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NSR database version of April 27, 2024.

Search: Author = E.B.Deleeuw

Found 2 matches.

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2019WO01      Phys.Rev.Lett. 122, 232701 (2019)

C.Wolf, C.Langer, F.Montes, J.Pereira, W.-J.Ong, T.Poxon-Pearson, S.Ahn, S.Ayoub, T.Baumann, D.Bazin, P.C.Bender, B.A.Brown, J.Browne, H.Crawford, R.H.Cyburt, E.Deleeuw, B.Elman, S.Fiebiger, A.Gade, P.Gastis, S.Lipschutz, B.Longfellow, Z.Meisel, F.M.Nunes, G.Perdikakis, R.Reifarth, W.A.Richter, H.Schatz, K.Schmidt, J.Schmitt, C.Sullivan, R.Titus, D.Weisshaar, P.J.Woods, J.C.Zamora, R.G.T.Zegers

Constraining the Neutron Star Compactness: Extraction ²³Al(p, γ) Reaction Rate for the rp Process

NUCLEAR REACTIONS ²H(²³Al, n), E=48 MeV/nucleon; measured reaction products, En, In, Eγ, Iγ; deduced J, π, σ, σ(θ), resonance widths and spectroscopic strengths, reaction rates.

doi: 10.1103/PhysRevLett.122.232701
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2458. Data from this article have been entered in the XUNDL database. For more information, click here.

2017ON01      Phys.Rev. C 95, 055806 (2017)

W.-J.Ong, C.Langer, F.Montes, A.Aprahamian, D.W.Bardayan, D.Bazin, B.A.Brown, J.Browne, H.Crawford, R.Cyburt, E.B.Deleeuw, C.Domingo-Pardo, A.Gade, S.George, P.Hosmer, L.Keek, A.Kontos, I.-Y.Lee, A.Lemasson, E.Lunderberg, Y.Maeda, M.Matos, Z.Meisel, S.Noji, F.M.Nunes, A.Nystrom, G.Perdikakis, J.Pereira, S.J.Quinn, F.Recchia, H.Schatz, M.Scott, K.Siegl, A.Simon, M.Smith, A.Spyrou, J.Stevens, S.R.Stroberg, D.Weisshaar, J.Wheeler, K.Wimmer, R.G.T.Zegers

Low-lying level structure of ⁵⁶Cu and its implications for the rp process

NUCLEAR REACTIONS ²H(⁵⁶Ni, ⁵⁶Cu), E AP 75 MeV/nucleon, [secondary ⁵⁶Ni beam from ⁹Be(⁵⁸Ni, X), E=160 MeV/nucleon primary reaction using A1900 separator at NSCL-MSU facility]; measured ΔE-TOF particle identification for ions, Eγ, Iγ, γγ-, (⁵⁶Cu ions)γ-coin using GRETINA array and S800 magnetic spectrograph. ⁵⁶Cu; deduced levels, J, π. Comparison with mirror nucleus ⁵⁶Co level scheme, and with shell-model calculations ⁵⁵Ni(p, γ)⁵⁶Cu, T₉=0.1-10; deduced Q value, astrophysical reaction rates as function of temperature, and impact on the r-process around ⁵⁶Ni.

NUCLEAR STRUCTURE ⁵⁶Cu; calculated levels, resonance energies, J, π, spectroscopic factors, Γ_p, Γ_γ using shell model with the GXPF1A interaction. Comparison with experimental data.

doi: 10.1103/PhysRevC.95.055806
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Data from this article have been entered in the XUNDL database. For more information, click here.

Note: The following list of authors and aliases matches the search parameter E.B.Deleeuw: , E.B.DELEEUW