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NSR database version of April 11, 2024.

Search: Author = X.Tang

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2024CH17      Eur.Phys.J. A 60, (2024)

Y.Chen, Y.Qiu, Q.Li, Sh.Tang, Y.Yang, Zh.Ren, W.Jiang, R.Fan, H.Yi, R.Liu, J.Tang, H.Jing, Ch.Lan, Y.Li, Zh.Tan, Q.An, J.Bai, J.Bao, Y.Bao, P.Cao, H.Chen, Q.Chen, Zh.Chen, Z.Cui, Ch.Feng, K.Gao, X.Gao, M.Gu, Ch.Han, Z.Han, G.He, Y.He, Y.Hong, Y.Hu, H.Huang, X.Huang, H.Jiang, Zh.Jiang, L.Kang, B.Li, Ch.Li, J.Li, X.Li, J.Liu, Sh.Liu, X.Liu, Z.Long, G.Luan, Ch.Ning, M.Niu, B.Qi, J.Ren, X.Ruan, Zh.Song, K.Sun, Zh.Sun, X.Tang, B.Tian, L.Wang, P.Wang, Zh.Wang, Zh.Wen, X.Wu, X.Wu, L.Xie, X.Yang, L.Yu, T.Yu, Y.Yu, G.Zhang, L.Zhang, Q.Zhang, X.Zhang, Y.Zhang, Zh.Zhang, L.Zhou, Zh.Zhou, K.Zhu

Measurement of the neutron flux of CSNS Back-n ES#1 under small collimators from 0.5 eV to 300 MeV

NUCLEAR REACTIONS 235U(n, F), 6Li(n, X), E=0.0000005-300 MeV; measured reaction products, En, In, TOF; deduced σ, neutron flux and uncertainties. China Spallation Neutron Source (CSNS).

doi: 10.1140/epja/s10050-024-01272-z
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2023GU03      Phys.Rev. C 107, 014318 (2023)

L.Guo, W.L.Lv, Y.F.Niu, D.L.Fang, B.S.Gao, K.A.Li, X.D.Tang

Spin-isospin excitations in the direction of β+ decay for 80Zn and 126Ru at finite temperature

RADIOACTIVITY 80Zn, 126Ru(β+); calculated Gamow-Teller (GT+) strength distribution with respect to the ground state of daughter nuclei, spin-dipole (SD) transition strength distributions, sum-rule values of GT and SD transitions. Self consistent finite-temperature proton-neutron relativistic quasiparticle RPA (FT-PNRQRPA) and finite-temperature proton-neutron relativistic RPA (FT-PNRRPA) model.

doi: 10.1103/PhysRevC.107.014318
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2023LI01      Appl.Radiat.Isot. 191, 110557 (2023)

B.Liu, G.Tian, R.Han, F.Shi, Y.Huang, Z.Chen, X.Zhang, H.Sun, X.Tang, Z.Zhang, P.Luo

Excitation functions for fast-neutron induced reactions on zinc

NUCLEAR REACTIONS 64Zn(n, p), 66,70Zn(n, 2n), Zn(n, X)67Cu, E=14 MeV; measured reaction products, Eγ, Iγ; deduced σ. Comparison with CENDL-3.2, ENDF/B-VIII.0, JENDL-5, BROND-3.1, JEFF-3.3 and EXFOR libraries, TALYS-1.95 calculations. The K-400 neutron generator at China Academy of Engineering Physics.

doi: 10.1016/j.apradiso.2022.110557
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2023RU05      Phys.Rev. C 107, 065803 (2023)

L.H.Ru, D.H.Xie, T.Y.Jiao, Z.An, F.Bai, J.W.Cai, X.Fang, Y.H.Fan, Y.X.Fan, B.S.Gao, Y.Z.Li, W.P.Lin, G.Liu, L.Ma, H.J.Ong, X.D.Tang, P.Wang, X.Zhang

Strength of the resonance of the 13C(α, n)16O reaction at Eα = 1055.63 keV

NUCLEAR REACTIONS 13C(α, n), E=960-1150 keV; measured In; deduced σ(E), resonance strengths at 1055.63 keV (used for neutron detector arrays calibration), resonance parameters for Eα= 1334.64 and 1338.27 keV. Comparison to previous experimental results and ENDF/B-VIII.0 evaluation. Low background neutron detector array consisting of 24 cylindrical 3He-filled proportional counters at 3 MV Tandetron accelerator (Sichuan University).

doi: 10.1103/PhysRevC.107.065803
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Data from this article have been entered in the XUNDL database. For more information, click here.


2023SH06      Astrophys.J. 945, 41 (2023)

Y.Shen, B.Guo, R.J.deBoer, E.Li, Z.Li, Y.Li, X.Tang, D.Pang, S.Adhikari, C.Basu, J.Su, S.Yan, Q.Fan, J.Liu, C.Chen, Z.Han, X.Li, G.Lian, T.Ma, W.Nan, W.Nan, Y.Wang, S.Zeng, H.Zhang, W.Liu

New Determination of the 12C(α, γ)16O Reaction Rate and Its Impact on the Black-hole Mass Gap

NUCLEAR REACTIONS 12C(11B, 7Li), (11B, 11B), E=50 MeV; measured reaction products. 16O; deduced σ(θ), the asymptotic normalization coefficient (ANC) for the 16O ground state (GS), astrophysical S-factor and the stellar rate. The HI-13 tandem accelerator of China Institute of Atomic Energy (CIAE) in Beijing, China.

doi: 10.3847/1538-4357/acb7de
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2023TA01      Appl.Radiat.Isot. 193, 110636 (2023)

X.Tang, G.Tian, Y.Huang, J.Ran, Z.Wen, J.Xu, S.Song, B.Liu, R.Han, F.Shi, X.Zhang, H.Sun, Y.Gong, Y.Li, Z.Zhang, Z.Chen, P.Luo

Activation cross sections for reactions induced by 14 MeV neutrons on natural titanium

NUCLEAR REACTIONS Ti(n, X)46Sc/47Sc/48Sc/47Ca, E ∼ 14 MeV; measured reaction products, Eγ, Iγ; deduced σ. Comparison with TALYS calculations, EXFOR library. The K-400 neutron generator at the China Academy of Engineering Physics (CAEP), China.

doi: 10.1016/j.apradiso.2022.110636
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2023WA05      Phys.Rev.Lett. 130, 092701 (2023)

L.H.Wang, J.Su, Y.P.Shen, J.J.He, M.Lugaro, B.Szanyi, A.I.Karakas, L.Y.Zhang, X.Y.Li, B.Guo, G.Lian, Z.H.Li, Y.B.Wang, L.H.Chen, B.Q.Cui, X.D.Tang, B.S.Gao, Q.Wu, L.T.Sun, S.Wang, Y.D.Sheng, Y.J.Chen, H.Zhang, Z.M.Li, L.Y.Song, X.Z.Jiang, W.Nan, W.K.Nan, L.Zhang, F.Q.Cao, T.Y.Jiao, L.H.Ru, J.P.Cheng, M.Wiescher, W.P.Liu

Measurement of the 18O(α, γ)22Ne Reaction Rate at JUNA and Its Impact on Probing the Origin of SiC Grains

NUCLEAR REACTIONS 18O(α, γ), E=470-787 keV; measured reaction products, Eγ, Iγ; deduced thick target yields, resonance energies and resonance strengths, total reaction rates. Comparison with available data. The Jinping Underground Nuclear Astrophysics experimental facility (JUNA).

doi: 10.1103/PhysRevLett.130.092701
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2023WA36      Phys.Rev. C 108, 065805 (2023)

B.Wang, Y.Xu, X.Tang

Effective energy window of the E1 photon strength function for astrophysical neutron-capture reaction rates

doi: 10.1103/PhysRevC.108.065805
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2023ZH26      Phys.Rev. C 107, 065801 (2023)

H.Zhang, J.Su, Z.H.Li, Y.J.Li, E.T.Li, C.Chen, J.J.He, Y.P.Shen, G.Lian, B.Guo, X.Y.Li, L.Y.Zhang, Y.D.Sheng, Y.J.Chen, L.H.Wang, L.Zhang, F.Q.Cao, W.Nan, W.K.Nan, G.X.Li, N.Song, B.Q.Cui, L.H.Chen, R.G.Ma, Z.C.Zhang, T.Y.Jiao, B.S.Gao, X.D.Tang, Q.Wu, J.Q.Li, L.T.Sun, S.Wang, S.Q.Yan, J.H.Liao, Y.B.Wang, S.Zeng, D.Nan, Q.W.Fan, W.P.Liu

Updated reaction rate of 25Mg(p, γ)26Al and its astrophysical implication

NUCLEAR REACTIONS 25Mg(p, γ), E=117-350 keV; measured Eγ, Iγ, sum of γ energies; deduced γ-ray branching ratios, resonances, resonance strengths, astrophysical reaction rate (T=0.01-2.0 GK), contribution of individual resonances to the reaction rate, ground-state and isomeric state contribution. Comaprison to other experimental data and NACRE compilation. Evaluated the impact of the obtained data on the 26Al yield in stellar environment (code MESA). BGO detector array in nearby 4π geometry composed of 8 identical segments at high-current 400 kV JUNA accelerator (China JinPing underground Laboratory).

doi: 10.1103/PhysRevC.107.065801
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Data from this article have been entered in the XUNDL database. For more information, click here.


2022LI28      Few-Body Systems 63, 43 (2022)

W.P.Liu, Z.H.Li, J.J.He, X.D.Tang, G.Lian, J.Su, Y.P.Shen, Z.An, F.Q.Chao, J.J.Chang, L.H.Chen, H.Chen, X.J.Chen, Y.H.Chen, Z.J.Chen, B.Q.Cui, X.C.Du, X.Fang, C.B.Fu, L.Gan, B.Guo, Z.Y.Han, X.Y.Guo, G.Z.He, J.R.He, A.Heger, S.Q.Hou, H.X.Huang, N.Huang, B.L.Jia, L.Y.Jiang, S.Kubono, J.M.Li, M.C.Li, K.A.Li, E.T.Li, T.Li, Y.J.Li, M.Lugaro, X.B.Luo, H.Y.Ma, S.B.Ma, D.M.Mei, W.Nan, W.K.Nan, N.C.Qi, Y.Z.Qian, J.C.Qin, J.Ren, C.S.Shang, L.T.Sun, W.L.Sun, W.P.Tan, I.Tanihata, S.Wang, P.Wang, Y.B.Wang, Q.Wu, S.W.Xu, S.Q.Yan, L.T.Yang, Y.Yang, X.Q.Yu, Q.Yue, S.Zeng, L.Zhang, H.Zhang, H.Y.Zhang, L.Y.Zhang, N.T.Zhang, P.Zhang, Q.W.Zhang, T.Zhang, X.P.Zhang, X.Z.Zhang, W.Zhao, J.F.Zhou, Y.Zho

Progress of Underground Nuclear Astrophysics Experiment JUNA in China

NUCLEAR REACTIONS 12C(α, γ), 13C(α, n), 25Mg(p, γ), 19F(p, α), E(cm)<600 keV; measured reaction products; deduced yields near the Gamow window. Comparison with available data.

doi: 10.1007/s00601-022-01735-3
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2022WA36      Chin.Phys.C 46, 104001 (2022)

