NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = C.Iliadis Found 94 matches. 2023IL01 Phys.Rev. C 107, 044610 (2023) Laboratory electron screening in nuclear resonance reactions NUCLEAR REACTIONS 17O(p, γ), E(cm)=64.5 keV;18O(p, γ), (p, α), E(cm)=90 keV;22Ne(p, γ), E=149.4 keV;25Mg(p, γ), E(cm)=92.2 keV;27Al(p, γ), E(cm)=956 keV;176Lu(p, n), E=805 keV; calculated electron screening factors, lengths, and potentials for narrow resonances, shift in resonance energy caused by electron screening for the case of 27Al(p, γ) and 176Lu(p, n) reactions. Comparison to the values derived from the published data.
doi: 10.1103/PhysRevC.107.044610
2022DO04 Phys.Rev. C 105, 055804 (2022) L.N.Downen, C.Iliadis, A.E.Champagne, T.B.Clegg, A.Coc, J.Dermigny Thermonuclear reaction rate of 29Si(p, γ)30P NUCLEAR REACTIONS 29Si(p, γ), E(cm)=200-420 keV; measured Eγ, Iγ, γγ-coin; deduced resonance energies, resonance strengths. 30P; deduced levels, J, π, branching ratios. 29Si(p, γ), T=0.01-5.0 GK; deduced total thermonuclear reaction rates. Investigated the influence of possibly unobserved resonances on the reaction rates. Comparison to other experimental data. HPGe detector surrounded by a 16-segment NaI(Tl) annulus comprising LENA γγ-coincidence spectrometer at TUNL.
doi: 10.1103/PhysRevC.105.055804
2022GR04 Phys.Rev. C 106, 014308 (2022) D.Gribble, C.Iliadis, R.V.F.Janssens, U.Friman-Gayer, Krishichayan, S.Finch Investigation of 11B and 40Ca levels at 8-9 MeV by nuclear resonance fluorescence NUCLEAR REACTIONS 11B, 40Ca(polarized γ, γ'), E=8-9 MeV nearly monoenergetic and linearly polarized photon beams from the HIγS facility at TUNL; measured Eγ, Iγ, γ(θ, pol) using three HPGe detectors. 11B, 40Ca; deduced levels, J, π, polarization asymmetries, and branching ratios. 11B; analyzed γ-ray multipolarity mixing ratios using (polarized γ, γ') data from the present experiment and those from 2009Ru04: Phys. Rev. C 79, 047601. Discussed relationship of different phase conventions in nuclear resonance fluorescence (NRF) experiments.
doi: 10.1103/PhysRevC.106.014308
2022IL04 Phys.Rev. C 106, 055802 (2022) C.Iliadis, V.Palanivelrajan, R.S.de Souza Bayesian estimation of the S factor and thermonuclear reaction rate for 16O(p, γ)17F NUCLEAR REACTIONS 16O(p, γ), E=0.002-2.5 MeV; analyzed data from several studies, analyzed S-factors by Bayesian R-matrix fit; calculated astrophysical S-factor, thermonuclear astrophysical reaction rates (range 0.003-3.5 GK). R-matrix approximation with Bayesian model. Single-particle model employing a Woods-Saxon potential.
doi: 10.1103/PhysRevC.106.055802
2022LO05 Phys.Rev. C 105, L042801 (2022) G.Lotay, D.T.Doherty, R.V.F.Janssens, D.Seweryniak, H.M.Albers, S.Almaraz-Calderon, M.P.Carpenter, A.E.Champagne, C.J.Chiara, C.R.Hoffman, C.Iliadis, A.Kankainen, T.Lauritsen, S.Zhu Revised decay properties of the key 93-keV resonance in the 25Mg(p, γ) reaction and its influence on the MgAl cycle in astrophysical environments NUCLEAR REACTIONS 11B(16O, n), E=19 MeV; measured Eγ, Iγ, γ(θ), γγγ-coin. 26Al; deduced levels J, π, branchings. Obtained ground state branching for 93-keV resonance of 25Mg+p system which corresponds to 6398 keV level in 26Al. Comparison to other experimental data. Discussed impact on the production of cosmic γ rays. Gammasphere array with 99 detectors at ATLAS accelerator (ANL).
doi: 10.1103/PhysRevC.105.L042801
2021IL01 Eur.Phys.J. A 57, 190 (2021) Linear polarization-direction correlations in γ-ray scattering experiments
doi: 10.1140/epja/s10050-021-00472-1
2021MO31 Astrophys.J. 923, 49 (2021) J.Moscoso, R.S.de Souza, A.Coc, C.Iliadis Bayesian Estimation of the D(p, γ)3He Thermonuclear Reaction Rate NUCLEAR REACTIONS 2H(p, γ), E<1 MeV; analyzed available data; deduced S-factor, reaction rates and their uncertainties.
doi: 10.3847/1538-4357/ac1db0
2020DE26 Phys.Rev. C 102, 014609 (2020) J.Dermigny, C.Iliadis, A.Champagne, R.Longland Thermonuclear reaction rate of 30Si (p, γ) 31P NUCLEAR REACTIONS 30Si(p, γ)31P, E=434.6, 501.1, 621.7 keV; measured Eγ, Iγ, γγ-coin using JN Van de Graaff electrostatic accelerator at LENA-TUNL facility; deduced γ-ray branching ratios for primary γ rays from the resonance states from singles and coincidence data, resonance strength, thermonuclear reaction rates in the T=0.01-10 GK range. Comparison with previous experimental results. Relevance to Mg-K anticorrelation observed in the globular cluster NGC 2419.
doi: 10.1103/PhysRevC.102.014609
2019DE03 Phys.Rev. C 99, 014619 (2019) R.S.de Souza, S.R.Boston, A.Coc, C.Iliadis Thermonuclear fusion rates for tritium + deuterium using Bayesian methods NUCLEAR REACTIONS 3H(d, n), E=5-270 keV; compiled data from several studies, analyzed S-factors by Bayesian R-matrix fit; calculated astrophysical S-factors using the single-level, two-channel approximation, marginalized posterior of the S-factor, S-factor normalization factors, densities for the electron screening potential, thermonuclear reaction rates for temperatures of 0.001 to 1.0 GK, and reactivities for kT=0.2 to 50.0 keV. R-matrix approximation with Bayesian model. Relevance to future commercial fusion reactors, and Big Bang nucleosynthesis.
doi: 10.1103/PhysRevC.99.014619
2019HU08 Phys.Rev. C 99, 045804 (2019) S.Hunt, C.Iliadis, A.Champagne, L.Downen, A.Cooper New measurement of the Elabα = 0.83 MeV resonance in 22Ne(α, γ)26Mg NUCLEAR REACTIONS 22Ne(α, γ)26Mg, E=815, 904 keV; 22Ne(p, γ)23Na, E=479 keV; measured Eγ, Iγ, γγ-coin using HPGe and NaI(Tl) detectors at the JN Van de Graaff accelerator of the Laboratory for Experimental Nuclear Astrophysics (LENA); deduced yield curves for 479-keV proton resonance in 23Na. 26Mg; deduced level, precise energy of the 830-keV resonance by γγ-coin method, resonance strength. Comparison with previous experimental results.
