Zobrazeno 1 - 10
of 174
pro vyhledávání: '"Li E. T."'
Autor:
Zhang, S., Li, G., Jiang, W., Wang, D. X., Ren, J., Li, E. T., Huang, M., Tang, J. Y., Ruan, X. C., Wang, H. W., Li, Z. H., Chen, Y. S., Liu, L. X., Li, X. X., Fan, Q. W., Fan, R. R., Hu, X. R., Wang, J. C., Li, X., Niu, 1D. D., Song, N., Gu, M.
The stellar (n, $\gamma$) cross section data for the mass numbers around A $\approx$ 160 are of key importance to nucleosynthesis in the main component of the slow neutron capture process, which occur in the thermally pulsing asymptotic giant branch
Externí odkaz:
http://arxiv.org/abs/2212.01820
Autor:
Zhang G. X., Hu S. P., Zhang G. L., Zhang H. Q., Yao Y. J., Huang Z., Wang M. L., Sun H. B., Valiente-Dobòn J. J., Testov D., Goasduff A., John P. R., Siciliano M., Galtarosa F., Francesco R., Mengoni D., Bazzacco D., Li E. T., Hao X.
Publikováno v:
EPJ Web of Conferences, Vol 178, p 03009 (2018)
Investigation of the breakup and transfer effect of weakly bound nuclei on the fusion process has been an interesting research topic in the past several years. In comparison with radioactive ion beam (RIB), the beam intensities of stable weakly bound
Externí odkaz:
https://doaj.org/article/7157dbd82ba342a099cc76341553e9d8
Autor:
Gao, B., Jiao, T. Y., Li, Y. T., Chen, H., Lin, W. P., An, Z., Ru, L. H., Zhang, Z. C., Tang, X. D., Wang, X. Y., Zhang, N. T., Fang, X., Xie, D. H., Fan, Y. H., Ma, L., Zhang, X., Bai, F., Wang, P., Fan, Y. X., Liu, G., Huang, H. X., Wu, Q., Zhu, Y. B., Chai, J. L., Li, J. Q., Sun, L. T., Wang, S., Cai, J. W., Li, Y. Z., Su, J., Zhang, H., Li, Z. H., Li, Y. J., Li, E. T., Chen, C., Shen, Y. P., Lian, G., Guo, B., Li, X. Y., Zhang, L. Y., He, J. J., Sheng, Y. D., Chen, Y. J., Wang, L. H., Zhang, L., Cao, F. Q., Nan, W., Nan, W. K., Li, G. X., Song, N., Cui, B. Q., Chen, L. H., Ma, R. G., Yan, S. Q., Liao, J. H., Wang, Y. B., Zeng, S., Nan, D., Fan, Q. W., Qi, N. C., Sun, W. L., Guo, X. Y., Zhang, P., Chen, Y. H., Zhou, Y., Zhou, J. F., He, J. R., Shang, C. S., Li, M. C., Kubono, S., Liu, W. P., deBoer, R. J., Wiescher, M., Pignatari, M.
Publikováno v:
Physical Review Letters 129, 132701 (2022)
The $^{13}$C($\alpha$,$n$)$^{16}$O reaction is the main neutron source for the slow-neutron-capture (s-) process in Asymptotic Giant Branch stars and for the intermediate (i-) process. Direct measurements at astrophysical energies in above-ground lab
Externí odkaz:
http://arxiv.org/abs/2210.03222
Autor:
Zhang G. L., Zhang G. X., Hu S. P., Zhang H. Q., Gomes P. R. S., Lubian J., Guo C. L., Wu X. G., Yang J. C., Zheng Y., Li C. B., He C. Y., Zhong J., Li G. S., Yao Y. J., Guo M. F., Sun H. B., Valiente-Dobòn J. J., Goasduff A., Siciliano M., Galtarosa F., Francesco R., Testov D., Mengoni D., Bazzacco D., John P. R., Qu W. W., Wang F., Zheng L., Yu L., Chen Q. M., Luo P. W., Li H. W., Wu Y. H., Zhou W. K., Zhu B. J., Li E. T., Hao X.
