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NSR database version of May 24, 2024.

Search: Author = D.N.Binh

Found 13 matches.

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2018KA11      Phys.Rev. C 97, 015802 (2018)

D.Kahl, H.Yamaguchi, S.Kubono, A.A.Chen, A.Parikh, D.N.Binh, J.Chen, S.Cherubini, N.N.Duy, T.Hashimoto, S.Hayakawa, N.Iwasa, H.S.Jung, S.Kato, Y.K.Kwon, S.Nishimura, S.Ota, K.Setoodehnia, T.Teranishi, H.Tokieda, T.Yamada, C.C.Yun, L.Y.Zhang

First measurement of 30S + α resonant elastic scattering for the 30S(α, p) reaction rate

NUCLEAR REACTIONS 4H(30S, α), E(cm)=1.9-5.5 MeV, [30S secondary beam from 3He(28Si, 30S), E=7.3 MeV/nucleon]; measured Eα, Iα, differential σ(E) using an array of silicon strip detectors (SSDs), and parallel plate avalanche counters (PPACs) for monitoring the 30S beam, ΔE-E plot for light ion particle using the CNS Radioactive Ion Beam separator (CRIB) facility, University of Tokyo, and RIKEN. 34Ar; deduced levels above 11 MeV, α-resonances, J, π, α-widths, proton-width. R-matrix analysis. 30s(α, p), T=1-10 GK; deduced stellar reaction rate using new resonance data, and compared with statistical model (SM) calculations from NON-SMOKER code. Astrophysical impact on one-zone postprocessing type I x-ray burst (XRBs) calculations.

doi: 10.1103/PhysRevC.97.015802
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2583. Data from this article have been entered in the XUNDL database. For more information, click here.


2016HA19      Phys.Rev. C 93, 065802 (2016)

S.Hayakawa, S.Kubono, D.Kahl, H.Yamaguchi, D.N.Binh, T.Hashimoto, Y.Wakabayashi, J.J.He, N.Iwasa, S.Kato, T.Komatsubara, Y.K.Kwon, T.Teranishi

First direct measurement of the 11C(α, p)14N stellar reaction by an extended thick-target method

NUCLEAR REACTIONS 4He(11C, p)14N, E(cm)=1.3-4.5 MeV, [11C secondary beam from 1H(11B, n) primary reaction, E=4.6 MeV/nucleon, using CRIB at RIKEN AVF cyclotron]; measured Ep, Ip, time of flight of protons for (α, p0), (α, p1), and (α, p2) transitions, energy loss of 11C beam in 4He gas, σ(E, θ) for p0, p1 and p2 by geometrically-extended thick-target inverse-kinematics method; deduced astrophysical S factors and reaction rates for p0, p1 and p2. Comparison

doi: 10.1103/PhysRevC.93.065802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2516.


2015CH41      Phys.Rev. C 92, 015805 (2015)

S.Cherubini, M.Gulino, C.Spitaleri, G.G.Rapisarda, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, S.Kubono, H.Yamaguchi, S.Hayakawa, Y.Wakabayashi, N.Iwasa, S.Kato, T.Komatsubara, T.Teranishi, A.Coc, N.de Sereville, F.Hammache, G.Kiss, S.Bishop, D.N.Binh

First application of the Trojan horse method with a radioactive ion beam: Study of the 18F(p, α)15O reaction at astrophysical energies

NUCLEAR REACTIONS 2H(18F, α15O), E=47.9 MeV, [18F secondary beam from 18O(p, n) primary reaction at CRIB-CNS-RIKEN facility]; measured Q-value spectra, σ for p-18F c.m. energy; deduced momentum distribution for the p-n intercluster motion in deuteron. 19Ne; deduced proton resonances, levels, J, π, and compared to previous experimental data and evaluations. 18F(p, α)15O, E<900 keV; deduced σ(E), astrophysical S(E) factor by Trojan horse method (THM) by considering interference effects.

doi: 10.1103/PhysRevC.92.015805
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2506. Data from this article have been entered in the XUNDL database. For more information, click here.


2015KI07      Phys.Rev. C 92, 035801 (2015)

A.Kim, N.H.Lee, M.H.Han, J.S.Yoo, K.I.Hahn, H.Yamaguchi, D.N.Binh, T.Hashimoto, S.Hayakawa, D.Kahl, T.Kawabata, Y.Kurihara, Y.Wakabayashi, S.Kubono, S.Choi, Y.K.Kwon, J.Y.Moon, H.S.Jung, C.S.Lee, T.Teranishi, S.Kato, T.Komatsubara, B.Guo, W.P.Liu, B.Wang, Y.Wang

Measurement of the 14O(α, p)17F cross section at Ec.m. ≈ 2.1-5.3MeV

NUCLEAR REACTIONS 4He(14O, p), E=2.5 MeV/nucleon, [secondary 14O beam from 1H(14N, n), E=8.4 MeV/nucleon primary reaction at RIBF-RIKEN]; measured E(p), I(p), pp-coin, energy distribution of single- and double-proton events, differential cross sections by thick target method. 18Ne; deduced levels, resonances, J, π, proton and α widths by R-matrix analysis, astrophysical reaction rates, strong single-proton decay events, but no strong double-proton events. Relevance to trigger reaction for the x-ray burst and nucleosynthesis of heavy nuclei up to Cd.

doi: 10.1103/PhysRevC.92.035801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2487. Data from this article have been entered in the XUNDL database. For more information, click here.


