NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = F.K.Thielemann Found 100 matches. 2023TH02 Eur.Phys.J. A 59, 12 (2023) From the slow to the rapid neutron capture process
doi: 10.1140/epja/s10050-023-00921-z
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
2019FR10 J.Phys.(London) G46, 084002 (2019) C.Frohlich, S.Curtis, K.Ebinger, S.Ghosh, A.Menon, A.Heger, A.Perego, F.-K.Thielemann Nucleosynthesis for SN 1987A from single star and binary-merger progenitors NUCLEAR REACTIONS 28Si(28Si, X), E not given; analyzed available data. 56,57,58Ni, 44Ti; calculated nucleosynthesis yields. Comparison with observed abundances.
doi: 10.1088/1361-6471/ab1ff7
2018EI01 J.Phys.(London) G45, 014001 (2018) M.Eichler, K.Nakamura, T.Takiwaki, T.Kuroda, K.Kotake, M.Hempel, R.Cabezon, M.Liebendorfer, F.-K.Thielemann Nucleosynthesis in 2D core-collapse supernovae of 11.2 and 17.0 M(.) progenitors: implications for Mo and Ru production ATOMIC MASSES 92,94Mo, 96,98Ru; calculated abundances of p-process nuclei.
doi: 10.1088/1361-6471/aa8891
2018XI04 Phys.Lett. B 781, 358 (2018) Y.M.Xing, K.A.Li, Y.H.Zhang, X.H.Zhou, M.Wang, Yu.A.Litvinov, K.Blaum, S.Wanajo, S.Kubono, G.Martinez-Pinedo, A.Sieverding, R.J.Chen, P.Shuai, C.Y.Fu, X.L.Yan, W.J.Huang, X.Xu, X.D.Tang, H.S.Xu, T.Bao, X.C.Chen, B.S.Gao, J.J.He, Y.H.Lam, H.F.Li, J.H.Liu, X.W.Ma, R.S.Mao, M.Si, M.Z.Sun, X.L.Tu, Q.Wang, J.C.Yang, Y.J.Yuan, Q.Zeng, P.Zhang, X.Zhou, W.L.Zhan, S.Litvinov, G.Audi, T.Uesaka, Y.Yamaguchi, T.Yamaguchi, A.Ozawa, C.Frohlich, T.Rauscher, F.-K.Thielemann, B.H.Sun, Y.Sun, A.C.Dai, F.R.Xu Mass measurements of neutron-deficient Y, Zr, and Nb isotopes and their impact on rp and νp nucleosynthesis processes ATOMIC MASSES 78,79Y, 80,81Zr, 82,83,84Nb, 84Mo; measured revolution time spectrum; deduced mass excess values and proton separation energies. Comparison with available data.
doi: 10.1016/j.physletb.2018.04.009
2017PA34 Phys.Atomic Nuclei 80, 657 (2017); Yad.Fiz. 80, 345 (2017) I.V.Panov, Yu.S.Lutostansky, M.Eichler, F.-K.Thielemann Determination of the Galaxy age by the method of uranium-thorium-plutonium isotopic ratios RADIOACTIVITY 244Pu, 238U(α); analyzed available data for 244Pu/238U ratio; deduced Galaxy age, T1/2.
doi: 10.1134/S1063778817040202
2016PA06 Nucl.Phys. A947, 1 (2016) I.V.Panov, Yu.S.Lutostansky, F.-K.Thielemann Beta-decay half-lives for the r-process nuclei RADIOACTIVITY 90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112Sr, 237,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262,263,264,265,266,267,268,269,270,271,272,273,274,275U(β-); calculated T1/2 using FFST (Finite Fermi Systems Theory) with masses from FRDM or ETFSI. Compared with other calculations and with data. Z=37-50(β-); calculated T1/2. Compared with data.
doi: 10.1016/j.nuclphysa.2015.12.001
2015PA29 Bull.Rus.Acad.Sci.Phys. 79, 437 (2015); Izv.Akad.Nauk RAS, Ser.Fiz 79, 478 (2015) I.V.Panov, Yu.S.Lutostansky, F.-K.Thielemann Half-life of short-lived neutron-excess nuclei that participate in the r -process NUCLEAR STRUCTURE A<220; calculated β-decay rates, T1/2 for r-process nuclei. A quasi-classic model of a strength function based on finite Fermi systems.
