NSR Query Results

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NSR database version of April 27, 2024.

Search: Author = E.J.Lingerfelt

Found 3 matches.

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2007MO20      Phys.Rev. C 75, 065801 (2007)

B.H.Moazen, D.W.Bardayan, J.C.Blackmon, K.Y.Chae, K.Chipps, C.P.Domizioli, R.Fitzgerald, U.Greife, W.R.Hix, K.L.Jones, R.L.Kozub, E.J.Lingerfelt, R.J.Livesay, C.D.Nesaraja, S.D.Pain, L.F.Roberts, J.F.Shriner, Jr., M.S.Smith, J.S.Thomas

Measurement of the 183 keV resonance in ¹⁷O(p, α)¹⁴N using a novel technique

NUCLEAR REACTIONS ¹H(¹⁷O, α)¹⁴N, E=3.3 MeV; measured resonance energy and strength. Discussed astrophysical implications.

doi: 10.1103/PhysRevC.75.065801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1567.

2006BA65      Phys.Rev. C 74, 045804 (2006)

D.W.Bardayan, J.A.Howard, J.C.Blackmon, C.R.Brune, K.Y.Chae, W.R.Hix, M.S.Johnson, K.L.Jones, R.L.Kozub, J.F.Liang, E.J.Lingerfelt, R.J.Livesay, S.D.Pain, J.P.Scott, M.S.Smith, J.S.Thomas, D.W.Visser

Astrophysically important ²⁶Si states studied with the ²⁸Si(p, t)²⁶Si reaction. II. Spin of the 5.914-MeV ²⁶Si level and galactic ²⁶Al production

NUCLEAR REACTIONS ²⁸Si(p, t), (p, d), E=40 MeV; measured particle spectra, angular distributions. ²⁶Si level deduced J, π. ²⁵Al(p, γ), E=low; deduced astrophysical reaction rate.

doi: 10.1103/PhysRevC.74.045804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1509. Data from this article have been entered in the XUNDL database. For more information, click here.

2004SM09      Nucl.Phys. A746, 569c (2004)

M.S.Smith, R.A.Meyer, D.W.Bardayan, J.C.Blackmon, K.Chae, M.W.Guidry, W.R.Hix, R.L.Kozub, E.J.Lingerfelt, Z.Ma, J.P.Scott

Nuclear data on unstable nuclei for astrophysics

doi: 10.1016/j.nuclphysa.2004.09.092
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