Zobrazeno 1 - 10
of 450
pro vyhledávání: '"Ma, J B"'
Autor:
Lucy L. Clarke, Benjamin Hine, Dawn England, Poppy P. M. S. Flew, Ritaj Alzahri, Stepheni N. Juriansz, Ma. J. B. C. Garcia
Publikováno v:
Frontiers in Sociology, Vol 9 (2024)
Previous research suggests that the portrayal of male and female protagonists in Disney animations may be changing over time. The current study examined the portrayal of gendered behaviors displayed within some of Disney's most successful animated fe
Externí odkaz:
https://doaj.org/article/433095b4e1c5469c81e75e22418550c3
Autor:
Yan, S. Q., Li, X. Y., Nishio, K., Lugaro, M., Li, Z. H., Makii, H., Pignatari, M., Wang, Y. B., Orlandi, R., Hirose, K., Tsukada, K., Mohr, P., Li, G. S., Wang, J. G., Gao, B. S., Han, Y. L., Guo, B., Li, Y. J., Shen, Y. P., Sato, T. K., Ito, Y., Suzaki, F., Su, J., Yang, Y. Y., Wang, J. S., Ma, J. B., Ma, P., Bai, Z., Xu, S. W., Ren, J., Fan, Q. W., Zeng, S., Han, Z. Y., Nan, W., Nan, W. K., Chen, C., Lian, G., Hu, Q., Duan, F. F., Jin, S. Y., Tang, X. D., Liu, W. P.
The long-lived $^{60}$Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutron-capture reaction $^{59}$Fe(n,$\gamma$)$^{60}$Fe on $^{59}$Fe (half-
Externí odkaz:
http://arxiv.org/abs/2109.12654
Autor:
Li, G., Lou, J. L., Ye, Y. L., Hua, H., Wang, H., Han, J. X., Liu, W., Bai, S. W., Tan, Z. W., Ma, K., Chen, J. H., Yang, L. S., Wang, S. J., Hu, Z. Y., Yu, H. Z., Zhu, H. Y., Xia, B. L., Jiang, Y., Liu, Y., Yang, X. F., Li, Q. T., Xu, J. Y., Wang, J. S., Yang, Y. Y., Ma, J. B., Chen, R. F., Ma, P., Bai, Z., Duan, F. F., Hu, L. Y., Li, J. W., Li, Y., Song, Y. S., Zhang, Suyalatu, Huang, M. R.
Two types of wedge-shaped CsI(Tl)s were designed to be placed behind the annular double-sided silicon detectors (ADSSDs) to identify the light charged particles with the $\Delta E-E$ method. The properties of CsI(Tl)s with different shapes and sizes,
Externí odkaz:
http://arxiv.org/abs/2103.02151
Autor:
Guo, S., Zhou, X. H., Petrache, C. M., Lawrie, E. A., Mthembu, S., Fang, Y. D., Wu, H. Y., Wang, H. L., Meng, H. Y., Li, G. S., Qiang, Y. H., Wang, J. G., Liu, M. L., Zheng, Y., Ding, B., Zhang, W. Q., Rohilla, A., Mukhi, K. R., Yang, Y. Y., Ong, H. J., Ma, J. B., Xu, S. W., Bai, Z., Fan, H. L., Huang, J. F., Li, J. H., Xu, J. H., Lv, B. F., Hua, W., Gan, Z. G., Zhang, Y. H.
Precession is a unique motion in which the orientation of the rotational axis of a rotating body is not fixed but moving, and it generally exists in the Universe from giant stars through tiny atomic nuclei. In principle, the precession of an atomic n
Externí odkaz:
http://arxiv.org/abs/2011.14354
Autor:
Liang, P. F., Sun, L. J., Lee, J., Hou, S. Q., Xu, X. X., Lin, C. J., Yuan, C. X., He, J. J., Li, Z. H., Wang, J. S., Wang, D. X., Wu, H. Y., Yang, Y. Y., Lam, Y. H., Ma, P., Duan, F. F., Gao, Z. H., Hu, Q., Bai, Z., Ma, J. B., Wang, J. G., Zhong, F. P., Wu, C. G., Luo, D. W., Jiang, Y., Liu, Y., Hou, D. S., Li, R., Ma, N. R., Ma, W. H., Shi, G. Z., Yu, G. M., Patel, D., Jin, S. Y., Wang, Y. F., Yu, Y. C., Zhou, Q. W., Wang, P., Hu, L. Y., Wang, X., Zang, H. L., Li, P. J., Zhao, Q. Q., Yang, L., Wen, P. W., Yang, F., Jia, H. M., Zhang, G. L., Pan, M., Wang, X. Y., Sun, H. H., Hu, Z. G., Chen, R. F., Liu, M. L., Yang, W. Q., Zhao, Y. M.