X.Y.Wang, N.T.Zhang, Z.C.Zhang, C.G.Lu, T.L.Pu, J.L.Zhang, L.M.Duan, B.S.Gao, K.A.Li, Y.T.Li, Y.Qian, L.H.Ru, B.Wang, X.D.Xu, H.Y.Zhao, W.P.Lin, Z.W.Cai, B.F.Ji, Q.T.Li, J.Y.Xu, X.D.Tang

Studies of the 2α and 3α channels of the 12C+12C reaction in the range of Ec.m.=8.9 MeV to 21 MeV using the active target Time Projection Chamber

NUCLEAR REACTIONS 12C(12C, 2α), (12C, 8Be), (12C, 3α), (12C, X), E(cm)=8.9-21 MeV; measured reaction products, Eα, Iα; deduced fusion σ. Comparison with available data. 1024-channel TPC named pMATE (prototype Multi-purpose time projection chamber for nuclear Astrophysical and Exotic beam experiments), the Heavy Ion Research Facility in Lanzhou (HIRFL), China.

doi: 10.1088/1674-1137/ac7a1d
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2022YA16      Astrophys.J. 933, 112 (2022)

Y.Yamazaki, Z.He, T.Kajino, G.J.Mathews, M.A.Famiano, X.Tang, J.Shi

Possibility to Identify the Contributions from Collapsars, Supernovae, and Neutron Star Mergers from the Evolution of the r-process Mass Abundance Distribution

doi: 10.3847/1538-4357/ac721c
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2022ZH67      Phys.Rev. C 106, 055803 (2022)

L.Y.Zhang, J.Su, J.J.He, R.J.deBoer, D.Kahl, M.Wiescher, D.Odell, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, B.Guo, X.D.Tang, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, J.P.Cheng, W.P.Liu

Direct measurement of the astrophysical 19F(p, αγ)16O reaction in a deep-underground laboratory

NUCLEAR REACTIONS 19F(p, αγ), E(cm)=72.4-344 keV; measured Eγ, Iγ; deduced astrophysical S-factor, thermonuclear astrophysical reaction rates (range 0.05–1 GK), contributions from different channels. R-matrix analysis with AZURE2 together with a MCMC Bayesian uncertainty estimation. Comparison to other experimental data. 4π BGO γ-array with proton beam from JUNA accelerator at China JinPing underground Laboratory (CJPL).

doi: 10.1103/PhysRevC.106.055803
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Data from this article have been entered in the XUNDL database. For more information, click here.


2021CH53      Nucl.Instrum.Methods Phys.Res. B509, 27 (2021)

Z.Chen, W.Chen, Y.Luo, X.Tang, F.Zhang, Y.Hu, X.Guo, H.Yang, L.Ding

New method for predicting heavy ion-induced SEE cross-section based on proton experimental data

doi: 10.1016/j.nimb.2021.08.014
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2021GA15      Phys.Rev.Lett. 126, 152701 (2021)

B.Gao, S.Giraud, K.A.Li, A.Sieverding, R.G.T.Zegers, X.Tang, J.Ash, Y.Ayyad-Limonge, D.Bazin, S.Biswas, B.A.Brown, J.Chen, M.DeNudt, P.Farris, J.M.Gabler, A.Gade, T.Ginter, M.Grinder, A.Heger, C.Hultquist, A.M.Hill, H.Iwasaki, E.Kwan, J.Li, B.Longfellow, C.Maher, F.Ndayisabye, S.Noji, J.Pereira, C.Qi, J.Rebenstock, A.Revel, D.Rhodes, A.Sanchez, J.Schmitt, C.Sumithrarachchi, B.H.Sun, D.Weisshaar

New 59Fe Stellar Decay Rate with Implications for the 60Fe Radioactivity in Massive Stars

NUCLEAR REACTIONS 59Co(t, 3He)59Fe, E=115 MeV/nucleon; measured reaction products, Eγ, Iγ; deduced γ-ray energies, J, π, σ(θ), B(GT), β-decay rates. Comparison with stellar evolution calculations.

doi: 10.1103/PhysRevLett.126.152701
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Data from this article have been entered in the XUNDL database. For more information, click here.


2021HA53      Astrophys.J. 915, L13 (2021)

S.Hayakawa, M.La Cognata, L.Lamia, H.Yamaguchi, D.Kahl, K.Abe, H.Shimizu, L.Yang, O.Beliuskina, S.M.Cha, K.Y.Chae, S.Cherubini, P.Figuera, Z.Ge, M.Gulino, J.Hu, A.Inoue, N.Iwasa, A.Kim, D.Kim, G.Kiss, S.Kubono, M.La Commara, M.Lattuada, E.J.Lee, J.Y.Moon, S.Palmerini, C.Parascandolo, S.Y.Park, V.H.Phong, D.Pierroutsakou, R.G.Pizzone, G.G.Rapisarda, S.Romano, C.Spitaleri, X.D.Tang, O.Trippella, A.Tumino, N.T.Zhang

Constraining the Primordial Lithium Abundance: New Cross Section Measurement of the 7Be + n Reactions Updates the Total 7Be Destruction Rate

NUCLEAR REACTIONS 2H(7Be, p7Li)1H, E=3.16 MeV/nucleon; measured reaction products. 8Be; deduced σ, low-lying resonance parameters, astrophysical reaction rates for 7Be(n, p) and 7Be(n, α) reactions. Comparison with available data. the Trojan Horse Method (THM), Center-for-Nuclear-Study RI Beam separator (CRIB), the University of Tokyo, located atthe RI Beam Factory, RIKEN.

doi: 10.3847/2041-8213/ac061f
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23652.


2021HU08      Chin.Phys.C 45, 024003 (2021)

M.Huang, A.Bonasera, S.Zhang, H.Zheng, D.X.Wang, J.C.Wang, N.Song, X.Tang, L.Lu, G.Zhang, Z.Kohley, M.R.D.Rodrigues, Y.G.Ma, S.J.Yennello

Four α correlations in nuclear fragmentation: a game of resonances

NUCLEAR REACTIONS 70Zn(70Zn, X), 64Zn(64Zn, X), 64Ni(64Ni, X), E=35 MeV/nucleon; measured reaction products, Eα, Iα. 4He; deduced yields, correlation functions, strong resonances among α-particles.

doi: 10.1088/1674-1137/abce52
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2021RE01      Nucl.Instrum.Methods Phys.Res. A985, 164703 (2021)

J.Ren, X.Ruan, W.Jiang, J.Bao, G.Luan, Q.Zhang, H.Huang, Y.Nie, Z.Ge, Q.An, H.Bai, Y.Bao, P.Cao, H.Chen, Q.Chen, Y.Chen, Y.Chen, Z.Chen, Z.Cui, R.Fan, C.Feng, K.Gao, M.Gu, C.Han, Z.Han, G.He, Y.He, Y.Hong, W.Huang, X.Huang, X.Ji, X.Ji, H.Jiang, Z.Jiang, H.Jing, L.Kang, M.Kang, B.Li, C.Li, J.Li, L.Li, Q.Li, X.Li, Y.Li, R.Liu, S.Liu, X.Liu, Q.Mu, C.Ning, B.Qi, Z.Ren, Y.Song, Z.Song, H.Sun, K.Sun, X.Sun, Z.Sun, Z.Tan, H.Tang, J.Tang, X.Tang, B.Tian, L.Wang, P.Wang, Q.Wang, T.Wang, Z.Wang, J.Wen, Z.Wen, Q.Wu, X.Wu, X.Wu, L.Xie, Y.Yang, H.Yi, L.Yu, T.Yu, Y.Yu, G.Zhang, L.Zhang, X.Zhang, Y.Zhang, Z.Zhang, Y.Zhao, L.Zhou, Z.Zhou, D.Zhu, K.Zhu, P.Zhu

Background study for (n, γ) cross section measurements with C6D6 detectors at CSNS Back-n

NUCLEAR REACTIONS 197Au, Pb, C, 181Ta, 59Co(n, γ), E<400 MeV; measured reaction products, Eγ, Iγ; deduced σ.

doi: 10.1016/j.nima.2020.164703
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2021ZH49      Nucl.Instrum.Methods Phys.Res. A1016, 165740 (2021)

Z.C.Zhang, X.Y.Wang, T.L.Pu, C.G.Lu, N.T.Zhang, J.L.Zhang, L.M.Duan, B.S.Gao, J.Gao, R.J.Hu, E.Q.Liu, K.A.Li, Q.T.Li, Y.T.Li, B.F.Lv, H.Y.Ma, J.B.Ma, H.J.Ong, Y.Qian, L.H.Ru, L.T.Sun, X.D.Tang, J.Y.Xu, X.D.Xu, Y.Yang, Y.H.Zhai, H.Y.Zhao, H.W.Zhao

Studying the heavy-ion fusion reactions at stellar energies using Time Projection Chamber

NUCLEAR REACTIONS 12C(12C, α)20Ne, E(cm)=3 MeV; measured reaction products, Eα, Iα; deduced preliminary σ, yields.

doi: 10.1016/j.nima.2021.165740
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2021ZH53      Phys.Rev.Lett. 127, 152702 (2021)

L.Y.Zhang, J.Su, J.J.He, M.Wiescher, R.J.deBoer, D.Kahl, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, X.D.Tang, H.W.Zhao, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, B.Guo, S.W.Xu, J.Y.Li, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, X.H.Zhou, Y.H.Zhang, F.S.Zhang, Z.G.Hu, H.S.Xu, J.P.Chen, W.P.Liu

Direct Measurement of the Astrophysical 19F(p, αγ)16O Reaction in the Deepest Operational Underground Laboratory

NUCLEAR REACTIONS 19F(p, α), E(cm)=72.4-188.8 keV; measured reaction products, Eγ, Iγ; deduced yields, S-factors, reaction rates. The China Jinping Underground Laboratory (CJPL), JUNA accelerator.

doi: 10.1103/physrevlett.127.152702
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2020BE07      Eur.Phys.J. A 56, 87 (2020)

C.Beck, A.M.Mukhamedzhanov, X.Tang

Status on 12C + 12C fusion at deep subbarrier energies: impact of resonances on astrophysical S* factors

doi: 10.1140/epja/s10050-020-00075-2
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2020GR14      Phys.Rev.X 10, 031037 (2020)

A.Green, H.Li, J.Hui S.Toh, X.Tang, K.C.McCormick, M.Li, E.Tiesinga, S.Kotochigova, S.Gupta

Feshbach Resonances in p-Wave Three-Body Recombination within Fermi-Fermi Mixtures of Open-Shell 6Li and Closed-Shell 173Yb Atoms

ATOMIC PHYSICS 6Li, 173Yb; measured frequencies; deduced magnetic Feshbach resonances as functions of magnetic field, dependence of magnetic Feshbach resonances on the nuclear Zeeman state.

doi: 10.1103/PhysRevX.10.031037
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2020JI06      Nucl.Instrum.Methods Phys.Res. A973, 164126 (2020)

