NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = K.Langanke Found 269 matches. Showing 1 to 100. [Next]2023MA24 Eur.Phys.J. A 59, 67 (2023) G.MartÃnez-Pinedo, K.Langanke Nuclear quests for the r-process
doi: 10.1140/epja/s10050-023-00987-9
2022LY02 Phys.Rev. C 105, 014327 (2022) N.Lyutorovich, V.Tselyaev, J.Speth, G.Martinez-Pinedo, K.Langanke, P.-G.Reinhard Self-consistent description of high-spin states in doubly magic 208Pb NUCLEAR STRUCTURE 208Pb; calculated natural and unnatural high-spin yrast levels of spins from 13-30, energy difference for the first two excited states in each angular momentum channel, discrete RPA (DRPA) results for the energies of the high-spin yrast states, energies and structures of 2p2h, 1p1h+phonon, and two-phonon energies of high spins. Self-consistent phonon-coupling model based on Skyrme functionals, with renormalized time-blocking approximation which evolves coherent one-particle-one-hole states of the random-phase approximation (RPA) to more complex configurations beyond RPA. Comparison with experimental data.
doi: 10.1103/PhysRevC.105.014327
2021CO05 Rev.Mod.Phys. 93, 015002 (2021) J.J.Cowan, C.Sneden, J.E.Lawler, A.Aprahamian, M.Wiescher, K.Langanke, G.Martinez-Pinedo, F.-K.Thielemann Origin of the heaviest elements: The rapid neutron-capture process
doi: 10.1103/RevModPhys.93.015002
2020DZ01 Phys.Rev. C 101, 025805 (2020) AlanA.Dzhioev, K.Langanke, G.Martinez-Pinedo, A.I.Vdovin, Ch.Stoyanov Unblocking of stellar electron capture for neutron-rich N=50 nuclei at finite temperature NUCLEAR STRUCTURE 78Ni, 82Ge, 86Kr, 88Sr; calculated electron-capture rates on neutron-rich nuclei at conditions of temperatures and densities relevant for collapse supernovae, GT+ strengths, neutron and proton single-particle energies, relative contribution of first forbidden transitions to the electron-capture rates. Thermal quasiparticle random-phase approximation (TQRPA) formalism.
doi: 10.1103/PhysRevC.101.025805
2019KI08 Phys.Rev.Lett. 123, 262701 (2019) O.S.Kirsebom, S.Jones, D.F.Stromberg, G.Martinez-Pinedo, K.Langanke, F.K.Ropke, B.A.Brown, T.Eronen, H.O.U.Fynbo, M.Hukkanen, A.Idini, A.Jokinen, A.Kankainen, J.Kostensalo, I.Moore, H.Moller, S.T.Ohlmann, H.Penttila, K.Riisager, S.Rinta-Antila, P.C.Srivastava, J.Suhonen, W.H.Trzaska, J.Aysto Discovery of an Exceptionally Strong β-Decay Transition of 20F and Implications for the Fate of Intermediate-Mass Stars RADIOACTIVITY 20F(β-) [from 19F(d, X), E=6 MeV]; measured decay products, Eβ, Iβ; deduced transition strength.
doi: 10.1103/PhysRevLett.123.262701
2019LA23 Eur.Phys.J. A 55, 226 (2019) The role of giant resonances in nuclear astrophysics: An overview
doi: 10.1140/epja/i2019-12760-0
2015ME10 Phys.Rev. C 92, 055805 (2015) J.Mendoza-Temis, M.-R.Wu, K.Langanke, G.Martinez-Pinedo, A.Bauswein, H.-T.Janka Nuclear robustness of the r process in neutron-star mergers ATOMIC MASSES A=108-288; calculated r-process abundances of slow ejecta for different mass models at different phases of the evolution in neutron star mergers using three-dimensional relativistic smoothed particle hydrodynamic simulation, and extended nuclear network of 7300 nuclei from free nucleons up to 313Ds, including spontaneous, β- and neutron-induced fission, fission yield distributions from the ABLA code. Comparison with observed r-process abundances. NUCLEAR REACTIONS 278Am(n, F); calculated fission fragment distributions as functions of charge, neutron number, and mass number for neutron using the ABLA code.
doi: 10.1103/PhysRevC.92.055805
2014KU23 Eur.Phys.J. A 50, 135 (2014) T.Kurtukian-Nieto, J.Benlliure, K.-H.Schmidt, L.Audouin, F.Becker, B.Blank, I.N.Borzov, E.Casarejos, F.Farget, M.Fernandez-Ordonez, J.Giovinazzo, D.Henzlova, B.Jurado, K.Langanke, G.Martinez-Pinedo, J.Pereira, O.Yordanov Beta-decay half-lives of new neutron-rich isotopes of Re, Os and Ir approaching the r-process path near N = 126
doi: 10.1140/epja/i2014-14135-5
2014LA18 Nucl.Phys. A928, 305 (2014) The role of electron capture in core-collapse supernovae NUCLEAR REACTIONS 20Ne(e, γ), T=0.4 GK; calculated electron capture rates vs density. Compared with Takahara data. NUCLEAR REACTIONS 45Sc, 48Ti, 50,51V, 54,56Fe, 55Mn, 58,60,62,64Ni, 58Co, 64Zn(e, γ), T=3-10 GK; calculated electron capture rates using large-scale shell model and within QRPA. Compared with some reaction data. NUCLEAR STRUCTURE A=12-70; calculated solar abundances using different electron capture rates, B(GT+) transition strength across N=40 the shell gap. Compared with data.
doi: 10.1016/j.nuclphysa.2014.04.015
2014MA25 Phys.Rev. C 89, 045806 (2014) G.Martinez-Pinedo, Y.H.Lam, K.Langanke, R.G.T.Zegers, C.Sullivan Astrophysical weak-interaction rates for selected A = 20 and A= 24 nuclei NUCLEAR REACTIONS 20Ne, 20F, 24Mg, 24Na(e-, ν), at T=0.1-10 GK; calculated electron capture rates and β- decay rates of 20F and 24Na at temperature and density conditions in the late-evolution stages of stars with 8-12 time the solar masses using recent experimental data and large-scale shell-model calculations. Comparison with other theoretical calculations. Analytical expressions for electron capture and β-decay rates. RADIOACTIVITY 20F, 24Na(β-)[from electron capture in 20Ne and 24Mg in stellar environments]; calculated β- decay rates at temperature and density conditions in the late-evolution stages using recent experimental data and large-scale shell-model calculations. Comparison with other theoretical calculations. Analytical expressions β-decay rates.
