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Akademický článek
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Publikováno v:
Physical Review A 95, 013835 (2017)
Polarized light microscopy using path-entangled $N$-photon states (i.e., the N00N states) has been demonstrated to surpass the shot-noise limit at very low light illumination. However, the microscopy images suffer from divergence of phase sensitivity
Externí odkaz:
http://arxiv.org/abs/1606.03267
Autor:
Liu, H., Benoit, M., Chen, H., Chen, K., Di Bello, F. A., Iacobucci, G., Lanni, F., Peric, I., Ristic, B., Pinto, M. Vicente Barreto, Wu, W., Xu, L., Jin, G.
High Voltage CMOS sensors are a promising technology for tracking detectors in collider experiments. Extensive R&D studies are being carried out by the ATLAS Collaboration for a possible use of HV-CMOS in the High Luminosity LHC upgrade of the Inner
Externí odkaz:
http://arxiv.org/abs/1603.07950
Autor:
Flay, D., Posik, M., Parno, D. S., Allada, K., Armstrong, W., Averett, T., Benmokhtar, F., Bertozzi, W., Camsonne, A., Canan, M., Cates, G. D., Chen, C., Chen, J. -P., Choi, S., Chudakov, E., Cusanno, F., Dalton, M. M., Deconinck, W., de Jager, C. W., Deng, X., Deur, A., Dutta, C., Fassi, L. El, Franklin, G. B., Friend, M., Gao, H., Garibaldi, F., Gilad, S., Gilman, R., Glamazdin, O., Golge, S., Gomez, J., Guo, L., Hansen, O., Higinbotham, D. W., Holmstrom, T., Huang, J., Hyde, C., Ibrahim, H. F., Jiang, X., Jin, G., Katich, J., Kelleher, A., Kolarkar, A., Korsch, W., Kumbartzki, G., LeRose, J. J., Lindgren, R., Liyanage, N., Long, E., Lukhanin, A., Mamyan, V., McNulty, D., Meziani, Z. -E., Michaels, R., Mihovilovič, M., Moffit, B., Muangma, N., Nanda, S., Narayan, A., Nelyubin, V., Norum, B., Oh, Y., Peng, J. C., Qian, X., Qiang, Y., Rakhman, A., Riordan, S., Saha, A., Sawatzky, B., Shabestari, M. H., Shahinyan, A., Širca, S., Solvignon, P., Subedi, R., Sulkosky, V., Tobias, A., Troth, W., Wang, D., Wang, Y., Wojtsekhowski, B., Yan, X., Yao, H., Ye, Y., Ye, Z., Yuan, L., Zhan, X., Zhang, Y., Zhang, Y. -W., Zhao, B., Zheng, X.
Publikováno v:
Phys. Rev. D 94, 052003 (2016)
We report on the results of the E06-014 experiment performed at Jefferson Lab in Hall A, where a precision measurement of the twist-3 matrix element $d_2$ of the neutron ($d_{2}^{n}$) was conducted. This quantity represents the average color Lorentz
Externí odkaz:
http://arxiv.org/abs/1603.03612
We show by direct numerical simulation (DNS) that the Lagrangian cross correlation of velocity gradients in homogeneous isotropic turbulence increases at short times, whereas its auto-correlation decreases. Kinematic considerations allow to show that
Externí odkaz:
http://arxiv.org/abs/1511.06501
Publikováno v:
In Analytical Biochemistry April 2021
Autor:
De Cat, P., Fu, J. N., Ren, A. B., Yang, X. H., Shi, J. R., Luo, A. L., Yang, M., Wang, J. L., Zhang, H. T., Shi, H. M., Zhang, W., Dong, Subo, Catanzaro, G., Corbally, C. J., Frasca, A., Gray, R. O., Molenda-Zakowicz, J., Uytterhoeven, K., Briquet, M., Bruntt, H., Frandsen, S., Kiss, L., Kurtz, D. W., Marconi, M., Niemczura, E., Oestensen, R. H., Ripepi, V., Smalley, B., Southworth, J., Szabo, R., Telting, J. H., Karoff, C., Aguirre, V. Silva, Wu, Y., Hou, Y. H., Jin, G., Zhou, X. L.
