References quoted in the ENSDF dataset: 59CA ADOPTED LEVELS
27 references found.
Clicking on a keynumber will list datasets that reference the given article.
Prog.Theor.Phys.(Kyoto) 83, 180 (1990)
Y.Suzuki, K.Ikeda, H.Sato
New Type of Dipole Vibration in Nuclei
NUCLEAR STRUCTURE 47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62Ca; calculated pygmy dipole resonance, GDR relative energy, dipole strength ratio. 128I, 134Cs, 142Pr, 160Tb, 166Ho, 170Tm, 176Lu, 182Ta, 198Au, 207Pb; calculated pygmy resonance energy, electric dipole strength. Hydrodynamic model.
Nucl.Phys. A586, 445 (1995); Erratum Nucl.Phys. A596, 716 (1996)
W.A.Richter, M.G.Van der Merwe, B.Brown
Shell-Model Calculations for Neutron-Rich Nuclei in the 0f1p Shell
NUCLEAR STRUCTURE 51,52,53,54,55,56,57,58,59,60Ca, 52,53,54,55,56,57,58,59,60,61Sc, 54,55,56,57,58,59,60,61,62Ti, 59,60,61,62,63V, 58,60,61,62,63,64Cr, 62,63,64,65Mn, 63,64,65,66Fe; calculated binding energies, mass defects. 51,50,52Ca, 52,53Ti, 51,52Sc; calculated levels. Shell model, empirical effective interaction.
doi: 10.1016/0375-9474(94)00802-T
Phys.Rev. C58, 2099 (1998)
B.A.Brown, W.A.Richter
Shell-Model Plus Hartree-Fock Calculations for the Neutron-Rich Ca Isotopes
NUCLEAR STRUCTURE 47,48,49,50,51,52,53,54,55,56,57,58,59,60Ca; calculated binding energies, levels, J, π. 48Ca calculated electron scattering form factors. Shell model plus Hartree-Fock approach.
Phys.Rev. C 76, 054602 (2007)
T.Dong, Z.Ren, Y.Guo
Elastic magnetic form factors of exotic nuclei
NUCLEAR STRUCTURE 17O, 41Ca; calculated rms radii, magnetic moments, spectroscopic factors. 23O, 17F, 15,17,19C, 49,59Ca; calculated configurations, form factors.
doi: 10.1103/PhysRevC.76.054602
Phys.Rev. C 77, 054309 (2008)
J.Margueron, H.Sagawa, K.Hagino
Effective pairing interactions with isospin density dependence
NUCLEAR STRUCTURE 36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62Ca, 52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90Ni, 100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162,163,164,165,166,167,168,169,170Sn, 182,183,184,185,186,187,188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262,263,264,265,266,267Pb; calculated odd-even mass staggering, binding energies, two-neutron separation energies, pairing gaps. Comparison with experimental data. 110,150Sn; calculated particle densities, neutron Fermi momentum. Hartree-Fock-Bogoliubov model.
doi: 10.1103/PhysRevC.77.054309
Phys.Rev. C 85, 034324 (2012)
M.A.Caprio, F.Q.Luo, K.Cai, V.Hellemans, Ch.Constantinou
Generalized seniority for the shell model with realistic interactions
NUCLEAR STRUCTURE 41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59Ca; calculated levels, J, π, orbital occupations, quadrupole moments, B(E2), magnetic moment. Comparison between seniority (ν=1-3) model space and full shell-model space.
doi: 10.1103/PhysRevC.85.034324
J.Phys.:Conf.Ser. 445, 012010 (2013)
B.A.Brown
Pairing and shell gaps in nuclei
NUCLEAR STRUCTURE 40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60Ca; calculated ground-state energy, 2+ energy, 1n separation energy, Q. Z=6-92; calculated energy differences, Q of neighbouring isotopes. Shell model. Compared with available data.
