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NSR database version of April 11, 2024.

Search: Author = F.K.Thielemann

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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1917.

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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22939.

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
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2010PA41      Astron.Astrophys. 513, A61 (2010)

I.V.Panov, I.Yu.Korneev, T.Rauscher, G.Martínez-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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22892.

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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22939.

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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22892.

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
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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
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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
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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
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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
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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
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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
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2004RA22      At.Data Nucl.Data Tables 88, 1 (2004)

T.Rauscher, F.-K.Thielemann

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
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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
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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
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2003PA35      Nucl.Phys. A718, 647c (2003)

I.V.Panov, F.-K.Thielemann

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
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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
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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
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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
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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
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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
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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
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2001RA36      At.Data Nucl.Data Tables 79, 47 (2001)

T.Rauscher, F.-K.Thielemann

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
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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
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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
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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
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2001TH04      Nucl.Phys. A685, 169c (2001)


Nuclear Physics as a Basic Milestone for Stellar Modeling

doi: 10.1016/S0375-9474(01)00538-3
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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
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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
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2000RA20      At.Data Nucl.Data Tables 75, 1 (2000)

T.Rauscher, F.-K.Thielemann

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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset21991.

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
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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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