doi: 10.1103/PhysRevC.89.045806
2013FI11 Phys.Rev. C 88, 065804 (2013) T.Fischer, K.Langanke, G.Martinez-Pinedo Neutrino-pair emission from nuclear de-excitation in core-collapse supernova simulations
doi: 10.1103/PhysRevC.88.065804
2013LA05 Phys.Scr. T152, 014011 (2013) The role of radioactive ion beams in nuclear astrophysics
doi: 10.1088/0031-8949/2013/T152/014011
2013ZH05 Phys.Rev. C 87, 025803 (2013) Q.Zhi, E.Caurier, J.J.Cuenca-Garcia, K.Langanke, G.Martinez-Pinedo, K.Sieja Shell-model half-lives including first-forbidden contributions for r-process waiting-point nuclei RADIOACTIVITY 129,131In, 205Au, 205,206Hg, 206,207Tl(β-); calculated logft, first-forbidden shape factors. 74Cr, 75Mn, 76Fe, 77Co, 78Ni, 79Cu, 80Zn, 81Ga, 82Ge, 124Mo, 125Tc, 126Ru, 127Rh, 128Pd, 129Ag, 130Cd, 131In, 192Dy, 193Ho, 194Er, 195Tm, 196Yb, 197Lu, 198Hf, 199Ta(β-), (β-n); calculated Q(β) values, T1/2, beta-delayed neutron emission probabilities, first-forbidden transition components, partial decay rates for N=50, Z=24-32; N=82, Z=42-49; N=126, Z=66-73 r-process waiting-point nuclei. Large-scale shell-model calculations. Comparison with other model calculations, and with experimental data.
doi: 10.1103/PhysRevC.87.025803
2012ER01 Phys.Rev. C 85, 025802 (2012) J.Erler, K.Langanke, H.P.Loens, G.Martinez-Pinedo, P.-G.Reinhard Fission properties for r-process nuclei NUCLEAR STRUCTURE 250,252,254,256,258No, 254,256,258,260Rf, 258,260,262,264,266Sg, 264,266Hs, 284Cn, 288Fl; calculated half-lives and fission barriers with three different Skyrme parameterizations. Comparison with experimental data. Z=82-120, N=120-260; calculated fission barriers of even-even nuclei for four different Skyrme parameterizations and four theoretical mass models HFB-14, ETFSI, FRDM, and TF. Z=100-120, N=120-260; calculated fission half-lives for even-even nuclei using the Skyrme parameterizations, minimal lifetime plots for competing α decay and spontaneous fission. Comparison with experimental data. Z=84-120, N=120-260; calculated α-decay half-lives using the Q(α) values and the semi empirical Viola-Seaborg formula. Z=96-108, N=180-206; calculated difference of ground state energies and fission barriers between reflection symmetric and asymmetric configurations with the Skyrme parameterization, comparison of symmetric and asymmetric fission barriers and half-lives. 286,294Rf; calculated PES for symmetric and asymmetric shapes with the Skyrme parameterization.
doi: 10.1103/PhysRevC.85.025802
2012LA30 J.Phys.:Conf.Ser. 381, 012016 (2012) Supernova Dynamics and Explosive Nucleosynthesis
doi: 10.1088/1742-6596/381/1/012016
2012LO04 Eur.Phys.J. A 48, 34 (2012) H.P.Loens, K.Langanke, G.Martinez-Pinedo, K.Sieja M1 strength functions from large-scale shell-model calculations and their effect on astrophysical neutron capture cross-sections NUCLEAR STRUCTURE 54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70Fe; calculated M1 transition strength distribution for ground state and low-lying states using shell model with 40,48Ca core and KB3Gmod interaction. Compared with single-particle calculation and Kopecky formula. NUCLEAR REACTIONS 53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69Fe(n, γ), E=0.001-1 MeV; calculated M1 σ. Compared with single-particle calculation and Kopecky formula.
doi: 10.1140/epja/i2012-12034-5
2012NE08 J.Phys.:Conf.Ser. 337, 012055 (2012) T.Neff, H.Feldmeier, K.Langanke Microscopic calculation of the 3He(α, γ)7Be reaction rate using realistic interactions NUCLEAR REACTIONS 3H, 3He(α, γ), E(cm)≈0.2-2.5 MeV; calculated S-factor, γ dipole strength using FMD (fermionic molecular dynamics). Compared with data.
doi: 10.1088/1742-6596/337/1/012055
2012PE14 Eur.Phys.J. A 48, 122 (2012) I.Petermann, K.Langanke, G.Martinez-Pinedo, I.V.Panov, P.-G.Reinhard, F.-K.Thielemann Have superheavy elements been produced in nature? NUCLEAR STRUCTURE Z=84-120; calculated fission barrier, neutron Q-value using ETF (extended Thomas-Fermi) and FRDM (finite-range droplet model). NUCLEAR REACTIONS Z=56-110(n, γ), E=low; calculated r-process yields using barriers from ETF and FRDM.
doi: 10.1140/epja/i2012-12122-6
2012SM07 Phys.Rev. C 86, 044604 (2012) C.Smorra, T.R.Rodriguez, T.Beyer, K.Blaum, M.Block, Ch.E.Dullmann, K.Eberhardt, M.Eibach, S.Eliseev, K.Langanke, G.Martinez-Pinedo, Sz.Nagy, W.Nortershauser, D.Renisch, V.M.Shabaev, I.I.Tupitsyn, N.A.Zubova Q value and half-life of double-electron capture in 184Os ATOMIC MASSES 184Os, 184W; measured time-of-flight and cyclotron frequency ratios using Penning-trap mass spectrometer TRIGA-TRAP; deduced mass excess, Q value for 2β decay. RADIOACTIVITY 184Os(2EC); measured Q-value using Penning-trap; calculated nuclear matrix element, T1/2. Energy density functional (EDF) calculations.
doi: 10.1103/PhysRevC.86.044604
2011AD03 Rev.Mod.Phys. 83, 195 (2011) E.G.Adelberger, A.Garcia, R.G.H.Robertson, K.A.Snover, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, D.Bemmerer, A.Junghans, D.Bemmerer, A.Junghans, C.A.Bertulani, K.-W.Chen, H.Costantini, P.Prati, M.Couder, E.Uberseder, M.Wiescher, R.Cyburt, B.Davids, S.J.Freedman, M.Gai, D.Gazit, L.Gialanella, G.Imbriani, U.Greife, M.Hass, W.C.Haxton, T.Itahashi, K.Kubodera, K.Langanke, D.Leitner, M.Leitner, P.Vetter, L.Winslow, L.E.Marcucci, T.Motobayashi, A.Mukhamedzhanov, R.E.Tribble, F.M.Nunes, T.-S.Park, R.Schiavilla, E.C.Simpson, C.Spitaleri, F.Strieder, H.-P.Trautvetter, K.Suemmerer, S.Typel Solar fusion cross sections. II. The pp chain and CNO cycles NUCLEAR REACTIONS 2H(p, γ), 3He(3He, 2p), (α, γ), (p, e), 7Be, 12C, 14N, 15N, 17O(p, γ), 15N, 16,17,18O(p, α), E<3 MeV; analyzed and evaluated experimental data; deduced recommended values and uncertainties.