doi: 10.1103/PhysRevC.99.045804
2019IL02 Phys.Rev. C 99, 065809 (2019) Calculation of resonance energies from Q values NUCLEAR REACTIONS 36Ar(p, γ), at T9=0.01-1; calculated thermonuclear reaction rates including energy shift to reaction Q values from electron binding energies, and compared with rates calculated without the electron binding energy shift; deduced 2-keV shift in the energy of the lowest-lying resonance in 37K. Discussed systematic bias introduced by adopting tabulated Q values based on atomic mass difference for the calculation of center-of-mass resonance energies which does not account for the difference in total electron binding energies before and after the nuclear interaction.
doi: 10.1103/PhysRevC.99.065809
2017AR04 Prog.Part.Nucl.Phys. 94, 1 (2017) A.Arcones, D.W.Bardayan, T.C.Beers, L.A.Bernstein, J.C.Blackmon, B.Messer, B.A.Brown, E.F.Brown, C.R.Brune, A.E.Champagne, A.Chieffi, A.J.Couture, P.Danielewicz, R.Diehl, M.El Eid, J.E.Escher, B.D.Fields, C.Frohlich, F.Herwig, W.R.Hix, C.Iliadis, W.G.Lynch, G.C.McLaughlin, B.S.Meyer, A.Mezzacappa, F.Nunes, B.W.O'Shea, M.Prakash, B.Pritychenko, S.Reddy, E.Rehm, G.Rogachev, R.E.Rutledge, H.Schatz, M.S.Smith, I.H.Stairs, A.W.Steiner, T.E.Strohmayer, F.X.Timmes, D.M.Townsley, M.Wiescher, R.G.T.Zegers, M.Zingale White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics
doi: 10.1016/j.ppnp.2016.12.003
2017KE01 Phys.Rev. C 95, 015806 (2017) K.J.Kelly, A.E.Champagne, L.N.Downen, J.R.Dermigny, S.Hunt, C.Iliadis, A.L.Cooper New measurements of low-energy resonances in the 22Ne (p, γ) 23Na reaction NUCLEAR REACTIONS 22Ne(p, γ), E=165, 192, 425, 441 keV; measured Eγ, Iγ, γγ-coin for resonances and direct capture process using HPGe-NaI detectors and plastic scintillator cosmic ray veto at LENA-TUNL facility. 23Na; deduced levels, resonance strengths, σγ for direct capture state, γ-ray branching ratios from singles and coincidence γ-ray data for resonant states, thermonuclear reaction rates.
doi: 10.1103/PhysRevC.95.015806
2017TI07 Nucl.Instrum.Methods Phys.Res. A871, 66 (2017) A.Tillett, J.Dermigny, M.Emamian, Y.Tonin, I.Bucay, R.L.Smith, M.Darken, C.Dearing, M.Orbon, C.Iliadis A low-background γγ-coincidence spectrometer for radioisotope studies RADIOACTIVITY 26Al(EC); measured decay products, Eγ, Iγ, γ-γ-coin; deduced cosmogenic activity, decay constant. Comparison with available data.
doi: 10.1016/j.nima.2017.07.057
2016DA05 Phys.Rev. C 94, 025803 (2016) S.Daigle, K.J.Kelly, A.E.Champagne, M.Q.Buckner, C.Iliadis, C.Howard Measurement of the Ec.m.r = 259 keV resonance in the 14N(p, g)15O reaction NUCLEAR REACTIONS 14N(p, γ)15O, E=270-310 keV; measured Eγ, Iγ using an HPGe detector and APEX array of NaI(Tl) detectors at LENA-TUNL facility. 15O; deduced levels, resonances, γ-ray branching ratios from the decay of the 259-keV proton resonance, resonance strength. Comparison with previous experimental data.
doi: 10.1103/PhysRevC.94.025803
2016DE36 Nucl.Instrum.Methods Phys.Res. 830, 427 (2016) J.R.Dermigny, C.Iliadis, M.Q.Buckner, K.J.Kelly γ-Ray spectroscopy using a binned likelihood approach NUCLEAR REACTIONS 18O, 25Mg(p, γ), E not given; measured reaction products, Eγ, Iγ; deduced a novel data-analysis method for γ-ray spectroscopy, resonance parameters. Comparison with Monte Carlo calculations.
doi: 10.1016/j.nima.2016.06.017
2015BU02 Phys.Rev. C 91, 015812 (2015) M.Q.Buckner, C.Iliadis, K.J.Kelly, L.N.Downen, A.E.Champagne, J.M.Cesaratto, C.Howard, R.Longland High-intensity-beam study of 17O(p, γ)18F and thermonuclear reaction rates for 17O + p NUCLEAR REACTIONS 17O(p, γ), E=170-530 keV; measured Eγ, Iγ, γγ-coin at LENA-TUNL facility. 18F; deduced levels, J, π, resonances, γ branching ratios from resonance capture, and from direct capture as function of E(p), resonance strengths, total S(E) factors. 17O(p, γ), (p, α); deduced thermonuclear reaction rates. Comparison with previous results.
doi: 10.1103/PhysRevC.91.015812
2014MO39 Phys.Rev. C 90, 065806 (2014) Thermonuclear reaction rate of 18Ne(α, p)21Na from Monte Carlo calculations NUCLEAR REACTIONS 18Ne(α, p), E=1-3 MeV; analyzed resonance strengths for α resonances in 22Mg from 40 keV to 5 MeV, astrophysical S(E) factor; deduced reaction rates for T9=0.1-3.0 using Monte Carlo method. Comparison with previous reaction rates.
doi: 10.1103/PhysRevC.90.065806
2013CE04 Phys.Rev. C 88, 065806 (2013) J.M.Cesaratto, A.E.Champagne, M.Q.Buckner, T.B.Clegg, S.Daigle, C.Howard, C.Iliadis, R.Longland, J.R.Newton, B.M.Oginni Measurement of the Erc.m.=138 keV resonance in the 23Na(p, γ)24Mg reaction and the abundance of sodium in AGB stars NUCLEAR REACTIONS 23Na(p, γ)24Mg, E<500 keV; measured Eγ, Iγ, on resonance γγ-coin spectra using ECRIS ion source at LENA-TUNL accelerator facility; deduced upper limit on the strength of the 138-keV proton resonance, probability density of the final 23Na abundance, (p, α)/(p, γ) reaction rate ratio, correlations between the final abundance of 23Na in AGB stars and the rate-variation factor. 23Na(p, α)20Ne, E at T9=0.010-10.0; deduced reaction rates for 138-keV resonance. Performed one-zone post-processing nucleosynthesis calculations.
doi: 10.1103/PhysRevC.88.065806
2013PA19 Prog.Part.Nucl.Phys. 68, 225 (2013) A.Parikh, J.Jose, G.Sala, C.Iliadis Nucleosynthesis in type I X-ray bursts
doi: 10.1016/j.ppnp.2012.11.002
2013PO05 Phys.Rev. C 88, 015808 (2013) I.Pogrebnyak, C.Howard, C.Iliadis, R.Longland, G.E.Mitchell Mean proton and α-particle reduced widths of the Porter-Thomas distribution and astrophysical applications NUCLEAR REACTIONS 27Al, 31P, 35Cl, 39K(p, α); 33S, 35Cl, 39K, 42Ca, 44Ca, 46Ti, 48Ti, 50Cr, 52Cr, 54Cr, 54Fe, 56Fe, 60Ni, 64Zn, 66Zn(p, p); analyzed previous experimental resonance data collected at TUNL facility. 28Si, 32S, 34Cl, 36Ar, 40Ca, 43,45Sc, 47,49V, 51,53,55Mn, 55,57Co, 61Cu, 65Ge, 67Ga; deduced mean reduced proton width and α widths. Porter-Thomas distributions. 40Ti(α, γ)44Ti; deduced thermonuclear reaction rates based on mean reduced α widths. Impact on 44Ti abundance in core-collapse novae.