2014KO41      Eur.Phys.J. A 50, 136 (2014)

T.Komatsubara, S.Kubono, T.Hayakawa, T.Shizuma, A.Ozawa, Y.Ito, Y.Ishibashi, T.Moriguchi, H.Yamaguchi, D.Kahl, S.Hayakawa, D.N.Binh, A.A.Chen, J.Chen, K.Setoodehnia, T.Kajino

Excited states above the proton threshold in 26Si

doi: 10.1140/epja/i2014-14136-4
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Data from this article have been entered in the XUNDL database. For more information, click here.


2014MC08      Nucl.Data Sheets 120, 88 (2014)

E.Mcneice, K.Setoodehnia, B.Singh, Y.Abe, D.N.Binh, A.A.Chen, J.Chen, S.Cherubini, S.Fukuoka, T.Hashimoto, T.Hayakawa, Y.Ishibashi, Y.Ito, D.Kahl, T.Komatsubara, S.Kubono, T.Moriguchi, D.Nagae, R.Nishikiori, T.Niwa, A.Ozawa, T.Shizuma, H.Suzuki, H.Yamaguchi, T.Yuasa

In-beam γ-ray Spectroscopy of 30P via the 28Si(3He, pγ)30P Reaction

NUCLEAR REACTIONS 28Si(3He, p), E=9 MeV; measured reaction products, Eγ, Iγ, γ-γ-coin.; deduced level structure, J, π, resonance states, γ-γ directional correlation of oriented nuclei. Comparison with available data.

doi: 10.1016/j.nds.2014.07.014
Citations: PlumX Metrics

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


2013GU04      Phys.Rev. C 87, 015803 (2013)

B.Guo, J.Su, Z.H.Li, Y.B.Wang, S.Q.Yan, Y.J.Li, N.C.Shu, Y.L.Han, X.X.Bai, Y.S.Chen, W.P.Liu, H.Yamaguchi, D.N.Binh, T.Hashimoto, S.Hayakawa, D.Kahl, S.Kubono, J.J.He, J.Hu, S.W.Xu, N.Iwasa, N.Kume, Z.H.Li

Determination of the astrophysical 12N(p, γ)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications

NUCLEAR REACTIONS 2H(12N, 13O)1n, E=59 MeV; measured reaction products, energy loss, time-of-flight, differential σ(θ); deduced ANC, astrophysical S factors. 12N(p, γ)13O, at T9=0.3-3.0; deduced stellar reaction rate. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.87.015803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2405. Data from this article have been entered in the XUNDL database. For more information, click here.


2013SE08      Phys.Rev. C 87, 065801 (2013)

K.Setoodehnia, A.A.Chen, D.Kahl, T.Komatsubara, J.Jose, R.Longland, Y.Abe, D.N.Binh, J.Chen, S.Cherubini, J.A.Clark, C.M.Deibel, S.Fukuoka, T.Hashimoto, T.Hayakawa, J.Hendriks, Y.Ishibashi, Y.Ito, S.Kubono, W.N.Lennard, T.Moriguchi, D.Nagae, R.Nishikiori, T.Niwa, A.Ozawa, P.D.Parker, D.Seiler, T.Shizuma, H.Suzuki, C.Wrede, H.Yamaguchi, T.Yuasa

Nuclear structure of 30S and its implications for nucleosynthesis in classical novae

NUCLEAR REACTIONS 32S(p, t), E=34.5 MeV; measured triton spectra, σ(θ) using Enge split-pole magnetic spectrograph at WNSL, Yale facility. 28Si(3He, n), E=9 MeV; measured Eγ, Iγ, γγ-coin, γ(θ), γγ(θ)(DCO) at UTTAC facility. 30S; deduced levels, resonances, J, π, multipolarity, σ/J, mixing ratio, branching ratios, proton and gamma widths, resonance strengths. DWBA and coupled reaction channel analyses of σ(θ) data in (p, t). 29P(p, γ)30S, at T=0.01-1.5 GK; deduced astrophysical reaction rates, nova isotopic abundances of Si to Ca mass region isotopes using 1D hydrodynamic model.

doi: 10.1103/PhysRevC.87.065801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2040. Data from this article have been entered in the XUNDL database. For more information, click here.