W.Jiang, H.Bai, H.Jiang, H.Yi, R.Fan, G.Zhang, J.Tang, Z.Sun, C.Ning, K.Sun, K.Gao, Z.Cui, Q.An, J.Bao, Y.Bao, P.Cao, H.Chen, Q.Chen, Y.Chen, Y.Chen, Z.Chen, C.Feng, M.Gu, F.Guo, C.Han, Z.Han, G.He, Y.He, Y.Hong, H.Huang, W.Huang, X.Huang, X.Ji, X.Ji, Z.Jiang, H.Jing, L.Kang, M.Kang, B.Li, C.Li, J.Li, L.Li, Q.Li, X.Li, Y.Li, R.Liu, S.Liu, X.Liu, G.Luan, Q.Mu, B.Qi, J.Ren, Z.Ren, X.Ruan, Y.Song, Z.Song, H.Sun, X.Sun, Z.Tan, H.Tang, X.Tang, B.Tian, L.Wang, P.Wang, Q.Wang, T.Wang, Y.Wang, Z.Wang, J.Wen, Z.Wen, Q.Wu, X.Wu, X.Wu, L.Xie, Y.Yang, L.Yu, T.Yu, Y.Yu, L.Zhang, Q.Zhang, X.Zhang, Y.Zhang, Z.Zhang, Y.Zhao, L.Zhou, L.Zhou, Z.Zhou, D.Zhu, K.Zhu, P.Zhu

Application of a silicon detector array in (n, lcp) reaction cross-section measurements at the CSNS Back-n white neutron source

NUCLEAR REACTIONS 6Li(n, t), 10B(n, α), E<1 MeV; measured reaction products, En, In; deduced σ. Comparison with experimental data, ENDF/B-VIII.0, JEFF-3.3, ROSFOND evaluated libraries.

doi: 10.1016/j.nima.2020.164126
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2020LI46      Chin.Phys.C 44, 115001 (2020)

Y.J.Li, X.Fang, B.Bucher, K.A.Li, L.H.Ru, X.D.Tang

Modified astrophysical S-factor of 12C+12C fusion reaction at sub-barrier energies

NUCLEAR REACTIONS 12C(12C, X), E=2-8.75 MeV/nucleon; analyzed available data; deduced S-factors using statistical model calculations.

doi: 10.1088/1674-1137/abae56
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2020SH09      Phys.Rev.Lett. 124, 162701 (2020)

Y.P.Shen, B.Guo, R.J.deBoer, Z.H.Li, Y.J.Li, X.D.Tang, D.Y.Pang, S.Adhikari, C.Basu, J.Su, S.Q.Yan, Q.W.Fan, J.C.Liu, C.Chen, Z.Y.Han, X.Y.Li, G.Lian, T.L.Ma, W.Nan, W.K.Nan, Y.B.Wang, S.Zeng, H.Zhang, W.P.Liu

Constraining the External Capture to the 16O ground State and the E2 S Factor of the 12C(α, γ)16O reaction

NUCLEAR REACTIONS 12C(11B, 7Li)16O, E=50 MeV; measured reaction products; deduced σ(θ), the ground state asymptotic normalization coefficients, S-factors. Comparison with available data.

doi: 10.1103/PhysRevLett.124.162701
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0230. Data from this article have been entered in the XUNDL database. For more information, click here.


2020ZH02      Phys.Lett. B 801, 135170 (2020), Corrigendum Phys.Lett. B 803, 135278 (2020)

N.T.Zhang, X.Y.Wang, D.Tudor, B.Bucher, I.Burducea, H.Chen, Z.J.Chen, D.Chesneanu, A.I.Chilug, L.R.Gasques, D.G.Ghita, C.Gomoiu, K.Hagino, S.Kubono, Y.J.Li, C.J.Lin, W.P.Lin, R.Margineanu, A.Pantelica, I.C.Stefanescu, M.Straticiuc, X.D.Tang, L.Trache, A.S.Umar, W.Y.Xin, S.W.Xu, Y.Xu

Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies

NUCLEAR REACTIONS 12C(13C, p)24Na, E=4.640-10.995 MeV; measured reaction products, Eγ, Iγ; deduced σ, branching ratio, S-factor.

doi: 10.1016/j.physletb.2019.135170
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0970.


2019HO18      J.Phys.(London) G46, 083001 (2019)

C.J.Horowitz, A.Arcones, B.Cote, I.Dillmann, W.Nazarewicz, I.U.Roederer, H.Schatz, A.Aprahamian, D.Atanasov, A.Bauswein, T.C.Beers, J.Bliss, M.Brodeur, J.A.Clark, A.Frebel, F.Foucart, C.J.Hansen, O.Just, A.Kankainen, G.C.McLaughlin, J.M.Kelly, S.N.Liddick, D.M.Lee, J.Lippuner, D.Martin, J.Mendoza-Temis, B.D.Metzger, M.R.Mumpower, G.Perdikakis, J.Pereira, B.W.O'Shea, R.Reifarth, A.M.Rogers, D.M.Siegel, A.Spyrou, R.Surman, X.Tang, T.Uesaka, M.Wang

r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos

doi: 10.1088/1361-6471/ab0849
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2019JI07      Chin.Phys.C 43, 124002 (2019)

H.Jiang, W.Jiang, H.Bai, Z.Cui, G.Zhang, R.Fan, H.Yi, C.Ning, L.Zhou, J.Tang, Q.An, J.Bao, Y.Bao, P.Cao, H.Chen, Q.Chen, Y.Chen, Y.Chen, Z.Chen, C.Feng, K.Gao, M.Gu, C.Han, Z.Han, G.He, Y.He, Y.Hong, H.Huang, W.Huang, X.Huang, X.Ji, X.Ji, Z.Jiang, H.Jing, L.Kang, M.Kang, B.Li, C.Li, J.Li, L.Li, Q.Li, X.Li, Y.Li, R.Liu, S.Liu, X.Liu, G.Luan, Q.Mu, B.Qi, J.Ren, Z.Ren, X.Ruan, Z.Song, Y.Song, H.Sun, K.Sun, X.Sun, Z.Sun, Z.Tan, H.Tang, X.Tang, B.Tian, L.Wang, P.Wang, Q.Wang, T.Wang, Z.Wang, J.Wen, Z.Wen, Q.Wu, X.Wu, X.Wu, L.Xie, Y.Yang, L.Yu, T.Yu, Y.Yu, L.Zhang, Q.Zhang, X.Zhang, Y.Zhang, Z.Zhang, Y.Zhao, L.Zhou, Z.Zhou, D.Zhu, K.Zhu, P.Zhu

Measurements of differential and angle-integrated cross sections for the 10B(n, α)7Li reaction in the neutron energy range from 1.0 eV to 2.5 MeV

NUCLEAR REACTIONS 10B(n, α), E=0.000001-2.5 MeV; measured reaction products, Eα, Iα; deduced σ(θ), σ and uncertainties. Comparison with ENDF/B-VIII.0, JEFF-3.3, CENDL-3.1 and JENDL 4.0 libraries.

doi: 10.1088/1674-1137/43/12/124002
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2019JI08      Chin.Phys.C 43, 124110 (2019)

H.Jiang, X.-L.Tang, J.-J.Shen, Y.Lei

Electromagnetic properties of neutron-rich Ge isotopes

NUCLEAR STRUCTURE 72,74,76,78,80,75,77,79Ge; calculated electric quadrupole and the dipole magnetic moments of low-lying states in the framework of the nucleon pair approximation (NPA) of the shell model. Comparison with available data.

doi: 10.1088/1674-1137/43/12/124110
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2018JI01      Phys.Rev. C 97, 012801 (2018)

C.L.Jiang, D.Santiago-Gonzalez, S.Almaraz-Calderon, K.E.Rehm, B.B.Back, K.Auranen, M.L.Avila, A.D.Ayangeakaa, S.Bottoni, M.P.Carpenter, C.Dickerson, B.DiGiovine, J.P.Greene, C.R.Hoffman, R.V.F.Janssens, B.P.Kay, S.A.Kuvin, T.Lauritsen, R.C.Pardo, J.Sethi, D.Seweryniak, R.Talwar, C.Ugalde, S.Zhu, D.Bourgin, S.Courtin, F.Haas, M.Heine, G.Fruet, D.Montanari, D.G.Jenkins, L.Morris, A.Lefebvre-Schuhl, M.Alcorta, X.Fang, X.D.Tang, B.Bucher, C.M.Deibel, S.T.Marley

Reaction rate for carbon burning in massive stars

NUCLEAR REACTIONS 12C(12C, p)23Na, (12C, α)20Ne, E=5.5-10 MeV; measured Eγ, Iγ, (particle)γ-coin, σ(E) using Gammasphere array and an array of three annular double-sided silicon strip detectors at the ATLAS-ANL facility; deduced S factors and astrophysical reaction rates. Comparison with previous measurements, and with data from other reactions. Relevance to carbon burning is a critical phase for nucleosynthesis in massive stars.

doi: 10.1103/PhysRevC.97.012801
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2018XI04      Phys.Lett. B 781, 358 (2018)

Y.M.Xing, K.A.Li, Y.H.Zhang, X.H.Zhou, M.Wang, Yu.A.Litvinov, K.Blaum, S.Wanajo, S.Kubono, G.Martinez-Pinedo, A.Sieverding, R.J.Chen, P.Shuai, C.Y.Fu, X.L.Yan, W.J.Huang, X.Xu, X.D.Tang, H.S.Xu, T.Bao, X.C.Chen, B.S.Gao, J.J.He, Y.H.Lam, H.F.Li, J.H.Liu, X.W.Ma, R.S.Mao, M.Si, M.Z.Sun, X.L.Tu, Q.Wang, J.C.Yang, Y.J.Yuan, Q.Zeng, P.Zhang, X.Zhou, W.L.Zhan, S.Litvinov, G.Audi, T.Uesaka, Y.Yamaguchi, T.Yamaguchi, A.Ozawa, C.Frohlich, T.Rauscher, F.-K.Thielemann, B.H.Sun, Y.Sun, A.C.Dai, F.R.Xu

Mass measurements of neutron-deficient Y, Zr, and Nb isotopes and their impact on rp and νp nucleosynthesis processes

ATOMIC MASSES 78,79Y, 80,81Zr, 82,83,84Nb, 84Mo; measured revolution time spectrum; deduced mass excess values and proton separation energies. Comparison with available data.

doi: 10.1016/j.physletb.2018.04.009
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2017DI02      Phys.Rev. C 95, 024301 (2017)

B.Ding, Z.Liu, D.Seweryniak, P.J.Woods, H.L.Wang, J.Yang, H.L.Liu, C.N.Davids, M.P.Carpenter, T.Davinson, R.V.F.Janssens, R.D.Page, A.P.Robinson, J.Shergur, S.Sinha, S.Zhu, X.D.Tang, J.G.Wang, T.H.Huang, W.Q.Zhang, M.D.Sun, X.Y.Liu, H.Y.Lu

First identification of excited states in 117Ba using the recoil-β-delayed proton tagging technique

NUCLEAR REACTIONS 64Zn(58Ni, 3n2p), E=305 MeV; measured Eγ, Iγ, (delayed protons)γ-coin, recoil-βp decay tagging using fragment mass analyzer (FMA), and Gammasphere array at ATLAS-ANL facility. 117Ba; deduced high-spin levels, J, π, bands, alignments, Routhian energies, configurations. Comparison with cranked shell-model calculations. Level-spacing systematics for negative- and positive-parity bands in 117,119,121,123,125,127,129Ba.

doi: 10.1103/PhysRevC.95.024301
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2017FA10      Phys.Rev. C 96, 045804 (2017)

X.Fang, W.P.Tan, M.Beard, R.J.deBoer, G.Gilardy, H.Jung, Q.Liu, S.Lyons, D.Robertson, K.Setoodehnia, C.Seymour, E.Stech, B.Vande Kolk, M.Wiescher, R.T.deSouza, S.Hudan, V.Singh, X.D.Tang, E.Uberseder

