Zobrazeno 1 - 10
of 771
pro vyhledávání: '"Chen, R. F."'
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:
Zhang, Z. Y., Yang, H. B., Huang, M. H., Gan, Z. G., Yuan, C. X., Qi, C., Andreyev, A. N., Liu, M. L., Ma, L., Zhang, M. M., Tian, Y. L., Wang, Y. S., Wang, J. G., Yang, C. L., Li, G. S., Qiang, Y. H., Yang, W. Q., Chen, R. F., Zhang, H. B., Lu, Z. W., Xu, X. X., Duan, L. M., Yang, H. R., Huang, W. X., Liu, Z., Zhou, X. H., Zhang, Y. H., Xu, H. S., Wang, N., Zhou, H. B., Wen, X. J., Huang, S., Hua, W., Zhu, L., Wang, X., Mao, Y. C., He, X. T., Wang, S. Y., Xu, W. Z., Li, H. W., Ren, Z. Z., Zhou, S. G.
Publikováno v:
Phys. Rev. Lett. 126, 152502 (2021)
A new $\alpha$-emitting isotope $^{214}$U, produced by fusion-evaporation reaction $^{182}$W($^{36}$Ar, 4n)$^{214}$U, was identified by employing the gas-filled recoil separator SHANS and recoil-$\alpha$ correlation technique. More precise $\alpha$-d
Externí odkaz:
http://arxiv.org/abs/2101.06023
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:
Zhang, L. Y., He, J. J., Parikh, A., Xu, S. W., Yamaguchi, H., Kahl, D., Kubono, S., Mohr, P., Hu, J., Ma, P., Chen, S. Z., Wakabayashi, Y., Wang, H. W., Tian, W. D., Chen, R. F., Guo, B., Hashimoto, T., Togano, Y., Hayakawa, S., Teranishi, T., Iwasa, N., Yamada, T., Komatsubara, T., Zhang, Y. H., Zhou, X. H.
The $^{18}$Ne($\alpha$,$p$)$^{21}$Na reaction is thought to be one of the key breakout reactions from the hot CNO cycles to the rp-process in type I x-ray bursts. In this work, the resonant properties of the compound nucleus $^{22}$Mg have been inves
Externí odkaz:
http://arxiv.org/abs/1403.4668
Autor:
Han, J L, Ma, J B, Cao, X G, Wang, Q, Wang, J S, Yang, Y Y, Ma, P, Huang, M R, Jin, S L, Rong, X J, Bai, Z, Fu, F, Hu, Q, Chen, R F, Xu, S W, Chen, J B, Jin, L, Li, Y, Zhao, M H, Xu, H S
The performance of a double sided silicon strip detector (DSSSD), used for position and energy detection of heavy ions, is reported. The analysis shows that the incomplete charge collection (ICC) and charge sharing (CS) effects of the DSSSD give rise
Externí odkaz:
http://arxiv.org/abs/1307.4148
Autor:
He, J. J., Zhang, L. Y., Parikh, A., Xu, S. W., Yamaguchi, H., Kahl, D., Kubono, S., Hu, J., Ma, P., Chen, S. Z., Wakabayashi, Y., Sun, B. H., Wang, H. W., Tian, W. D., Chen, R. F., Guo, B., Hashimoto, T., Togano, Y., Hayakawa, S., Teranishi, T., Iwasa, N., Yamada, T., Komatsubara, T.
The $^{18}$Ne($\alpha$,$p$)$^{21}$Na reaction provides a pathway for breakout from the hot CNO cycles to the $rp$-process in type I x-ray bursts. To better determine this astrophysical reaction rate, the resonance parameters of the compound nucleus $
Externí odkaz:
http://arxiv.org/abs/1301.4283
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Akademický článek
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