Zobrazeno 1 - 10
of 2 017
pro vyhledávání: '"WANG, B. Y."'
Autor:
Rossi, M., Lu, H., Lee, K., Goodge, B. H., Choi, J., Osada, M., Lee, Y., Li, D., Wang, B. Y., Jost, D., Agrestini, S., Garcia-Fernandez, M., Shen, Z. X., Zhou, Ke-Jin, Been, E., Moritz, B., Kourkoutis, L. F., Devereaux, T. P., Hwang, H. Y., Lee, W. S.
We conducted a comparative study of the rare-earth infinite-layer nickelates films, RNiO2 (R = La, Pr, and Nd) using resonant inelastic X-ray scattering (RIXS). We found that the gross features of the orbital configurations are essentially the same,
Externí odkaz:
http://arxiv.org/abs/2312.16444
Autor:
Xu, X. H., Wang, Y., Wei, F. S., Feng, X. S., Bo, M. H., Tang, H. W., Wang, D. S., Lei, B., Wang, B. Y., Zuo, P. B., Jiang, C. W., Xu, X. J., Zhou, Z. L., Li, Z., Zou, P., Wang, L. D., Gu, Y. X., Chen, Y. L., Zhang, W. Y., Sun, P.
Analyzing the effects of space weather on aviation is a new and developing topic. It has been commonly accepted that the flight time of the polar flights may increase during solar proton events because the flights have to change their route to avoid
Externí odkaz:
http://arxiv.org/abs/2209.07703
Autor:
Xu, X. H., Wang, Y., Wei, F. S., Feng, X. S., Bo, M. H., Tang, H. W., Wang, D. S., Bian, L., Wang, B. Y., Zhang, W. Y., Huang, Y. S., Li, Z., Guo, J. P., Zuo, P. B., Jiang, C. W., Xu, X. J., Zhou, Z. L., Zou, P.
Solar flare is one of the severest solar activities on the sun, and it has many important impacts on the near-earth space. It has been found that flight arrival delays will increase during solar flare. However, the detailed intrinsic mechanism of how
Externí odkaz:
http://arxiv.org/abs/2209.07701
Autor:
Wang, Y., Xu, X. H., Wei, F. S., Feng, X. S., Bo, M. H., Tang, H. W., Wang, D. S., Bian, L., Wang, B. Y., Zhang, W. Y., Huang, Y. S., Li, Z., Guo, J. P., Zuo, P. B., Jiang, C. W., Xu, X. J., Zhou, Z. L., Zou, P.
Although the sun is really far away from us, some solar activities could still influence the performance and reliability of space-borne and ground-based technological systems on Earth. Those time-varying conditions in space caused by the sun are also
Externí odkaz:
http://arxiv.org/abs/2209.07700
Autor:
Lu, H., Rossi, M., Nag, A., Osada, M., Li, D. F., Lee, K., Wang, B. Y., Garcia-Fernandez, M., Agrestini, S., Shen, Z. X., Been, E. M., Moritz, B., Devereaux, T. P., Zaanen, J., Hwang, H. Y., Zhou, Ke-Jin, Lee, W. S.
Publikováno v:
Science 373, 213-216 (2021)
The discovery of superconductivity in infinite-layer nickelates brings us tantalizingly close to a new material class that mirrors the cuprate superconductors. Here, we report on magnetic excitations in these nickelates, measured using resonant inela
Externí odkaz:
http://arxiv.org/abs/2105.11300
Autor:
Rossi, M., Lu, H., Nag, A., Li, D., Osada, M., Lee, K., Wang, B. Y., Agrestini, S., Garcia-Fernandez, M., Chuang, Y. -D., Shen, Z. X., Hwang, H. Y., Moritz, B., Zhou, Ke-Jin, Devereaux, T. P., Lee, W. S.
The recent discovery of superconductivity in Nd$_{1-x}$Sr$_{x}$NiO$_2$ has drawn significant attention in the field. A key open question regards the evolution of the electronic structure with respect to hole doping. Here, we exploit x-ray absorption
Externí odkaz:
http://arxiv.org/abs/2011.00595
Akademický článek
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Autor:
Maser, Daniel L., Hoenig, Eli, Wang, B. -Y., Rupasinghe, P. M., Porsev, S. G., Safronova, M. S., Majumder, P. K.
Publikováno v:
Phys. Rev. A 100, 052506 (2019)
We have completed a measurement of the $(6s^26p^2)\, ^3\!P_0 \rightarrow \, ^3\!P_2$ 939 nm electric quadrupole ($E2$) transition amplitude in atomic lead. Using a Faraday rotation spectroscopy technique and a sensitive polarimeter, we have measured
Externí odkaz:
http://arxiv.org/abs/1909.10581
Akademický článek
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Autor:
Vilas, N. B., Wang, B. -Y., Rupasinghe, P. M., Maser, D. L., Safronova, M. S., Safronova, U. I., Majumder, P. K.
Publikováno v:
Phys. Rev. A 97, 022507 (2018)
We report measurements of the $^{115}$In $7p_{1/2}$ and $7p_{3/2}$ scalar and tensor polarizabilities using two-step diode laser spectroscopy in an atomic beam. The scalar polarizabilities are one to two orders of magnitude larger than for lower lyin
Externí odkaz:
http://arxiv.org/abs/1712.07706