Zobrazeno 1 - 10
of 175
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:
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
Akademický článek
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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
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
Autor:
Fallis, J., Parikh, A., Bertone, P. F., Bishop, S., Buchmann, L., Chen, A. A., Christian, G., Clark, J. A., D'Auria, J. M., Davids, B., Deibel, C. M., Fulton, B. R., Greife, U., Guo, B., Hager, U., Herlitzius, C., Hutcheon, D. A., José, J., Laird, A. M., Li, E. T., Li, Z. H., Lian, G., Liu, W. P., Martin, L., Nelson, K., Ottewell, D., Parker, P. D., Reeve, S., Rojas, A., Ruiz, C., Setoodehnia, K., Sjue, S., Vockenhuber, C., Wang, Y. B., Wrede, C.
The 33S(p,\gamma)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abundance of 33S in oxygen-neon nova ejecta. This overproduction fac
Externí odkaz:
http://arxiv.org/abs/1309.3543
Autor:
Guo, B., Li, Z. H., Lugaro, M., Buntain, J., Pang, D. Y., Li, Y. J., Su, J., Yan, S. Q., Bai, X. X., Chen, Y. S., Fan, Q. W., Jin, S. J., Karakas, A. I., Li, E. T., Li, Z. C., Lian, G., Liu, J. C., Liu, X., Shi, J. R., Shu, N. C., Wang, B. X., Wang, Y. B., Zeng, S., Liu, W. P.
Publikováno v:
Astrophys. J. 756, 193, 2012
We present a new measurement of the $\alpha$-spectroscopic factor ($S_\alpha$) and the asymptotic normalization coefficient (ANC) for the 6.356 MeV 1/2$^+$ subthreshold state of $^{17}$O through the $^{13}$C($^{11}$B, $^{7}$Li)$^{17}$O transfer react
Externí odkaz:
http://arxiv.org/abs/1208.0714
Autor:
Hu, J., He, J. J., Xu, S. W., Chen, Z. Q., Zhang, X. Y., Wang, J. S., Yu, X. Q., Li, L., Zhang, L. Y., Yang, Y. Y., Ma, P., Zhang, X. H., Hu, Z. G., Guo, Z. Y., Xu, X., Yuan, X. H., Lu, W., Yu, Y. H., Zang, Y. D., Tang, S. W., Ye, R. P., Chen, J. D., Jin, S. L., Du, C. M., Wang, S. T., Ma, J. B., Liu, L. X., Bai, Z., Lei, X. G., Sun, Z. Y., Zhang, Y. H., Zhou, X. H., Xu, H. S., Su, J., Li, E. T., Wang, H. W., Tian, W. D., Li, X. Q.
Properties of proton resonances in $^{18}$Ne have been investigated efficiently by utilizing a technique of proton resonant elastic scattering with a $^{17}$F radioactive ion (RI) beam and a thick proton target. A 4.22~MeV/nucleon $^{17}$F RI beam wa
Externí odkaz:
http://arxiv.org/abs/1009.1206