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NSR database version of April 11, 2024.

Search: Author = D.Mocelj

Found 10 matches.

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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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