doi: 10.3103/S1062873815040243
2013BU08 Nucl.Phys. A907, 13 (2013) N.Buyukcizmeci, A.S.Botvina, I.N.Mishustin, R.Ogul, M.Hempel, J.Schaffner-Bielich, F.-K.Thielemann, S.Furusawa, K.Sumiyoshi, S.Yamada, H.Suzuki A comparative study of statistical models for nuclear equation of state of stellar matter
doi: 10.1016/j.nuclphysa.2013.03.010
2013PA05 Phys.Atomic Nuclei 76, 88 (2013); Yad.Fiz. 76, 90 (2013) I.V.Panov, I.Yu.Korneev, Yu.S.Lutostansky, F.-K.Thielemann Probabilities of delayed processes for nuclei involved in the r-process NUCLEAR STRUCTURE A=249-260; calculated delayed fission and neutron emission probabilities, B(GT), fission barriers. Generalized Thomas-Fermi model, comparison with available data.
doi: 10.1134/S1063778813010081
2012DR08 J.Phys.(London) G39, 105201 (2012) R.Dressler, M.Ayranov, D.Bemmerer, M.Bunka, Y.Dai, C.Lederer, J.Fallis, A.StJ.Murphy, M.Pignatari, D.Schumann, T.Stora, T.Stowasser, F.-K.Thielemann, P.J.Woods 44Ti, 26Al and 53Mn samples for nuclear astrophysics: the needs, the possibilities and the sources
doi: 10.1088/0954-3899/39/10/105201
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
2011DI11 Phys.Rev. C 84, 015802 (2011) I.Dillmann, L.Coquard, C.Domingo-Pardo, F.Kappeler, J.Marganiec, E.Uberseder, U.Giesen, A.Heiske, G.Feinberg, D.Hentschel, S.Hilpp, H.Leiste, T.Rauscher, F.-K.Thielemann Cross sections for proton-induced reactions on Pd isotopes at energies relevant for the γ process NUCLEAR REACTIONS 102,104Pd(p, γ), 105Pd(p, n), E=2.75-9 MeV; measured Eγ, Iγ, total cross sections. 104Pd(p, n), 105Pd(p, γ)106mAg, 106Pd(p, n)106mAg, 110Pd(p, n)110mAg, E=2.75-9 MeV; measured Eγ, Iγ, partial cross sections; deduced S factors. Activation method. Relevant cross sections measured close to the astrophysical Gamow window of the γ process. Comparison with previous measurements and theoretical predictions from Hauser-Feshbach model "NON-SMOKER". RADIOACTIVITY 104Ag(EC); measured precise Iγ.
doi: 10.1103/PhysRevC.84.015802
2011PA18 Bull.Rus.Acad.Sci.Phys. 75, 484 (2011) I.V.Panov, I.Yu.Korneev, T.Rauscher, F.-K.Thielemann Neutron-induced reaction rates for the r-process NUCLEAR REACTIONS 235,238U(n, γ), E not given; calculated r-process reaction rates, neutron capture rates for Z=84-118, β-delayed fission.
doi: 10.3103/S106287381104037X
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
2010CY01 Astrophys.J.Suppl.Ser. 189, 240 (2010) R.H.Cyburt, A.M.Amthor, R.Ferguson, Z.Meisel, K.Smith, S.Warren, A.Heger, R.D.Hoffman, T.Rauscher, A.Sakharuk, H.Schatz, F.K.Thielemann, M.Wiescher The JINA REACLIB Database: Its Recent Updates and Impact on Type-I X-ray Bursts
doi: 10.1088/0067-0049/189/1/240
2010DI01 Phys.Rev. C 81, 015801 (2010) I.Dillmann, C.Domingo-Pardo, M.Heil, F.Kappeler, S.Walter, S.Dababneh, T.Rauscher, F.-K.Thielemann Stellar (n, γ) cross sections of p-process isotopes Part I: 102Pd, 120Te, 130, 132Ba, and 156Dy NUCLEAR REACTIONS 102Pd, 120Te, 130Ba, 132Ba, 156Dy, 197Au(n, γ), E=0-120 keV; measured Eγ, Iγ, Maxwellian-averaged σ by activation technique; deduced reaction rates for p process. Comparison with standard Hauser-Feshbach models and with results from various reaction libraries including ENDF-B/VII.0.
