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NSR database version of April 11, 2024.

Search: Author = M.B.Aufderheide

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2001GO25      Nucl.Instrum.Methods Phys.Res. A462, 545 (2001)

C.D.Goodman, M.Bhattacharya, M.B.Aufderheide, S.D.Bloom, P.Zupranski

Data Analysis Techniques for Extracting Gamow-Teller Strengths from 0° (p, n) Data

NUCLEAR REACTIONS ⁷Li, ¹³C, ²³Na(p, n), E=120, 160 MeV; analyzed neutron spectra; deduced Gamow-Teller matrix elements.

doi: 10.1016/S0168-9002(00)01317-6
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1996AU05      Phys.Rev. C53, 3139 (1996)

M.B.Aufderheide, S.D.Bloom, G.J.Mathews, D.A.Resler

Importance of (n, p) Reactions for Stellar Beta Decay Rates

NUCLEAR STRUCTURE ^54,56Mn, ⁵⁸Co, ⁵⁹Fe; calculated Gamow-Teller resonances; deduced newly calibrated stellar β-decay rates related features. Data from (n, p) reactions considered.

doi: 10.1103/PhysRevC.53.3139
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1996RE06      Phys.Rev. C53, 2505 (1996)

M.T.Ressell, G.J.Mathews, M.B.Aufderheide, S.D.Bloom, D.A.Resler

Strange Neutral Currents in Nuclei

NUCLEAR STRUCTURE ^{50,52,54,56,58,60,62,64,66}Fe, ⁵⁶Ni, ²⁸Si, ²⁴Mg, ²⁰Ne, ¹⁴N, ¹²C; calculated total neutral current Gamow-Teller transition strength change, strength function. Shell model, finite contribution from polarized strange quark sea.

doi: 10.1103/PhysRevC.53.2505
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1994AU01      Phys.Rev. C49, 678 (1994)

M.B.Aufderheide, S.D.Bloom, D.A.Resler, C.D.Goodman

Comparison of Gamow-Teller Strength in ³⁷Ar and ³⁷K and ³⁷Cl Neutrino Cross Sections

NUCLEAR STRUCTURE ³⁷Ar; analyzed Gamow-Teller transition strength; deduced ³⁷Cl(ν, X) reaction σ for solar, supernova, μ⁺-decay neutrinos. ³⁷K level deduced β^--delayed proton emission suppression features. Shell model.

doi: 10.1103/PhysRevC.49.678
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1993AU02      Phys.Rev. C47, 2961 (1993)

M.B.Aufderheide, S.D.Bloom, D.A.Resler, G.J.Mathews

Implications of the Recent ⁵⁹Co(n, p)⁵⁹Fe Experiment for Stellar Electron Capture Rates

NUCLEAR REACTIONS ⁵⁹Co(p, n), E not given; calculated Gamow-Teller transition strength; deduced stellar electron capture rate (in ⁵⁹Co) implications. Shell model.

NUCLEAR STRUCTURE ⁵⁹Co, ⁵⁹Fe; calculated levels. ⁶⁰Co; calculated Gamow-Teller transition strengths. ^59,60Co; calculated stellar electron capture rate vs temperature. Shell model.

doi: 10.1103/PhysRevC.47.2961
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1993AU06      Phys.Rev. C48, 1677 (1993)

M.B.Aufderheide, S.D.Bloom, D.A.Resler, G.J.Mathews

Shell-Model Calculations of Gamow-Teller Strength in ⁵¹V, ⁵⁴Fe, and ⁵⁹Co

NUCLEAR REACTIONS ⁵¹V, ⁵⁴Fe, ⁵⁹Co(p, n), (n, p), E not given; calculated normalized Gamow-Teller transition strength; deduced quenching reaction dependence. Shell model.

doi: 10.1103/PhysRevC.48.1677
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1993RE14      Phys.Rev. D48, 5519 (1993)

M.T.Ressell, M.B.Aufderheide, S.D.Bloom, K.Griest, G.J.Mathews, D.A.Resler

Nuclear Shell Model Calculations of Neutralino-Nucleus Cross Sections for ²⁹Si and ⁷³Ge

NUCLEAR REACTIONS ²⁹Si, ⁷³Ge(X, X), E not given; calculated neutralino scattering matrix elements; deduced non-nuclear uncertainities. Shell model target wave functions.

NUCLEAR STRUCTURE ²⁹Si, ⁷³Ge; calculated levels, spectroscopic factors, g factors. Shell model target wave functions.

doi: 10.1103/PhysRevD.48.5519
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1992AU05      Phys.Rev. C46, 2251 (1992)

M.B.Aufderheide, S.D.Bloom, D.A.Resler, C.D.Goodman

Gamow-Teller Strength in A = 37 Nuclei

NUCLEAR STRUCTURE A=37; analyzed Gamow-Teller transition strength from ³⁷Ca(β⁺) decay, ³⁷Cl(p, n) reaction data; deduced branching ratios sum possible values range, relevance to solar, supernova ν σ of ³⁷Cl.

doi: 10.1103/PhysRevC.46.2251
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1992GO13      Phys.Rev.Lett. 69, 2445 (1992)

C.D.Goodman, M.B.Aufderheide, S.D.Bloom, D.A.Resler

Comment on ' Is the Weak Axial-Vector Current Renormalized in Nuclei ( Question ) '

NUCLEAR STRUCTURE ³⁷K, ³⁷Ar; analyzed Gamow-Teller transition strength data; deduced β-decay, (p, n) reaction probe consistency evidence.

doi: 10.1103/PhysRevLett.69.2445
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1991AU01      Nucl.Phys. A526, 161 (1991)

M.B.Aufderheide

Stellar Electron Capture Rates and the ⁵⁴Fe(n, p) Experiment

NUCLEAR REACTIONS ⁵⁴Fe(n, p), E=200 MeV; analyzed data. ^54,55Fe, ⁵³Mn, ^59,60Co deduced stellar electron capture rate limits.

doi: 10.1016/0375-9474(91)90304-O
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