Experimental measurement of 12C + 16O fusion at stellar energies

NUCLEAR REACTIONS 12C(16O, p), (16O, n), (16O, α), E=8.5-11.7 MeV in steps of 100 or 200 keV; measured Eγ, Iγ, Ep, Ip, pγ-coin, charged particles, partial and total fusion σ(E) at the (ANA) accelerator laboratory (NSL) of University of Notre Dame; deduced S factors, astrophysical reaction rates, uncertainty range of the reaction rate within the temperature range of late stellar burning environments. Results analyzed using Statistical model calculations with SAPPHIRE code. 27Al, 24Mg, 27Si; deduced levels, relative γ strengths of the observed transitions with respect to the strength of the ground state transition of the first excited states.

doi: 10.1103/PhysRevC.96.045804
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2017GU05      Phys.Rev. C 95, 025807 (2017)

G.L.Guardo, C.Spitaleri, L.Lamia, M.Gulino, M.La Cognata, X.Tang, R.deBoer, X.Fang, V.Goldberg, J.Mrazek, A.Mukhamedzhanov, M.Notani, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Wiescher

Assessing the near threshold cross section of the 17O(n, α)14C reaction by means of the Trojan horse method

NUCLEAR REACTIONS 2H(17O, α14C), E=43.5 MeV; measured reaction products, particle spectra, (particle)(particle)-coin, angular distributions using two telescopes of ionization chambers (IC) and silicon position-sensitive detector (PSD) at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced normalized reaction yields, experimental momentum distribution, quasifission (QF) cross sections and best fit from R-matrix analysis. 18O; deduced levels, resonances, J, π, and Trojan horse method (THM) analysis of Γn, Γα and total widths. 17O(n, α)14C, T9=0.01-10; deduce astrophysical reaction rates by THM method.

doi: 10.1103/PhysRevC.95.025807
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23332. Data from this article have been entered in the XUNDL database. For more information, click here.


2016FR01      Phys.Rev. C 93, 014321 (2016)

A.Fritsch, S.Beceiro Novo, D.Suzuki, W.Mittig, J.J.Kolata, T.Ahn, D.Bazin, F.D.Becchetti, B.Bucher, Z.Chajecki, X.Fang, M.Febbraro, A.M.Howard, Y.Kanada-En'yo, W.G.Lynch, A.J.Mitchell, M.Ojaruega, A.M.Rogers, A.Shore, T.Suhara, X.D.Tang, R.Torres-Isea, H.Wang

One-dimensionality in atomic nuclei: A candidate for linear-chain α clustering in 14C

NUCLEAR REACTIONS 4He(10Be, α), E=39.7 MeV, [secondary 10Be beam from 13C(11B, 10B), E=46 MeV primary reaction]; measured particle spectra, differential cross sections for elastic and inelastic scattering, angular distributions using the prototype active target-time projection chamber (PAT-TPC) at Notre Dame TwinSol facility. 14C; deduced levels, α-resonances, J, π, band, α-widths, L-transfers, spectroscopic factors. R-matrix analysis. Comparison with predictions of antisymmetrized molecular dynamics (AMD) theory, and evidence for a 3α-linear chain structure in 14C.

doi: 10.1103/PhysRevC.93.014321
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2016LI53      Phys.Rev. C 94, 065807 (2016)

K.A.Li, Y.H.Lam, C.Qi, X.D.Tang, N.T.Zhang

β-decay rate of 59Fe in shell burning environment and its influence on the production of 60Fe in a massive star

RADIOACTIVITY 59Fe(β-); calculated B(GT) values for allowed β transitions from low-lying states of 59Fe to 59Co, stellar β-decay rate as a function of stellar temperatures from 0.5-2 GK; deduced impact on the relative abundance of 60Fe from 59Fe(n, γ) in the C-shell burning scenario. Shell model calculations using GXPF1a and GXPF1j interactions. Comparison with experimental logft values taken from NNDC databases.

NUCLEAR STRUCTURE 59Fe; calculated levels, J, π using shell model with GXPF1a and GXPF1j interactions. Comparison with experimental values.

doi: 10.1103/PhysRevC.94.065807
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2016SU10      Phys.Lett. B 756, 323 (2016)

J.Su, W.P.Liu, N.T.Zhang, Y.P.Shen, Y.H.Lam, N.A.Smirnova, M.MacCormick, J.S.Wang, L.Jing, Z.H.Li, Y.B.Wang, B.Guo, S.Q.Yan, Y.J.Li, S.Zeng, G.Lian, X.C.Du, L.Gan, X.X.Bai, Z.C.Gao, Y.H.Zhang, X.H.Zhou, X.D.Tang, J.J.He, Y.Y.Yang, S.L.Jin, P.Ma, J.B.Ma, M.R.Huang, Z.Bai, Y.J.Zhou, W.H.Ma, J.Hu, S.W.Xu, S.B.Ma, S.Z.Chen, L.Y.Zhang, B.Ding, Z.H.Li, G.Audi

Revalidation of the isobaric multiplet mass equation at A = 53, T = 3/2

RADIOACTIVITY 53Ni(EC), (ECp) [from Be(58Ni, X)53Ni, E=68.3 MeV/nucleon]; measured decay products, Eγ, Iγ; deduced T1/2, level scheme, J, π, isobaric analog state, mass excess, explanation of unexpected deviation from the isobaric multiplet mass equation (IMME) at A=53, T=3/2.

doi: 10.1016/j.physletb.2016.03.024
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2015BU08      Phys.Rev.Lett. 114, 251102 (2015)

B.Bucher, X.D.Tang, X.Fang, A.Heger, S.Almaraz-Calderon, A.Alongi, A.D.Ayangeakaa, M.Beard, A.Best, J.Browne, C.Cahillane, M.Couder, R.J.deBoer, A.Kontos, L.Lamm, Y.J.Li, A.Long, W.Lu, S.Lyons, M.Notani, D.Patel, N.Paul, M.Pignatari, A.Roberts, D.Robertson, K.Smith, E.Stech, R.Talwar, W.P.Tan, M.Wiescher, S.E.Woosley

First Direct Measurement of 12C(12C, n)23Mg at Stellar Energies

NUCLEAR REACTIONS 12C(12C, n), E=7.5, 9.5 MeV; measured reaction products, Eγ, Iγ, En, In; deduced yields, S-factors, astrophysical reaction rate. Comparison with available data.

doi: 10.1103/PhysRevLett.114.251102
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2168.


2015SE08      Phys.Rev. C 91, 065803 (2015)

M.L.Sergi, C.Spitaleri, M.La Cognata, L.Lamia, R.G.Pizzone, G.G.Rapisarda, X.D.Tang, B.Bucher, M.Couder, P.Davies, R.deBoer, X.Fang, L.Lamm, C.Ma, M.Notani, S.O'Brien, D.Roberson, W.Tan, M.Wiescher, B.Irgaziev, A.Mukhamedzhanov, J.Mrazek, V.Kroha

Improvement of the high-accuracy 17O(p, α)14N reaction-rate measurement via the Trojan Horse method for application to 17O nucleosynthesis

NUCLEAR REACTIONS 2H(17O, α14N)n, E=41, 43.5 MeV; measured particle spectra, (14N)α-coin at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced Q-value spectra, yields as function of 14N and α emission angles, E(14N-α) versus E(α-n) plots, neutron momentum distributions, (14N)α-coincidence yields for different neutron momentum ranges, differential σ(E) of the Trojan-Horse reaction. 18F; deduced parameters for the two resonance levels, resonance strengths for the 65-keV resonance. 17O(p, α)14N; deduced reaction rates via Trojan Horse Method (THM). 18F; compiled resonance energies, J, π, Γp, Γα, Γγ for 24 resonances from -3.12 keV to 1684.5 keV. Relevance to destruction of 17O and the formation of 18F in stellar sites.

doi: 10.1103/PhysRevC.91.065803
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2015SH16      Phys.Rev. C 91, 047304 (2015)

Y.P.Shen, W.P.Liu, J.Su, N.T.Zhang, L.Jing, Z.H.Li, Y.B.Wang, B.Guo, S.Q.Yan, Y.J.Li, S.Zeng, G.Lian, X.C.Du, L.Gan, X.X.Bai, J.S.Wang, Y.H.Zhang, X.H.Zhou, X.D.Tang, J.J.He, Y.Y.Yang, S.L.Jin, P.Ma, J.B.Ma, M.R.Huang, Z.Bai, Y.J.Zhou, W.H.Ma, J.Hu, S.W.Xu, S.B.Ma, S.Z.Chen, L.Y.Zhang, B.Ding, Z.H.Li

Measurement of the 52Fe mass via the precise proton-decay energy of 53Com

RADIOACTIVITY 53mCo(p)[from 9Be(58Ni, X), E=68.3 MeV/nucleon]; 41Ti(β+p); measured Ep, Ip, at RIBLL-HIRFL-Lanzhou facility; deduced mass excess of 52Fe and compared with AME-2012 evaluation. 51Fe, 52Co(β+); measured half-lives and compared with evaluated data in ENSDF.

ATOMIC MASSES 52Fe; deduced mass excess from Q value of proton decay of 3174.1 keV, 19/2- isomer in 53Co determined from measured proton energy. Comparison with previous experimental results.

doi: 10.1103/PhysRevC.91.047304
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2014ZH27      Nucl.Instrum.Methods Phys.Res. B335, 85 (2014)

H.Zhang, X.Tang, L.Shi

Elastic recoil cross section determination of 1H by 4He ions at 30 degree and energy range of 1.6-6.0 MeV

NUCLEAR REACTIONS 1H(α, α), E=1.6-6.0 MeV; measured reaction products; deduced σ(θ). Comparison with available data.

doi: 10.1016/j.nimb.2014.06.012
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0204.


2013GU02      Phys.Rev. C 87, 012801 (2013)

M.Gulino, C.Spitaleri, X.D.Tang, G.L.Guardo, L.Lamia, S.Cherubini, B.Bucher, V.Burjan, M.Couder, P.Davies, R.deBoer, X.Fang, V.Z.Goldberg, Z.Hons, V.Kroha, L.Lamm, M.La Cognata, C.Li, C.Ma, J.Mrazek, A.M.Mukhamedzhanov, M.Notani, S.O'Brien, R.G.Pizzone, G.G.Rapisarda, D.Roberson, M.L.Sergi, W.Tan, I.J.Thompson, M.Wiescher

Suppression of the centrifugal barrier effects in the off-energy-shell neutron + 17O interaction

NUCLEAR REACTIONS 2H(17O, α14C), E=41, 43.5 MeV; measured α and 14C particle spectra, (14C)α-coin, angular distributions, yields using position-sensitive silicon detectors (PSD) at LNS, Catania, and at NSL, Notre Dame. CD2 target; deduced momentum distributions, Q value. DWBA analysis. 17O(n, α)14C, E(cm)=0-350 keV; deduced yields, angular distributions, neutron from quasifree breakup of deuteron. 18O; deduced resonances, J, π, and excitation functions. Trojan Horse method (THM), and suppression of centrifugal barrier. Comparison with previous studies. Relevance to neutron-induced reactions in nuclear reactors, and nucleosynthesis in astrophysics.

doi: 10.1103/PhysRevC.87.012801
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2013MO01      Phys.Rev. C 87, 014611 (2013)

G.Montagnoli, A.M.Stefanini, H.Esbensen, C.L.Jiang, L.Corradi, S.Courtin, E.Fioretto, A.Goasduff, J.Grebosz, F.Haas, M.Mazzocco, C.Michelagnoli, T.Mijatovic, D.Montanari, C.Parascandolo, K.E.Rehm, F.Scarlassara, S.Szilner, X.D.Tang, C.A.Ur

