NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = Tang Xuetian Found 48 matches. 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
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
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
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
2023WA36 Phys.Rev. C 108, 065805 (2023) Effective energy window of the E1 photon strength function for astrophysical neutron-capture reaction rates
doi: 10.1103/PhysRevC.108.065805
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
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
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
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
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
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
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
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
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
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
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
2014ZH27 Nucl.Instrum.Methods Phys.Res. B335, 85 (2014) 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
2011ES08 Phys.Rev. C 84, 064613 (2011) 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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
2001GA41 Nucl.Phys. A688, 536c (2001) C.A.Gagliardi, A.Azhari, V.Burjan, F.Carstoiu, V.Kroha, A.M.Mukhamedzhanov, X.Tang, L.Trache, R.E.Tribble Astrophysical S Factors Determined from Asymptotic Normalization Coefficients Measured in Peripheral Transfer Reactions NUCLEAR REACTIONS 10B, 14N(7Be, 8B), E=12 MeV/nucleon; measured σ(θ), asymptotic normalization coefficients. 7Be(p, γ), E=low; calculated S-factor from transfer reaction data. Comparison with other measurements. DWBA analysis.
doi: 10.1016/S0375-9474(01)00780-1
2001KR12 Czech.J.Phys. 51, 471 (2001) V.Kroha, P.Bem, V.Burjan, J.Novak, S.Piskor, E.Simeckova, J.Vincour, A.Azhari, C.A.Gagliardi, A.M.Mukhamedzhanov, X.Tang, L.Trache, R.E.Tribble, F.Carstoiu Asymptotic Normalization Constants in Nuclear Astrophysics NUCLEAR REACTIONS 16O(3He, d), E=29.7 MeV; 13C(3He, d), E=26.3 MeV; measured σ(E, θ). 13C(14N, 14N), (14N, 13C), E ≈ 162 MeV; 9Be(10B, 10B), (10B, 9Be), E=100 MeV; analyzed σ(θ). 16O(p, γ), E ≈ 0.2-1.2 MeV; deduced S-factors. 9Be, 13C(p, γ), E=low; deduced asymptotic normalization constants, S-factors.
doi: 10.1023/A:1017504100371
1999AZ04 Phys.Rev. C60, 055803 (1999) A.Azhari, V.Burjan, F.Carstoiu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, X.Tang, L.Trache, R.E.Tribble The 14N(7Be, 8B)13C Reaction and the 7Be(p, γ)8B S Factor NUCLEAR REACTIONS 14N(7Be, 8B), E=85 MeV; measured σ(E), σ(θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E not given; deduced astrophysical S-factor. 14N(7Be, 7Be), E=85 MeV; measured σ(θ).
doi: 10.1103/PhysRevC.60.055803
1999TR12 Pramana 53, 585 (1999) R.E.Tribble, A.Azhari, H.L.Clark, C.A.Gagliardi, Y.-W.Lui, A.M.Mukhamedzhanov, A.Sattaroy, X.Tang, L.Trache, V.Burjan, J.Cejpek, V.Kroha, S.Piskor, J.Vincour, F.Carstoiu Astrophysical S-Factors from Asymptotic Normalization Coefficients
doi: 10.1007/s12043-999-0035-6
1997LI05 Nucl.Phys. A616, 131c (1997) W.Liu, X.Bai, S.Zhou, Z.Ma, Z.Li, Y.Wang, A.Li, Z.Ma, B.Chen, X.Tang, Y.Han, Q.Shen, J.Xu Measurement of the Angular Distribution for the 7Be(d, n)8B Reaction and Determination of the Astrophysical S Factor for the 7Be(p, γ)8B Reaction NUCLEAR REACTIONS, ICPND 7Be(d, n), E(cm)=5.8 MeV; measured σ(θ), reaction σ; deduced 7Be(p, γ) reaction astrophysical S-factor, model parameters.
doi: 10.1016/S0375-9474(97)00082-1
1996LI12 Phys.Rev.Lett. 77, 611 (1996) W.Liu, X.Bai, S.Zhou, Z.Ma, Z.Li, Y.Wang, A.Li, Z.Ma, B.Chen, X.Tang, Y.Han, Q.Shen Angular Distribution for the 7Be(d, n)8B Reaction at E(c.m.) = 5.8 MeV and the S17(0) Factor for the 7Be(p, γ)8B Reaction NUCLEAR REACTIONS, ICPND 2H(7Be, n), E(cm)=5.8 MeV; measured σ(θ); deduced astrophysical S-factor for 7Be(p, γ). DWBA analysis.
doi: 10.1103/PhysRevLett.77.611
1993TA25 Chin.Phys.Lett. 10, 209 (1993) A Nuclear Detector Using Scanning Tunneling Microscopy
doi: 10.1088/0256-307X/10/4/005
1992TA23 Chin.Phys.Lett. 9, 508 (1992) X.Tang, Y.Wu, S.Zhang, Q.Chen, X.Xie New Upper Limit of γ-Rays Emitted by Tritium Nucleus RADIOACTIVITY 3H(β-); measured γ-ray energy distribution; deduced upper limit for Eγ. Low background hyperpure Ge detector.
1985TA26 Chin.J.Nucl.Phys. 7, 263 (1985) Tang Xuetian, Gao Liangjun, Tian Ye Generalization of the Goldhaber Theory NUCLEAR STRUCTURE 11C, 19O; calculated momentum distribution widths. Generalized Goldhaber theory.
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