NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = N.Zinner Found 25 matches. 2018HO02 Phys.Rev.Lett. 120, 052502 (2018) D.Hove, E.Garrido, P.Sarriguren, D.V.Fedorov, H.O.U.Fynbo, A.S.Jensen, N.T.Zinner Emergence of Clusters: Halos, Efimov States, and Experimental Signals NUCLEAR STRUCTURE 70,72Ca; calculated rms radii, single-particle energy distributions for neutrons, halo structure parameters.
doi: 10.1103/PhysRevLett.120.052502
2018HO07 J.Phys.(London) G45, 073001 (2018) D.Hove, E.Garrido, P.Sarriguren, D.V.Fedorov, H.O.U.Fynbo, A.S.Jensen, N.T.Zinner Combined few-body and mean-field model for nuclei
doi: 10.1088/1361-6471/aac6de
2018HO08 Phys.Lett. B 782, 42 (2018) D.Hove, E.Garrido, A.S.Jensen, P.Sarriguren, H.O.U.Fynbo, D.V.Fedorov, N.T.Zinner Two-proton capture on the 68Se nucleus with a new self-consistent cluster model NUCLEAR REACTIONS 68Se(2p, γ)70Kr, E not given; calculated E2 electromagnetic two-proton dissociation and capture σ; deduced the temperature dependent capture rates.
doi: 10.1016/j.physletb.2018.05.002
2017HO12 Phys.Rev. C 95, 061301 (2017) D.Hove, E.Garrido, P.Sarriguren, D.V.Fedorov, H.O.U.Fynbo, A.S.Jensen, N.T.Zinner Combined mean-field and three-body model tested on the 26O nucleus NUCLEAR STRUCTURE 26O; calculated ground-state energy, probability distribution of the two valence neutrons in 26O, invariant mass spectra of core neutron, single-particle energy distributions after decay of the ground-state resonance. New self-consistent three-body model (core+two valence neutrons) with meanfield approximation and effective Skyrme interaction. 25,26O; comparison with experimental data.
doi: 10.1103/PhysRevC.95.061301
2016HO04 Phys.Rev. C 93, 024601 (2016) D.Hove, A.S.Jensen, H.O.U.Fynbo, N.T.Zinner, D.V.Fedorov, E.Garrido Capture reactions into Borromean two-proton systems at rp waiting points NUCLEAR REACTIONS 64Ge, 68Se, 72Kr(2p, γ); calculated two-proton radiative capture reaction rates for E1 and E2 photon emissions for temperatures of about 0.1-10 GK using three-body Faddeev formalism for even-even two-proton Borromean systems at prominent intermediate heavy waiting points for the rapid proton (rp) capture process.
doi: 10.1103/PhysRevC.93.024601
2014BE35 Few-Body Systems 55, 847 (2014) F.F.Bellotti, T.Frederico, M.T.Yamashita, D.V.Fedorov, A.S.Jensen, N.T.Zinner Mass-Imbalanced Three-Body Systems in 2D: Bound States and the Analytical Approach to the Adiabatic Potential
doi: 10.1007/s00601-014-0842-2
2014BE36 Few-Body Systems 55, 1025 (2014) F.F.Bellotti, T.Frederico, M.T.Yamashita, D.V.Fedorov, A.S.Jensen, N.T.Zinner Universality of Three-Body Systems in 2D: Parametrization of the Bound States Energies
doi: 10.1007/s00601-014-0845-z
2014HO17 Phys.Rev. C 90, 064311 (2014) D.Hove, D.V.Fedorov, H.O.U.Fynbo, A.S.Jensen, K.Riisager, N.T.Zinner, E.Garrido Borromean structures in medium-heavy nuclei NUCLEAR STRUCTURE 142Ba, 148Nd; calculated low-lying levels, J, π considering Borromean two-alpha structures 134Te+α+α and 140Ba+α+α at the α drip line, spatial structures and probability distribution contours, B(E2), B(E1), charge radii. Adiabatic hyperspherical expansion method for three-body calculations. Comparison with experimental data.
doi: 10.1103/PhysRevC.90.064311
2014HO18 Eur.Phys.J. A 50, 181 (2014) D.Hove, D.V.Fedorov, A.S.Jensen, K.Riisager, N.T.Zinner Assessing the accuracy of Hartree-Fock-Bogoliubov calculations by use of mass relations NUCLEAR STRUCTURE Z=10-112; calculated Q, mass excess using different interactions.