Effects of transfer channels on near- and sub-barrier fusion of 32S + 48Ca

NUCLEAR REACTIONS 48Ca(32S, X), E=60.0-89.4 MeV; measured reaction products, σ(θ, E), fusion σ(E) at Legnaro facility; deduced logarithmic slope. 48Ca(32S, X), (36S, X), E(cm)=35-60 MeV; analyzed fusion σ(E) data, energy-weighted fusion cross sections, astrophysical S factor. Coupled channel analysis with M3Y+repulsion, double-folding potential.

doi: 10.1103/PhysRevC.87.014611
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2013QU01      Phys.Rev. C 88, 011603 (2013)

S.J.Quinn, A.Spyrou, A.Simon, A.Battaglia, M.Couder, P.A.DeYoung, A.C.Dombos, X.Fang, J.Gorres, A.Kontos, Q.Li, S.Lyons, B.S.Meyer, G.F.Peaslee, D.Robertson, K.Smith, M.K.Smith, E.Stech, W.P.Tan, X.D.Tang, M.Wiescher

Probing the production mechanism of the light p-process nuclei

NUCLEAR REACTIONS 74Ge(p, γ)75As, E=1.6-4.2 MeV; measured Eγ, Iγ, σ(E) using the NSCL SuN detector at Notre Dame facility; deduced astrophysical S(E) factors, reaction rates at T9=0.10-10.0, cumulative mass fraction of 74Se in a Type II Supernova model. Comparison with previous experimental data, and with theoretical predictions using NON-SMOKER and TALYS nuclear reaction codes.

doi: 10.1103/PhysRevC.88.011603
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2013SI11      Phys.Rev. C 87, 055802 (2013)

A.Simon, A.Spyrou, T.Rauscher, C.Frohlich, S.J.Quinn, A.Battaglia, A.Best, B.Bucher, M.Couder, P.A.DeYoung, X.Fang, J.Gorres, A.Kontos, Q.Li, L.-Y.Lin, A.Long, S.Lyons, A.Roberts, D.Robertson, K.Smith, M.K.Smith, E.Stech, B.Stefanek, W.P.Tan, X.D.Tang, M.Wiescher

Systematic study of (p, γ) reactions on Ni isotopes

NUCLEAR REACTIONS 58,60,61,62,64Ni(p, γ), E=2.0-6.0 MeV; measured Eγ, Iγ, σ(E) using the NSCL-SuN gamma detector utilizing γ-summing technique at Notre Dame; deduced sensitivity of the reaction σ(E) with variation of γ- and particle width. Comparison with theoretical predictions from NON-SMOKER and SMARAGD computer code calculations, and with previous experimental data. Predicted astrophysical reaction rates on all stable nickel isotopes including that for 56Ni(p, γ)57Cu.

doi: 10.1103/PhysRevC.87.055802
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2013SI35      Nucl.Instrum.Methods Phys.Res. A 703, 16 (2013)

A.Simon, S.J.Quinn, A.Spyrou, A.Battaglia, I.Beskin, A.Best, B.Bucher, M.Couder, P.A.Deyoung, X.Fang, J.Gorres, A.Kontos, Q.Li, S.N.Liddick, A.Long, S.Lyons, K.Padmanabhan, J.Peace, A.Roberts, D.Robertson, K.Smith, M.K.Smith, E.Stech, B.Stefanek, W.P.Tan, X.D.Tang, M.Wiescher

SuN: Summing NaI(Tl) gamma-ray detector for capture reaction measurements

NUCLEAR REACTIONS 27Al(p, γ), E=2.3-3.9 MeV; measured products, Eγ, Iγ; deduced resonance parameters. Data were imported from EXFOR entry C1967.

doi: 10.1016/j.nima.2012.11.045
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2013SP04      Phys.Rev. C 88, 045802 (2013)

A.Spyrou, S.J.Quinn, A.Simon, T.Rauscher, A.Battaglia, A.Best, B.Bucher, M.Couder, P.A.DeYoung, A.C.Dombos, X.Fang, J.Gorres, A.Kontos, Q.Li, L.Y.Lin, A.Long, S.Lyons, B.S.Meyer, A.Roberts, D.Robertson, K.Smith, M.K.Smith, E.Stech, B.Stefanek, W.P.Tan, X.D.Tang, M.Wiescher

Measurement of the 90, 92Zr(p, γ)91, 93Nb reactions for the nucleosynthesis of elements near A=90

NUCLEAR REACTIONS 90,92Zr(p, γ)91Nb/93Nb, E=2.0-5.0 MeV; measured Eγ, Iγ, σ(E) using NSCL SuN detector at Notre Dame accelerator facility; deduced astrophysical S factors, reaction rates, sensitivity of reaction to widths in Hauser-Feshbach model. Comparison with standard NON-SMOKER model, and two TALYS calculations. Relevance to synthesis and abundances of light p nuclei.

doi: 10.1103/PhysRevC.88.045802
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2013ST14      Eur.Phys.J. A 49, 63 (2013)

A.M.Stefanini, G.Montagnoli, F.Scarlassara, C.L.Jiang, H.Esbensen, E.Fioretto, L.Corradi, B.B.Back, C.M.Deibel, B.Di Giovine, J.P.Greene, H.D.Henderson, S.T.Marley, M.Notani, N.Patel, K.E.Rehm, D.Sewerinyak, X.D.Tang, C.Ugalde, S.Zhu

Fusion of 60Ni + 100Mo near and below the Coulomb barrier - Multi-phonon and transfer couplings down to the hindrance region

NUCLEAR REACTIONS 100Mo(60Ni, X), (64Ni, X), E=196-262 MeV; measured particle tracks; deduced fusion σ, logarithmic excitation function slope; calculated fusion σ using CCFULL CC code.

doi: 10.1140/epja/i2013-13063-2
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2013SU10      Phys.Rev. C 87, 054301 (2013)

D.Suzuki, A.Shore, W.Mittig, J.J.Kolata, D.Bazin, M.Ford, T.Ahn, F.D.Becchetti, S.Beceiro Novo, D.Ben Ali, B.Bucher, J.Browne, X.Fang, M.Febbraro, A.Fritsch, E.Galyaev, A.M.Howard, N.Keeley, W.G.Lynch, M.Ojaruega, A.L.Roberts, X.D.Tang

Resonant α scattering of 6He: Limits of clustering in 10Be

NUCLEAR REACTIONS 4He(6He, 6He), (6He, 6He'), (6He, 2n)8Be, [secondary 6He beam from 7Li(d, 3He), E=29.2 MeV primary reaction], E=15 MeV; measured reactions products, 6He spectra, elastic and inelastic σ(E, θ) using PAT-TPC system at Notre Dame TwinSol facility. 4,6He, 8Be; deduced levels, cross sections for g.s. and first 2+ states. 10Be; deduced level, resonance, J, π, α width. Discussed α clustering in high-spin states. Comparison with antisymmetric molecular dynamics calculations.

doi: 10.1103/PhysRevC.87.054301
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2012BU19      J.Phys.:Conf.Ser. 381, 012121 (2012)

B.Bucher, J.Browne, S.Almaraz-Calderon, A.Alongi, A.D.Ayangeakaa, A.Best, M.Couder, J.DeBoer, X.Fang, W.Lu, M.Notani, D.Patel, N.Paul, A.Roberts, R.Talwar, W.Tan, X.D.Tang, A.Villano

The Role of 12C(12C, n) in the Astrophysical S-Process

NUCLEAR REACTIONS 12C(12C, n), E(cm)=3.54-8.74 MeV; measured thin and thick target (4.23-8.74 MeV and 3.54-4.74 MeV, respectively) β-delayed γ rays; deduced modified S-factor, reaction rates. Compared with other data and predictions.

doi: 10.1088/1742-6596/381/1/012121
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2012KI16      Science 335, 1614 (2012)

N.Kinoshita, M.Paul, Y.Kashiv, P.Collon, C.M.Deibel, B.DiGiovine, J.P.Greene, D.J.Henderson, C.L.Jiang, S.T.Marley, T.Nakanishi, R.C.Pardo, K.E.Rehm, D.Robertson, R.Scott, C.Schmitt, X.D.Tang, R.Vondrasek, A.Yokoyama

A Shorter 146Sm Half-Life Measured and Implications for 146Sm-142Nd Chronology in the Solar System

RADIOACTIVITY 146Sm(α); measured decay products, Eα, Iα; deduced T1/2 and its uncertainty and 146Sm/144Sm ratio. 146Sm - 142Nd clock, comparison with available data.

doi: 10.1126/science.1215510
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2012MO05      Phys.Rev. C 85, 024607 (2012)

G.Montagnoli, A.M.Stefanini, C.L.Jiang, H.Esbensen, L.Corradi, S.Courtin, E.Fioretto, A.Goasduff, F.Haas, A.F.Kifle, C.Michelagnoli, D.Montanari, T.Mijatovic, K.E.Rehm, R.Silvestri, PushpendraP.Singh, F.Scarlassara, S.Szilner, X.D.Tang, C.A.Ur

Fusion of 40Ca+40Ca and other Ca+Ca systems near and below the barrier

NUCLEAR REACTIONS 40Ca(40Ca, X), E=98-130 MeV; measured evaporation residue spectra, σ(E); deduced barrier distribution, astrophysical S factor. 48Ca(48Ca, X), E(cm)=45-70 MeV; analyzed fusion σ(E), barrier distributions. Comparison with previous experimental data and with coupled-channel calculations based on Woods-Saxon (WS), M3Y+repulsion potentials.

doi: 10.1103/PhysRevC.85.024607
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2012NO01      Phys.Rev. C 85, 014607 (2012)

M.Notani, H.Esbensen, X.Fang, B.Bucher, P.Davies, C.L.Jiang, L.Lamm, C.J.Lin, C.Ma, E.Martin, K.E.Rehm, W.P.Tan, S.Thomas, X.D.Tang, E.Brown

Correlation between the 12C+12C, 12C+13C, and 13C+13C fusion cross sections

NUCLEAR REACTIONS 12C(13C, p)24Na, 13C(13C, np)24Na, E(cm)=2.6-4.8 MeV; measured Eγ, Iγ, βγ-coin from 24Na decay; deduced thick target yield by activation method, GEANT4 simulation, fusion cross section, S factors. 12C(12C, X), (13C, X), 13C(13C, X), E(cm)=2.5-6.5 MeV; analyzed fusion cross sections, fusion barrier parameters, spectroscopic factors by fitting with Wong formula. Comparison of experimental data with two coupled-channels calculations using ingoing wave boundary condition (IWBC).

doi: 10.1103/PhysRevC.85.014607
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2012TA13      J.Phys.:Conf.Ser. 337, 012016 (2012)

X.D.Tang, X.Fang, B.Bucher, H.Esbensen, C.L.Jiang, K.E.Rehm, C.J.Lin

Upper Limit on the molecular resonance strengths in the 12C+ 12C fusion reaction

NUCLEAR REACTIONS 12,13C(12C, X), (13C, X), E(cm)=2-6.5 MeV; analyzed published data on fusion reaction S-factor; deduced average S-factor, resonances, upper limit for molecular resonance strengths, empirical relationship using CRC-AW and EWS (equivalent square well).

doi: 10.1088/1742-6596/337/1/012016
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2012TA24      J.Phys.:Conf.Ser. 381, 012120 (2012)

X.D.Tang, H.Esbensen, X.Fang, B.Bucher, C.L.Jiang, K.E.Rehm, C.J.Lin, E.Brown

Does the 12C+12C fusion reaction trigger superburst?

