NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = L.Van Wormer Found 7 matches. 2003BL11 Nucl.Phys. A718, 127c (2003) J.C.Blackmon, D.W.Bardayan, W.Bradfield-Smith, R.Brummitt, A.E.Champagne, A.A.Chen, T.Davinson, L.Dessieux, M.W.Guidry, K.I.Hahn, G.M.Hale, W.R.Hix, R.L.Kozub, Z.Ma, P.D.Parker, G.Rajbaidya, R.C.Runkle, C.M.Rowland, A.C.Shotter, M.S.Smith, L.A.Van Wormer, D.W.Visser, P.J.Woods The 14O(α, p)17F Reaction Rate NUCLEAR REACTIONS 1H(17F, 17F), (17F, 17F'), (17F, 14O), E(cm) ≈ 1-4 MeV; measured particle spectra. 17F(p, p'), E(cm)=2-2.5 MeV; deduced σ. 14O(α, p), E=low; deduced astrophysical reaction rate. R-matrix analysis.
doi: 10.1016/S0375-9474(03)00689-4
2002SM11 Nucl.Instrum.Methods Phys.Res. A488, 342 (2002) D.L.Smith, D.G.Naberejnev, L.A.Van Wormer Large Errors and Severe Conditions RADIOACTIVITY 53V(β-); analyzed T1/2 uncertainties. NUCLEAR REACTIONS 31P(p, γ), E not given; analyzed astrophysical reaction rates, uncertainties.
doi: 10.1016/S0168-9002(02)00467-9
1997SC20 Nucl.Phys. A621, 417c (1997) H.Schatz, A.Aprahamian, B.A.Brown, J.Gorres, H.Herndl, K.-L.Kratz, P.Moller, B.Pfeiffer, T.Rauscher, J.F.Rembges, F.-K.Thielemann, M.Wiescher, L.van Wormer The Endpoint of the rp-Process NUCLEAR STRUCTURE A=50-100; analyzed rp-process endpoint associated X-ray bursts related features; deduced mass=80-100 region production enhancement. Large nuclear reaction network.
doi: 10.1016/S0375-9474(97)00283-2
1995HE18 Phys.Rev. C52, 1078 (1995) H.Herndl, J.Gorres, M.Wiescher, B.A.Brown, L.Van Wormer Proton Capture Reaction Rates in the rp Process NUCLEAR STRUCTURE 34,35Ar, 23,24Al, 31,32Cl, 27P, 35K, 26Si, 30S, 42Ti; calculated (p, γ) reaction rate for these targets; deduced rp process nucleosynthesis implications. 24,25Si, 27P, 31Cl, 28Si, 32,33Ar, 35,36K, 43V, 36Ca deduced resonances, spectroscopic amplitudes. Shell model.
doi: 10.1103/PhysRevC.52.1078
1994TH03 Nucl.Phys. A570, 329c (1994) F.-K.Thielemann, K.-L.Kratz, B.Pfeiffer, T.Rauscher, L.van Wormer, M.C.Wiescher Astrophysics and Nuclei Far from Stability ATOMIC MASSES A=60-200; analyzed mass models analyses; deduced r-process abundance fits. NUCLEAR STRUCTURE A=60-200; analyzed mass models analyses; deduced r-process abundance fits.
doi: 10.1016/0375-9474(94)90299-2
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
1992WA13 Nucl.Instrum.Methods Phys.Res. A314, 113 (1992) R.E.Warner, R.J.Orr, W.F.Waite, C.P.Browne, S.E.Darden, A.Rollefson, J.J.Kolata, L.Van Wormer, A.Galonsky, D.Sackett, F.D.Becchetti Measurement of the 6Li + (nat)Si Reaction Cross Section at 18 to 28 MeV with a Magnetic Spectrograph and Position-Sensitive Si Detector NUCLEAR REACTIONS, ICPND Si(6Li, X), E=18-28 MeV; measured average reaction σ. Two-dimensional position-sensitive Si detector in magnetic spectrograph focal plane.
doi: 10.1016/0168-9002(92)90503-V
Back to query form Note: The following list of authors and aliases matches the search parameter L.Van Wormer: , L.A.VAN WORMER |