doi: 10.1103/RevModPhys.83.195
2011HU03 Eur.Phys.J. A 47, 10 (2011) L.Huther, H.P.Loens, G.Martinez-Pinedo, K.Langanke s-process stellar enhancement factors obtained within the statistical model with parity-dependent level densities NUCLEAR REACTIONS 204Pb(n, γ), E=0.086 eV-860 keV; calculated σ, reaction rates. A=24-210(n, γ), E=8, 30, 90 keV; calculated s-process reaction rates, stellar enhancement factors. Hilaire-Goriely and BSFG densities with parity.
doi: 10.1140/epja/i2011-11010-y
2011MA47 Eur.Phys.J. A 47, 98 (2011) G.Martinez-Pinedo, B.Ziebarth, T.Fischer, K.Langanke Effect of collective neutrino flavor oscillations on νp-process nucleosynthesis
doi: 10.1140/epja/i2011-11098-y
2011NE02 Prog.Part.Nucl.Phys. 66, 341 (2011) T.Neff, H.Feldmeier, K.Langanke Towards microscopic ab initio calculations of astrophysical S-factors NUCLEAR REACTIONS 3H, 3He(α, γ), E<2.5 MeV; calculated S-factors, p-wave scattering phase shifts, dipole strengths. Fermionic Molecular Dynamics, Argonne V18 potential.
doi: 10.1016/j.ppnp.2011.01.031
2011TH01 Prog.Part.Nucl.Phys. 66, 346 (2011) F.-K.Thielemann, A.Arcones, R.Kappeli, M.Liebendorfer, T.Rauscher, C.Winteler, C.Frohlich, I.Dillmann, T.Fischer, G.Martinez-Pinedo, K.Langanke, K.Farouqi, K.-L.Kratz, I.Panov, I.K.Korneev What are the astrophysical sites for the r-process and the production of heavy elements?
doi: 10.1016/j.ppnp.2011.01.032
2011ZH17 Nucl.Phys. A859, 172 (2011) Q.Zhi, K.Langanke, G.Martinez Pinedo, F.Nowacki, K.Sieja The 76Se Gamow-Teller strength distribution and its importance for stellar electron capture rates RADIOACTIVITY 76Se(EC); calculated β-decay B(GT) strength using shell model with RG interaction.
doi: 10.1016/j.nuclphysa.2011.04.010
2010DE35 Phys.Rev.Lett. 105, 212504 (2010) D.J.Dean, K.Langanke, H.Nam, W.Nazarewicz Pairing Reentrance Phenomenon in Heated Rotating Nuclei in the Shell-Model Monte Carlo Approach NUCLEAR STRUCTURE 72Ge; calculated rotational motion of heated nucleus, neutron occupation, pairing strength, angular momentum. Microscopic shell-model Monte Carlo approach.
doi: 10.1103/PhysRevLett.105.212504
2010DZ02 Phys.Rev. C 81, 015804 (2010) A.A.Dzhioev, A.I.Vdovin, V.Yu.Ponomarev, J.Wambach, K.Langanke, G.Martinez-Pinedo Gamow-Teller strength distributions at finite temperatures and electron capture in stellar environments NUCLEAR STRUCTURE 54,56Fe, 76,78,80Ge; calculated Gammow-Teller strength distributions, electron capture rates, strength distributions for first forbidden transitions, and occupation numbers in hot nuclei in stellar environments using thermal quasiparticle random-phase approximation (TQRPA) model. Comparison with experimental data and large-scale shell-model (LSSM) calculations.
doi: 10.1103/PhysRevC.81.015804
2010JU04 Nucl.Phys. A848, 454 (2010) A.Juodagalvis, K.Langanke, W.R.Hix, G.Martinez-Pinedo, J.M.Sampaio Improved estimate of electron capture rates on nuclei during stellar core collapse
doi: 10.1016/j.nuclphysa.2010.09.012
2010KI02 Phys.Rev. C 81, 025802 (2010) L.-T.Kizivat, G.Martinez-Pinedo, K.Langanke, R.Surman, G.C.McLaughlin ψ-ray bursts black hole accretion disks as a site for the νp process
doi: 10.1103/PhysRevC.81.025802
2010LA10 Nucl.Phys. A834, 608c (2010) Nuclear input for supernova simulations and nucleosynthesis
doi: 10.1016/j.nuclphysa.2010.01.105
2010PE01 Phys.Rev. C 81, 014308 (2010) I.Petermann, K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, F.Nowacki, A.Richter Scales in the fine structure of the magnetic dipole resonance: A wavelet approach to the shell model NUCLEAR STRUCTURE 50Ti, 52Cr, 54,56Fe; calculated M1 strength distributions, and power spectra using shell model and KB3G interaction. Comparison with experimental data from (e, e') reactions.
doi: 10.1103/PhysRevC.81.014308
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
2010TH06 J.Phys.:Conf.Ser. 202, 012006 (2010) F.-K.Thielemann, I.Dillmann, K.Farouqi, T.Fischer, C.Frohlich, A.Kelic-Heil, I.Korneev, K.-L.Kratz, K.Langanke, M.Liebendorfer, I.V.Panov, G.Martinez-Pinedo, T.Rauscher The r-, p-, and νp-Process NUCLEAR REACTIONS 252Cf(n, F), E=0.002-20 MeV; calculated fission σ using different barrier predicions. Compared with data and JENDL-3.3. A≈220-260(n, F), E not given; calculated fission σ using different barrier predictions. Compared with data.
doi: 10.1088/1742-6596/202/1/012006
2009KU28 Nucl.Phys. A827, 587c (2009) T.Kurtukian-Nieto, J.Benlliure, K.-H.Schmidt, L.Audouin, F.Becker, B.Blank, I.N.Borzov, E.Casarejos, M.Fernandez-Ordonez, J.Giovinazzo, D.Henzlova, B.Jurado, K.Langanke, G.Martinez-Pinedo, J.Pereira, F.Rejmund, O.Yordanov Recent progress in measuring β half-lives of nuclei approaching the r-process waiting point A = 195 RADIOACTIVITY 194,195,196Re, 199,200Os, 198,199,200Ir(β-) [from Be(208Pb, X), E=1 GeV/nucleon]; measured T1/2. Comparison with two QRPA models.