NUCLEAR REACTIONS 12C(12C, X), (13C, X), E(cm)≈2.0-6.5 MeV;13C(13C, X), E(cm)≈2.9-6.5 MeV; calculated fusion reaction rate, modified S-factor using CC with IWBC (incoming wave boundary condition) and different interactions. Discussed role of possible resonance near E(cm)≈1.5 MeV.

doi: 10.1088/1742-6596/381/1/012120
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2011ES08      Phys.Rev. C 84, 064613 (2011)

H.Esbensen, X.Tang, C.L.Jiang

Effects of mutual excitations in the fusion of carbon isotopes

NUCLEAR REACTIONS 13C(13C, X), E(cm)=0-18 MeV; 13C(12C, X), E(cm)=2-7 MeV; 12C(12C, X), E(cm)=1-9 MeV; calculated fusion cross section, S factors. Coupled-channels calculations based on the M3Y+repulsion, double-folding potential. Comparison with experimental data.

doi: 10.1103/PhysRevC.84.064613
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2011JI14      J.Phys.:Conf.Ser. 312, 042011 (2011)

C.L.Jiang, B.B.Back, H.Esbensen, R.V.F.Janssens, K.E.Rehm, X.D.Tang

Do we understand heavy-ion fusion reactions of importance in stellar evolution?

NUCLEAR REACTIONS 10B(10B, X), E≈0.9-3.5 MeV;16O(16O, X), E≈5.5-11.5 MeV;30Si(28Si, X), E≈23-30 MeV;48Ca(36S, X), E≈36-48 MeV;48Ca(40Ca, X), E≈46-56 MeV;48Ca(48Ca, X), E≈46-56 MeV;45Sc(27Al, X), E≈31=39 MeV;64Ni(28Si, X), E≈43-52 MeV;64Ni(64Ni, X), E≈84-100 MeV;92Zr(90Zr, X), E≈165-177 MeV; re-analyzed S-factors in fusion reactions; calculated S-factors, fusion hinderance effect.

doi: 10.1088/1742-6596/312/4/042011
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2011LI28      Phys.Lett. B 702, 24 (2011)

Z.Liu, D.Seweryniak, P.J.Woods, C.N.Davids, M.P.Carpenter, T.Davinson, R.V.F.Janssens, R.D.Page, A.P.Robinson, J.Shergur, S.Sinha, X.D.Tang, F.R.Xu, S.Zhu

Structure of the proton emitter 117La studied by proton and γ-ray spectroscopy

RADIOACTIVITY 117La(p) [from 64Zn(58Ni, 4np), E=305 MeV]; measured reaction products, Eγ, Iγ; deduced ground-state proton decay, Q-value, T1/2, prompt γ-rays, no evidence of isomeric state. Comparison with theoretical predictions.

doi: 10.1016/j.physletb.2011.06.058
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2010JI03      Phys.Rev. C 81, 024611 (2010)

C.L.Jiang, K.E.Rehm, H.Esbensen, B.B.Back, R.V.F.Janssens, P.Collon, C.M.Deibel, B.DiGiovine, J.M.Figueira, J.P.Greene, D.J.Henderson, H.Y.Lee, M.Notani, S.T.Marley, R.C.Pardo, N.Patel, D.Seweryniak, X.D.Tang, C.Ugalde, S.Zhu

Fusion hindrance for 27Al+45Sc and other systems with a positive Q value

NUCLEAR REACTIONS 45Sc(27Al, X), E=51-82 MeV; measured fragment spectra, σ, astrophysical S-factor. Comparison with coupled-channels calculations. 14N(14N, X), E=4-11 MeV; 30Si(28Si, X), E=25-31 MeV; 45Sc(27Al, X), E=32-39 MeV; 64Ni(28Si, X), E=44-51 MeV; 40Ca(40Ca, X), E=49-57 MeV; 48Ca(48Ca, X), E=46-56 MeV; 48Ca(36S, X), E=37-48 MeV; comparison of measured cross sections and astrophysical S-factors with coupled-channel calculations.

doi: 10.1103/PhysRevC.81.024611
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2010JI14      Phys.Rev. C 82, 041601 (2010)

C.L.Jiang, A.M.Stefanini, H.Esbensen, K.E.Rehm, L.Corradi, E.Fioretto, P.Mason, G.Montagnoli, F.Scarlassara, R.Silvestri, P.P.Singh, S.Szilner, X.D.Tang, C.A.Ur

Fusion hindrance for Ca+Ca systems: Influence of neutron excess

NUCLEAR REACTIONS 48Ca(40Ca, X), E=89.2, 107.7 MeV; measured particle spectra, σ(E, θ); deduced S factors. Comparisons of experimental σ(E) for 40Ca+40Ca, 40Ca+48Ca, 48Ca+48Ca, 40Ca+90Zr, 40Ca+96Zr and 48Ca+96Zr systems with coupled-channel calculations.

doi: 10.1103/PhysRevC.82.041601
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2010LE02      Phys.Rev. C 81, 015802 (2010)

H.Y.Lee, J.P.Greene, C.L.Jiang, R.C.Pardo, K.E.Rehm, J.P.Schiffer, A.H.Wuosmaa, N.J.Goodman, J.C.Lighthall, S.T.Marley, K.Otsuki, N.Patel, M.Beard, M.Notani, X.D.Tang

Experimental study of the 11, 12B(n, γ) reactions and their influence on r-process nucleosynthesis of light elements

NUCLEAR REACTIONS 2H(11B, p), E=81 MeV; 2H(12B, p), E=75 MeV; measured proton and 11,12,13B particle spectra, σ(θ). 12,13B; deduced levels, J, π, l-transfers. Comparison with DWBA calculations. 11B, 12B(n, γ); deduced reaction rates of astrophysical relevance, and abundances of 11B and 12B in r process.

doi: 10.1103/PhysRevC.81.015802
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2010NO04      Nucl.Phys. A834, 192c (2010)

M.Notani, P.Davies, B.Bucher, X.Fang, L.Lamm, C.Ma, E.Martin, W.Tan, X.D.Tang, S.Thomas, C.L.Jiang

Study of the hindrance effect in sub-barrier fusion reactions

NUCLEAR REACTIONS 12C(13C, p), E(cm)=2.6-5.0 MeV; measured Eβ, Iβ, Eγ, Iγ, βγ-coin, thick target yield; deduced σ, astrophysical S-factor. Comparison with data and calculations.

doi: 10.1016/j.nuclphysa.2009.12.037
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2010SU30      Eur.Phys.J. A 46, 69 (2010)

J.Su, Z.H.Li, L.C.Zhu, G.Lian, X.X.Bai, Y.B.Wang, B.Guo, B.X.Wang, S.Q.Yan, S.Zeng, Y.J.Li, E.T.Li, S.J.Jin, X.Liu, Q.W.Fan, J.L.Zhang, X.Y.Jiang, J.X.Lu, X.F.Lan, X.Z.Tang, W.P.Liu

Alpha decay half-life of 147Sm in metal samarium and Sm2O3

RADIOACTIVITY 147Sm(α); measured Eα, Iα for metalic Sm and Sm oxide; deduced T1/2. Halflives in both forms are different.

doi: 10.1140/epja/i2010-11028-7
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2010TA05      Phys.Rev. C 81, 045809 (2010)

X.D.Tang, K.E.Rehm, I.Ahmad, C.R.Brune, A.Champagne, J.P.Greene, A.Hecht, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, D.Kahl, E.F.Moore, M.Notani, R.C.Pardo, N.Patel, M.Paul, G.Savard, J.P.Schiffer, R.E.Segel, S.Sinha, A.H.Wuosmaa

Determination of the E1 component of the low-energy 12C(α, γ)16O cross section

RADIOACTIVITY 16N(β-α); measured Eα, Iα, α12C-coin, half-life; deduced E1 component of the S factor for 12C(α, γ)16O reaction using a set of twin ionization chambers. R-matrix analysis. Comparison with previous studies.

NUCLEAR REACTIONS 2H(15N, p)15N/16N/16O/20Ne, E=82 MeV; measured fragment yields.

doi: 10.1103/PhysRevC.81.045809
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2008JI04      Phys.Rev. C 78, 017601 (2008)

C.L.Jiang, B.B.Back, H.Esbensen, J.P.Greene, R.V.F.Janssens, D.J.Henderson, H.Y.Lee, C.J.Lister, M.Notani, R.C.Pardo, N.Patel, K.E.Rehm, D.Seweryniak, B.Shumard, X.Wang, S.Zhu, S.Misicu, P.Collon, X.D.Tang

Fusion hindrance for a positive Q-value system

NUCLEAR REACTIONS 30Si(28Si, X), E=48.5-71 MeV; measured excitation functions, fusion σ. 12C(12C, X); systematics of Q-values. Comparisons with model calculations.

doi: 10.1103/PhysRevC.78.017601
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2008KI05      J.Phys.(London) G35, 014033 (2008)

N.Kinoshita, T.Hashimoto, T.Nakanishi, A.Yokoyama, H.Amakawa, T.Mitsugashira, T.Ohtsuki, N.Takahashi, I.Ahmad, J.P.Greene, D.J.Henderson, C.L.Jiang, M.Notani, R.C.Pardo, N.Patel, K.E.Rehm, R.Scott, R.Vondrasek, L.Jisonna, P.Collon, D.Robertson, C.Schmitt, X.D.Tang, Y.Kashiv, H.Nassar, M.Paul

Ultra-sensitive detection of p-process nuclide 146Sm produced by (γ, n), (p, 2nε) and (n, 2n) reactions

doi: 10.1088/0954-3899/35/1/014033
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2008WU05      Phys.Rev. C 78, 041302 (2008)

A.H.Wuosmaa, J.P.Schiffer, K.E.Rehm, J.P.Greene, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, J.C.Lighthall, S.T.Marley, E.F.Moore, R.C.Pardo, N.Patel, M.Paul, D.Peterson, S.C.Pieper, G.Savard, R.E.Segel, R.H.Siemssen, X.D.Tang, R.B.Wiringa

Structure of 7He by proton removal from 8Li with the (d, 3He) reaction

NUCLEAR REACTIONS 2H(8Li, 3He), E=76 MeV; 2H(7Li, t), (7Li, 3He), E=81 MeV; measured charged particle spectra, (particle)(particle)-coin, angular distributions, σ, σ(θ), spectroscopic factors. 7He; deduced levels, J, π. Comparisons with data from 2H(6He, p) experiment. Comparisons with nuclear structure models and variational quantum Monte Carlo calculations.

doi: 10.1103/PhysRevC.78.041302
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2007FR10      Phys.Rev. C 75, 051301 (2007)

S.J.Freeman, J.P.Schiffer, A.C.C.Villari, J.A.Clark, C.Deibel, S.Gros, A.Heinz, D.Hirata, C.L.Jiang, B.P.Kay, A.Parikh, P.D.Parker, J.Qian, K.E.Rehm, X.D.Tang, V.Werner, C.Wrede

Pair correlations in nuclei involved in neutrinoless double Β decay: 76Ge and 76Se

NUCLEAR REACTIONS 74,76Ge, 76,78Se(p, t), E=23 MeV; measured yields, cross sections and angular distributions. Compared results to DWBA calculations.

doi: 10.1103/PhysRevC.75.051301
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2007HA49      J.Nucl.Radiochem.Sci. 8, 109 (2007)

T.Hashimoto, T.Nakanishi, A.Yokoyama, H.Amakawa, T.Mitsugashira, T.Ohtsuki, N.Takahashi, I.Ahmad, J.P.Greene, D.J.Henderson, C.L.Jiang, M.Notani, R.C.Pardo, N.Patel, K.E.Rehm, R.Scott, R.Vondrasek, L.Jisonna, P.Collon, D.Robertson, C.Schmitt, X.D.Tang, Y.Kashiv, M.Paul

Technological Development for Half-life Measurement of 146Sm Nuclide

NUCLEAR REACTIONS 147Sm(γ, n), E < 50 MeV; 147Sm(n, 2n), E=6-10 MeV; 147Sm(p, 2n), E=21 MeV; measured Eα, Iα.


