NSR Query Results


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NSR database version of April 11, 2024.

Search: Author = X.Fang

Found 55 matches.

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2023AN14      Sci. Rep. 13, 12657 (2023)

Z.An, W.Qiu, W.Jiang, G.Yang, X.Li, Z.Liao, Z.Zhuang, X.Zhang, S.Chen, C.Guo, E.Xiao, X.Fang, X.Li, H.Wang, X.Hu, Bi.Jiang, W.Shen, J.Wang, J.Ren, X.Ruan, D.Wang, S.-Y.Zhang, W.Luo, Z.Zhu, H.Lan, Z.Cao, X.Ma, Y.Liu, P.Wang, Y.Yang, P.Su, X.Deng, W.He, Y.Ma, C.Ma, Y.Wang, P.He, R.Tang, T.Zhou, J.Wang, H.Yi, Y.Zhang, Y.Chen, R.Fan, K.Gao, Q.Li, K.Sun, Z.Tan, M.Gu, H.Jing, J.Tang

Measurement of the 181Ta(n, γ) cross sections up to stellar s-process temperatures at the CSNS Back-n

NUCLEAR REACTIONS 181Ta(n, γ), E=0.001-800 keV; measured reaction products, En, In, TOF; deduced σ, resonance parameters using the R-Matrix code SAMMY, Maxwellian average cross sections (MACS). Comparison with available data. The back-streaming white neutron facility (Back-n) of China spallation neutron source (CSNS).

doi: 10.1038/s41598-023-39603-7
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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.


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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2021HU23      Phys.Rev.Lett. 127, 172701 (2021)

J.Hu, H.Yamaguchi, Y.H.Lam, A.Heger, D.Kahl, A.M.Jacobs, Z.Johnston, S.W.Xu, N.T.Zhang, S.B.Ma, L.H.Ru, E.Q.Liu, T.Liu, S.Hayakawa, L.Yang, H.Shimizu, C.B.Hamill, A.St J.Murphy, J.Su, X.Fang, K.Y.Chae, M.S.Kwag, S.M.Cha, N.N.Duy, N.K.Uyen, D.H.Kim, R.G.Pizzone, M.La Cognata, S.Cherubini, S.Romano, A.Tumino, J.Liang, A.Psaltis, M.Sferrazza, D.Kim, Y.Y.Li, S.Kubono

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New 22Mg(α, p)25Al Reaction Rate Determined at the Gamow Energy

NUCLEAR REACTIONS 1H(25Al, p), (25Al, p'), (25Al, X), E=142 MeV; measured reaction products, Ep, Ip, Eγ, Iγ. 26Si; deduced σ(θ), level energies, J, π, resonance parameters, astrophysical reaction rates. Comparison with available data.

doi: 10.1103/physrevlett.127.172701
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2724. Data from this article have been entered in the XUNDL database. For more information, click here.


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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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2288.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2812.


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.


2016CU02      Phys.Rev. C 94, 034313 (2016)

N.Curtis, S.Almaraz-Calderon, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, X.Fang, M.Freer, G.Goldring, F.Jung, S.R.Lesher, W.Lu, J.D.Malcolm, A.Roberts, W.P.Tan, C.Wheldon, V.A.Ziman

8Be + 8Be and 12C + α breakup states in 16O populated via the 13C(4He, 4α)n reaction

NUCLEAR REACTIONS 13C(α, 16O), E=22.0, 27.0, 27.5, 28.0 MeV; measured reaction products using four position-sensitive double-sided Si strip detectors, at Notre Dame FN Tandem accelerator facility. 16O; deduced levels identified through the 8Be+8Be and 12C*+α channels, J, π, centroids, cross sections. Comparison with previous studies using 12C(α, 8Be)8Be and 12C(16O, 4α)12C reactions. Relevance to 4α chain structure in 16O.

doi: 10.1103/PhysRevC.94.034313
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2239. 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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Data from this article have been entered in the XUNDL database. For more information, click here.


