
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