doi: 10.1016/j.nuclphysa.2009.05.129
2009LI13 Nucl.Phys. A823, 26 (2009) E.Litvinova, H.P.Loens, K.Langanke, G.Martinez-Pinedo, T.Rauscher, P.Ring, F.-K.Thielemann, V.Tselyaev Low-lying dipole response in the relativistic quasiparticle time blocking approximation and its influence on neutron capture cross sections NUCLEAR STRUCTURE 106,116,132,140Sn; calculated E1 strength function using microscopic quasiparticle time blocking approximation. Comparison with other models. NUCLEAR REACTIONS 105,115,131,139Sn(n, γ), E=0.001-20 MeV; calculated σ. 67,69,71,73,75,77Ni, 105,109,113,115,119,123,129,131,133,135,137,139Sn(n, γ), E≈80-100 keV; calculated stellar capture rate ratio between various models.
doi: 10.1016/j.nuclphysa.2009.03.009
2009LI20 Phys.Rev. C 79, 054312 (2009) E.Litvinova, P.Ring, V.Tselyaev, K.Langanke Relativistic quasiparticle time blocking approximation. II. Pygmy dipole resonance in neutron-rich nuclei NUCLEAR STRUCTURE 68,70,72,74,76,78Ni, 116,118,120,122,124,126,128,130,132,134,136,138,140Sn, 208Pb; calculated dipole excitation spectra, σ, proton and neutron transition densities, pygmy strength, mean energies for giant dipole resonance (GDR) and pygmy dipole resonance (PDR) using relativistic quasiparticle random-phase approximation (RQRPA) and relativistic quasiparticle time-blocking approximation (RQTBA). Comparison with experimental data.
doi: 10.1103/PhysRevC.79.054312
2009SI14 Phys.Rev. C 79, 064310 (2009); Erratum Phys.Rev. C 80, 019905 (2009) K.Sieja, F.Nowacki, K.Langanke, G.Martinez-Pinedo Shell model description of zirconium isotopes NUCLEAR STRUCTURE 90,91,92,93,94,95,96,97,98Zr; calculated B(E2), B(M1), levels, occupation numbers, and g-factors using shell model. Comparison with experimental data.
doi: 10.1103/PhysRevC.79.064310
2008AR06 Phys.Rev. C 78, 015806 (2008) A.Arcones, G.Martinez-Pinedo, E.O'Connor, A.Schwenk, H.-Th.Janka, C.J.Horowitz, K.Langanke Influence of light nuclei on neutrino-driven supernova outflows NUCLEAR REACTIONS 3H(ν-bar, ν-bar), (ν-bar, e+), E=11-100 MeV; calculated σ.
doi: 10.1103/PhysRevC.78.015806
2008BA08 Phys.Rev. C 77, 024304 (2008) C.Barbieri, E.Caurier, K.Langanke, G.Martinez-Pinedo Pygmy dipole response of proton-rich argon nuclei in random-phase approximation and no-core shell model NUCLEAR STRUCTURE 32,34Ar; calculated B(E1), isovector dipole strength.particle transition energies. Investigated pygmy dipole resonances.
doi: 10.1103/PhysRevC.77.024304
2008BA36 Phys.Rev. C 78, 039802 (2008) C.Barbieri, E.Caurier, K.Langanke, G.Martinez-Pinedo Reply to "Comment on `Pygmy dipole response of proton-rich argon nuclei in random-phase approximation and no-core shell model'"
doi: 10.1103/PhysRevC.78.039802
2008BO35 Nucl.Phys. A814, 159 (2008) I.N.Borzov, J.J.Cuenca-Garcia, K.Langanke, G.Martinez-Pinedo, F.Montes Beta-decay of Z < 50 nuclei near the N = 82 closed neutron shell RADIOACTIVITY Zr, Nb, Mo, Tc, Ru, Rh, Pd, Ag, Cd, In(β-); calculated β-decay Q-values, T1/2 using QRPA with local energy-density functional theory. Comparison with other models and data.
doi: 10.1016/j.nuclphysa.2008.09.010
2008GR10 Phys.Rev. C 77, 064303 (2008) E.-W.Grewe, C.Baumer, H.Dohmann, D.Frekers, M.N.Harakeh, S.Hollstein, H.Johansson, K.Langanke, G.Martinez-Pinedo, F.Nowacki, I.Petermann, L.Popescu, S.Rakers, D.Savran, K.Sieja, H.Simon, J.H.Thies, A.M.van den Berg, H.J.Wortche, A.Zilges Studies on the double-β decay nucleus 64Zn using the (d, 2He) reaction NUCLEAR REACTIONS 64Zn(d, 2He), E=183 MeV; measured charged particle energies, angular distributions, σ(θ). 64Cu; deduced levels, J, π, Gamow-Teller strengths. 64Ni(3He, t); analyzed Gamow-Teller strength distribution. Comparison with shell model calculations.
doi: 10.1103/PhysRevC.77.064303
2008JU03 J.Phys.(London) G35, 014031 (2008) A.Juodagalvis, J.M.Sampaio, K.Langanke, W.R.Hix Extended pool of electron-capture rates for core-collapse supernovae simulations
doi: 10.1088/0954-3899/35/1/014031
2008WE10 Phys.Rev. C 78, 054310 (2008) C.Weber, V.-V.Elomaa, R.Ferrer, C.Frohlich, D.Ackermann, J.Aysto, G.Audi, L.Batist, K.Blaum, M.Block, A.Chaudhuri, M.Dworschak, S.Eliseev, T.Eronen, U.Hager, J.Hakala, F.Herfurth, F.P.Hessberger, S.Hofmann, A.Jokinen, A.Kankainen, H.-J.Kluge, K.Langanke, A.Martin, G.Martinez-Pinedo, M.Mazzocco, I.D.Moore, J.B.Neumayr, Yu.N.Novikov, H.Penttila, W.R.Plass, A.V.Popov, S.Rahaman, T.Rauscher, C.Rauth, J.Rissanen, D.Rodriguez, A.Saastamoinen, C.Scheidenberger, L.Schweikhard, D.M.Seliverstov, T.Sonoda, F.-K.Thielemann, P.G.Thirolf, G.K.Vorobjev Mass measurements in the vicinity of the r p-process and the ν p-process paths with the Penning trap facilities JYFLTRAP and SHIPTRAP ATOMIC MASSES 84Y, 87Zr, 88,89Mo, 88,89,90,91,92Tc, 90,91,92,93Ru, 92,93,94,95Rh, 94,95,95m,96Pd; measured masses. Comparison with evaluated data.