2016SM02      Phys.Rev. C 94, 014320 (2016)

R.Smith, C.Wheldon, M.Freer, N.Curtis, Tz.Kokalova, S.Almaraz-Calderon, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, X.Fang, G.Goldring, F.Jung, S.R.Lesher, W.Lu, J.D.Malcolm, A.Roberts, W.P.Tan, V.A.Ziman

Evidence for a 3.8 MeV state in 9Be

NUCLEAR REACTIONS 9Be(α, n3α), E=22, 26 MeV; measured Eα, Iα using an array of double-sided silicon strip detectors (DSSSDs) at the Notre Dame FN Tandem Van de Graaff accelerator facility; extracted sum energy spectra for all four final-state particles, assumed to be 3α+n, 9Be excitation spectrum. 9Be; deduced levels, new state at 3.8 MeV, J, π, width, ratios of reduced widths to Wigner limits (decays to 8Be ground state). 9Be, 9B; comparison of levels and widths in mirror nuclei.

doi: 10.1103/PhysRevC.94.014320
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Data from this article have been entered in the XUNDL database. For more information, click here.


2016TA09      Phys.Rev. C 93, 055803 (2016)

R.Talwar, T.Adachi, G.P.A.Berg, L.Bin, S.Bisterzo, M.Couder, R.J.deBoer, X.Fang, H.Fujita, Y.Fujita, J.Gorres, K.Hatanaka, T.Itoh, T.Kadoya, A.Long, K.Miki, D.Patel, M.Pignatari, Y.Shimbara, A.Tamii, M.Wiescher, T.Yamamoto, M.Yosoi

Probing astrophysically important states in the 26Mg nucleus to study neutron sources for the s process

NUCLEAR REACTIONS 26Mg(α, α'), E=206 MeV; 22Ne(6Li, d)26Mg, E=82.3 MeV; measured Eα, Iα, E(d), I(d), σ(θ) using Grand Raiden (GR) spectrometer at RCNP-Osaka. 26Mg; deduced α-unbound resonance energies, levels, J, π, α-spectroscopic factors, resonance strengths. Angular distributions for inelastic scattering analyzed by coupled channel code PTOLEMY and for transfer reactions by FRESCO code. 22Ne(α, γ)26Mg, 22Ne(α, n)25Mg, T9=0.01-10; deduced astrophysical reaction rates from resonance parameters. Comparison with previous results. Relevance to slow neutron capture process (s process) in massive stars.

doi: 10.1103/PhysRevC.93.055803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2514. Data from this article have been entered in the XUNDL database. For more information, click here.


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.


2015NA14      Phys.Rev. C 92, 025804 (2015)

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

Proton capture cross section of 72Ge and astrophysical implications

NUCLEAR REACTIONS 72,74Ge(p, γ), E=1.8-3.6 MeV; measured Eγ, Iγ, σ(E) using γ-summing detector SuN at Notre Dame Tandem Van de Graff accelerator facility. Natural Ge target. Comparison with calculations using TALYS1.6 code and different combinations of optical model potentials (OMPs), nuclear level densities (NLDs), and γ-ray strength functions, and with data in standard astrophysical libraries BRUSLIB and REACLIB. Relevance to astrophysical p-process.

doi: 10.1103/PhysRevC.92.025804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2183.


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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Data from this article have been entered in the XUNDL database. For more information, click here.


2015XU11      Phys.Rev. C 92, 015807 (2015)

J.Xu, E.Shields, F.Calaprice, S.Westerdale, F.Froborg, B.Suerfu, T.Alexander, A.Aprahamian, H.O.Back, C.Casarella, X.Fang, Yo.K.Gupta, A.Ianni, E.Lamere, W.H.Lippincott, Q.Liu, S.Lyons, K.Siegl, M.Smith, W.Tan, B.Vande Kolk

Scintillation efficiency measurement of Na recoils in NaI(Tl) below the DAMA/LIBRA energy threshold

NUCLEAR REACTIONS Na, I(n, n'), E=690 keV pulsed beam; measured Na-recoil spectra, double-TOF spectrum for coincidence events of Na recoils, E(n), I(n), 127I excitation events at Notre Dame accelerator facility; deduced Na-recoil quenching factors, spectral fits of the DAMA/LIBRA modulation amplitudes to standard WIMP model. Comparison with other experimental results for Na-recoil quenching factors. Relevance to DAMA/LIBRA dark matter claims.

doi: 10.1103/PhysRevC.92.015807
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2014HE01      Chin.Phys.C 38, 024101 (2014)

C.-Y.He, X.-G.Wu, Y.Zheng, C.-B.Li, X.Fang

Description of the shape evolution in the yrast states of 186Pt

NUCLEAR STRUCTURE 186Pt; calculated E(4+)/E(2+), B(E2), Routhian surfaces. IBM-1 and X(3) models, comparison with experimental data.