doi: 10.1140/epja/i2014-14181-y
2014MA74 Few-Body Systems 55, 1045 (2014) O.V.Marchukov, A.G.Volosniev, D.V.Fedorov, A.S.Jensen, N.T.Zinner Spin-Orbit Coupling in Deformed Harmonic Traps
doi: 10.1007/s00601-014-0825-3
2014VO10 Few-Body Systems 55, 839 (2014) A.G.Volosniev, D.V.Fedorov, A.S.Jensen, N.T.Zinner, M.Valiente Multicomponent Strongly Interacting Few-Fermion Systems in One Dimension
doi: 10.1007/s00601-013-0776-0
2014ZI02 Few-Body Systems 55, 599 (2014) Few-Body Physics in a Many-Body World
doi: 10.1007/s00601-014-0802-x
2013ZI02 J.Phys.(London) G40, 053101 (2013) Comparing and contrasting nuclei and cold atomic gases
doi: 10.1088/0954-3899/40/5/053101
2010PA41 Astron.Astrophys. 513, A61 (2010) I.V.Panov, I.Yu.Korneev, T.Rauscher, G.MartÃnez-Pinedo, A.Kelic-Heil, N.T.Zinner, F.-K.Thielemann Neutron-induced astrophysical reaction rates for translead nuclei NUCLEAR REACTIONS 235,236,238U, 237Np, 238,239,240,241,242Pu(n, F), (n, γ), E<1 MeV; calculated astrophysical reaction rates. Comparison with JENDL-3.3 library.
doi: 10.1051/0004-6361/200911967
2010PE18 J.Phys.:Conf.Ser. 202, 012008 (2010) I.Petermann, G.Martinez-Pinedo, A.Arcones, W.R.Hix, A.Kelic, K.Langanke, I.Panov, T.Rauscher, K.-H.Schmidt, F.-K.Thielemann, N.Zinner Network calculations for r-process nucleosynthesis
doi: 10.1088/1742-6596/202/1/012008
2008ZI04 Phys.Rev. C 78, 041306 (2008) Nuclear α-particle condensates: Definitions, occurrence conditions, and consequences
doi: 10.1103/PhysRevC.78.041306
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
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
2007ZI01 Nucl.Phys. A781, 81 (2007) Alpha decay rate enhancement in metals: An unlikely scenario RADIOACTIVITY 210Po, 226Ra, 232Th(α); calculated T1/2 corrections for sources embedded in metal.
doi: 10.1016/j.nuclphysa.2006.10.071
2006FR05 Phys.Rev.Lett. 96, 142502 (2006) C.Frohlich, G.Martinez-Pinedo, M.Liebendorfer, F.-K.Thielemann, E.Bravo, W.R.Hix, K.Langanke, N.T.Zinner Neutrino-Induced Nucleosynthesis of A > 64 Nuclei: The νp Process
doi: 10.1103/PhysRevLett.96.142502
2006ZI01 Phys.Rev. C 74, 024326 (2006) N.T.Zinner, K.Langanke, P.Vogel Muon capture on nuclei: Random phase approximation evaluation versus data for 6 ≤ Z ≤ 94 nuclei NUCLEAR REACTIONS Z=6-94(μ-, ν), E at rest; calculated muon capture rates. RPA approach, in-medium renormalization, comparison with data.
doi: 10.1103/PhysRevC.74.024326
2005FR25 Nucl.Phys. A758, 27c (2005) C.Frohlich, P.Hauser, M.Liebendorfer, G.Martinez-Pinedo, E.Bravo, W.R.Hix, N.T.Zinner, F.-K.Thielemann The Innermost Ejecta of Core Collapse Supernovae
doi: 10.1016/j.nuclphysa.2005.05.009
2005KE02 Phys.Lett. B 616, 48 (2005) A.Kelic, N.Zinner, E.Kolbe, K.Langanke, K.-H.Schmidt Cross sections and fragment distributions from neutrino-induced fission on r-process nuclei NUCLEAR REACTIONS 200Yb, 199,215Lu, 202,214Hf, 199Ta, 200W, 201,215Re, 200,214,226Os, 199Ir, 200Pt, 215Au, 216,234Hg, 233Tl, 216Pb, 231,245Bi, 215,233At, 234Rn, 215,233,261Fr, 216,230,246Ra, 215,231Ac, 230,274Th, 216,229,259,275Pa, 216,232,238,246,254,262,270,278,286,294,302U, 231,281Np, 286Pu, 245,275,293Am, 296Cm, 245,259,297Bk, 276,300Cf, 301Es, 246,260,304Fm, 307Md, 276,308No, 261,313Lr, 314Rf, 321Db, 276,322Sg, 261,325Bh, 324Hs, 276Ds, 276Cn(ν, F), (ν, X), (ν, xn), E=spectrum; calculated total, fission, neutron evaporation σ, fission fragment mass distributions.
doi: 10.1016/j.physletb.2005.04.074
2003ZI02 Eur.Phys.J. A 17, 625 (2003) N.T.Zinner, K.Langanke, K.Riisager, E.Kolbe Muon capture on nickel and tin isotopes NUCLEAR REACTIONS 48,50,52,54,56,58,60,62,64,66,68,70,72,74,76,78,80,82,84,86Ni, 100,104,108,112,114,116,118,120,122,124,128,132,136,140,144,148,152,156,160Sn(μ, X), E at rest; calculated muon capture rates; deduced nuclear structure effects.
doi: 10.1140/epja/i2003-10020-8
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