doi: 10.1103/PhysRevC.78.054310
2007BY02 Phys.Rev.Lett. 98, 082501 (2007) A.Byelikov, T.Adachi, H.Fujita, K.Fujita, Y.Fujita, K.Hatanaka, A.Heger, Y.Kalmykov, K.Kawase, K.Langanke, G.Martinez-Pinedo, K.Nakanishi, P.von Neumann-Cosel, R.Neveling, A.Richter, N.Sakamoto, Y.Sakemi, A.Shevchenko, Y.Shimbara, Y.Shimizu, F.D.Smit, Y.Tameshige, A.Tamii, S.E.Woosley, M.Yosoi Gamow-Teller Strength in the Exotic Odd-Odd Nuclei 138La and 180Ta and Its Relevance for Neutrino, Nucleosynthesis NUCLEAR REACTIONS 138Ba, 180Hf(3He, t), E=140 MeV/nucleon; measured particle spectra. 138La, 180Ta deduced Gamow-Teller strength distributions. Implications for stellar nucleosynthesis discussed.
doi: 10.1103/PhysRevLett.98.082501
2007CU03 Eur.Phys.J. A 34, 99 (2007) J.J.Cuenca-Garcia, G.Martinez-Pinedo, K.Langanke, F.Nowacki, I.N.Borzov Shell model half-lives for r-process N = 82 nuclei RADIOACTIVITY 124Mo, 125Tc, 126Ru, 127Rh, 128Pd, 129Ag, 130Cd, 131In(β-); calculated T1/2, Q-values, Gamow-Teller strength distributions, two-neutron separation energies and one-neutron emission probabilities using a shell model with enlarged model space. Comparison with other models and data.
doi: 10.1140/epja/i2007-10477-3
2007FU04 Phys.Rev. C 75, 034310 (2007) H.Fujita, Y.Fujita, T.Adachi, A.D.Bacher, G.P.A.Berg, T.Black, E.Caurier, C.C.Foster, H.Fujimura, K.Hara, K.Harada, K.Hatanaka, J.Janecke, J.Kamiya, Y.Kanzaki, K.Katori, T.Kawabata, K.Langanke, G.Martinez-Pinedo, T.Noro, D.A.Roberts, H.Sakaguchi, Y.Shimbara, T.Shinada, E.J.Stephenson, H.Ueno, T.Yamanaka, M.Yoshifuku, M.Yosoi Isospin structure of Jπ = 1+ states in 58Ni and 58Cu studied by 58Ni(p, p') and 58Ni(3He, t)58Cu measurements NUCLEAR REACTIONS 58Ni(p, p'), E=160 MeV; measured Ep, σ(θ=0°). 58Ni(3He, t), E=140 MeV/nucleon; measured triton spectra, σ(θ=0°). 58Ni, 58Cu deduced 1+ level energies, B(GT), isospin symmetry features. Comparison with shell model predictions.
doi: 10.1103/PhysRevC.75.034310
2007GR19 Rep.Prog.Phys. 70, 1525 (2007) H.Grawe, K.Langanke, G.Martinez-Pinedo Nuclear structure and astrophysics NUCLEAR STRUCTURE Li, Sn; A=60, 80, 130, 140, 195, 208; analyzed level energies, single particle energies, and spectroscopic factors. Discussed astrophysical *implications.
doi: 10.1088/0034-4885/70/9/R02
2007JU05 Phys.Rev.Lett. 99, 132501 (2007) A.Jungclaus, L.Caceres, M.Gorska, M.Pfutzner, S.Pietri, E.Werner-Malento, H.Grawe, K.Langanke, G.Martinez-Pinedo, F.Nowacki, A.Poves, J.J.Cuenca-Garcia, D.Rudolph, Z.Podolyak, P.H.Regan, P.Detistov, S.Lalkovski, V.Modamio, J.Walker, P.Bednarczyk, P.Doornenbal, H.Geissel, J.Gerl, J.Grebosz, I.Kojouharov, N.Kurz, W.Prokopowicz, H.Schaffner, H.J.Wollersheim, K.Andgren, J.Benlliure, G.Benzoni, A.M.Bruce, E.Casarejos, B.Cederwall, F.C.L.Crespi, B.Hadinia, M.Hellstrom, R.Hoischen, G.Ilie, J.Jolie, A.Khaplanov, M.Kmiecik, R.Kumar, A.Maj, S.Mandal, F.Montes, S.Myalski, G.S.Simpson, S.J.Steer, S.Tashenov, O.Wieland Observation of Isomeric Decays in the r-Process Waiting-Point Nucleus 130Cd82 RADIOACTIVITY 130Cd(IT) [from Be(136Xe, 6n), E=750 MeV/nucleon]; measured Eγ, Iγ, γγ-coinc. 130Cd deduced levels, J, π.
doi: 10.1103/PhysRevLett.99.132501
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
2007KA58 Phys.Rev.Lett. 99, 202502 (2007) Y.Kalmykov, C.Ozen, K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, A.Richter Spin- and Parity-Resolved Level Densities from the Fine Structure of Giant Resonances NUCLEAR REACTIONS 58Ni, 90Zr(p, p'), (e, e'), E not given; 90Zr(3He, t), E not given; analyzed cross sections. deduced level densities.
doi: 10.1103/PhysRevLett.99.202502
2007LA15 Prog.Part.Nucl.Phys. 59, 66 (2007) K.Langanke, H.Feldmeier, G.Martinez-Pinedo, T.Neff Astrophysically important nuclear reactions
doi: 10.1016/j.ppnp.2006.12.010
2007LI37 Acta Phys.Pol. B38, 1359 (2007) A.F.Lisetskiy, E.Caurier, K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, F.Nowacki, A.Richter sd - pf Shell Model Studies of M1 Strength in Ar Isotopes NUCLEAR STRUCTURE 36,38Ar; calculated B(M1) distribution as a function of excitation energy using the nuclear shell model.