2007HU22      Chin.Phys.Lett. 24, 2792 (2007)

Y.-S.Huang, N.-Y.Wang, X.-J.Duan, X.-F.Lan, Z.-X.Tan, X.-Z.Tang, Y.-X.Ye

Neutron Generation and Kinetic Energy of Expanding Laser Plasmas

doi: 10.1088/0256-307X/24/10/022
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2007NA27      Phys.Rev. C 76, 054604 (2007)

R.S.Naik, W.Loveland, P.H.Sprunger, A.M.Vinodkumar, D.Peterson, C.L.Jiang, S.Zhu, X.Tang, E.F.Moore, P.Chowdhury

Measurement of the fusion probability PCN for the reaction of 50Ti with 208Pb

NUCLEAR REACTIONS 208Pb(50Ti, X), E(cm)=183.7, 186.2, 190.2, 194.2, 202.3 MeV; measured fission fragments, cross sections, angular distributions; deduced fusion probabilities and survival probabilities for compound nuclei Z=102-113.

doi: 10.1103/PhysRevC.76.054604
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2007TA34      Phys.Rev.Lett. 99, 052502 (2007)

X.D.Tang, K.E.Rehm, I.Ahmad, C.R.Brune, A.Champagne, J.P.Greene, A.A.Hecht, D.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, D.Kahl, E.F.Moore, M.Notani, R.C.Pardo, N.Patel, M.Paul, G.Savard, J.P.Schiffer, R.E.Segel, S.Sinha, B.Shumard, A.H.Wuosmaa

New Determination of the Astrophysical S Factor SE1 of the 12C(α, γ)16O Reaction

RADIOACTIVITY 16N(β-), (β-α); measured Eα, Iα, 12Cα-coin. 12C(α, γ); deduced astrophysical S-factor.

doi: 10.1103/PhysRevLett.99.052502
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2007WU05      Eur.Phys.J. Special Topics 150, 79 (2007)

A.H.Wuosmaa, K.E.Rehm, J.P.Greene, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, J.C.Lighthall, S.T.Marley, E.F.Moore, R.C.Pardo, N.Patel, M.Paul, D.Peterson, S.C.Pieper, G.Savard, J.P.Schiffer, R.E.Segal, R.H.Siemssen, S.Sinha, X.Tang, R.B.Wiringa

Nucleon transfer reactions with exotic beams at ATLAS

doi: 10.1140/epjst/e2007-00271-y
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2006JI06      Phys.Lett. B 640, 18 (2006)

C.L.Jiang, B.B.Back, H.Esbensen, R.V.F.Janssens, S.Misicu, K.E.Rehm, P.Collon, C.N.Davids, J.Greene, D.J.Henderson, L.Jisonna, S.Kurtz, C.J.Lister, M.Notani, M.Paul, R.Pardo, D.Peterson, D.Seweryniak, B.Shumard, X.D.Tang, I.Tanihata, X.Wang, S.Zhu

First evidence of fusion hindrance for a small Q-value system

NUCLEAR REACTIONS 64Ni(28Si, X), E=63-95 MeV; measured fusion-evaporation σ, fusion excitation function; deduced hindrance at sub-barrier energies. Coupled-channels analysis.

doi: 10.1016/j.physletb.2006.07.007
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2006MU15      Eur.Phys.J. A 27, Supplement 1, 205 (2006)

A.M.Mukhamedzhanov, L.D.Blokhintsev, B.A.Brown, V.Burjan, S.Cherubini, C.A.Gagliardi, B.F.Irgaziev, V.Kroha, F.M.Nunes, F.Pirlepesov, R.G.Pizzone, S.Romano, C.Spitaleri, X.D.Tang, L.Trache, R.E.Tribble, A.Tumino

Indirect techniques in nuclear astrophysics: Asymptotic Normalization Coefficient and Trojan Horse

NUCLEAR REACTIONS 14N(3He, d), E=26.3 MeV; measured σ(θ). 14N(p, γ), E ≈ 100-600 keV; deduced astrophysical S-factor. 11C, 13N(p, γ), E not given; analyzed resonant and nonresonant amplitudes. Asymptotic normalization coefficient and Trojan horse techniques discussed.

doi: 10.1140/epja/i2006-08-032-7
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2006PE21      Phys.Rev. C 74, 024306 (2006)

K.Perajarvi, C.Fu, G.V.Rogachev, G.Chubarian, V.Z.Goldberg, F.Q.Guo, D.Lee, D.M.Moltz, J.Powell, B.B.Skorodumov, G.Tabacaru, X.D.Tang, R.E.Tribble, B.A.Brown, A.Volya, J.Cerny

Structure of 12N using 11C+p resonance scattering

NUCLEAR REACTIONS 1H(11C, p), E(cm)=2.2-11.0 MeV; measured recoil proton spectra, σ(θ), excitation functions. 12N deduced levels, J, π, widths. R-matrix analysis.

doi: 10.1103/PhysRevC.74.024306
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2006TA09      Phys.Rev. C 73, 025808 (2006)

G.Tabacaru, A.Azhari, J.Brinkley, V.Burjan, F.Carstoiu, C.Fu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, X.Tang, L.Trache, R.E.Tribble, S.Zhou

Scattering of 7Be and 8B and the astrophysical S17 factor

NUCLEAR REACTIONS H, C, N(7Be, 7Be), E=87 MeV; C(8B, 8B), E=95 MeV; measured σ(θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S-factor.

doi: 10.1103/PhysRevC.73.025808
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2005JI02      Phys.Rev. C 71, 044613 (2005)

C.L.Jiang, K.E.Rehm, H.Esbensen, R.V.F.Janssens, B.B.Back, C.N.Davids, J.P.Greene, D.J.Henderson, C.J.Lister, R.C.Pardo, T.Pennington, D.Peterson, D.Seweryniak, B.Shumard, S.Sinha, X.D.Tang, I.Tanihata, S.Zhu, P.Collon, S.Kurtz, M.Paul

Hindrance of heavy-ion fusion at extreme sub-barrier energies in open-shell colliding systems

NUCLEAR REACTIONS 100Mo(64Ni, X), E=196-262 MeV; measured fusion-evaporation σ, fusion excitation function; deduced hindrance at sub-barrier energies. 58,60,64Ni, 74Ge, 90,91,94Zr, 92,100Mo, 124Sn(58Ni, X), 89Y(60Ni, X), 64Ni, 74Ge, 92,96Zr, 92,100Mo, 124Sn(64Ni, X), E(cm) ≈ 120 MeV; analyzed fusion σ, sub-barrier hindrance.

doi: 10.1103/PhysRevC.71.044613
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2005NA08      Phys.Rev.Lett. 94, 092504 (2005)

H.Nassar, M.Paul, I.Ahmad, D.Berkovits, M.Bettan, P.Collon, S.Dababneh, S.Ghelberg, J.P.Greene, A.Heger, M.Heil, D.J.Henderson, C.L.Jiang, F.Kappeler, H.Koivisto, S.O'Brien, R.C.Pardo, N.Patronis, T.Pennington, R.Plag, K.E.Rehm, R.Reifarth, R.Scott, S.Sinha, X.Tang, R.Vondrasek

Stellar (n, γ) Cross Section of 62Ni

NUCLEAR REACTIONS 62Ni(n, γ), E=spectrum; measured total σ. Fast-neutron activation, accelerator mass spectrometry. Astrophysical implications discussed.

doi: 10.1103/PhysRevLett.94.092504
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2005WU03      Phys.Rev.Lett. 94, 082502 (2005)

A.H.Wuosmaa, K.E.Rehm, J.P.Greene, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, E.F.Moore, R.C.Pardo, M.Paul, D.Peterson, S.C.Pieper, G.Savard, J.P.Schiffer, R.E.Segel, S.Sinha, X.Tang, R.B.Wiringa

Neutron Spectroscopic Factors in 9Li from 2H(8Li, p)9Li

NUCLEAR REACTIONS 2H(8Li, p), E ≈ 76 MeV; measured Ep, excitation energy spectra, σ(θ). 9Li deduced levels, J, π, spectroscopic factors. Comparison with model predictions.

doi: 10.1103/PhysRevLett.94.082502
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2005WU08      Phys.Rev. C 72, 061301 (2005)

A.H.Wuosmaa, K.E.Rehm, J.P.Greene, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, L.Jisonna, E.F.Moore, R.C.Pardo, M.Paul, D.Peterson, Steven C.Pieper, G.Savard, J.P.Schiffer, R.E.Segel, S.Sinha, X.Tang, R.B.Wiringa

Search for excited states in 7He with the (d, p) reaction

NUCLEAR REACTIONS 2H(6He, p), E=69 MeV; 2H(7Li, p), E=81 MeV; measured particle spectra, σ(θ). 7He deduced ground-state J, π, excited state energy, width.

doi: 10.1103/PhysRevC.72.061301
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2004GO15      Phys.Rev. C 69, 031302 (2004)

V.Z.Goldberg, G.G.Chubarian, G.Tabacaru, L.Trache, R.E.Tribble, A.Aprahamian, G.V.Rogachev, B.B.Skorodumov, X.D.Tang

Low-lying levels in 15F and the shell model potential for drip-line nuclei

NUCLEAR REACTIONS 1H(14O, 14O), E(cm)=1.0-3.4 MeV; measured excitation functions, σ(θ). 15F deduced ground and excited states J, π, resonance features. Woods-Saxon potential model analysis.

doi: 10.1103/PhysRevC.69.031302
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2004MO19      Phys.Rev. C 69, 044604 (2004)

S.Moretto, D.Fabris, M.Lunardon, S.Pesente, V.Rizzi, G.Viesti, M.Barbui, M.Cinausero, E.Fioretto, G.Prete, A.Brondi, E.Vardaci, F.Lucarelli, A.Azhari, X.D.Tang, K.Hagel, Y.Ma, A.Makeev, M.Murray, J.B.Natowitz, L.Qin, P.Smith, L.Trache, R.E.Tribble, R.Wada, J.Wang

Search for temperature and N/Z dependent effects in the decay of A = 98 compound nuclei

NUCLEAR REACTIONS 87Rb(11B, X), (11C, X), E=110 MeV; measured particle spectra, (light particle)(evaporation residue)-coin, relative proton, α-particle yields. Comparison with statistical model predictions.

doi: 10.1103/PhysRevC.69.044604
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2004NA39      Nucl.Phys. A746, 613c (2004)