doi: 10.1103/PhysRevC.81.015801
2010FA02 Astrophys.J. 712, 1359 (2010) K.Farouqi, K.-L.Kratz, B.Pfeiffer, T.Rauscher, F.-K.Thielemann, J.W.Truran Charged-particle and neutron-capture processes in the high-entropy wind of core-collapse supernovae
doi: 10.10///0004-637X/712/2/1359
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
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
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
2009LI69 Nucl.Phys. A827, 573c (2009) M.Liebendorfer, T.Fischer, M.Hempel, A.Mezzacappa, G.Pagliara, I.Sagert, J.Schaffner-Bielich, S.Scheidegger, F.-K.Thielemann, S.C.Whitehouse Supernovae as Nuclear and Particle Physics Laboratories
doi: 10.1016/j.nuclphysa.2009.05.126
2009PA23 Phys.Atomic Nuclei 72, 1026 (2009); Yad.Fiz. 72, 1070 (2009) I.V.Panov, I.Yu.Korneev, F.-K.Thielemann Superheavy elements and r-process
doi: 10.1134/S1063778809060155
2008DI05 J.Phys.(London) G35, 014029 (2008) I.Dillmann, T.Rauscher, M.Heil, F.Kappeler, W.Rapp, F.-K.Thielemann p-Process simulations with a modified reaction library
doi: 10.1088/0954-3899/35/1/014029
2008LI10 J.Phys.(London) G35, 014056 (2008) M.Liebendorfer, T.Fischer, C.Frohlich, F.-K.Thielemann, S.Whitehouse Nuclear physics with spherically symmetric supernova models
doi: 10.1088/0954-3899/35/1/014056
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
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
2006DI02 Phys.Rev. C 73, 015803 (2006) I.Dillmann, M.Heil, F.Kappeler, T.Rauscher, F.-K.Thielemann Experimental (n, γ) cross sections of the p-process nuclei 74Se and 84Sr NUCLEAR REACTIONS 74Se, 84Sr(n, γ), E=spectrum; measured capture σ; deduced Maxwellian averaged σ. Activation technique, astrophysical implications discussed.
doi: 10.1103/PhysRevC.73.015803
2006DI12 Eur.Phys.J. A 27, Supplement 1, 129 (2006) I.Dillmann, M.Heil, F.Kappeler, R.Plag, T.Rauscher, F.-K.Thielemann (n, γ) cross-sections of light p nuclei: Towards an updated database for the p process NUCLEAR REACTIONS 74Se, 84Sr, 120Te, 130,132Ba(n, γ), E=spectrum; measured σ. Activation technique.
doi: 10.1140/epja/i2006-08-018-5
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
2005DI15 Nucl.Phys. A758, 513c (2005) I.Dillmann, M.Heil, F.Kappeler, T.Rauscher, F.-K.Thielemann The (n, γ) cross sections of the p-process nuclei 74Se and 84Sr at kT=25 keV NUCLEAR REACTIONS 74Se, 84Sr(n, γ), E=spectrum; measured σ, isomer ratio. Activation technique.
doi: 10.1016/j.nuclphysa.2005.05.093
2005FA13 Nucl.Phys. A758, 631c (2005) K.Farouqi, C.Freiburghaus, K.-L.Kratz, B.Pfeiffer, T.Rauscher, F.-K.Thielemann Astrophysical conditions for an r-process in the high-entropy wind scenario of type II supernovae
doi: 10.1016/j.nuclphysa.2005.05.187
2005FI06 Nucl.Phys. A752, 604c (2005) J.L.Fisker, E.F.Brown, M.Liebendorfer, F.-K.Thielemann, M.Wiescher The reactions and ashes of thermonuclear explosions on neutron stars
doi: 10.1016/j.nuclphysa.2005.02.063
2005FI13 Nucl.Phys. A758, 447c (2005) J.L.Fisker, E.Brown, M.Liebendorfer, H.Schatz, F.-K.Thielemann The nuclear reaction flow of type I X-ray bursts
doi: 10.1016/j.nuclphysa.2005.05.082
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
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
2005PA06 Nucl.Phys. A747, 633 (2005) I.V.Panov, E.Kolbe, B.Pfeiffer, T.Rauscher, K.-L.Kratz, F.-K.Thielemann Calculations of fission rates for r-process nucleosynthesis NUCLEAR STRUCTURE A=250-320; calculated neutron-induced and β-delayed fission rates, related features. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2004.09.115
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
2004RA22 At.Data Nucl.Data Tables 88, 1 (2004) Predicted cross-sections for photon-induced particle emission COMPILATION Z=22-83; calculated, compiled cross sections for photon-induced particle emission.