doi: 10.1103/PhysRevC.88.015808
2013RA23 Phys.Rev.Lett. 111, 112501 (2013) R.Raut, A.P.Tonchev, G.Rusev, W.Tornow, C.Iliadis, M.Lugaro, J.Buntain, S.Goriely, J.H.Kelley, R.Schwengner, A.Banu, N.Tsoneva Cross-Section Measurements of the 86Kr(γ, n) Reaction to Probe the s-Process Branching at 85Kr NUCLEAR REACTIONS 86Kr, 197Au(γ, n), E<9.86-13 MeV; measured reaction products, Eγ, Iγ; deduced σ for direct and inverse reactions, 82,86Kr isotopic ratios. Comparison with HFB+QRPA calculations, TALYS code.
doi: 10.1103/PhysRevLett.111.112501
2012AR01 Phys.Rev. C 85, 044605 (2012) C.W.Arnold, T.B.Clegg, C.Iliadis, H.J.Karwowski, G.C.Rich, J.R.Tompkins, C.R.Howell Cross-section measurement of 9Be(γ, n)8Be and implications for α+α+n → 9Be in the r process NUCLEAR REACTIONS 9Be(γ, n)8Be, E=1.5-5.2 MeV; measured neutron spectra, Eγ, σ(E) using HIγS facility at TUNL. 9Be; deduced resonance energies, neutron and gamma widths, B(E1), B(M1), neutron branching ratios. Deduced astrophysical reaction rate for 4He(αn, γ)9Be reaction for r-process nucleosynthesis sites. Comparison with previous studies using (γ, n) and (e, e') reactions.
doi: 10.1103/PhysRevC.85.044605
2012BU16 Phys.Rev. C 86, 065804 (2012) M.Q.Buckner, C.Iliadis, J.M.Cesaratto, C.Howard, T.B.Clegg, A.E.Champagne, S.Daigle Thermonuclear reaction rate of 18O(p, γ)19F NUCLEAR REACTIONS 18O(p, γ)19F, E=95 keV; measured Eγ, Iγ, γγ-coin; deduced resonance strength, direct capture S factor using LENA facility. Improved thermonuclear reaction rates.
doi: 10.1103/PhysRevC.86.065804
2012LO07 Phys.Rev. C 85, 065809 (2012) R.Longland, C.Iliadis, A.I.Karakas Reaction rates for the s-process neutron source 22Ne + α NUCLEAR REACTIONS 22Ne(α, n)25Mg, 22Ne(α, γ)26Mg, E=830-2040 keV; analyzed resonance strengths, resonance energies, spectroscopic factors, partial widths; deduced astrophysical reactions rates, reaction rate probability densities, nucleosynthesis uncertainties; calculated element abundances. Monte Carlo sampling. Relevance to s-process nucleosynthesis in massive and AGB stars.
doi: 10.1103/PhysRevC.85.065809
2012LO11 J.Phys.:Conf.Ser. 337, 012047 (2012) Current Status of the 22Ne+α s-Process Neutron Source NUCLEAR REACTIONS 22Ne(α, γ), (α, n), E≈10 keV-1 MeV; re-analyzed, evaluated reaction rates; calculated isotopic abundances vs mass.
doi: 10.1088/1742-6596/337/1/012047
2012MO17 Nucl.Instrum.Methods Phys.Res. A688, 62 (2012) Recommended cross-section of the 16O(p, γ)17F reaction below 2.5 MeV: A potential tool for quantitative analysis and depth profiling of oxygen NUCLEAR REACTIONS 16O(p, γ), E=0.5-2.5 MeV; analyzed available data; deduced recommended σ and uncertainties. Comparison with available data.
doi: 10.1016/j.nima.2012.05.084
2012RA21 J.Phys.:Conf.Ser. 337, 012048 (2012) R.Raut, A.Banu, C.Iliadis, J.H.Kelley, G.Rusev, R.Schwengner, A.P.Tonchev, W.Tornow Cross-Section Measurements of the 86Kr(γ, n) Reaction to Probe the s-Process Branching at 85Kr NUCLEAR REACTIONS 86Kr(γ, n), E=9.970, 10.115, 10.170, 10.290, 10.360, 10.490, 11.005 MeV; measured En, In using 3He proportional counters; deduced σ; calculated σ using TALYS code with different parameter sets.
doi: 10.1088/1742-6596/337/1/012048
2011JO06 Rep.Prog.Phys. 74, 096901 (2011) Nuclear astrophysics: the unfinished quest for the origin of the elements
doi: 10.1088/0034-4885/74/9/096901
2011OG02 Phys.Rev. C 83, 025802 (2011) B.M.Oginni, C.Iliadis, A.E.Champagne Theoretical evaluation of the reaction rates for 26Al(n, p)26Mg and 26Al(n, α)23Na NUCLEAR REACTIONS 26Al(n, p)26Mg, E=0.01-10 MeV; 26Al(n, α)23Na, E=0.01-10 MeV; evaluated σ, fractional contribution to total σ, astrophysical reaction rates using EMPIRE, TALYS, and NON-SMOKER codes. Effects of different level density models and optical model potentials.
doi: 10.1103/PhysRevC.83.025802
2010DE29 Phys.Rev. C 82, 025802 (2010) R.J.de Boer, M.Wiescher, J.Gorres, R.Longland, C.Iliadis, G.Rusev, A.P.Tonchev Photoexcitation of astrophysically important states in 26Mg. II. Ground-state-transition partial widths NUCLEAR REACTIONS 26Mg(γ, γ'), E=10.5-11.7 MeV; measured Eγ, Iγ; deduced levels, J, π, resonances, branching ratios, total widths, partial widths. GEANT4 Monte-Carlo simulation of γ-ray spectra. Relevance to predictions of neutron production for the s-process in nucleosynthesis.
doi: 10.1103/PhysRevC.82.025802
2010IL04 Nucl.Phys. A841, 31 (2010) C.Iliadis, R.Longland, A.E.Champagne, A.Coc, R.Fitzgerald Charged-particle thermonuclear reaction rates: II. Tables and graphs of reaction rates and probability density functions NUCLEAR REACTIONS 14C, 16,17,18O, 17,18F, 19,20,21,22Ne, 21,22,23Na, 22,23,24,25,26Mg, 23,24,25,26,27Al, 26,27,28,29,30Si, 27,29,31P, 30,31,32S, 31,32,35Cl, 34,35,36Ar, 35K, 39,40Ca(p, γ), 14C, 14,15N, 15,16,18O, 20,22Ne, 24Mg(α, γ), 17,18O, 18F, 23Na, 27Al, 31P, 35Cl(p, α), 22Ne(α, n), E(cm)≤ 15 MeV; analyzed/evaluated total thermonuclear reaction rates. Tabulations from T=0.01-10 GK given.