The nearly continuous light curves with micromagnitude precision provided by the space mission Kepler are revolutionising our view of pulsating stars. They have revealed a vast sea of low-amplitude pulsation modes that were undetectable from Earth. T
Externí odkaz:
http://arxiv.org/abs/1508.06391
Publikováno v:
Phys. Rev. E 92, 043307 (2015)
The precise calculations of the Wigner's d-matrix are important in various research fields. Due to the presence of large numbers, direct calculations of the matrix using the Wigner's formula suffer from loss of precision. We present a simple method t
Externí odkaz:
http://arxiv.org/abs/1507.04535
Autor:
Luo, A. -L., Zhao, Y. -H., Zhao, G., Deng, L. -C., Liu, X. -W., Jing, Y. -P., Wang, G., Zhang, H. -T, Shi, J. -R., Cui, X. -Q., Chu, Y. -Q., Li, G. -P., Bai, Z. -R., Cai, Y., Cao, S. -Y., Cao, Z. -H, Carlin, J. L., Chen, H. Y., Chen, J. -J., Chen, K. -X., Chen, L., Chen, X. -L., Chen, X. -Y., Chen, Y., Christlieb, N., Chu, J. -R., Cui, C. -Z., Dong, Y. -Q., Du, B., Fan, D. -W., Feng, L., Fu, J. -N, Gao, P., Gong, X. -F., Gu, B. -Z., Guo, Y. -X., Han, Z. -W., He, B. -L., Hou, J. -L., Hou, Y. -H., Hou, W., Hu, H. -Z., Hu, N. -S., Hu, Z. -W., Huo, Z. -Y., Jia, L., Jiang, F. -H., Jiang, X., Jiang, Z. -B., Jin, G., Kong, X., Lei, Y. -J., Li, A. -H., Li, C. -H., Li, G. -W., Li, H. -N., Li, J., Li, Q., Li, S., Li, S. -S., Li, X. -N., Li, Y., Li, Y. -B., Li, Y. -P., Liang, Y., Lin, C. -C., Liu, C., Liu, G. -R., Liu, G. -Q., Liu, Z. -G., Lu, W. -Z., Luo, Y., Mao, Y. -D., Newberg, H., Ni, J. -J., Qi, Z. -X., Qi, Y. -J., Shen, S. -Y., Shi, H. -M., Song, J., Song, Y. -H., Su, D. -Q., Su, H. -J., Tang, Z. -H., Tao, Q. -S., Tian, Y., Wang, D., Wang, D. -Q., Wang, F. -F., Wang, G. -M., Wang, H., Wang, H. -C., Wang, J., Wang, J. -N., Wang, J. -L., Wang, J. -P., Wang, J. -X., Wang, L., Wang, M. -X., Wang, S. -G., Wang, S. -Q., Wang, X., Wang, Y. -N., Wang, Y., Wang, Y. -F., Wei, P., Wei, M. -Z., Wu, H., Wu, K. -F., Wu, X. -B., Wu, Y., Wu, Y. Z., Xing, X. -Z., Xu, L. -Z., Xu, X. -Q., Xu, Y., Yan, T. -S., Yang, D. -H., Yang, H. -F., Yang, H. -Q., Yang, M., Yao, Z. -Q., Yu, Y., Yuan, H., Yuan, H. -B., Yuan, H. -L., Yuan, W. -M., Zhai, C., Zhang, E. -P., Zhang, H. W., Zhang, J. -N., Zhang, L. -P., Zhang, W., Zhang, Y., Zhang, Y. -X., Zhang, Z. -C., Zhao, M., Zhou, F., Zhou, X., Zhu, J., Zhu, Y. -T., Zou, S. -C., Zuo, F.
The Large sky Area Multi-Object Spectroscopic Telescope (LAMOST) General Survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects both i
Externí odkaz:
http://arxiv.org/abs/1505.01570