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NSR database version of May 24, 2024.

Search: Author = K.Yildiz

Found 7 matches.

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1999YI01      Phys.Rev. C60, 028801 (1999)

K.O.Yildiz, N.P.T.Bateman, Y.M.Butt, A.A.Chen, K.B.Swartz, P.D.Parker

Thick Target Yields of 26Alg.s. from the 16O(16O, x)26Alg.s. and 16O(14N, x)26Alg.s. Reactions

NUCLEAR REACTIONS 16O(16O, X)26Al, E=80-150 MeV; 16O(14N, X)26Al, E=115 MeV; measured thick target yields; deduced production of 26Al in proto-solar nebula. Previous measurements included in analysis. Comparison with model predictions.

doi: 10.1103/PhysRevC.60.028801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1235.

1998BA19      Phys.Rev. C57, 2022 (1998)

N.P.T.Bateman, D.W.Bardayan, Y.M.Butt, A.A.Chen, K.O.Yildiz, B.M.Young, P.D.Parker

Thick Target Yield of 26Al from the 12C(16O, x)26Al(g.s.) Reaction

NUCLEAR REACTIONS 12C(16O, X)26Al, E=45, 65, 140 MeV; measured thick target yield; deduced σ. Activation method.

doi: 10.1103/PhysRevC.57.2022
Citations: PlumX Metrics

1998UT02      Phys.Rev. C57, 2731 (1998); Erratum Phys.Rev. C58, 1354 (1998)

S.Utku, J.G.Ross, N.P.T.Bateman, D.W.Bardayan, A.A.Chen, J.Gorres, A.J.Howard, C.Iliadis, P.D.Parker, M.S.Smith, R.B.Vogelaar, M.Wiescher, K.Yildiz

Breakout from the Hot CNO Cycle: The 18F(p, γ) vs 18F(p, α) branching ratio

NUCLEAR REACTIONS 19F(3He, t), (3He, tα), (3He, pt), E=29.8 MeV; 16O(6Li, t), (6Li, 3He), E=32 MeV; measured particle spectra, tp-, tα-coin; deduced reaction rates for 18F + p. 19F deduced levels, resonance features. Astrophysical implications.

doi: 10.1103/PhysRevC.57.2731
Citations: PlumX Metrics

1997BA51      Nucl.Phys. A621, 60c (1997)

N.P.T.Bateman, D.W.Bardayan, Y.M.Butt, A.A.Chen, K.O.Yildiz, B.M.Young, P.D.Parker, A.E.Champagne

The Production of 26Al in the Early Solar System by Oxygen Rich Cosmic Rays

NUCLEAR REACTIONS 12C(16O, X)26Al, E=45, 65, 140 MeV; measured residual decay associated βγ(t); deduced residual yield, astrophysical consequences.

doi: 10.1016/S0375-9474(97)00213-3
Citations: PlumX Metrics

1997MA60      J.Phys.(London) G23, 1215 (1997)

J.C.Mahon, L.L.Lee, Jr., J.F.Liang, C.R.Morton, N.T.P.Bateman, K.Yildiz, B.M.Young

Fusion and Transfer in 37Cl + 98,100Mo, 93Nb at Near Barrier Energies

NUCLEAR REACTIONS, ICPND 100Mo(37Cl, X), E=118.1, 121.8, 125.1; measured σ(θ) for one-, two-proton stripping; deduced transfer form factors. 93Nb, 92,98,100Mo(37Cl, X), E(cm)=82-95 MeV; 93Nb, 92,98,100Mo(32S, X), E(cm)=78-90 MeV; measured fusion σ; deduced sub-barrier enhancement.

doi: 10.1088/0954-3899/23/10/008
Citations: PlumX Metrics

1996HA26      Phys.Rev. C54, 1999 (1996)

K.I.Hahn, A.Garcia, E.G.Adelberger, P.V.Magnus, A.D.Bacher, N.Bateman, G.P.A.Berg, J.C.Blackmon, A.E.Champagne, B.Davis, A.J.Howard, J.Liu, B.Lund, Z.Q.Mao, D.M.Markoff, P.D.Parker, M.S.Smith, E.J.Stephenson, K.B.Swartz, S.Utku, R.B.Vogelaar, K.Yildiz

Structure of 18Ne and the Breakout from the Hot CNO Cycle

NUCLEAR REACTIONS, ICPND 12C(12C, 6He), E=80 MeV; 16O(3He, n), E=10.9-14.5 MeV; 20Ne(p, t), E=44, 88 MeV; measured σ(θ). 18Ne deduced levels, Γ, J, π. 14O(α, p), E(cm) ≤ 2.5 MeV; calculated astrophysical S-factor vs E, astrophysical reaction rate vs temperature.

doi: 10.1103/PhysRevC.54.1999
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1144.

1995HO25      Nucl.Instrum.Methods Phys.Res. B99, 346 (1995)

M.A.Hofstee, J.C.Blackmon, A.E.Champagne, N.P.T.Bateman, P.D.Parker, K.Yildiz, B.M.Young, R.B.Vogelaar, M.S.Smith, A.J.Howard

Investigating the Astrophysically Important E(x) = 2.646 MeV State in 20Na

NUCLEAR REACTIONS 20Ne(3He, t), E=27 MeV; measured triton spectra, tγ-coin. 20Na level deduced Γγ/Γ.

doi: 10.1016/0168-583X(95)00307-X
Citations: PlumX Metrics

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Note: The following list of authors and aliases matches the search parameter K.Yildiz: , K.O.YILDIZ