doi: 10.1016/j.nuclphysa.2010.04.009
2010IL05 Nucl.Phys. A841, 251 (2010) C.Iliadis, R.Longland, A.E.Champagne, A.Coc Charged-particle thermonuclear reaction rates: III. Nuclear physics input
doi: 10.1016/j.nuclphysa.2010.04.010
2010IL06 Nucl.Phys. A841, 323 (2010) C.Iliadis, R.Longland, A.E.Champagne, A.Coc Charged-particle thermonuclear reaction rates: IV. Comparison to previous work NUCLEAR REACTIONS 14C, 16,17,18O, 17,18F, 19,20,21,22Ne, 21,22,23Na, 22,23,24,25,26Mg, 23,24,25,26,27Al, 26,27,28,29,30Si, 27,29,31P, 30,31,32S, 31,32,35Cl, 34,35,36Ar, 35K, 39,40Ca(p, γ), 14C, 14,15N, 15,16,18O, 20,22Ne, 24Mg(α, γ), 17,18O, 18F, 23Na, 27Al, 31P, 35Cl(p, α), 22Ne(α, n), E(cm)≤ 15 MeV; analyzed/evaluated total thermonuclear reaction rates. Graphical comparison with other data from T=0.01-10 GK.
doi: 10.1016/j.nuclphysa.2010.04.012
2010LO05 Phys.Rev. C 81, 055804 (2010) R.Longland, C.Iliadis, J.M.Cesaratto, A.E.Champagne, S.Daigle, J.R.Newton, R.Fitzgerald Resonance strength in 22Ne(p, γ)23Na from depth profiling in aluminum NUCLEAR REACTIONS 22Ne, 27Al(p, γ), E=400-505 keV; measured Eγ, Iγ, yields and resonance strengths. Comparison with previous data. Relevance to of resonance strengths in the 22Ne(p, γ)23Na hydrogen-burning reaction and in the 22Ne(α, γ) s-process neutron-source reactions.
doi: 10.1103/PhysRevC.81.055804
2010LO11 Nucl.Phys. A841, 1 (2010) R.Longland, C.Iliadis, A.E.Champagne, J.R.Newton, C.Ugalde, A.Coc, R.Fitzgerald Charged-particle thermonuclear reaction rates: I. Monte Carlo method and statistical distributions
doi: 10.1016/j.nuclphysa.2010.04.008
2010NE03 Phys.Rev. C 81, 045801 (2010) J.R.Newton, C.Iliadis, A.E.Champagne, J.M.Cesaratto, S.Daigle, R.Longland Measurement of 17O(p, γ)18F between the narrow resonances at Erlab=193 and 519 keV NUCLEAR REACTIONS 17O(p, γ)18O, E=151, 275, 300, 325, 400, 450, 500, 519 keV; measured Eγ, Iγ; deduced levels, total yields, σ, and total S factors. Compared with previous work.
doi: 10.1103/PhysRevC.81.045801
2009LO06 Phys.Rev. C 80, 055803 (2009) R.Longland, C.Iliadis, G.Rusev, A.P.Tonchev, R.J.de Boer, J.Gorres, M.Wiescher Photoexcitation of astrophysically important states in 26Mg NUCLEAR REACTIONS 26Mg(polarized γ, γ'), E=10.8, 11.0, 11.2, 11.4 MeV; measured Eγ, Iγ, and γγ(θ) at TUNL HIγS facility. 26Mg; deduced levels, J, π, and branching ratios. Comparison with Monte Carlo simulations. Implications for the reaction rates for 22Ne(α, γ)26Mg of astrophysical interest.
doi: 10.1103/PhysRevC.80.055803
2009PA18 Phys.Rev. C 79, 045802 (2009) A.Parikh, J.Jose, C.Iliadis, F.Moreno, T.Rauscher Impact of uncertainties in reaction Q values on nucleosynthesis in type I x-ray bursts NUCLEAR REACTIONS 25Si, 26P, 30S, 42Ti, 45,46Cr, 50Fe, 55Ni, 60Zn, 64Ge, 68Se, 89Ru, 98Cd, 105,106Sn(p, γ); calculated Q-values. A=1-113, Z=1-50; calculated yields and abundances using K04, F08, S01 and XRB models for, long, short, high temperature, low temperature, low Z and high Z. Implications for nucleosynthesis in type I x-ray bursts.
doi: 10.1103/PhysRevC.79.045802
2008IL02 Phys.Rev. C 77, 045802 (2008) C.Iliadis, C.Angulo, P.Descouvemont, M.Lugaro, P.Mohr New reaction rate for 16O(p, γ)17F and its influence on the oxygen isotopic ratios in massive AGB stars NUCLEAR REACTIONS 16O(p, γ), E<3.5 MeV; evaluated σ, deduced astrophysical S-factor, reaction rate. Compared with rate of 17O(p, α) reaction.
doi: 10.1103/PhysRevC.77.045802
2008NE10 Phys.Rev. C 78, 025805 (2008) J.R.Newton, R.Longland, C.Iliadis Matching of experimental and statistical-model thermonuclear reaction rates at high temperatures NUCLEAR REACTIONS 20Ne, 24Mg(α, γ), E=0-2000 keV; 21,22Ne, 23Na, 24,25,26Mg, 27Al, 28,29,30Si, 31P, 32S, 35Cl, 36Ar, 40Ca(p, γ), E=thermal; 23Na, 27Al, 31P, 35Cl(p, α), E=thermal; calculated stellar reaction rates.
doi: 10.1103/PhysRevC.78.025805
2007NE07 Phys.Rev. C 75, 045801 (2007) J.R.Newton, C.Iliadis, A.E.Champagne, A.Coc, Y.Parpottas, C.Ugalde Gamow peak in thermonuclear reactions at high temperatures NUCLEAR REACTIONS 27Al(p, γ), 24Mg(α, γ), E not given; calculated reaction rates, resonance contributions. 21,22Ne, 23Na, 25,26Mg, 27Al, 29,30Si, 31P, 35Cl(p, γ), E ≈ 0-2.5 MeV; calculated Gamow peak vs effective thermonuclear energy range.
doi: 10.1103/PhysRevC.75.045801
2007NE08 Phys.Rev. C 75, 055808 (2007) J.R.Newton, C.Iliadis, A.E.Champagne, R.Longland, C.Ugalde Remeasurement of the 193 keV resonance in 17O(p, α)14N NUCLEAR REACTIONS 17O(p, α), E=140-210 keV; measured yields and resonance strength for the 193 keV resonance.
doi: 10.1103/PhysRevC.75.055808
2007UG01 Phys.Rev. C 76, 025802 (2007) C.Ugalde, A.E.Champagne, S.Daigle, C.Iliadis, R.Longland, J.R.Newton, E.Osenbaugh-Stewart, J.A.Clark, C.Deibel, A.Parikh, P.D.Parker, C.Wrede Experimental evidence for a natural parity state in 26Mg and its impact on the production of neutrons for the s process NUCLEAR REACTIONS 22Ne(6Li, d), E=30 MeV; measured deuteron energy spectra. 26Mg deduced level energies.
