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NSR database version of April 11, 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 ²⁶Al_g.s. from the ¹⁶O(¹⁶O, x)²⁶Al_g.s. and ¹⁶O(¹⁴N, x)²⁶Al_g.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
Citations: PlumX Metrics
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

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