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NSR database version of April 27, 2024.

Search: Author = K.O.Yildiz

Found 3 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
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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
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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
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