doi: 10.1088/1674-1137/38/2/024101
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2013CU04      Phys.Rev. C 88, 064309 (2013)

N.Curtis, S.Almaraz-Calderon, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, X.Fang, M.Freer, G.Goldring, F.Jung, S.R.Lesher, W.Lu, J.D.Malcolm, A.Roberts, W.P.Tan, C.Wheldon, V.A.Ziman

Investigation of the 4α linear chain state in 16O

NUCLEAR REACTIONS 12C(α, 8Be)8Be, (α, 12C), [12C* decaying to 8Be+α], E=12.2-20.0 MeV; measured Eα, Iα, α(θ), αα-coin, σ(E, θ) at Notre Dame FN tandem facility. Phase shift analysis of σ(θ) data. 16O; deduced levels, resonances, J. Comparison with previous experimental results. No evidence found for rigid, 4α-linear chain in 16O.

doi: 10.1103/PhysRevC.88.064309
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Data from this article have been entered in the XUNDL database. For more information, click here.


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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2013KO15      Phys.Rev. C 87, 057309 (2013)

Tz.Kokalova, M.Freer, N.Curtis, N.I.Ashwood, M.Barr, J.D.Malcolm, C.Wheldon, V.A.Ziman, S.Almaraz-Calderon, A.Aprahamian, B.Bucher, M.Couder, X.Fang, F.Jung, W.Lu, A.Roberts, W.P.Tan, P.Copp, S.R.Lesher

Yield measurements for resonances above the multi-α threshold in 20Ne

NUCLEAR REACTIONS 16O(α, X), E=23.0-29.0 MeV; measured α and particle spectra, (particle)(particle)α-coin, yields for 8Be+8Be+α, and 8Be+12C(second 0+) channels. Measurements at Notre Dame facility. 20Ne; deduced levels, resonances, J. Monte Carlo simulations.

doi: 10.1103/PhysRevC.87.057309
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Data from this article have been entered in the XUNDL database. For more information, click here.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2046.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2026.


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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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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2012CU04      J.Phys.:Conf.Ser. 381, 012079 (2012)

N.Curtis, S.Almaraz-Calderon, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, X.Fang, M.Freer, G.Goldring, F.Jung, S.R.Lesher, W.Lu, J.D.Malcolm, A.Roberts, W.P.Tan, C.Wheldon, V.A.Ziman

Does a 4-α linear chain exist in 16O?

NUCLEAR REACTIONS 12C(α, 8Be), E=12.2-20.0 MeV; measured Eα, Iα from 8Be decay using DSSSD; deduced σ(θ=900), doublet 6+ resonance and its components.

doi: 10.1088/1742-6596/381/1/012079
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2012FR11      J.Phys.:Conf.Ser. 381, 012009 (2012)

M.Freer, S.Almaraz-Calderon, J.Carter, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, N.Curtis, X.Fang, F.Jung, S.Lesher, W.Lu, J.D.Malcolm, A.Roberts, R.Smit, W.P.Tan, C.Wheldon, V.A.Ziman

Simplicity from Complexity

doi: 10.1088/1742-6596/381/1/012009
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1785.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1785.


2011FR02      Phys.Rev. C 83, 034314 (2011)

M.Freer, S.Almaraz-Calderon, A.Aprahamian, N.I.Ashwood, M.Barr, B.Bucher, P.Copp, M.Couder, N.Curtis, X.Fang, F.Jung, S.Lesher, W.Lu, J.D.Malcolm, A.Roberts, W.P.Tan, C.Wheldon, V.A.Ziman

Evidence for a new 12C state at 13.3 MeV

NUCLEAR REACTIONS 9Be, 12C(α, 3α), E=22-30 MeV; measured Eα, Iα, 12C-α angular correlations; deduced Dalitz plot. 12C; deduced levels, J, π, width. Possible collective excitation of Hoyle state.

doi: 10.1103/PhysRevC.83.034314
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2011LI18      Chin.Phys.Lett. 28, 052102 (2011)

E.-T.Li, Z.-H.Li, J.Su, B.Guo, Y.-J.Li, S.-Q.Yan, X.-X.Bai, Y.-B.Wang, B.-X.Wang, G.Lian, S.Zeng, X.Fang, W.-J.Zhao, W.-P.Liu

