NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = D.Mocelj Found 10 matches. 2007KA46 Nucl.Phys. A788, 136c (2007) Y.Kalmykov, K.Langanke, G.Martinez-Pinedo, D.Mocelj, P.von Neumann-Cosel, I.Poltoratska, V.Yu.Ponomarev, A.Richter, A.Shevchenko, J.Wambach Spin- and Parity-Resolved Level Densities from High-Resolution Hadron and Electron Scattering Studies of Giant Resonances NUCLEAR REACTIONS 90Zr(3He, t), E=140 MeV/nucleon; 90Zr(e, e'), E=42.5, 66.4, 82.3 MeV; 90Zr(p, p'), E=200 MeV; analyzed excitation energy spectra. 90Zr, 90Nb deduced Gamow-Teller resonance and GQR energies and level densities. 58Ni(3He, t), (e, e'), (p, p'), E not given; analyzed excitation energy spectra. 58Ni, 58Cu deduced level densities. Discrete wavelet transform and fluctuation analysis, back-shifted Fermi gas and Hartree-Fock-BCS models.
doi: 10.1016/j.nuclphysa.2007.01.059
2007MA36 Prog.Part.Nucl.Phys. 59, 199 (2007) G.Martinez-Pinedo, D.Mocelj, N.T.Zinner, A.Kelic, K.Langanke, I.Panov, B.Pfeiffer, T.Rauscher, K.-H.Schmidt, F.-K.Thielemann The role of fission in the r-process
doi: 10.1016/j.ppnp.2007.01.018
2007MO15 Phys.Rev. C 75, 045805 (2007) D.Mocelj, T.Rauscher, G.Martinez-Pinedo, K.Langanke, L.Pacearescu, A.Faessler, F.-K.Thielemann, Y.Alhassid Large-scale prediction of the parity distribution in the nuclear level density and application to astrophysical reaction rates NUCLEAR STRUCTURE 56,58,60,62,64,66Fe, 47,48,49,50,66,68,70,72Ni, 66,70Zn, 76,78,80,82Sr, 89Y, 90Zr, 91Nb, 92Mo, 118,120,122,124Sn; calculated parity-projected level density ratios. NUCLEAR REACTIONS 67,69Se(n, γ), (p, γ), E=low; 94Nb, 95Zr(p, γ), E=low; calculated astrophysical reaction rates.
doi: 10.1103/PhysRevC.75.045805
2007TH05 Prog.Part.Nucl.Phys. 59, 74 (2007) F.-K.Thielemann, C.Frohlich, R.Hirschi, M.Liebendorfer, I.Dillmann, D.Mocelj, T.Rauscher, G.Martinez-Pinedo, K.Langanke, K.Farouqi, K.-L.Kratz, B.Pfeiffer, I.Panov, D.K.Nadyozhin, S.Blinnikov, E.Bravo, W.R.Hix, P.Hoflich, N.T.Zinner Production of intermediate-mass and heavy nuclei
doi: 10.1016/j.ppnp.2006.12.019
2007TH10 Int.J.Mod.Phys. E16, 1149 (2007) F.-K.Thielemann, D.Mocelj, I.Panov, E.Kolbe, T.Rauscher, K.-L.Kratz, K.Farouqi, B.Pfeiffer, G.Martinez-Pinedo, A.Kelic, K.Langanke, K.-H.Schmidt, N.Zinner The R-process: Supernovae and other sources of the heaviest elements
doi: 10.1142/S0218301307006587
2005MO27 Nucl.Phys. A758, 154c (2005) D.Mocelj, T.Rauscher, K.Langanke, G.Martinez Pinedo, L.Pacearescu, A.Faessler, F.-K.Thielemann Parity-Dependence in the Nuclear Level Density NUCLEAR STRUCTURE 48Ti, 56Fe, 58Ni, 54,58,62,66,70,74Zn; calculated parity dependent level densities. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2005.05.032
2005MO36 J.Phys.(London) G31, S1927 (2005) D.Mocelj, T.Rauscher, F.-K.Thielemann, G.Martinez Pinedo, K.Langanke, L.Pacearescu, A.Faessler Towards a parity-dependent level density for astrophysics NUCLEAR STRUCTURE 48Ti, 56Fe, 58Ni, 54,58,62,66,70,74Zn; calculated parity ratio of level densities vs excitation energy.
doi: 10.1088/0954-3899/31/10/103
2005TH04 Nucl.Phys. A751, 301c (2005) F.-K.Thielemann, D.Argast, F.Brachwitz, J.L.Fisker, C.Frohlich, R.Hirschi, E.Kolbe, D.Mocelj, T.Rauscher Nuclear Physics: A Key Ingredient in Astrophysical Modeling
doi: 10.1016/j.nuclphysa.2005.02.111
2004RO35 Phys.Rev.Lett. 93, 182501 (2004) D.Rohe, C.S.Armstrong, R.Asaturyan, O.K.Baker, S.Bueltmann, C.Carasco, D.Day, R.Ent, H.C.Fenker, K.Garrow, A.Gasparian, P.Gueye, M.Hauger, A.Honegger, J.Jourdan, C.E.Keppel, G.Kubon, R.Lindgren, A.Lung, D.J.Mack, J.H.Mitchell, H.Mkrtchyan, D.Mocelj, K.Normand, T.Petitjean, O.Rondon, E.Segbefia, I.Sick, S.Stepanyan, L.Tang, F.Tiefenbacher, W.F.Vulcan, G.Warren, S.A.Wood, L.Yuan, M.Zeier, H.Zhu, B.Zihlmann, and the E97-006 Collaboration Correlated Strength in the Nuclear Spectral Function NUCLEAR REACTIONS 12C(e, e'p), E=3.3 GeV; measured Ep, electron spectra; deduced spectral function, correlated strength.
doi: 10.1103/PhysRevLett.93.182501
2003MO25 Nucl.Phys. A718, 650c (2003) D.Mocelj, T.Rauscher, G.Martinez-Pinedo, Y.Alhassid Influence of Parity-Dependence in the nuclear Level Density on the Prediction of Astrophysical Reaction Rates NUCLEAR REACTIONS 64Co, 66Cu, 66Ga(n, p), 63Fe, 65Ni, 65Zn(n, γ), 67Ni, 69Zn, 69Ge(n, α), E=low; calculated astrophysical reaction rates, effects of parity dependence in level density.
doi: 10.1016/S0375-9474(03)00876-5
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