2007LI56 Nucl.Phys. A789, 114 (2007) A.F.Lisetskiy, E.Caurier, K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, F.Nowacki, A.Richter Magnetic dipole probes of the sd and pf shell crossing in the 36, 38Ar isotopes NUCLEAR STRUCTURE 36,38Ar; calculated level energies, J, π, and magnetic dipole strength distributions within a large scale shell model study.
doi: 10.1016/j.nuclphysa.2007.01.074
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
2007OZ03 Phys.Rev. C 75, 064307 (2007) C.Ozen, K.Langanke, G.Martinez-Pinedo, D.J.Dean Parity-projected shell model Monte Carlo level densities for fp-shell nuclei NUCLEAR STRUCTURE 58,62,65,66Fe, 58,59Ni; calculated level densities, occupation numbers and pairing strength for neutrons using shell model monte carlo method.
doi: 10.1103/PhysRevC.75.064307
2007PE35 Eur.Phys.J. A 34, 319 (2007) I.Petermann, G.Martinez-Pinedo, K.Langanke, E.Caurier Breaking of the SU(4) limit for the Gamow-Teller strength in N ∼ Z nuclei NUCLEAR STRUCTURE 46,48,50Ti, 50,52,54Cr, 54,56,58Fe, 62Ge; calculated Gamow-Teller strength distributions with a large-scale shell model.
doi: 10.1140/epja/i2007-10502-7
2007SC26 Phys.Rev. C 75, 064321 (2007) C.Scholl, P.Petkov, V.Werner, A.Linnemann, T.Adachi, A.Dewald, A.Fitzler, C.Fransen, Y.Fujita, J.Jolie, K.Langanke, A.F.Lisetskiy, G.Martinez-Pinedo, D.Mucher, J.N.Orce, N.Pietralla, N.Warr, K.O.Zell, P.von Brentano New spin assignments in the odd-odd N = Z nucleus 42Sc and the breaking of the 40Ca core NUCLEAR REACTIONS 40Ca(3He, p)42Sc, E=9 MeV; measured Eγ, Iγ, γγ-coinc, and angular correlations. 42Sc deduced levels, J, π, B(E2), B(M1), multipole mixing ratios. Compared results to model calculations.
doi: 10.1103/PhysRevC.75.064321
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
2006CA23 Phys.Lett. B 639, 32 (2006) W.Cassing, M.Kant, K.Langanke, P.Vogel Transport study of charged current interactions in neutrino-nucleus reactions NUCLEAR REACTIONS 1n, 1H(ν, μ-X), E=0.4-2.0 GeV; 12C(ν, μ-X), E=0.5-1.5 GeV; calculated π+ production σ. 12C, 56Fe(ν, μ-X), E=1.0 GeV; calculated pion spectra. Dynamical transport model, final state interactions discussed.
doi: 10.1016/j.physletb.2006.03.074
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
2006GR20 Phys.Lett. B 641, 254 (2006) L.V.Grigorenko, K.Langanke, N.B.Shulgina, M.V.Zhukov Soft dipole mode in 17Ne and the astrophysical 2p capture on 15O NUCLEAR STRUCTURE 16F, 17Ne; calculated level energies, E1 transitions strength function. Three-body model. NUCLEAR REACTIONS Au, Pb(17Ne, 15OX), E=50, 240, 500 MeV/nucleon; calculated two-proton removal σ. Two-proton capture rates in astrophysical conditions discussed.
doi: 10.1016/j.physletb.2006.08.054
2006LA04 Prog.Part.Nucl.Phys. 57, 324 (2006) Neutrino-nucleus reactions in core-collapse supernovae
doi: 10.1016/j.ppnp.2005.11.027
2006LA24 Nucl.Phys. A778, 233 (2006) Shell model Monte Carlo studies of pairing correlations and level densities in medium-mass nuclei NUCLEAR STRUCTURE 70,71Ga, 72,75Ge, 76As, 80Zr; calculated level densities, pairing strength distributions. Shell model Monte Carlo approach.
doi: 10.1016/j.nuclphysa.2006.08.005
2006LA29 Phys.Scr. T125, 26 (2006) Shell model and supernovae
doi: 10.1088/0031-8949/2006/T125/006
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
2005AP02 Prog.Part.Nucl.Phys. 54, 535 (2005) A.Aprahamian, K.Langanke, M.Wiescher Nuclear structure aspects in nuclear astrophysics
doi: 10.1016/j.ppnp.2004.09.002
2005BA14 Phys.Rev. C 71, 024603 (2005); Erratum Phys.Rev. C 71, 029903 (2005) C.Baumer, A.M.van den Berg, B.Davids, D.Frekers, D.De Frenne, E.-W.Grewe, P.Haefner, M.N.Harakeh, F.Hofmann, S.Hollstein, M.Hunyadi, M.A.de Huu, E.Jacobs, B.C.Junk, A.Korff, K.Langanke, G.Martinez-Pinedo, A.Negret, P.von Neumann-Cosel, L.Popescu, S.Rakers, A.Richter, H.J.Wortche Determination of the Gamow-Teller strength distribution from the odd-odd nucleus 50V measured through 50V(d, 2He)50Ti and astrophysical implications NUCLEAR REACTIONS 50V(d, 2p), E=171 MeV; measured Ep, pp-coin, σ(E, θ). 50V deduced Gamow-Teller strength distribution. Comparison with model predictions.
doi: 10.1103/PhysRevC.71.024603
2005HA03 Phys.Rev. C 71, 014606 (2005) M.Hagemann, C.Baumer, A.M.van den Berg, D.De Frenne, D.Frekers, V.M.Hannen, M.N.Harakeh, J.Heyse, M.A.de Huu, E.Jacobs, K.Langanke, G.Martinez-Pinedo, A.Negret, L.Popescu, S.Rakers, R.Schmidt, H.J.Wortche Spin-isospin excitations in the medium-mass nucleus 58Co investigated with the (d, 2He) reaction NUCLEAR REACTIONS 58Ni(d, 2p), E=170 MeV; measured Ep, pp-coin, σ(E, θ). 58Co deduced levels, Gamow-Teller strengths, related features. 58Ni, 58Co deduced analog states Coulomb displacement energy. Comparison with large-scale shell model calculations.
doi: 10.1103/PhysRevC.71.014606
2005HE02 Phys.Lett. B 606, 258 (2005) A.Heger, E.Kolbe, W.C.Haxton, K.Langanke, G.Martinez-Pinedo, S.E.Woosley Neutrino nucleosynthesis
doi: 10.1016/j.physletb.2004.12.017
2005HI18 Nucl.Phys. A758, 31c (2005) W.R.Hix, O.E.B.Messer, A.Mezzacappa, J.Sampaio, K.Langanke, G.Martinez-Pinedo, M.Liebendorfer, D.J.Dean Nuclear electron capture in core collapse supernovae
doi: 10.1016/j.nuclphysa.2005.05.010
2005JU02 Nucl.Phys. A747, 87 (2005) A.Juodagalvis, K.Langanke, G.Martinez-Pinedo, W.R.Hix, D.J.Dean, J.M.Sampaio Neutral-current neutrino-nucleus cross sections for A ∼ 50-65 nuclei NUCLEAR REACTIONS 50,51,52,53,54,55,56,57,58,59,60Mn, 52,53,54,55,56,57,58,59,60,61Fe, 54,55,56,57,58,59,60,61,62,63Co, 56,57,58,59,60,61,62,63,64Ni(ν, ν'), E=0-50 MeV; calculated neutral-current inelastic σ, neutrino spectra. NUCLEAR STRUCTURE 50,51,52,53,54,55,56,57,58,59,60Mn, 52,53,54,55,56,57,58,59,60,61Fe, 54,55,56,57,58,59,60,61,62,63Co, 56,57,58,59,60,61,62,63,64Ni; calculated Gamow-Teller strength distributions.