Astrophysical Rates for the 6He(p, γ)7Li Reaction

NUCLEAR REACTIONS 1H(6He, γ), 2H(6He, n), E(cm)=9.1 MeV; measured reaction products; deduced σ(θ), S-factors, temperature-dependent reaction rates. Comparison with DWBA analysis, REACLIB library.

doi: 10.1088/0256-307X/
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2010GU16      Phys.Rev. C 82, 034318 (2010)

J.-Y.Guo, X.-Z.Fang, P.Jiao, J.Wang, B.-M.Yao

Application of the complex scaling method in relativistic mean-field theory

NUCLEAR STRUCTURE 120Sn; calculated energies and widths of low-lying single-neutron resonant states using complex scaling method (CSM) in the framework of relativistic mean field (RMF) model. Comparison with results from real stabilization method, the scattering phase-shift method, and the analytic continuation in the coupling constant approach.

doi: 10.1103/PhysRevC.82.034318
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2010GU18      Phys.Rev. C 82, 047301 (2010)

J.-Y.Guo, P.Jiao, X.-Z.Fang

Microscopic description of nuclear shape evolution from spherical to octupole-deformed shapes in relativistic mean-field theory

NUCLEAR STRUCTURE 210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246Th; calculated binding energies, β2, β3 and β4 deformation parameters, matter density distribution contours, and potential energy surfaces using relativistic mean-field (RMF) theory.

doi: 10.1103/PhysRevC.82.047301
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2010GU23      Eur.Phys.J. A 45, 179 (2010)

J.-Y.Guo, X.-Z.Fang

Research on the contributions from different fields of mesons and photons to pseudospin symmetry

doi: 10.1140/epja/i2010-10990-2
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2010JI02      Chin.Phys.Lett. 27, 032102 (2010)

S.-J.Jin, Y.-B.Wang, B.-X.Wang, X.-X.Bai, X.Fang, B.Guo, E.-T.Li, Y.-J.Li, Z.-H.Li, G.Lian, J.Su, s.-Q.Yan, S.Zeng, Z.-E.Yao, W.-P.Liu

Excited States in 18Ne Studied via 17F+p

NUCLEAR REACTIONS 1H(17F, α), (17F, γ), E=55.5 MeV; measured recoil nuclei, Eα, Iα; deduced σ(θ), excitation function, 18Ne resonance states, J, π.

doi: 10.1088/0256-307X/27/3/032102
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0065. Data from this article have been entered in the XUNDL database. For more information, click here.


2010LI19      Eur.Phys.J. A 44, 1 (2010)

Z.H.Li, E.T.Li, B.Guo, X.X.Bai, Y.J.Li, S.Q.Yan, Y.B.Wang, G.Lian, J.Su, B.X.Wang, S.Zeng, X.Fang, W.P.Liu

First measurement of the 2H(6He, 7Li)n angular distribution and proton spectroscopic factor in 7Li

NUCLEAR REACTIONS 2H(7Li, 6He)n, E=46 MeV; measured reaction products; deduced σ(θ), proton spectroscopic factor of 7Li ground state, optical potential parameters. Comparison with DWBA calculations.

doi: 10.1140/epja/i2010-10944-8
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0061. Data from this article have been entered in the XUNDL database. For more information, click here.


2010LI38      Nucl.Phys. A834, 661c (2010)

Z.H.Li, J.Su, B.Guo, E.T.Li, Z.C.Li, X.X.Bai, Y.J.Li, J.C.Liu, S.Q.Yan, B.X.Wang, Y.B.Wang, G.Lian, S.Zeng, X.Fang, W.P.Liu, Y.S.Chen, N.C.Shu, Q.W.Fan

2H(6He, 7Li)n, 12C(7Li, 6He)13N reactions and 12C(p, γ)13N astrophysical S(E) factors

NUCLEAR REACTIONS 2H(6He, 7Li), E not given; 12C(7Li, 6He), E=44.0 MeV; measured σ(θ); deduced 12C(p, γ) S-factor; calculated S-factor using DWBA and asymptotic normalization coefficient. Comparison with other data.

doi: 10.1016/j.nuclphysa.2010.01.117
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1785.