Publikováno v:
Phys. Rev. C 101, 024305 (2020)
$\beta$ decay of $^{26}$P was used to populate the astrophysically important $E_x=$5929.4(8) keV $J^{\pi}=3{^+}$ state of $^{26}$Si. Both $\beta$-delayed proton at 418(8) keV and gamma ray at 1742(2) keV emitted from this state were measured simultan
Externí odkaz:
http://arxiv.org/abs/1909.11377
Autor:
Sun, L. J., Xu, X. X., Hou, S. Q., Lin, C. J., José, J., Lee, J., He, J. J., Li, Z. H., Wang, J. S., Yuan, C. X., Wang, D. X., Wu, H. Y., Liang, P. F., Yang, Y. Y., Lam, Y. H., Ma, P., Duan, F. F., Gao, Z. H., Hu, Q., Bai, Z., Ma, J. B., Wang, J. G., Zhong, F. P., Wu, C. G., Luo, D. W., Jiang, Y., Liu, Y., Hou, D. S., Li, R., Ma, N. R., Ma, W. H., Shi, G. Z., Yu, G. M., Patel, D., Jin, S. Y., Wang, Y. F., Yu, Y. C., Zhou, Q. W., Wang, P., Hu, L. Y., Wang, X., Zang, H. L., Li, P. J., Zhao, Q. Q., Yang, L., Wen, P. W., Yang, F., Jia, H. M., Zhang, G. L., Pan, M., Wang, X. Y., Sun, H. H., Hu, Z. G., Chen, R. F., Liu, M. L., Yang, W. Q., Zhao, Y. M., Zhang, H. Q.
Publikováno v:
Phys. Rev. C 99, 064312 (2019)
Background: Beta-decay spectroscopy provides valuable nuclear physics input for thermonuclear reaction rates of astrophysical interest and stringent test for shell-model theories far from the stability line. Purpose: The available decay properties of
Externí odkaz:
http://arxiv.org/abs/1809.02987
Autor:
Sun, L. J., Xu, X. X., Hou, S. Q., Lin, C. J., José, J., Lee, J., He, J. J., Li, Z. H., Wang, J. S., Yuan, C. X., Herwig, F., Keegans, J., Budner, T., Wang, D. X., Wu, H. Y., Liang, P. F., Yang, Y. Y., Lam, Y. H., Ma, P., Duan, F. F., Gao, Z. H., Hu, Q., Bai, Z., Ma, J. B., Wang, J. G., Zhong, F. P., Wu, C. G., Luo, D. W., Jiang, Y., Liu, Y., Hou, D. S., Li, R., Ma, N. R., Ma, W. H., Shi, G. Z., Yu, G. M., Patel, D., Jin, S. Y., Wang, Y. F., Yu, Y. C., Zhou, Q. W., Wang, P., Hu, L. Y., Wang, X., Zang, H. L., Li, P. J., Zhao, Q. Q., Yang, L., Wen, P. W., Yang, F., Jia, H. M., Zhang, G. L., Pan, M., Wang, X. Y., Sun, H. H., Hu, Z. G., Chen, R. F., Liu, M. L., Yang, W. Q., Zhao, Y. M., Zhang, H. Q.
The mass of $^{27}$P was predicted to impact the X-ray burst (XRB) model predictions of burst light curves and the composition of the burst ashes. To address the uncertainties and inconsistencies in the reported $^{27}$P masses in literature, a wealt
Externí odkaz:
http://arxiv.org/abs/1809.02980
Autor:
Ma, W. H., Wang, J. S., Patel, D., Yang, Y. Y., Ma, J. B., Jin, S. L., Ma, P., Hu, Q., Bai, Z., Huang, M. R., Liu, X. Q., Zhou, Y. J., Chen, J., Gao, Z. H., Wang, Q., Lubian, J., Li, J. X., Wang, T. F., Mukherjee, S., Ju, X. Y., Yu, Y. S., Wu, T. W., Ni, C., Jia, X. D., Liu, Q. B., Zhang, Y. H., Xu, H. S., Xiao, G. Q.
Publikováno v:
Phys. Rev. C 103, 061302 (2021)
$^{6}$He+$t$ cluster states of exited $^{9}$Li have been measured by 32.7 MeV/nucleon $^{9}$Li beams bombarding on $^{208}$Pb target. Two resonant states are clearly observed with the excitation energies at 9.8 MeV and 12.6 MeV and spin-parity of 3/2
Externí odkaz:
http://arxiv.org/abs/1709.02515
Autor:
Teng, X. Z., Teh, C. E., Lee, J., Xu, X. X., Lin, C. J., Sun, L. J., Wang, J. S., Fang, D. Q., Leblond, S., Li, Z. H., Li, J., Ma, N. R., Ma, J. B., Zang, H. L., Ma, P., Jin, S. L., Huang, M. R., Bai, Z., Liu, J. J., Lokotko, T., Yang, F., Jia, H. M., Wang, D. X., Yang, Y. Y., Hu, Z. G., Wang, M., Zhang, H. Q.
Fragmentation cross section of $^{28}$Si + $^{9}$Be reaction at 75.8 MeV/u was analyzed for studying the decay mode of single-proton emission in $^{21}$Al (the proton-rich nucleus with neutron closed-shell of $N = 8$ and $T_z = -5/2$). With the compa
Externí odkaz:
http://arxiv.org/abs/1704.03249