doi: 10.1016/j.adt.2004.07.001
2003FI11 Nucl.Phys. A718, 614c (2003) J.L.Fisker, W.R.Hix, M.Liebendorfer, F.-K.Thielemann The transition to stable burning on an accreting neutron star
doi: 10.1016/S0375-9474(03)00902-3
2003LI43 Nucl.Phys. A719, 144c (2003) M.Liebendorfer, A.Mezzacappa, O.E.B.Messer, G.Martinez-Pinedo, W.R.Hix, F.-K.Thielemann The neutrino signal in stellar core collapse and postbounce evolution
doi: 10.1016/S0375-9474(03)00984-9
2003PA35 Nucl.Phys. A718, 647c (2003) Final r-process yields and the influence of fission: The competition between neutron-induced and β-delayed fission
doi: 10.1016/S0375-9474(03)00875-3
2003TH05 Nucl.Phys. A718, 139c (2003) F.-K.Thielemann, D.Argast, F.Brachwitz, W.R.Hix, P.Hoflich, M.Liebendorfer, G.Martinez-Pinedo, A.Mezzacappa, I.Panov, T.Rauscher Nuclear cross sections, nuclear structure and stellar nucleosynthesis
doi: 10.1016/S0375-9474(03)00704-8
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
2002WI15 Eur.Phys.J. A 15, 59 (2002) M.Wiescher, V.Barnard, J.L.Fisker, J.Gorres, K.Langanke, G.Martinez-Pinedo, F.Rembges, H.Schatz, F.K.Thielemann Nuclear-reaction rates in the thermonuclear runaway phase of accreting neutron stars NUCLEAR REACTIONS 46Cr, 55Cu, 59Ga(p, γ), E=low; calculated astrophysical reaction rates.
doi: 10.1140/epja/i2001-10226-8
2001NA37 Astrophys.J. 555, 880 (2001) T.Nakamura, H.Umeda, K.Iwamoto, K.Nomoto, M.-A.Hashimoto, W.R.Hix, F.-K.Thielemann Explosive Nucleosynthesis in Hypernovae
doi: 10.1086/321495
2001PA24 Nucl.Phys. A688, 587c (2001) I.V.Panov, C.Freiburghaus, F.-K.Thielemann Could Fission Provide the Formation of Chemical Elements with A ≤ 120 in Metal-Poor Stars ?
doi: 10.1016/S0375-9474(01)00797-7
2001PF04 Nucl.Phys. A693, 282 (2001) B.Pfeiffer, K.-L.Kratz, F.-K.Thielemann, W.B.Walters Nuclear Structure Studies for the Astrophysical r-Process
doi: 10.1016/S0375-9474(01)01141-1
2001RA36 At.Data Nucl.Data Tables 79, 47 (2001) Table of Nuclear Cross Sections and Reaction Rates: An addendum to the paper ' Astrophysical Reaction Rates from Statistical Model Calculations ' COMPILATION Z=10-83; compiled nuclear levels, cross sections and reaction rates for n-, p-, and α-induced reactions. Addendum to 2000Ra20.
doi: 10.1006/adnd.2001.0863
2001RO16 Nucl.Phys. A688, 344c (2001) S.Rosswog, C.Freiburghaus, F.-K.Thielemann Nucleosynthesis Calculations for the Ejecta of Neutron Star Coalescences
doi: 10.1016/S0375-9474(01)00724-2
2001SC21 Phys.Rev.Lett. 86, 3471 (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher End Point of the rp Process on Accreting Neutron Stars NUCLEAR STRUCTURE Z=27-54; calculated astrophysical abundances; deduced rp-process endpoint.
doi: 10.1103/PhysRevLett.86.3471
2001SC29 Nucl.Phys. A688, 150c (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher The Endpoint of the rp-Process on Accreting Neutron Stars
doi: 10.1016/S0375-9474(01)00688-1
2001TH04 Nucl.Phys. A685, 169c (2001) Nuclear Physics as a Basic Milestone for Stellar Modeling
doi: 10.1016/S0375-9474(01)00538-3
2001TH08 Prog.Part.Nucl.Phys. 46, 5 (2001) F.-K.Thielemann, F.Brachwitz, C.Freiburghaus, E.Kolbe, G.Martinez-Pinedo, T.Rauscher, F.Rembges, W.R.Hix, M.Liebendorfer, A.Mezzacappa, K.-L.Kratz, B.Pfeiffer, K.Langanke, K.Nomoto, S.Rosswog, H.Schatz, M.Wiescher Element Synthesis in Stars
doi: 10.1016/S0146-6410(01)00103-X
2000RA19 Nucl.Phys. A675, 695 (2000) T.Rauscher, F.-K.Thielemann, J.Gorres, M.Wiescher Capture of α Particles by Isospin-Symmetric Nuclei NUCLEAR REACTIONS 20Ne, 24Mg, 28Si, 32S, 36Ar, 40Ca(α, γ), E(cm)=0.07-5.5 MeV; calculated capture resonance parameters, σ, reaction rates. Comparison with data, astrophysical relevance discussed.
doi: 10.1016/S0375-9474(00)00182-2
2000RA20 At.Data Nucl.Data Tables 75, 1 (2000) Astrophysical Reaction Rates from Statistical Model Calculations COMPILATION Z=10-83; calculated neutron-, proton-, alpha-induced astrophysical reaction rates. Statistical model.