2010WA18      Nucl.Phys. A834, 100c (2010)

Y.B.Wang, B.X.Wang, S.J.Jin, X.Qin, X.X.Bai, W.P.Liu, Z.H.Li, G.Lian, S.Zeng, B.Guo, S.Q.Yan, J.Su, Y.J.Li, E.T.Li, X.Fang

Elastic resonance scattering of 13N+p and 17F+p

NUCLEAR REACTIONS 2H(12C, 13N), (16O, 17F), E not given; 1H(13N, 13N), (17F, 17F), E=47.8 MeV; measured reaction products, proton spectrum; 14O, 18Ne; deduced resonance parameters, J, π, σ(θ); R-matrix analysis.

doi: 10.1016/j.nuclphysa.2010.01.030
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2009HU19      Chin.Phys.C 33, Supplement 1, 148 (2009)

H.Hua, Z.-Y.Li, S.-Y.Wang, J.Meng, Z.-H.Li, X.-Q.Li, F.-R.Xu, H.-L.Liu, S.-Q.Zhang, S.-G.Zhou, Y.-L.Ye, D.-X.Jiang, T.Zheng, L.-H.Zhu, X.-G.Wu, G.-S.Li, C.-Y.He, L.-Y.Ma, F.Lu, F.-Y.Fan, L.-Y.Han, H.Wang, J.Xiao, X.-Q.Li, D.Chen, X.Fang, J.-L.Lou, Y.Liu, X.Hao, B.Pan, L.-H.Li

Structure change of 156Yb at high-spin states

NUCLEAR REACTIONS 144Sm(16O, 4n)156Yb, E=102 MeV; measured Eγ, Iγ, γ-γ-coin.; deduced high-spin states, level scheme, yrast states, J, π, energies.

doi: 10.1088/1674-1137/33/S1/047
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2009LI27      Chin.Phys.Lett. 26, 072401 (2009)

E.-T.Li, Z.-H.Li, Y.-J.Li, S.-Q.Yan, X.-X.Bai, B.Guo, J.Su, Y.-B.Wang, B.-X.Wang, G.Lian, S.Zeng, X.Fang, W.-J.Zhao, W.-P.Liu

Angular Distribution of the 12C(6He, 7Li)11B Reaction

NUCLEAR REACTIONS 12C(6He, 7Li), E = 34.6 MeV; measured σ(θ). comparison with DWBA calculation.

doi: 10.1088/0256-307X/26/7/072401
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2009ZH49      Chin.Phys.C 33, Supplement 1, 140 (2009)

L.-D.Zhang, J.-Y.Guo, X.-Z.Fang

With the alpha-cluster model to explain the change of separating energy

NUCLEAR STRUCTURE 4,6,8He, 6,8,10Li, 8,10,12Be, 10,12,14B, 12,14,16C, 14,16,18N, 16,18O, 18,20F; calculated separation energy of nn pair, two nn pairs, binding energy for Hydrogen isotopes.

doi: 10.1088/1674-1137/33/S1/044
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2008GU03      Int.J.Mod.Phys. E17, 539 (2008)

J.Y.Guo, X.Z.Fang, Z.Q.Sheng

Shape phase transitions and possible E(5) symmetry nuclei for Ti isotopes

NUCLEAR STRUCTURE 42,44,46,48,50,52,54,56,58,60,62,64Ti; calculated potential energy surfaces and ground state deformations using relativistic mean field theory.

doi: 10.1142/S0218301308009860
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2008LI23      Phys.Rev. C 77, 064323 (2008), Erratum Phys.Rev. C 106, 049901 (2022)

Z.Y.Li, H.Hua, S.Y.Wang, J.Meng, Z.H.Li, X.Q.Li, F.R.Xu, H.L.Liu, S.Q.Zhang, Y.L.Ye, D.X.Jiang, T.Zheng, L.Y.Ma, F.Lu, F.Y.Fan, L.Y.Han, H.Wang, J.Xiao, D.Chen, X.Fang, J.L.Lou, S.G.Zhou, L.H.Zhu, X.G.Wu, G.S.Li, C.Y.He, Y.Liu, X.Q.Li, X.Hao, B.Pan, L.H.Li

High-spin states in 156Yb and structure evolutions at large angular momenta in even-A Yb isotopes

NUCLEAR REACTIONS 144Sm(16O, 4n), E=102 MeV; measured Eγ, Iγ, γγ-coin, angular distributions. 156Yb; deduced levels, J, π, bands; calculated deformation parameters. 150,152,154,156,158,160,162,164,166,168,170Dy, 152,154,156,158,160,162,164,166,168,170,172Er, 154,156,158,160,162,164,166,168,170,172,174Yb, 156,158,160,162,164,166,168,170,172,174,176,178,180Hf; discussed level systematics. Comparison with cranked Woods-Saxon-Strutinsky model.