doi: 10.1103/PhysRevC.76.025802
2006JO13 Nucl.Phys. A777, 550 (2006) Nucleosynthesis in classical novae
doi: 10.1016/j.nuclphysa.2005.02.121
2005FO03 Phys.Rev. C 71, 055801 (2005) C.Fox, C.Iliadis, A.E.Champagne, R.P.Fitzgerald, R.Longland, J.Newton, J.Pollanen, R.Runkle Thermonuclear reaction rate of 17O(p, γ)18F NUCLEAR REACTIONS 17O(p, γ), E=140-540 keV; measured Eγ, Iγ; deduced resonance parameters, excitation functions, thermonuclear reaction rates.
doi: 10.1103/PhysRevC.71.055801
2005IL02 Nucl.Phys. A758, 73c (2005) Nuclear Astrophysics: Direct measurements with stable beams NUCLEAR REACTIONS 17O(p, γ), E ≈ 190, 519 keV; measured Eγ, Iγ; deduced resonance excitation functions. 23Na(p, γ), E ≈ 150 keV; measured Eγ, Iγ, γγ-coin; deduced resonance strength upper limit. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2005.05.019
2005IL03 J.Phys.(London) G31, S1785 (2005) C.Iliadis, A.Champagne, J.Jose Explosive hydrogen burning of 23Na in classical novae NUCLEAR REACTIONS 23Na(p, γ), (p, α), E=130-155 keV; measured Eγ, Iγ; deduced resonance strength upper limits, astrophysical reaction rates.
doi: 10.1088/0954-3899/31/10/073
2005RU04 Phys.Rev.Lett. 94, 082503 (2005) R.C.Runkle, A.E.Champagne, C.Angulo, C.Fox, C.Iliadis, R.Longland, J.Pollanen Direct Measurement of the 14N(p, γ)15O S Factor NUCLEAR REACTIONS 14N(p, γ), E=155-524 keV; measured Eγ, excitation function; deduced S-factor. R-matrix analysis, astrophysical implications discussed.
doi: 10.1103/PhysRevLett.94.082503
2004BL21 Nucl.Phys. A746, 365c (2004) J.C.Blackmon, D.W.Bardayan, C.R.Brune, F.Carstoiu, A.E.Champagne, R.Crespo, T.Davinson, J.C.Fernandes, C.A.Gagliardi, U.Greife, C.J.Gross, P.A.Hausladen, C.Iliadis, C.C.Jewett, R.L.Kozub, T.A.Lewis, F.Liang, B.H.Moazen, A.M.Mukhamedzhanov, C.D.Nesaraja, F.M.Nunes, P.D.Parker, D.C.Radford, L.Sahin, J.P.Scott, D.Shapira, M.S.Smith, J.S.Thomas, L.Trache, R.E.Tribble, P.J.Woods, C.-H.Yu The 17F(p, γ)18Ne direct capture cross section NUCLEAR REACTIONS 12C, 14N(17F, 17F), E=170 MeV; 14N(17F, 18Ne), E=170 MeV; measured σ(θ).
doi: 10.1016/j.nuclphysa.2004.09.054
2004FO12 Phys.Rev.Lett. 93, 081102 (2004) C.Fox, C.Iliadis, A.E.Champagne, A.Coc, J.Jose, R.Longland, J.Newton, J.Pollanen, R.Runkle Explosive Hydrogen Burning of 17O in Classical Novae NUCLEAR REACTIONS 17O(p, γ), E=180-210 keV; measured reaction products, Eγ, Iγ; deduced γ-ray yields, resonance parameters, reaction rates. 1 MV Van de Graaff accelerator, the Laboratory for Experimental Nuclear Astrophysics, located at the Triangle Universities Nuclear Laboratory
doi: 10.1103/PhysRevLett.93.081102
2004HA50 Phys.Rev. C 70, 045802 (2004) S.E.Hale, A.E.Champagne, C.Iliadis, V.Y.Hansper, D.C.Powell, J.C.Blackmon Investigation of the 23Na(p, γ)24Mg and 23Na(p, α)20Ne reactions via (3He, d) spectroscopy NUCLEAR REACTIONS 23Na(3He, d), E=20 MeV; measured deuteron spectra, σ(E, θ). 24Mg deduced levels, J, π, spectroscopic factors. 23Na(p, γ), (p, α), E=low; deduced resonance features, reaction rates. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.70.045802
2004IL02 Phys.Rev. C 69, 064305 (2004) Spectroscopic factors from direct proton capture NUCLEAR REACTIONS 16,17,18O, 20,22Ne, 24Mg, 27Al, 28Si, 32S, 40Ca(p, γ), E ≈ 800-1900 keV; 16,17,18O, 24Mg, 32S(3He, d), E=15, 25 MeV; analyzed data; deduced spectroscopic factors. Comparison of direct capture and transfer reaction results.
doi: 10.1103/PhysRevC.69.064305
2003BA85 Nucl.Phys. A718, 505c (2003) D.W.Bardayan, J.C.Blackmon, A.E.Champagne, A.K.Dummer, T.Davinson, U.Greife, D.Hill, C.Iliadis, B.A.Johnson, R.L.Kozub, C.S.Lee, M.S.Smith, P.J.Woods Study of 26Si States Important for 26Al Nucleosynthesis in Novae NUCLEAR REACTIONS 28Si(p, t), E=40, 42 MeV; measured σ(E, θ). 26Si deduced levels, J, π. Astrophysical implications discussed.
doi: 10.1016/S0375-9474(03)00825-X
2003BA86 Nucl.Phys. A718, 590c (2003) D.W.Bardayan, J.C.Batchelder, J.C.Blackmon, A.E.Champagne, T.Davinson, R.Fitzgerald, W.R.Hix, C.Iliadis, R.L.Kozub, Z.Ma, S.Parete-Koon, P.D.Parker, N.Shu, M.S.Smith, P.J.Woods Measurement of the 18F(p, α)15O Cross Section at Nova Energies NUCLEAR REACTIONS 1H(18F, α), E(cm) ≈ 0.3-0.8 MeV; measured σ; deduced resonance parameters. 18F(p, α), E(cm) ≈ 0.2-1.0 MeV; deduced σ.
doi: 10.1016/S0375-9474(03)00873-X
2003BL12 Nucl.Phys. A718, 587c (2003) J.C.Blackmon, D.W.Bardayan, C.R.Brune, A.E.Champagne, R.Crespo, T.Davinson, J.C.Fernandes, C.A.Gagliardi, U.Greife, C.J.Gross, P.A.Hausladen, C.Iliadis, C.C.Jewett, R.L.Kozub, T.A.Lewis, F.Liang, B.H.Moazen, A.M.Mukhamedzhanov, C.D.Nesaraja, F.M.Nunes, P.D.Parker, D.C.Radford, L.Sahin, J.P.Scott, D.Shapira, M.S.Smith, J.S.Thomas, L.Trache, R.E.Tribble, P.J.Woods, C.-H.Yu The 17F(p, γ)18Ne Direct Capture Cross Section NUCLEAR REACTIONS 14N(17F, 18Ne), E=170 MeV; measured Eγ, Iγ, particle spectra, (particle)γ-coin, σ(θ).