doi: 10.1006/adnd.2000.0834
1999HE33 Phys.Rev. C60, 064614 (1999) H.Herndl, R.Hofinger, J.Jank, H.Oberhummer, J.Gorres, M.Wiescher, F.-K.Thielemann, B.A.Brown Reaction Rates for Neutron Capture Reactions to C, N, and O Isotopes to the Neutron Rich Side of Stability NUCLEAR REACTIONS 13,14,15,16C, 15,16,17,18N, 18,19,20,21O(n, γ), E=stellar; analyzed data; deduced capture rates. Comparison with previous results.
doi: 10.1103/PhysRevC.60.064614
1999HO26 Astrophys.J. 521, 735 (1999) R.D.Hoffman, S.E.Woosley, T.A.Weaver, T.Rauscher, F.-K.Thielemann The Reaction Rate Sensitivity of Nucleosynthesis in Type II Supernovae NUCLEAR REACTIONS 32S, 39K, 45,46Ca, 50V, 69,70Zn(n, γ), 33S, 43Ca, 44Sc(p, γ), 33S, 40K, 45Ti(n, α), 40K, 45Ti(n, p), 44Ti(α, p), 24Mg, 28Si, 32S, 36Ar, 40Ca, 44Ti(α, γ), E not given; analyzed stellar reactions rates. Several libraries compared.
doi: 10.1086/307568
1999NA28 Astrophys.J. 517, 193 (1999) T.Nakamura, H.Umeda, K.Nomoto, F.-K.Thielemann, A.Burrows Nucleosynthesis in Type II Supernovae and the Abundances in Metal-Poor Stars
doi: 10.1086/307167
1998KA63 Ann.Rev.Nucl.Part.Sci. 48, 175 (1998) F.Kappeler, F.-K.Thielemann, M.Wiescher Current Quests in Nuclear Astrophysics and Experimental Approaches
1998KO65 Eur.Phys.J. A 3, 389 (1998) E.Kolbe, K.Langanke, F.-K.Thielemann The Role of Strange Sea Quarks on Neutrino-Nucleus Reactions in Superkamiokande and in the Supernova r-Process NUCLEAR REACTIONS 16O(ν, ν'X), (ν, ν'n), (ν, ν'p), E < 300 MeV; calculated total σ, γ-emission probability; deduced role of strange component of axial vector form factor. 130Cd(ν, ν'n), E not given; calculated total σ vs strange form factor. Implications for astrophysical r-process discussed.
doi: 10.1007/s100500050194
1998KR03 Nucl.Phys. A630, 352c (1998) K.-L.Kratz, B.Pfeiffer, F.-K.Thielemann Nuclear-Structure Input to r-Process Calculations NUCLEAR STRUCTURE A=60-210; analyzed abundances; deduced r-process calculations model dependences.
doi: 10.1016/S0375-9474(97)00773-2
1998KR29 Nuovo Cim. 111A, 1043 (1998) K.-L.Kratz, B.Pfeiffer, M.Hannawald, F.-K.Thielemann, J.Gorres, H.Schatz, M.Wiescher Nuclear Physics Far from Stability and Explosive Nucleosynthesis Processes
doi: 10.1007/BF03035991
1998SC21 Phys.Rep. 294, 167 (1998) H.Schatz, A.Aprahamian, J.Gorres, M.Wiescher, T.Rauscher, J.F.Rembges, F.-K.Thielemann, B.Pfeiffer, P.Moller, K.-L.Kratz, H.Herndl, B.A.Brown, H.Rebel rp-Process Nucleosynthesis at Extreme Temperature and Density Conditions
doi: 10.1016/S0370-1573(97)00048-3
1998TH08 Acta Phys.Pol. B29, 3503 (1998) F.-K.Thielemann, C.Freiburghaus, T.Rauscher, F.Rembges, S.Rosswog, B.Pfeiffer, K.-L.Kratz, H.Schatz, M.C.Wiescher Explosive Nucleosynthesis Close to the Drip Lines
1997FR13 Nucl.Phys. A621, 405c (1997) Ch.Freiburghaus, T.Rauscher, F.-K.Thielemann, K.-L.Kratz, B.Pfeiffer The r-Process in the High Entropy Bubble NUCLEAR STRUCTURE A=50-150; analyzed abundances; deduced r-process pattern dependence on electron abundances. High entropy bubble approach.