doi: 10.1103/PhysRevC.77.064323
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2006GU19      Phys.Rev. C 74, 024320 (2006)

J.Y.Guo, X.Z.Fang

Isospin dependence of pseudospin symmetry in nuclear resonant states

NUCLEAR STRUCTURE Sn; A=108-168; calculated single-particle resonant states energies and widths, energy splitting for pseudospin and spin-orbit doublets. 108,118,128,138,148,158,168Sn; calculated neutron potentials. Relativistic mean-field theory, analytic continuation of the coupling constant method.

doi: 10.1103/PhysRevC.74.024320
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2005GU23      Nucl.Phys. A757, 411 (2005)

J.-Y.Guo, X.-Z.Fang, F.-X.Xu

Pseudospin symmetry in the relativistic harmonic oscillator

NUCLEAR STRUCTURE 208Pb; calculated neutron single-particle levels, pseudospin symmetry features. Relativistic harmonic oscillator, Dirac equation.

doi: 10.1016/j.nuclphysa.2005.04.017
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2005GU35      Phys.Rev. C 72, 054319 (2005)

J.-Y.Guo, R.-D.Wang, X.-Z.Fang

Pseudospin symmetry in the resonant states of nuclei

NUCLEAR STRUCTURE 208Pb; calculated resonant states energies, pseudospin splitting.

doi: 10.1103/PhysRevC.72.054319
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2001FA07      Chin.Phys.Lett. 18, 193 (2001)

X.-Z.Fang, T.-N.Ruan

Analysis of the Yrast Bands with q-Deformed Moment of Inertia

NUCLEAR STRUCTURE 156Gd, 162,164Dy, 164,166Er, 168,170,172,174,176Yb, 170,172,174,176,178Hf, 228,230,232Th, 236,238U, 236,238,240,242,244Pu, 248Cm; calculated yrast rotational band parameters. Comparisons with data.

doi: 10.1088/0256-307X/18/2/313
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1994FA01      Phys.Rev. C49, R608 (1994)

X.S.Fang, C.M.Ko, G.Q.Li, Y.M.Zheng

Medium Effects on Subthreshold Kaon Production in Heavy-Ion Collisions

NUCLEAR REACTIONS 197Au(197Au, X), E=1 GeV/nucleon; analyzed kaon production σ(θ) vs momentum. Relativistic transport model, kaon degrees of freedom.

doi: 10.1103/PhysRevC.49.R608
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1994FA08      Nucl.Phys. A575, 766 (1994)

X.S.Fang, C.M.Ko, G.Q.Li, Y.M.Zheng

The Relativistic Transport Model Description of Subthreshold Kaon Production in Heavy-Ion Collisions

NUCLEAR REACTIONS 197Au(197Au, X), E=1 GeV/nucleon; calculated kaon production σ, momentum spectra. Relativistic transport model.

doi: 10.1016/0375-9474(94)90165-1
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1994LI02      Phys.Rev. C49, 1139 (1994)

G.Q.Li, C.M.Ko, X.S.Fang, Y.M.Zheng

Subthreshold Antiproton Production in Nucleus-Nucleus Collisions

NUCLEAR REACTIONS 28Si(28Si, p-barX), E=2.1 GeV/nucleon; calculated primordial p-bar production probability, differential momentum distribution. Relativistic transport model.

doi: 10.1103/PhysRevC.49.1139
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1994LI36      Phys.Lett. 329B, 149 (1994)

G.Q.Li, C.M.Ko, X.S.Fang

Subthreshold Antikaon Production in Nucleus-Nucleus Collisions

NUCLEAR REACTIONS 59Ni(58Ni, X), E=1.85 GeV/nucleon; 197Au(197Au, X), E=1 GeV/nucleon; calculated anti-kaon production σ. Relativistic transport model, anti-kaon degree of freedom.

doi: 10.1016/0370-2693(94)90752-8
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1991LI41      Chin.J.Nucl.Phys. 13, No 3, 223 (1991)

X.Li, X.Zhao, X.Fang

Equilibrium Deformation and Pairing Force in Light Nuclei

NUCLEAR STRUCTURE 17,18O, 19F, 20,21Ne, 22,23Na, 24,25,26Mg, 27Al, 28,29Si; calculated equilibrium deformations; deduced pairing force role.


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Note: The following list of authors and aliases matches the search parameter X.Fang: , X.S.FANG, X.Z.FANG