doi: 10.1016/S0375-9474(03)00872-8
2002BA25 Phys.Rev. C65, 032801 (2002) D.W.Bardayan, J.C.Blackmon, A.E.Champagne, A.K.Dummer, T.Davinson, U.Greife, D.Hill, C.Iliadis, B.A.Johnson, R.L.Kozub, C.S.Lee, M.S.Smith, P.J.Woods Astrophysically Important 26Si States Studied with the 28Si(p, t)26Si Reaction NUCLEAR REACTIONS 28Si(p, t), E=40, 42 MeV; measured triton spectra, σ(θ). 26Si deduced levels, J, π. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.65.032801
2002BB02 Phys.Rev.Lett. 89, 262501 (2002) D.W.Bardayan, J.C.Batchelder, J.C.Blackmon, A.E.Champagne, T.Davinson, R.Fitzgerald, W.R.Hix, C.Iliadis, R.L.Kozub, Z.Ma, S.Parete-Koon, P.D.Parker, N.Shu, M.S.Smith, P.J.Woods Strength of the 18F(p, α)15O Resonance at Ec.m.=330 keV NUCLEAR REACTIONS 1H(18F, α), E(cm)=330 keV; measured Eα, Iα(θ), σ; deduced resonance parameters. 18F(p, α), E=astrophysical; calculated reaction rates.
doi: 10.1103/PhysRevLett.89.262501
2002BE87 Phys.Rev. C 66, 055804 (2002) P.F.Bertone, A.E.Champagne, M.Boswell, C.Iliadis, S.E.Hale, V.Y.Hansper, D.C.Powell 14N(3He, d)15O as a probe of direct capture in the 14N(p, γ)15O reaction NUCLEAR REACTIONS 14N(3He, d), E=20 MeV; measured deuteron spectra, σ(θ). 15O deduced spectroscopic factors, asymptotic normalization coefficients. 14N(p, γ), E(cm)=0-3.5 MeV; calculated astrophysical S-factors.
doi: 10.1103/PhysRevC.66.055804
2002CH61 Phys.Rev. C 66, 064316 (2002) J.C.Chow, J.D.King, N.P.T.Bateman, R.N.Boyd, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, A.C.Morton, J.Powell, A.Shotter β-delayed particle decay of 17Ne into p+α+12C through the isobaric analog state in 17F RADIOACTIVITY 17Ne(β+α), (β+p); measured Ep, Eα pα(12C)-coin following decay of intermediate IAS state; deduced branching ratios. 17F deduced branching ratios for particle decay from IAS.
doi: 10.1103/PhysRevC.66.064316
2002HA03 Phys.Rev. C65, 015801 (2002) S.E.Hale, A.E.Champagne, C.Iliadis, V.Y.Hansper, D.C.Powell, J.C.Blackmon Investigation of the 22Ne(p, γ)23Na Reaction via (3He, d) Spectroscopy NUCLEAR REACTIONS 22Ne(3He, d), E=20 MeV; measured deuteron spectra, σ(θ). 23Na levels deduced spectroscopic factors. 22Ne(p, γ), E=spectrum; deduced astrophysical reaction rates. 22Ne(3He, 3He), E=20 MeV; measured σ(θ).
doi: 10.1103/PhysRevC.65.015801
2002IL05 Astrophys.J.Suppl.Ser. 142, 105 (2002) Ch.Iliadis, A.Champagne, J.Jose, S.Starrfield, P.Tupper The Effects of Thermonuclear Reaction-Rate Variations on Nova Nucleosynthesis: A Sensitivity Study NUCLEAR REACTIONS 3He, 7Be, 15O(α, γ), 7Be, 8B, 12,13C, 13,14,15N, 16,17,18O(p, γ), 15N, 17O, 18,19F, 23Na(p, α), 17,18F, 19,20,21,22Ne, 21,22,23Na, 23,24,25Mg(p, γ), E not given; calculated astrophysical abundances; deduced impact of σ and reaction rates uncertainties.
doi: 10.1086/341400
2002MO19 Nucl.Phys. A706, 15 (2002) A.C.Morton, J.C.Chow, J.D.King, R.N.Boyd, N.P.T.Bateman, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, W.Galster, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, J.Powell, G.Roy, A.Shotter Beta-Delayed Particle Decay of 17Ne RADIOACTIVITY 17Ne(β+p), (β+α); measured Ep, Eα, pγ-coin, angular correlations; deduced log ft, Gamow-Teller strength. 17F deduced levels, J, π, particle decay branching ratios.
doi: 10.1016/S0375-9474(02)00862-X
2002RO13 Nucl.Instrum.Methods Phys.Res. A480, 610 (2002) C.Rowland, C.Iliadis, A.E.Champagne, A.K.Dummer, R.Fitzgerald, E.C.T.Harley, J.Mosher, R.Runkle Studies of Weak Capture-γ-Ray Resonances via Coincidence Techniques NUCLEAR REACTIONS 26Mg(p, γ), E < 350 keV; measured Eγ, Iγ, γγ-coin.
doi: 10.1016/S0168-9002(01)01231-1
2002RO22 Phys.Rev. C65, 064609 (2002) C.Rowland, C.Iliadis, A.E.Champagne, J.Mosher Measurement of the ER = 338 keV Resonance Strength for 23Na(p, α)20Ne NUCLEAR REACTIONS 23Na(p, α), (p, p), E < 480 keV; measured Eα, Ep, yields. 23Na(p, α), E ≈ 338 keV; deduced resonance strength. Comparison with previous results.
doi: 10.1103/PhysRevC.65.064609
2002RU11 Phys.Rev. C66, 022801 (2002) R.C.Runkle, A.E.Champagne, C.Fox, C.Iliadis, J.Pollanen, A.Stephan, C.Westerfeldt Search for a resonance in the 14N(p, γ) 15O reaction at E p =127 keV NUCLEAR REACTIONS 14N(p, γ), E=135-300 keV; measured Eγ, Iγ; deduced resonance strength upper limit.
doi: 10.1103/PhysRevC.66.022801
2001BA17 Phys.Rev. C63, 035803 (2001) N.Bateman, K.Abe, G.Ball, L.Buchmann, J.Chow, J.M.D'Auria, Y.Fuchi, C.Iliadis, H.Ishiyama, K.P.Jackson, S.Karataglidis, S.Kato, S.Kubono, K.Kumagai, M.Kurokawa, X.Liu, S.Michimasa, P.Strasser, M.H.Tanaka Measurement of the 24Mg(p, t)22Mg Reaction and Implications for the 21Na(p, γ)22Mg Stellar Reaction Rate NUCLEAR REACTIONS 24Mg(p, t), E=37.925 MeV; measured particle spectra. 22Mg deduced levels, possible J, π. 21Na(p, γ), E not given; deduced astrophysical reaction rates. Shell model calculations.
doi: 10.1103/PhysRevC.63.035803
2001BE57 Phys.Rev.Lett. 87, 152501 (2001) P.F.Bertone, A.E.Champagne, D.C.Powell, C.Iliadis, S.E.Hale, V.Y.Hansper Lifetime of the 6793-keV State in 15O NUCLEAR REACTIONS 14N(p, γ), E=300 keV; measured Eγ, Iγ, DSA. 15O levels deduced T1/2. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.87.152501
2001IL02 Astrophys.J.Suppl.Ser. 134, 151 (2001) C.Iliadis, J.M.D'Auria, S.Starrfield, W.J.Thompson, M.Wiescher Proton-Induced Thermonuclear Reaction Rates for A = 20-40 Nuclei NUCLEAR REACTIONS 20,21,22Ne, 20,21,22,23Na, 22,23,24,25,26Mg, 23,24,25,26,27Al, 26,27,28,29,30Si, 27,28,29,30,31P, 30,31,32,33,34S, 31,32,33,34,35Cl, 34,35,36Ar, 35,36,37,38,39K, 39,40Ca(p, γ), E=low; 23Na, 27Al, 31P, 35Cl, 39K(p, α), E=low; compiled, analyzed astrophysical reaction rates.