doi: 10.1016/S0375-9474(97)00280-7
1997NO02 Nucl.Phys. A616, 79c (1997) K.Nomoto, M.Hashimoto, T.Tsujimoto, F.K.Thielemann, N.Kishimoto, Y.Kubo, N.Nakasato Nucleosynthesis in Type II Supernovae
doi: 10.1016/S0375-9474(97)00076-6
1997NO08 Nucl.Phys. A621, 467c (1997) K.Nomoto, K.Iwamoto, N.Nakasato, F.-K.Thielemann, F.Brachwitz, T.Tsujimoto, Y.Kubo, N.Kishimoto Nucleosynthesis in Type Ia Supernovae NUCLEAR STRUCTURE A=16-70; calculated integrated abundances ratio, normalized to 56Fe, relative to solar abundances; deduced synthesized mass. Delayed detonation model.
doi: 10.1016/S0375-9474(97)00291-1
1997PF01 Z.Phys. A357, 235 (1997) B.Pfeiffer, K.-L.Kratz, F.-K.Thielemann Analysis of the Solar-System r-Process Abundance Pattern with the New ETFSI-Q Mass Formula NUCLEAR STRUCTURE A=106-124; calculated neutron separation energies. A ≈ 68-208; 203,205Tl, 204Hg, 207,208Pb, 209Bi, 232Th, 235,238U, 244Pu; calculated global r-abundances after α-, β-decays. 232Th, 238,235U, 244Pu; calculated r-process chronometers production ratios. New ETFSI-Q mass formula.
doi: 10.1007/s002180050237
1997RA24 Nucl.Phys. A621, 331c (1997) T.Rauscher, F.-K.Thielemann, K.-L.Kratz Applicability of the Hauser-Feshbach Approach for the Determination of Astrophysical Reaction Rates NUCLEAR STRUCTURE Z=10-82; N=8-165; calculated level densities; deduced applicability of statistical model for stellar reaction rates.
doi: 10.1016/S0375-9474(97)00266-2
1997RA25 Phys.Rev. C56, 1613 (1997) T.Rauscher, F.-K.Thielemann, K.-L.Kratz Nuclear Level Density and the Determination of Thermonuclear Rates for Astrophysics NUCLEAR STRUCTURE A=10-250; calculated level densities, neutron capture σ; deduced astrophysical applications. Statistical model.
doi: 10.1103/PhysRevC.56.1613
1997RE18 Nucl.Phys. A621, 413c (1997) J.-F.Rembges, Ch.Freiburghaus, F.-K.Thielemann, H.Schatz, M.Wiescher An Approximation Scheme for the rp-Process
doi: 10.1016/S0375-9474(97)00282-0
1997RE30 Astrophys.J. 484, 412 (1997) F.Rembges, C.Freiburghaus, T.Rauscher, F.-K.Thielemann, H.Schatz, M.Wiescher An Approximation for the rp-Process
doi: 10.1086/304300
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
1997TH01 Nucl.Phys. A621, 477c (1997) F.-K.Thielemann, F.Brachwitz, K.Nomoto, K.Iwamoto Nucleosynthesis in SNe Ia as a Function of the Burning Front Propagation NUCLEAR STRUCTURE 48Ca, 54,56,58Fe, 56,58,60Ni, 60,62Zn, 50Ti, 54Cr; calculated abundance plots; deduced astrophysical models constraints.
doi: 10.1016/S0375-9474(97)00292-3
1997WO07 Nucl.Phys. A621, 445c (1997) S.E.Woosley, R.D.Hoffman, F.X.Timmes, T.A.Weaver, F.-K.Thielemann Nucleosynthesis in Massive Stars and Supernovae
doi: 10.1016/S0375-9474(97)00288-1
1995CH55 Phys.Lett. 355B, 37 (1995) B.Chen, J.Dobaczewski, K.-L.Kratz, K.Langanke, B.Pfeiffer, F.-K.Thielemann, P.Vogel Influence of Shell-Quenching Far from Stability on the Astrophysical r-Process NUCLEAR STRUCTURE A=80-140; analyzed r-process paths, abundances data; deduced far from stability nuclear structure properties testing possibility.
doi: 10.1016/0370-2693(95)00737-6
1995GO02 Phys.Rev. C51, 392 (1995) J.Gorres, M.Wiescher, F.-K.Thielemann Bridging the Waiting Points: The role of two-proton capture reactions in the rp process NUCLEAR REACTIONS 18Ne, 15O, 38Ca(p, p), 19Na, 19F, 39Sc(p, γ), 38Ca, 18Ne(α, p), E=stellar; calculated reaction rate. 15O, 18Ne, 38Ca(p, p), 19Na, 39Sc, 19F(p, γ), 18Ne(α, p), E=resonance; calculated Γp, Γγ, resonance strength; deduced two-proton capture reactions role in rp process.