H.Nassar, S.Ghelberg, M.Paul, S.Dababneh, M.Heil, F.Kappeler, R.Plag, I.Ahmad, J.P.Greene, D.J.Henderson, C.L.Jiang, R.C.Pardo, T.Pennington, K.E.Rehm, R.Scott, S.Sinha, X.Tang, R.Vondrasek, H.Koivisto, D.Berkovits, M.Bettan, R.Reifarth, P.Collon, S.O'Brien, N.Patronis

Production and isobaric separation of 63Ni ions for determination of the 62Ni(n, γ)63Ni reaction cross section at stellar temperatures

NUCLEAR REACTIONS 62Ni(n, γ), E=fast; measured yields.

doi: 10.1016/j.nuclphysa.2004.09.140
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2004RE31      Nucl.Phys. A746, 354c (2004)

K.E.Rehm, C.L.Jiang, J.P.Greene, D.Henderson, R.V.F.Janssens, E.F.Moore, G.Mukherjee, R.C.Pardo, T.Pennington, J.P.Schiffer, S.Sinha, X.D.Tang, R.H.Siemssen, L.Jisonna, R.E.Segel, A.H.Wuosmaa

First studies of the 8B(α, p)11C reaction

NUCLEAR REACTIONS 1H(11C, α), E=98-110 MeV; measured σ(θ). 8B(α, p), E*=8.7-9.8 MeV; deduced excitation function, astrophysical reaction rate.

doi: 10.1016/j.nuclphysa.2004.09.052
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2004TA15      Phys.Rev. C 69, 055807 (2004)

X.Tang, A.Azhari, C.Fu, C.A.Gagliardi, A.M.Mukhamedzhanov, F.Pirlepesov, L.Trache, R.E.Tribble, V.Burjan, V.Kroha, F.Carstoiu, B.F.Irgaziev

Determination of the direct capture contribution for 13N(p, γ)14O from the 14O → 13N + p asymptotic normalization coefficient

NUCLEAR REACTIONS 14N(13N, 14O), E=11.8 MeV/nucleon; measured σ(θ); deduced asymptotic normalization coefficient. 12C, 14N(13N, 13N), E=11.8 MeV/nucleon; measured elastic σ(θ). 13N(p, γ), E=low; deduced astrophysical S-factor, reaction rates.

doi: 10.1103/PhysRevC.69.055807
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2004WA23      Phys.Rev.Lett. 93, 142501 (2004)

L.-B.Wang, P.Mueller, K.Bailey, G.W.F.Drake, J.P.Greene, D.Henderson, R.J.Holt, R.V.F.Janssens, C.L.Jiang, Z.-T.Lu, T.P.O'Connor, R.C.Pardo, K.E.Rehm, J.P.Schiffer, X.D.Tang

Laser Spectroscopic Determination of the 6He Nuclear Charge Radius

NUCLEAR MOMENTS 4,6He; measured isotope shift. 6He deduced charge radius. Laser spectroscopy.

doi: 10.1103/PhysRevLett.93.142501
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2003HA20      Phys.Rev.Lett. 91, 082501 (2003)

J.C.Hardy, V.E.Iacob, M.Sanchez-Vega, R.G.Neilson, A.Azhari, C.A.Gagliardi, V.E.Mayes, X.Tang, L.Trache, R.E.Tribble

High Precision Measurement of the Superallowed 0+ → 0+ β Decay of 22Mg

RADIOACTIVITY 22Mg(β+) [from 1H(23Na, 2n)]; measured Eγ, Iγ, βγ-coin, T1/2; deduced superallowed branching ratio, log ft. 22Na levels deduced β-feeding intensities.

doi: 10.1103/PhysRevLett.91.082501
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2003HY02      Phys.Rev. C 68, 015501 (2003)

B.C.Hyman, V.E.Iacob, A.Azhari, C.A.Gagliardi, J.C.Hardy, V.E.Mayes, R.G.Neilson, M.Sanchez-Vega, X.Tang, L.Trache, R.E.Tribble

Beta decay of 62Ga

RADIOACTIVITY 62Ga(EC) [from 1H(64Zn, 62Ga)]; measured Eγ, Iγ, T1/2, branching ratios. 62Zn levels deduced β-feeding intensities. Mass separator.

NUCLEAR REACTIONS 1H(64Zn, X), E=41, 42 MeV/nucleon; measured fragments isotopic yields.

doi: 10.1103/PhysRevC.68.015501
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2003KR14      Nucl.Phys. A719, 119c (2003)

V.Kroha, A.Azhari, P.Bem, V.Burjan, C.A.Gagliardi, A.M.Mukhamedzhanov, J.Novak, S.Piskor, E.Simeckova, X.Tang, L.Trache, R.E.Tribble, J.Vincour

Asymptotic Normalization Coefficients in nuclear astrophysics

NUCLEAR REACTIONS 9Be, 11,13C(p, γ), E=low; analyzed asymptotic normalization coefficients, astrophysical S-factors.

doi: 10.1016/S0375-9474(03)00979-5
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2003MU18      Nucl.Phys. A725, 279 (2003)

A.M.Mukhamedzhanov, A.Azhari, V.Burjan, C.A.Gagliardi, V.Kroha, A.Sattarov, X.Tang, L.Trache, R.E.Tribble

Asymptotic normalization coefficients from proton transfer reactions and astrophysical S factors for the CNO 13C(p, γ)14N radiative capture process

NUCLEAR REACTIONS 13C(14N, 13C), (3He, d), E not given; 13C(p, γ), E(cm)=100-900 keV; analyzed data; deduced asymptotic normalization coefficients. 13C(p, γ), E=0-900 keV; deduced astrophysical S-factors. R-matrix approach.

doi: 10.1016/S0375-9474(03)01618-X
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2003TA02      Phys.Rev. C 67, 015804 (2003)

X.Tang, A.Azhari, C.A.Gagliardi, A.M.Mukhamedzhanov, F.Pirlepesov, L.Trache, R.E.Tribble, V.Burjan, V.Kroha, F.Carstoiu

Determination of the astrophysical S factor for 11C(p, γ)12N from the 12N → 11C+p asymptotic normalization coefficient

NUCLEAR REACTIONS 14N(11C, 12N), E=110 MeV; measured particle spectra, σ(θ); deduced asymptotic normalization coefficient. 11C(p, γ), E(cm)=0-0.7 MeV; deduced astrophysical S-factor, reaction rate.

doi: 10.1103/PhysRevC.67.015804
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2003TR04      Phys.Rev. C 67, 062801 (2003)

L.Trache, A.Azhari, F.Carstoiu, H.L.Clark, C.A.Gagliardi, Y.-W.Lui, A.M.Mukhamedzhanov, X.Tang, N.Timofeyuk, R.E.Tribble

Asymptotic normalization coefficients for 8B → 7Be + p from a study of 8Li → 7Li + n

NUCLEAR REACTIONS 13C(7Li, 8Li), E=63 MeV; measured σ(θ); deduced spectroscopic factors, asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S-factor.

doi: 10.1103/PhysRevC.67.062801
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2003TR09      Nucl.Phys. A718, 147c (2003)

R.E.Tribble, A.Azhari, P.Bem, V.Burjan, F.Carstoiu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, J.Novak, F.Pirlepesov, S.Piskor, A.Sattarov, E.Simeckova, X.Tang, L.Trache, J.Vincour

New Results for 8B(p, γ)9C, 11C(p, γ)12N, 13C(p, γ)14N and 14N(p, γ)15O at stellar energies

NUCLEAR REACTIONS 8B, 11,13C, 14N(p, γ), E=low; analyzed asymptotic normalization coefficients; deduced astrophysical reaction rates, S-factors.

doi: 10.1016/S0375-9474(03)00705-X
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2002GA11      Eur.Phys.J. A 13, 227 (2002)

C.A.Gagliardi, A.Azhari, V.Burjan, F.Carstoiu, V.Kroha, A.M.Mukhamedzhanov, A.Sattarov, X.Tang, L.Trache, R.E.Tribble

Asymptotic Normalization Coefficients and Astrophysical Direct Capture Rates

NUCLEAR REACTIONS 16O(3He, d), E not given; analyzed σ(E, θ). 16O(p, γ), E=0-1.3 MeV; 9Be(p, γ), E(cm)=0-1.6 MeV; analyzed S-factors. 10B, 14N(7Be, 7Be), (7Be, 8B), E=12 MeV/nucleon; 1H, 14N(11C, 12N), (11C, 11C), E not given; measured σ(θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E not given; deduced reaction rate.

doi: 10.1007/s10050-002-8747-8
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2002GA44      Eur.Phys.J. A 15, 69 (2002)

C.A.Gagliardi, A.Azhari, V.Burjan, F.Carstoiu, V.Kroha, A.M.Mukhamedzhanov, A.Sattarov, X.Tang, L.Trache, R.E.Tribble

Asymptotic normalization coefficients in nuclear astrophysics and structure

NUCLEAR REACTIONS 11C, 16O(p, γ), E ≈ 0.2-1.4 MeV; 9Be(8B, p7Be), E=41 MeV/nucleon; analyzed astrophysical S-factors, asymptotic normalization coefficients.

doi: 10.1140/epja/i2001-10228-6
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2002MU14      Phys.Rev. C66, 027602 (2002)

A.M.Mukhamedzhanov, A.Azhari, V.Burjan, C.A.Gagliardi, V.Kroha, A.Sattarov, X.Tang, L.Trache, R.E.Tribble

Astrophysical S factor for 13C(p, γ) 14N and asymptotic normalization coefficients

NUCLEAR REACTIONS 13C(p, γ), E ≈ 0-800 keV; analyzed astrophysical S-factors, asymptotic normalization coefficients.

doi: 10.1103/PhysRevC.66.027602
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2002TR08      Nucl.Phys. A701, 278c (2002)

R.E.Tribble, A.Azhari, C.A.Gagliardi, J.C.Hardy, A.Mukhamedzhanov, X.Tang, L.Trache, S.J.Yennello

Radioactive Beams at Texas A and M University

doi: 10.1016/S0375-9474(01)01597-4
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2001AZ01      Phys.Rev. C63, 055803 (2001)

A.Azhari, V.Burjan, F.Carstoiu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, F.M.Nunes, X.Tang, L.Trache, R.E.Tribble

Asymptotic Normalization Coefficients and the 7Be(p, γ)8B Astrophysical S Factor

NUCLEAR REACTIONS 10B, 14N(7Be, 7Be), E=85 MeV; measured σ(θ). 10B, 14N(7Be, 8B), E=85 MeV; measured σ(E, θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S factor.

doi: 10.1103/PhysRevC.63.055803
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2001GA19      Nucl.Phys. A682, 369c (2001)

C.A.Gagliardi, A.Azhari, P.Bem, V.Burjan, F.Carstoiu, J.Cejpek, H.L.Clark, V.Kroha, Y.-W.Lui, A.M.Mukhamedzhanov, J.Novak, S.Piskor, A.Sattarov, E.Simeckova, X.Tang, L.Trache, R.E.Tribble, J.Vincour

Asymptotic Normalization Coefficients from Direct Transfer Reactions and Astrophysical S Factors

NUCLEAR REACTIONS 10B, 14N(7Be, 7Be), (7Be, 8B), E=12 MeV/nucleon; measured σ(θ). 7Be(p, γ), E not given; deduced asymptotic nomalization coefficients, astrophysical capture rate. Other reactions discussed.

doi: 10.1016/S0375-9474(00)00662-X
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Note: The following list of authors and aliases matches the search parameter X.Tang: , X.D.TANG, X.L.TANG, X.N.TANG, X.P.TANG, X.T.TANG, X.Z.TANG