Publikováno v:
EPJ Web of Conferences, Vol 163, p 00066 (2017)
Investigation of the breakup and transfer effect of weakly bound nuclei on the fusion process has been an interesting research topic in the past several years. However, owing to the low intensities of the presently available radioactive ion beam (RIB
Externí odkaz:
https://doaj.org/article/36b29cd7477b4a43b4c357f77e4711b4
Autor:
Gan L., Li Z. H., Sun H. B., Su J., Li Y. J., Yan S. Q., Wang Y. B., Zeng S., Bai X. X., Du X. C., Wu Z. D., Jin S. J., Zhang W. J., Liu W. P., Li E. T.
Publikováno v:
EPJ Web of Conferences, Vol 109, p 04002 (2016)
The angular distributions of 12C + 90,92,94,96Zr elastic scattering were measured with the Q3D magnetic spectrometer at the HI-13 tandem accelerator, Beijing. The real part of optical potential were extracted by analysing these angular distributions.
Externí odkaz:
https://doaj.org/article/861d0186e1f34c6aa02c1931397c3d2b
Aluminium-26 is a short-lived radionuclide with a half-life of 0.72Myr, which is observed today in the Galaxy via gamma-ray spectroscopy and is inferred to have been present in the early Solar System via analysis of meteorites. Massive stars are cons
Externí odkaz:
http://arxiv.org/abs/1909.04433
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Autor:
Shen, Y. P., Guo, B., Li, Z. H., Li, Y. J., Pang, D. Y., Adhikari, S., An, Z. D., Su, J., Yan, S. Q., Du, X. C., Fan, Q. W., Gan, L., Han, Z. Y., Li, D. H., Li, E. T., Lian, G., Liu, J. C., Ma, T. L., Pei, C. J., Su, Y., Wang, Y. B., Zhou, Y., Liu, W. P.
Publikováno v:
Phys. Rev. C 99, 025805 (2019)
The ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction plays a key role in the evolution of stars with masses of $M >$ 0.55 $M_\odot$. The cross-section of the ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction within the Gamow wi
Externí odkaz:
http://arxiv.org/abs/1811.06220
Autor:
Wu, Z. D., Guo, B., Li, Z. H., Li, Y. J., Su, J., Pang, D. Y., Yan, S. Q., Li, E. T., Bai, X. X., Du, X. C., Fan, Q. W., Gan, L., He, J. J., Jin, S. J., Jing, L., Li, L., Li, Z. C., Lian, G., Liu, J. C., Shen, Y. P., Wang, Y. B., Yu, X. Q., Zeng, S., Zhang, D. H., Zhang, L. Y., Zhang, W. J., Liu, W. P.
All the 16F levels are unbound by proton emission. To date the four low-lying 16F levels below 1 MeV have been experimentally identified with well established spin-parity values and excitation energies with an accuracy of 4 - 6 keV. However, there ar
Externí odkaz:
http://arxiv.org/abs/1403.6912
Autor:
Guo, B., Li, Z. H., Li, Y. J., Su, J., Pang, D. Y., Yan, S. Q., Wu, Z. D., Li, E. T., Bai, X. X., Du, X. C., Fan, Q. W., Gan, L., He, J. J., Jin, S. J., Jing, L., Li, L., Li, Z. C., Lian, G., Liu, J. C., Shen, Y. P., Wang, Y. B., Yu, X. Q., Zeng, S., Zhang, L. Y., Zhang, W. J., Liu, W. P.
Publikováno v:
Phys. Rev. C 89, 012801(R) (2014)
Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggested to be asymptotic giant branch (AGB) stars. In these stars the 15N(n
Externí odkaz:
http://arxiv.org/abs/1401.0067