doi: 10.1103/PhysRevC.51.392
1995KO40 Phys.Rev. C52, 3437 (1995) E.Kolbe, K.Langanke, F.-K.Thielemann, P.Vogel Inclusive 12C(ν(μ), μ)12N Reaction in the Continuum Random Phase Approximation NUCLEAR REACTIONS 12C(ν, μ-X), (ν, μ+X), (ν-bar, μ+X), E not given; 12C(ν, e-), (ν, e+), (ν-bar, e-), (ν-bar, e+), E=20-250 MeV; calculated total, partial σ, branching ratios for several exit channels. Continuum RPA.
doi: 10.1103/PhysRevC.52.3437
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
1993KR05 Astrophys.J. 403, 216 (1993) K.-L.Kratz, J.-P.Bitouzet, F.-K.Thielemann, P.Moller, B.Pfeiffer Isotopic r-Process Abundances and Nuclear Structure Far from Stability: Implications for the r-process mechanism NUCLEAR STRUCTURE A ≤ 205; analyzed data; deduced isotopic r-process abundances pattern causing conditions. Unified model.
doi: 10.1086/172196
1993SO06 Phys.Rev. C47, 2941 (1993) O.Sorlin, D.Guillemaud-Mueller, A.C.Mueller, V.Borrel, S.Dogny, F.Pougheon, K.-L.Kratz, H.Gabelmann, B.Pfeiffer, A.Wohr, W.Ziegert, Yu.E.Penionzhkevich, S.M.Lukyanov, V.S.Salamatin, R.Anne, C.Borcea, L.K.Fifield, M.Lewitowicz, M.G.Saint-Laurent, D.Bazin, C.Detraz, F.-K.Thielemann, W.Hillebrandt Decay Properties of Exotic N ≈ 28 S and Cl Nuclei and the 48Ca/46Ca Abundance Ratio RADIOACTIVITY 44S, 45,46,47Cl(β-) [from 64Ni(48Ca, X), E=60 MeV/nucleon]; measured β-decay T1/2, neutron emission probabilities; deduced solar system 48Ca/46Ca abundance ratio implications. Model comparison.
doi: 10.1103/PhysRevC.47.2941
1992KO07 Nucl.Phys. A540, 599 (1992) E.Kolbe, K.Langanke, S.Krewald, F.-K.Thielemann Inelastic Neutrino Scattering on 12C and 16O Above the Particle Emission Threshold NUCLEAR REACTIONS 12C(ν, ν'), E ≈ 20-35 MeV; 16O(ν, ν'), E ≈ 12-38 MeV; 12C(ν-bar, ν-bar'), (ν-bar, e+), (ν, e-), E ≈ 15-40 MeV; 16O(ν-bar, ν-bar'), (ν-bar, e+), (ν, e-), E ≈ 13-39 MeV; calculated angle integrated σ. Extended continuum RPA theory.
doi: 10.1016/0375-9474(92)90175-J
1992WA16 Phys.Lett. 284B, 196 (1992) R.-P.Wang, F.-K.Thielemann, D.H.Feng, C.-L.Wu Microscopic Nuclear Masses and Their Astrophysical Implications NUCLEAR STRUCTURE A ≈ 210-260; calculated masses; deduced accurate level densities. Microscopic fermion dynamical symmetry model.
doi: 10.1016/0370-2693(92)90419-5
1990KR04 Z.Phys. A336, 357 (1990) K.-L.Kratz, V.Harms, W.Hillebrandt, B.Pfeiffer, F.-K.Thielemann, A.Wohr Origin of the Odd-Even Staggering in the A ≈ 80 Solar R-Abundance Peak NUCLEAR STRUCTURE A=75-85; analyzed β-delayed n-branching in decay; deduced r-abundances features.
1989WI24 Astrophys.J. 343, 352 (1989) M.Wiescher, J.Gorres, S.Graff, L.Buchmann, F.K.Thielemann The Hot Proton-Proton Chains in Low Metallicity Objects NUCLEAR REACTIONS 8B(p, γ), 9C(α, p), 8B(α, p), 11C(p, γ), 12N(p, γ), 13O(α, p), E<1.5 MeV; calculated astrophysical reaction rates, S-factors using level parameters, equilibrium mass abundances. Comparison with Hauser-Feshbach predictions and compilations.
doi: 10.1086/167709
1988KR08 J.Phys.(London) G14, Supplement S331 (1988) K.-L.Kratz, F.-K.Thielemann, W.Hillebrandt, P.Moller, V.Harms, A.Wohr, J.W.Truran Constraints on r-Process Conditions from Beta-Decay Properties Far Off Stability and r-Abundances NUCLEAR STRUCTURE 130Cd, 80Zn; analyzed β-decay data; deduced A ≈ 130, 80 r-abundances. Shell model imput.
