Zobrazeno 1 - 10
of 8 958
pro vyhledávání: '"Dai G."'
Autor:
Matsuura, K., Roppongi, M., Qiu, M., Sheng, Q., Cai, Y., Yamakawa, K., Guguchia, Z., Day, R. P., Kojima, K. M., Damascelli, A., Sugimura, Y., Saito, M., Takenaka, T., Ishihara, K., Mizukami, Y., Hashimoto, K., Gu, Y., Guo, S., Fu, L., Zhang, Z., Ning, F., Zhao, G., Dai, G., Jin, C., Beare, J. W., Luke, G. M., Uemura, Y. J., Shibauchi, T.
Publikováno v:
Proc. Natl. Acad. Sci. USA 120, e2208276120 (2023)
Iron-chalcogenide superconductors FeSe$_{1-x}$S$_x$ possess unique electronic properties such as non-magnetic nematic order and its quantum critical point. The nature of superconductivity with such nematicity is important for understanding the mechan
Externí odkaz:
http://arxiv.org/abs/2304.03409
Autor:
Chen, Y. P., Li, J., Xiong, S. L., Ji, L., Zhang, S., Peng, W. X., Qiao, R., Li, X. Q., Wen, X. Y., Song, L. M., Zheng, S. J., Song, X. Y., Zhao, X. Y., Huang, Y., Lu, F. J., Zhang, S. N., Xiao, S., Cai, C., Zhang, B. X., An, Z. H., Chen, C., Chen, G., Chen, W., Dai, G. Q., Du, Y. Q., Gao, M., Gong, K., Guo, D. Y., Guo, Z. W., He, J. J., Li, B., Li, C., Li, C. Y., Li, G., Li, J. H., Li, L., Li, Q. X., Li, X. B., Li, Y. G., Liang, J., Liang, X. H., Liao, J. Y., Liu, J. C., Liu, X. J., Liu, Y. Q., Luo, Q., Ma, X., Meng, B., Ou, G., Shi, D. L., Shi, F., Shi, J. Y., Sun, G. X., Sun, X. L., Tuo, Y. L., Wang, C. W., Wang, H., Wang, H. Y., Wang, J., Wang, J. Z., Wang, P., Wang, Y. S., Wang, Y. X., Wen, X., Wu, H., Xie, S. L., Xu, Y. B., Xu, Y. P., Xue, W. C., Yang, S., Yao, M., Ye, J. Y., Yi, Q. B., Zhang, C. M., Zhang, C. Y., Zhang, D. L., Zhang, Fan, Zhang, Fei, Zhang, H. M., Zhang, K., Zhang, P., Zhang, X. L., Zhang, Y. Q., Zhang, Z., Zhao, G. Y., Zhao, S. Y., Zhao, Y., Zheng, C., Zhou, X., Zhu, Y.
One month after launching Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM), a bright thermonuclear X-ray burst from 4U~0614+09, was observed on January 24, 2021. We report the time-resolved spectroscopy of the burst
Externí odkaz:
http://arxiv.org/abs/2112.04790
Publikováno v:
Advances in Astronomy, Vol 2010 (2010)
Magnetic fields are everywhere in nature, and they play an important role in every astronomical environment which involves the formation of plasma and currents. It is natural therefore to suppose that magnetic fields could be present in the turbulent
Externí odkaz:
https://doaj.org/article/9b7c8339458a4e18be8bb6bc95891fa5
Publikováno v:
Journal of the European Optical Society-Rapid Publications, Vol 9, p 14003 (2014)
In the present paper, we propose a 2D-Fourier transform method as a simple and efficient algorithm for stochastical and numerical studies to investigate the systematic impacts of line edge roughness on light diffraction pattern of periodic line-space
Externí odkaz:
https://doaj.org/article/9188b079532740f78e8b0841629f1da3
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
International Journal of General Medicine, Vol Volume 15, Pp 7241-7248 (2022)
GuiYing Dai,1,* JunYu Wang,1 FengLi Gao,2 WenHong Liu,1 Ping Li,1 Bing Wei,1 Jun Yang1,* 1Emergency Medicine Clinical Research Center, Beijing Chao-Yang Hospital, Capital Medical University, & Beijing Key Laboratory of Cardiopulmonary Cerebra
Externí odkaz:
https://doaj.org/article/324a501af7e4426aba9e71f4b2adb0c2
Autor:
Wang, C. G., Li, Z., Yang, J., Xing, L. Y., Dai, G. Y., Wang, X. C., Jin, C. Q., Zhou, R., Zheng, Guo-qing
Publikováno v:
Phys. Rev. Lett. 121, 167004 (2018)
A magnetic order can be completely suppressed at zero temperature($T$), by doping carriers or applying pressure, at a quantum critical point(QCP), around which physical properties change drastically. However, the situation is unclear for an electroni
Externí odkaz:
http://arxiv.org/abs/1810.08777
Autor:
Yamazaki, Dai G.
Publikováno v:
Phys. Rev. D 97, 103525 (2018)
We discuss the manner in which the primordial magnetic field (PMF) suppresses the cosmic microwave background (CMB) $B$ mode due to the weak-lensing (WL) effect. The WL effect depends on the lensing potential (LP) caused by matter perturbations, the
Externí odkaz:
http://arxiv.org/abs/1805.09903
Publikováno v:
International Journal of General Medicine, Vol Volume 15, Pp 3447-3458 (2022)
Hong Wang,1,* Tao Yang,2,* Xiaodan Yu,3,* Zhihong Chen,4 Yajuan Ran,5 Jiajia Wang,6 Guangming Dai,1 Huojin Deng,7 Xinglong Li,8 Tao Zhu8 1Respiratory Medicine, First People’s Hospital of Suining City, Suining, 629000, Sichuan, People’
Externí odkaz:
https://doaj.org/article/89e8009108b24469b19eaae9979b269b
Autor:
Akahori, Takuya, Nakanishi, Hiroyuki, Sofue, Yoshiaki, Fujita, Yutaka, Ichiki, Kiyotomo, Ideguchi, Shinsuke, Kameya, Osamu, Kudoh, Takahiro, Kudoh, Yuki, Machida, Mami, Miyashita, Yoshimitsu, Ohno, Hiroshi, Ozawa, Takeaki, Takahashi, Keitaro, Takizawa, Motokazu, Yamazaki, Dai G.
Magnetic field is ubiquitous in the Universe and it plays essential roles in various astrophysical phenomena, yet its real origin and evolution are poorly known. This article reviews current understanding of magnetic fields in the interstellar medium
Externí odkaz:
http://arxiv.org/abs/1709.02072