doi: 10.1016/j.nuclphysa.2004.09.005
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
2005LA22 Nucl.Phys. A757, 360 (2005) K.Langanke, D.J.Dean, W.Nazarewicz Thermal properties of N = 40 isotones NUCLEAR STRUCTURE 68Ni, 70Zn, 72Ge, 80Zr; calculated B(E2) distributions, pairing strengths, thermodynamic quantities, deformation effects. Shell-model Monte Carlo approach.
doi: 10.1016/j.nuclphysa.2005.04.023
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
2004HA01 Phys.Lett. B 579, 251 (2004) M.Hagemann, A.M.van den Berg, D.De Frenne, V.M.Hannen, M.N.Harakeh, J.Heyse, M.A.de Huu, E.Jacobs, K.Langanke, G.Martinez-Pinedo, H.J.Wortche High-resolution determination of GT strength distributions relevant to the presupernova evolution using the (d, 2He) reaction NUCLEAR REACTIONS 58Ni(d, 2p), E=170 MeV; measured Ep, pp-coin, σ(E, θ); deduced Gamow-Teller strength distributions. Astrophysical implications discussed.
doi: 10.1016/j.physletb.2003.09.101
2004KO13 Phys.Rev.Lett. 92, 111101 (2004) E.Kolbe, K.Langanke, G.M.Fuller Neutrino-Induced Fission of Neutron-Rich Nuclei NUCLEAR REACTIONS 232,240,248,256Po, 228,236,244,252,260Rn, 230,238,246,254,262Ra, 232,240,248,256,264Th, 238,246,254,262,270U(ν, F), E=spectrum; calculated neutrino-induced fission σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.92.111101
2004LA05 Nucl.Phys. A731, 365 (2004) Supernova neutrino-nucleus reactions NUCLEAR REACTIONS 56,59Fe, 56,59Co(ν, ν'), E=0-20 MeV; 40Ar(ν, e), E=0-100 MeV; 138Ba(ν, exnypzα), E=3-10 MeV; calculated σ. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2003.11.049
2004LA25 Phys.Rev.Lett. 93, 202501 (2004) K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, A.Richter Supernova Inelastic Neutrino-Nucleus Cross Sections from High-Resolution Electron Scattering Experiments and Shell-Model Calculations NUCLEAR REACTIONS 50Ti, 52Cr, 54Fe(e, e'), E* ≈ 6-14 MeV; analyzed data; deduced magnetic dipole strength distributions. 50Ti, 52Cr, 54Fe(ν, ν'), E=threshold-40 MeV; calculated σ, σ(E).
doi: 10.1103/PhysRevLett.93.202501
2004NI17 Nucl.Phys. A746, 513c (2004) T.Nilsson, J.Aysto, K.Langanke, K.Riisager, G.Martinez-Pinedo, E.Kolbe Muonic radioactive atoms - a unique probe for nuclear structure
doi: 10.1016/j.nuclphysa.2004.09.139
2004RA05 Eur.Phys.J. A 19, 283 (2004) F.Raiola, L.Gang, C.Bonomo, G.Gyurky, M.Aliotta, H.W.Becker, R.Bonetti, C.Broggini, P.Corvisiero, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, M.Junker, P.Prati, V.Roca, C.Rolfs, M.Romano, E.Somorjai, F.Strieder, F.Terrasi, G.Fiorentini, K.Langanke, J.Winter Enhanced electron screening in d(d, p)t for deuterated metals NUCLEAR REACTIONS 2H(d, p), E=low; measured yields in deuterated metals; deduced electron screening effect, astrophysical S-factors.
doi: 10.1140/epja/i2003-10125-0
2003BA77 Phys.Rev. C 68, 031303 (2003) C.Baumer, A.M.van den Berg, B.Davids, D.Frekers, D.De Frenne, E.-W.Grewe, P.Haefner, M.N.Harakeh, F.Hofmann, M.Hunyadi, E.Jacobs, B.C.Junk, A.Korff, K.Langanke, G.Martinez-Pinedo, A.Negret, P.von Neumann-Cosel, L.Popescu, S.Rakers, A.Richter, H.J.Wortche High-resolution study of the Gamow-Teller strength distribution in 51Ti measured through 51V(d, 2He)51Ti NUCLEAR REACTIONS 51V(d, 2p), E=171 MeV; measured Ep, pp-coin. 51Ti deduced levels, Gamow-Teller strength distribution. Comparison with large-scale shell model predictions.
doi: 10.1103/PhysRevC.68.031303
2003BO29 Nucl.Phys. A719, 37c (2003) C.Bonomo, G.Fiorentini, Z.Fulop, L.Gang, G.Gyurky, K.Langanke, F.Raiola, C.Rolfs, E.Somorjai, F.Strieder, J.Winter, M.Aliotta Enhanced electron screening in d(d, p)t for deuterated metals: a possible classical explanation NUCLEAR REACTIONS 2H(d, p), E not given; analyzed yields in several deuterated materials; deduced electron screening effect.
doi: 10.1016/S0375-9474(03)00955-2
2003FE06 Nucl.Phys. A727, 41 (2003) F.W.Fearick, G.Hartung, K.Langanke, G.Martinez-Pinedo, P.von Neumann-Cosel, A.Richter Low-energy magnetic dipole response in 56Fe from high-resolution electron scattering NUCLEAR REACTIONS 56Fe(e, e'), E=29.8-157.2; measured electron spectra, σ(E, θ). 56Fe deduced levels, J, π, excitation B(M1), scissors mode. Comparison with shell model results.