doi: 10.1086/320364
2001ST18 Nucl.Phys. A688, 110c (2001) S.Starrfield, C.Iliadis, J.W.Truran, M.Wiescher, W.M.Sparks Nuclear Reaction Rates and the Nova Outburst NUCLEAR STRUCTURE 12,13C, 14,15N, 22Na, 26,27Al, 32S; analyzed, surveyed astrophysical nuclear reaction rates; deduced nova luminosity, yields.
doi: 10.1016/S0375-9474(01)00679-0
2000GE09 Phys.Rev. C61, 064310 (2000) E.Gete, L.Buchmann, R.E.Azuma, D.Anthony, N.Bateman, J.C.Chow, J.M.D'Auria, M.Dombsky, U.Giesen, C.Iliadis, K.P.Jackson, J.D.King, D.F.Measday, A.C.Morton β-Delayed Particle Decay of 9C and the A = 9, T = 1/2 Nuclear System: Experiment, data, and phenomenological analysis RADIOACTIVITY 9C(β+); measured Eβ, Iβ, β-delayed particle spectra, coincidences, angular correlations. 9B levels deduced excitation and decay branching ratios.
doi: 10.1103/PhysRevC.61.064310
2000HA06 Phys.Rev. C61, 028801 (2000) V.Y.Hansper, A.E.Champagne, S.E.Hale, C.Iliadis, D.C.Powell Measurement of the 40Ca(3He, t)40Sc Reaction NUCLEAR REACTIONS 40Ca(3He, t), E=26 MeV; measured triton spectra. 40Sc deduced levels, resonances. Comparison with proton capture results.
doi: 10.1103/PhysRevC.61.028801
1999IL01 Astrophys.J. 524, 434 (1999) C.Iliadis, P.M.Endt, N.Prantzos, W.J.Thompson Explosive Hydrogen Burning of 27Si, 31S, 35Ar, and 39Ca in Novae and X-Ray Bursts NUCLEAR REACTIONS 27Si, 31S, 35Ar, 39Ca(p, γ), E not given; calculated astrophysical reaction rates vs temperature.
doi: 10.1086/307778
1999PO25 Nucl.Phys. A660, 349 (1999) D.C.Powell, C.Iliadis, A.E.Champagne, C.A.Grossmann, S.E.Hale, V.Y.Hansper, L.K.McLean Reaction Rate of 24Mg(p, γ)25Al NUCLEAR REACTIONS 24Mg(p, γ), E=0.2-1.7 MeV; measured Eγ, Iγ, DSA; deduced proton, γ-ray resonances partial widths, strengths, stellar reaction rates.
doi: 10.1016/S0375-9474(99)00390-5
1999TH03 Nucl.Phys. A647, 259 (1999) Error Analysis for Resonant Thermonuclear Reaction Rates NUCLEAR REACTIONS 32S, 39Ca(p, γ), E not given; analyzed resonance data; deduced reaction rates, uncertainties. Astrophysical implications discussed.
doi: 10.1016/S0375-9474(98)00617-4
1998CH05 Phys.Rev. C57, R475 (1998) J.C.Chow, A.C.Morton, R.E.Azuma, N.Bateman, R.N.Boyd, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, W.Galster, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, J.D.King, G.Roy, T.Shoppa, A.Shotter Three-Particle Breakup of the Isobaric Analog State in 17F RADIOACTIVITY 17Ne(β+) [from Mg, O(p, X)]; measured β-delayed pα(12C)-coin. 17F deduced IAS p, α branching ratios. Implications for stellar helium burning discussed.
doi: 10.1103/PhysRevC.57.R475
1998HE25 Phys.Rev. C58, 1798 (1998) H.Herndl, M.Fantini, C.Iliadis, P.M.Endt, H.Oberhummer Thermonuclear Reaction Rate of 23Mg(p, γ)24Al NUCLEAR REACTIONS 23Mg(p, γ), E not given; calculated reaction rate vs stellar temperature; deduced parameters. Comparison with previous results. Astrophysical implications.
doi: 10.1103/PhysRevC.58.1798
1998PO20 Nucl.Phys. A644, 263 (1998) D.C.Powell, C.Iliadis, A.E.Champagne, S.E.Hale, V.Y.Hansper, R.A.Surman, K.D.Veal Low-Energy Resonance Strengths for Proton Capture on Mg and Al Nuclei NUCLEAR REACTIONS 24,25,26Mg, 27Al(p, p), E ≈ 330-450 MeV; measured σ(θ). 24,25,26Mg, 27Al(p, γ), E ≈ 330-450 MeV; measured Eγ, Iγ; deduced γ-ray brancing ratios, resonance strengths.
doi: 10.1016/S0375-9474(98)00593-4
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
1997IL02 Nucl.Phys. A618, 166 (1997) Proton Single-Particle Reduced Widths for Unbound States NUCLEAR REACTIONS 12C, 23Na, 31P, 40Ca(p, p), E ≤ 1 MeV; calculated single particle reduced widths vs E. Comparison of partial proton widths from optical models, R-matrix methods.
doi: 10.1016/S0375-9474(97)00065-1
1997IL03 Nucl.Phys. A621, 211c (1997) C.Iliadis, R.E.Azuma, J.Chow, J.D.King, A.C.Morton, L.Buchmann, M.Dombsky, K.P.Jackson, J.M.D'Auria, U.Giesen, J.G.Ross, H.Schatz, M.Wiescher Decay Studies of Importance to Explosive Hydrogen Burning RADIOACTIVITY 36K(β+p), (β+α) [from Ca(p, X), E=500 MeV]; measured α-, proton spectra; deduced log ft. 36Ar deduced α-emitting resonance.
doi: 10.1016/S0375-9474(97)00240-6
1997KI19 Nucl.Phys. A621, 169c (1997) J.D.King, R.E.Azuma, C.Iliadis, A.C.Morton, L.Buchmann, M.Dombsky, K.P.Jackson, J.M.D'Auria, U.Giesen, G.Roy, T.Davinson, A.Shotter, W.Galster, R.N.Boyd Investigation of the 12C(α, γ)16O Reaction Via the β-Delayed Proton Decay of 17Ne RADIOACTIVITY 17Ne(β+p); measured β-delayed proton spectra, pγ-coin. 16O levels deduced β-delayed proton branching ratios. Implications for 12C(α, γ) reaction.
doi: 10.1016/S0375-9474(97)00232-7
1996IL01 Phys.Rev. C53, 475 (1996) C.Iliadis, L.Buchmann, P.M.Endt, H.Herndl, M.Wiescher New Stellar Reaction Rates for 25Mg(p, γ)26Al and 25Al(p, γ)26Si NUCLEAR REACTIONS 25Mg(3He, d), E=18 MeV; 27Al(3He, α), 24Mg(3He, n), E not given; analyzed σ(θ); deduced 25Mg, 25Al(p, γ) stellar reaction rates. 26Al deduced levels, J, π, T, spectroscopic factors, resonance parameters, γ-branching ratios. 26Mg, 26Si deduced Coulomb displacement energies. Shell model.