doi: 10.1088/0305-4616/14/S/034
1988WI08 Astrophys.J. 326, 384 (1988) M.Wiescher, J.Gorres, F.-K.Thielemann 17F(p, γ)18Ne in Explosive Hydrogen Burning NUCLEAR REACTIONS, ICPND 17F(p, γ), E(cm) ≤ 0.7 MeV; calculated capture σ, S-factor vs E. 18Ne deduced level, J, π.
doi: 10.1086/166100
1986KR17 Z.Phys. A325, 489 (1986) K.-L.Kratz, H.Gabelmann, W.Hillebrandt, B.Pfeiffer, K.Schlosser, F.-K.Thielemann, and the ISOLDE collaboration The Beta-Decay Half-Life of 13048Cd82 and Its Importance for Astrophysical r-Process Scenarios RADIOACTIVITY 130Cd(β-n) [from U(p, X), E=600 MeV]; measured T1/2; deduced neutron emission probability, astrophysical r-process relevance. 130In deduced neutron binding energy. 129Ag deduced approximate T1/2. Neutron long-counter, 3He proportional counters.
1986LA16 Z.Phys. A324, 147 (1986) K.Langanke, M.Wiescher, F.-K.Thielemann The Triple-Alpha-Reaction at Low Temperatures NUCLEAR REACTIONS, ICPND 4He(α, γ), E ≈ resonance; calculated thermonuclear reaction rate vs temperature. 9Be(α, γ), E ≤ 1.1 MeV; calculated direct capture σ component to astrophysical S-factor vs E, triple-α production rate.
1986ZI04 Radiat.Eff. 94, 311 (1986) W.Ziegert, M.Wiescher, K.-L.Kratz, F.-K.Thielemann, W.Hillebrandt, J.Krumlinde, P.Moller Beta-Decay Properties of Neutron-Rich S to K Nuclei and Their Implication for Solar and Meteoritic Ca-Ti Isotopic Abundances NUCLEAR STRUCTURE 46,48Ca, 47,49,50Ti; analyzed neutron rich nuclei β-decay characteristics; deduced solar, meteoritic Ca-Ti isotopic abundance implication.
doi: 10.1080/00337578608208399
1985BO49 Phys.Lett. 164B, 22 (1985) U.Bosch, W.-D.Schmidt-Ott, P.Tidemand-Petersson, E.Runte, W.Hillebrandt, M.Lechle, F.-K.Thielemann, R.Kirchner, O.Klepper, E.Roeckl, K.Rykaczewski, D.Schardt, N.Kaffrell, M.Bernas, Ph.Dessagne, W.Kurcewicz Beta-Decay Half-Lives of New Neutron-Rich Chromium-to-Nickel Isotopes and Their Consequences for the Astrophysical R-Process RADIOACTIVITY 58,59Cr, 63Mn, 66,67Co, 69Ni(β-) [from W(76Ge, X), E=11.4 MeV/nucleon]; measured Eγ, Eβ, βγ-coin; deduced T1/2, r-process implications. Other data considered.
doi: 10.1016/0370-2693(85)90023-1
1985LE23 Z.Phys. A322, 531 (1985) B.Leist, W.Ziegert, M.Wiescher, K.-I.Kratz, F.-K.Thielemann Neutron Capture Cross Sections for Neutron-Rich Isotopes NUCLEAR REACTIONS 86Kr, 136Xe(n, γ), E not given; calculated reaction rates. Hauser-Feshbach, Breit-Wigner methods.
doi: 10.1007/BF01412093
1983TH01 Z.Phys. A309, 301 (1983) F.-K.Thielemann, J.Metzinger, H.V.Klapdor Beta-Delayed Fission and Neutron Emission: Consequences for the astrophysical r-process and the age of the galaxy RADIOACTIVITY Z=10-100; Z=75-100; calculated β-delayed neutron emission, fission probabilites, r-process production ratios; deduced maximum fission probability Z, N, age of galaxy.
doi: 10.1007/BF01413833
1981KL04 Z.Phys. A299, 213 (1981) H.V.Klapdor, T.Oda, J.Metzinger, W.Hillebrandt, F.K.Thielemann The Beta Strength Function and the Astrophysical Site of the r-Process RADIOACTIVITY, Fission A=70-280; calculated β-strength function, β-decay T1/2, β-delayed neutron emission probabilities, β-delayed fission rates; deduced r-process astrophysical site. Schematical Brown-Bolsterli model.
doi: 10.1007/BF01443939
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