doi: 10.1016/j.nuclphysa.2003.07.016
2003HE16 Nucl.Phys. A718, 159c (2003) A.Heger, S.E.Woosley, K.Langanke, E.Kolbe, T.Rauscher, R.D.Hoffman Nucleosynthesis of heavy elements in massive stars
doi: 10.1016/S0375-9474(03)00708-5
2003KO50 J.Phys.(London) G29, 2569 (2003) E.Kolbe, K.Langanke, G.Martinez-Pinedo, P.Vogel Neutrino-nucleus reactions and nuclear structure NUCLEAR REACTIONS 16O(ν, eX), (ν, μ-X), E=100-500 MeV; calculated σ, σ(θ). 12C(ν, μ-), E=120-240 MeV; calculated σ. 16O, 56Fe, 208Pb(ν, ν'), (ν, ν'n), (ν, ν'p), (ν, ν'X), (ν-bar, e+), (ν-bar, e+n), (ν-bar, e+α), (ν-bar, e+X), 16O, 56Fe, 138Ba, 208Pb(ν, ep), 16O(ν, ν'np), (ν, ν'2n), (ν, ν'2p), (ν, ν'nα), (ν, ν'pα), (ν, enpα), (ν-bar, e+nα), (ν-bar, e+2n), (ν-bar, e+np), 16O, 138Ba(ν, enp), (ν, e2p), (ν, epα), 16O, 56Fe, 138Ba(ν, eα), 16O, 56Fe(ν, eX), 56Fe(ν, ν'α), 56Fe, 208Pb(ν, e), (ν-bar, e+p), 56Fe, 138Ba, 208Pb(ν, en), 138Ba(ν, e2n), (ν, enα), (ν, e2α), E=spectrum; calculated σ, σ(E).
doi: 10.1088/0954-3899/29/11/010
2003LA05 Phys.Rev. C 67, 044314 (2003) K.Langanke, J.Terasaki, F.Nowacki, D.J.Dean, W.Nazarewicz How magic is the magic 68Ni nucleus? NUCLEAR STRUCTURE 56,58,60,62,64,66,68,70,72,74,76,78,80Ni; calculated 2+ level energies, B(E2) strength distributions; deduced shell features. Shell model Monte Carlo, quasiparticle RPA, large-scale diagonalization shell model.
doi: 10.1103/PhysRevC.67.044314
2003LA10 Rev.Mod.Phys. 75, 819 (2003) Nuclear weak-interaction processes in stars
doi: 10.1103/RevModPhys.75.819
2003LA14 Nucl.Phys. A718, 92c (2003) Weak-interaction processes in stars
doi: 10.1016/S0375-9474(03)00684-5
2003LA18 Nucl.Phys. A728, 109 (2003) K.Langanke, D.J.Dean, W.Nazarewicz Shell model Monte Carlo studies of nuclei in the A ∼ 80 mass region NUCLEAR STRUCTURE 72,74,76Kr, 76,78,80Sr, 80,82,84Zr; calculated ground-state configurations, deformations, transitions B(E2). Shell model Monte Carlo approach.
doi: 10.1016/j.nuclphysa.2003.08.024
2003MA45 Nucl.Phys. A718, 452c (2003) G.Martinez-Pinedo, D.J.Dean, K.Langanke, J.Sampaio Neutrino-nucleus Interactions in Core-collapse Supernova NUCLEAR REACTIONS 60,62Ni, 59,61Fe, 60,62Co(ν, X), (ν-bar, X), E=0-50 MeV; calculated absorption σ vs temperature, chemical potential. 56Fe, 59Co(ν, ν'), calculated inelastic σ, neutrino spectra.
doi: 10.1016/S0375-9474(03)00849-2
2003SA32 Nucl.Phys. A718, 440c (2003) J.M.Sampaio, K.Langanke, G.Martinez-Pinedo, E.Kolbe, D.J.Dean Electron capture rates for core collapse supernovae NUCLEAR REACTIONS 1H, 70Cu, 72Zn, 76Ga, 93Kr(e, ν), E=stellar; calculated neutrino energies, capture rates vs chemical potential, temperature. Implications for supernovae core collapse discussed.
doi: 10.1016/S0375-9474(02)00832-7
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
2002BE18 Phys.Rev. C65, 035801 (2002) D.Belic, C.Arlandini, J.Besserer, J.de Boer, J.J.Carroll, J.Enders, T.Hartmann, F.Kappeler, H.Kaiser, U.Kneissl, E.Kolbe, K.Langanke, M.Loewe, H.J.Maier, H.Maser, P.Mohr, P.von Neumann-Cosel, A.Nord, H.H.Pitz, A.Richter, M.Schumann, F.-K.Thielemann, S.Volz, A.Zilges Photo-Induced Depopulation of the 180Tam Isomer via Low-Lying Intermediate States: Structure and astrophysical implications NUCLEAR REACTIONS 180mTa(γ, γ'), E=0.8-3.1 MeV bremsstrahlung; measured delayed Eγ, Iγ, X-ray spectra; deduced activation yields. 180Ta deduced intermediate states energies, transition strengths. Astrophysical implications discussed. Comparisons with previous results, model predictions. RADIOACTIVITY 180Ta(EC), (β-); measured T1/2.
doi: 10.1103/PhysRevC.65.035801
2002CU07 Eur.Phys.J. A 15, 291 (2002) R.Cussons, K.Langanke, T.Liolios Potential resonant screening effects on stellar 12C + 12C reaction rates NUCLEAR REACTIONS 12C(12C, X), E=400-1500 keV; calculated resonant screening correction factor. Astrophysical implications discussed.
doi: 10.1140/epja/i2002-10063-3
2002DE49 Phys.Rev. C66, 045802 (2002) D.J.Dean, K.Langanke, J.M.Sampaio Temperature dependence of the symmetry energy NUCLEAR STRUCTURE 56,59Mn, 56Cr, 56,59Fe, 56Co, 56,59,66Ni, 59,61,63,64Cu, 66Zn, 61,63,64Ga; calculated temperature dependence of symmetry energy. Shell model Monte Carlo approach.
doi: 10.1103/PhysRevC.66.045802
2002FU07 Eur.Phys.J. A 13, 411 (2002) Y.Fujita, H.Fujita, T.Adachi, G.P.A.Berg, E.Caurier, H.Fujimura, K.Hara, K.Hatanaka, Z.Janas, J.Kamiya, T.Kawabata, K.Langanke, G.Martinez-Pinedo, T.Noro, E.Roeckl, Y.Shimbara, T.Shinada, S.Y.van der Werf, M.Yoshifuku, M.Yosoi, R.G.T.Zegers Gamow-Teller Transitions from 58Ni to Discrete States of 58Cu the Study of Isospin Symmetry in Atomic Nuclei NUCLEAR REACTIONS 58Ni(3He, t), E=150 MeV/nucleon; measured triton spectra, σ(θ=0°). 58Cu deduced levels, Gamow-Teller strength distribution. 58Ni deduced excitation B(M1). Comparison with shell model.
doi: 10.1007/s10050-002-8771-8
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