doi: 10.1103/PhysRevC.53.475
1996IL02 Nucl.Phys. A609, 237 (1996) C.Iliadis, R.E.Azuma, L.Buchmann, J.Chow, J.M.D'Auria, M.Dombsky, U.Giesen, J.D.King, A.C.Morton Beta-Delayed Particle Decay of 36K RADIOACTIVITY 36K(β+); measured decay products, β-delayed Ep, Ip, Eα, Iα. 36Ar; deduced levels, particle branching ratios, associated log ft upper limits. Microchannel plate in back-to-back geometry, surface barrier detector.
doi: 10.1016/0375-9474(96)00297-7
1995RO22 Phys.Rev. C52, 1681 (1995) J.G.Ross, J.Gorres, C.Iliadis, S.Vouzoukas, M.Wiescher, R.B.Vogelaar, S.Utku, N.P.T.Bateman, P.D.Parker Indirect Study of Low-Energy Resonances in 31P(p, α)28Si and 35Cl(p, α)32S NUCLEAR REACTIONS 31P, 35Cl(3He, d), E=25 MeV; measured particle spectra, γd-, (particle)d-coin; deduced (p, γ), (p, α) reaction rates for 31P, 35Cl. 36Ar deduced levels Γ, J, π, T. 32S deduced levels Γ, J, π, T, resonance strength.
doi: 10.1103/PhysRevC.52.1681
1994IL01 Nucl.Phys. A571, 132 (1994) C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, R.E.Azuma, G.Roters, H.P.Trautvetter, H.C.Evans Explosive Hydrogen Burning of 35Cl NUCLEAR REACTIONS 35Cl(3He, d), E=15 MeV; measured σ(θ), σ(Ed). 32S(6Li, d), E=32 MeV; measured σ(Ed). 32S(α, γ), E ≈ resonance; measured Eγ, Iγ. 35Cl(p, γ), E ≈ 200-800 keV; measured γ yield vs E , stellar rates. 35Cl(p, X), E=177 keV; measured particle spectra. 36Ar deduced levels, J, π, L, spectroscopic factors, γ-branching ratios, resonance strengths. Deduced no evidence for (p, α) reactions.
doi: 10.1016/0375-9474(94)90345-X
1994VO12 Phys.Rev. C50, 1185 (1994) S.Vouzoukas, C.P.Browne, U.Giesen, J.Gorres, S.M.Graff, H.Herndl, C.Iliadis, L.O.Lamm, J.Meissner, J.G.Ross, K.Scheller, L.van Wormer, M.Wiescher, A.A.Rollefson Reaction Rate for 31S(p, γ)32Cl and Its Influence on the SiP Cycle in Hot Stellar Hydrogen Burning NUCLEAR REACTIONS 32S(3He, t), E=22.5-25 MeV; measured σ(Et), σ(θ); deduced 31S(p, γ) reaction rate, hot stellar hydrogen burning implications. 32Cl deduced level, J, π, C2S, Γγ.
doi: 10.1103/PhysRevC.50.1185
1993GI04 Nucl.Phys. A561, 95 (1993) U.Giesen, C.P.Browne, J.Gorres, S.Graff, C.Iliadis, H.-P.Trautvetter, M.Wiescher, V.Harms, K.L.Kratz, B.Pfeiffer, R.E.Azuma, M.Buckby, J.D.King The Astrophysical Implications of Low-Energy Resonances in 22Ne + α NUCLEAR REACTIONS 22Ne(6Li, d), E=32 MeV; measured σ(θ), σ(Ed). 22Ne(α, n), E=0.6-9 MeV; measured neutron yield vs E; deduced model parameters, resonance yield, reaction rates. 26Mg deduced resonances, J, π, α-spectroscopic factors, resonance strength.
doi: 10.1016/0375-9474(93)90167-V
1993IL01 Nucl.Phys. A559, 83 (1993) C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, C.Grama, Th.Schange, H.P.Trautvetter, H.C.Evans Explosive Hydrogen Burning of 31P NUCLEAR REACTIONS, ICPND 31P(p, γ), (p, α), E=160-370 keV; 28Si(α, γ), E=2.4-2.6 MeV; measured γ yield vs E; deduced stellar reaction rates, temperature dependence. 32S deduced proton thershold state features.
doi: 10.1016/0375-9474(93)90181-V
1993IL02 Phys.Rev. C48, R1479 (1993) C.Iliadis, J.Hohne, F.Kappeler, J.Meissner, H.P.Trautvetter, M.Wiescher Measurement of the Resonance at E(R) = 1422 keV in 36Ar(p, γ)37K NUCLEAR REACTIONS 36Ar(p, γ), E=0.90-1.45 MeV; measured γ yield, θγ=45°, Eγ, Iγ. 37K deduced level, Γγ/Γp, resonance strength, Gamow-Teller transition strength.
doi: 10.1103/PhysRevC.48.R1479
1992IL01 Nucl.Phys. A539, 97 (1992) C.Iliadis, U.Giesen, J.Gorres, M.Wiescher, S.M.Graff, R.E.Azuma, C.A.Barnes Direct Proton Capture on 32S NUCLEAR REACTIONS, ICPND 32S(p, γ), E=0.4-2 MeV; measured Eγ, Iγ, absolute γ yield vs E; deduced stellar reaction rate. 33Cl levels deduced C2S.
doi: 10.1016/0375-9474(92)90237-E
1992IL03 Phys.Rev. C45, 2989 (1992) C.Iliadis, J.G.Ross, J.Gorres, M.Wiescher, S.M.Graff, R.E.Azuma Reaction 36Ar(p, γ)37K in Explosive Hydrogen Burning NUCLEAR REACTIONS, ICPND 36Ar(p, γ), E=0.32-0.93 MeV; measured Eγ, Iγ, γ yield vs E; calculated thermonuclear reaction rate vs temperature. 37K levels deduced branching ratios, resonance strength.
doi: 10.1103/PhysRevC.45.2989
1991IL01 Nucl.Phys. A533, 153 (1991) C.Iliadis, U.Giesen, J.Gorres, S.Graff, M.Wiescher, R.E.Azuma, J.King, M.Buckby, C.A.Barnes, T.R.Wang The Reaction Branching 31P(p, γ)/31P(p, α) in the rp-Process NUCLEAR REACTIONS, ICPND 31P(p, γ), E=0.28-0.62 MeV; 31P(p, α), E=0.28-0.45 MeV; measured σ(E), relative yield. 32S, 28Si deduced resonances, J, π, resonance strengths. Hauser-Feshbach calculations.
doi: 10.1016/0375-9474(91)90824-P
1990IL01 Nucl.Phys. A512, 509 (1990) Ch.Iliadis, Th.Schange, C.Rolfs, U.Schroder, E.Somorjai, H.P.Trautvetter, K.Wolke, P.M.Endt, S.W.Kikstra, A.E.Champagne, M.Arnould, G.Paulus Low-Energy Resonances in 25Mg(p, γ)26Al, 26Mg(p, γ)27Al and 27Al(p, γ)28Si NUCLEAR REACTIONS 25,26Mg, 27Al(p, γ), E < 340 keV; measured γ-spectra, γ-branchings. 26,27Al, 28Si deduced resonances, J, π, Γ, γ-branching ratios.
doi: 10.1016/0375-9474(90)90084-Y
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