2013YA04      Phys.Rev. C 87, 034303 (2013)

H.Yamaguchi, D.Kahl, Y.Wakabayashi, S.Kubono, T.Hashimoto, S.Hayakawa, T.Kawabata, N.Iwasa, T.Teranishi, Y.K.Kwon, D.N.Binh, L.H.Khiem, N.N.Duy

α-resonance structure in 11C studied via resonant scattering of 7Be+α and with the 7Be(α, p) reaction

NUCLEAR REACTIONS 4He(7Be, p)10B, 4He(7Be, α)7Be, 4He(7Be, α'), [7Be beam from 1H(7Li, n), E=5.0 MeV/nucleon], E=15.43 MeV; measured particle spectra, Eγ, Iγ, Ep, Eα, energy loss, αγ-, pγ-, 7Beαγ-coin, σ(E, θ) using CRIB facility at RIKEN. 11C; deduced levels, resonances, J, π, resonance parameters, proton and α widths, 2α+3He-cluster band. R-matrix analysis. 7Be(α, γ)11C, at T9>1.5; deduced resonant reaction rate. Comparison with previous studies.

doi: 10.1103/PhysRevC.87.034303
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2431. Data from this article have been entered in the XUNDL database. For more information, click here.


2012ZH21      Eur.Phys.J. A 48, 65 (2012)

G.L.Zhang, C.L.Zhang, H.Q.Zhang, C.J.Lin, D.Y.Pang, X.K.Wu, H.M.Jia, G.P.An, Z.D.Wu, X.X.Xu, F.Yang, Z.H.Liu, S.Kubono, H.Yamaguchi, S.Hayakawa, D.N.Binh, Y.K.Kwon, N.Iwasa, M.Mazzocco, M.La Commara, M.Romoli, C.Signorini

Quasi-elastic scattering of the proton drip line nucleus 17F on 12C at 60 MeV

NUCLEAR REACTIONS 12C(17F, 17F'), E=60 MeV; measured E(17F), I(17F, θ); deduced σ(θ), σ; calculated σ(θ) using optical model and CDCC; deduced parameters. Compared with data, also for nearby projectiles.

doi: 10.1140/epja/i2012-12065-x
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2377.


2011SE03      Phys.Rev. C 83, 018803 (2011)

K.Setoodehnia, A.A.Chen, T.Komatsubara, S.Kubono, D.N.Binh, J.F.Carpino, J.Chen, T.Hashimoto, T.Hayakawa, Y.Ishibashi, Y.Ito, D.Kahl, T.Moriguchi, H.Oishi, A.Ozawa, T.Shizuma, Y.Sugiyama, H.Yamaguchi

Spins and parities of astrophysically important 30S states from 28Si(3He, nγ )30S

NUCLEAR REACTIONS 28Si(3He, n), E=9 MeV; measured Eγ, Iγ, γγ-coin, natural Si target. 30S; deduced levels, J, π. Comparison with mirror nucleus 30Si. Astrophysical relevance to the reaction rates for 29P(p, γ).

doi: 10.1103/PhysRevC.83.018803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2040. Data from this article have been entered in the XUNDL database. For more information, click here.


2011YA02      Phys.Rev. C 83, 034306 (2011)

H.Yamaguchi, T.Hashimoto, S.Hayakawa, D.N.Binh, D.Kahl, S.Kubono, Y.Wakabayashi, T.Kawabata, T.Teranishi

α resonance structure in 11B studied via resonant scattering of 7Li+α

NUCLEAR REACTIONS 4He(7Li, 7Li), (7Li, 7Li'), (7Li, p), E=13.7 MeV; measured Eα, Iα, Ep, Et, Eγ, Iγ, γγ-coin, excitation functions, σ(E, θ), 11B; deduced levels, J, π, l-values, widths, resonance parameters, rotational band. R-matrix analysis of σ(E) data. 7Li(α, γ)11B, E=11.29, 12.63, 13.03 MeV; calculated reaction rates and comparison with NACRE evaluation. Relevance to 11B production in core-collapse supernovae.

doi: 10.1103/PhysRevC.83.034306
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2326. Data from this article have been entered in the XUNDL database. For more information, click here.


2010KU20      Nucl.Phys. A834, 647c (2010)

S.Kubono, D.N.Binh, S.Hayakawa, H.Hashimoto, D.Kahl, Y.Wakabayashi, H.Yamaguchi, T.Teranishi, N.Iwasa, T.Komatsubara, S.Kato, L.H.Khiem

Nuclear Clusters in Astrophysics

doi: 10.1016/j.nuclphysa.2010.01.113
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