doi: 10.1088/1742-6596/445/1/012010
Phys.Rev. C 90, 024312 (2014)
J.D.Holt, J.Menendez, J.Simonis, A.Schwenk
Three-nucleon forces and spectroscopy of neutron-rich calcium isotopes
NUCLEAR STRUCTURE 40,41,42,43,44,45,46,47,48,49,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70Ca; calculated ground-state energies in pf and pfg9/2 shells, convergence of 42Ca and 48Ca ground-state energies as a function of increasing intermediate-state excitations; calculated levels, J, π, B(E2), B(M1) for 43,44,45,46,47,48,49,51,52,53,54,55,56,57Ca, energy convergence. Chiral two- and three-nucleon (NN and 3N) interactions, and many-body perturbation theory (MBPT). Comparison with coupled-cluster calculations, and with available experimental data for A=43-57 Ca isotopes.
doi: 10.1103/PhysRevC.90.024312
Phys.Rev. C 92, 024314 (2015)
G.Co, V.De Donno, M.Anguiano, R.N.Bernard, A.M.Lallena
Electric quadrupole and magnetic dipole moments of odd nuclei near the magic ones in a self-consistent approach
NUCLEAR STRUCTURE 16,22,24O, 40,48,60Ca, 90Zr, 100,132Sn, 208Pb; calculated energies and B(E2) of first 2+ states, energies and B(M1) of low-lying 1+ states using D1M and D1S Gogny interactions, and comparison with experimental data. Hartree-Fock and random phase approximation (RPA) calculations.
NUCLEAR MOMENTS 15,21,23N, 17,23,25F, 15,17,21,23,25O, 39,47,59K, 41,49,61Sc, 39,41,47,49,59,61Ca, 89Y, 91Nb, 89,91Zr, 99,131In, 101,133Sb, 99,101,131,133Sn, 207Tl, 209Bi, 207,209Pb; calculated magnetic dipole and electric quadrupole moments of ground states and in some cases excited states using D1M and D1S Gogny interactions and 16,22,24O, 40,48,60Ca, 90Zr, 100,132Sn, 208Pb as core nuclei and associated single-particle states. Hartree-Fock random phase approximation (RPA), independent particle model (IPM) first-order perturbation theory, and finite Fermi systems (FFS) calculations.
doi: 10.1103/PhysRevC.92.024314
Phys.Rev.Lett. 121, 022501 (2018)
O.B.Tarasov, D.S.Ahn, D.Bazin, N.Fukuda, A.Gade, M.Hausmann, N.Inabe, S.Ishikawa, N.Iwasa, K.Kawata, T.Komatsubara, T.Kubo, K.Kusaka, D.J.Morrissey, M.Ohtake, H.Otsu, M.Portillo, T.Sakakibara, H.Sakurai, H.Sato, B.M.Sherrill, Y.Shimizu, A.Stolz, T.Sumikama, H.Suzuki, H.Takeda, M.Thoennessen, H.Ueno, Y.Yanagisawa, K.Yoshida
Discovery of 60Ca and Implications For the Stability of 70Ca
NUCLEAR REACTIONS 9Be(70Zn, X)47P/49S/52Cl/54Ar/57K/59Ca/60Ca/62Sc, E=345 MeV/nucleon; measured reaction products. 59K; deduced new isotopes discovery. Comparison with the drip-line predictions of a wide variety of mass models.
doi: 10.1103/physrevlett.121.022501
Phys.Rev. C 100, 044308 (2019)
B.Bally, A.Sanchez-Fernandez, T.R.Rodriguez
Variational approximations to exact solutions in shell-model valence spaces: Calcium isotopes in the pf shell
NUCLEAR STRUCTURE 48Ca; calculated total energy surfaces (TES) as a function of the quadrupole degrees of freedom in the (β2, γ) plane, intrinsic pairing energy, particle-number projected, and particle-number and angular-momentum projected total energy surfaces as a function of the axial quadrupole (β2, γ=0 or 180 degrees) and nn-pairing degrees of freedom, levels, J, π, wave functions, B(E2), spectroscopic electric quadrupole moments, occupation numbers. 42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60Ca; calculated ground-state energies, energy difference between the approximate and exact ground-state energies computed with different variational approaches, excitation energies as a function of the angular momentum. Calculations used several projected generator coordinate methods (PGCM) in reproducing the exact eigenstates of the shell-model Hamiltonian KB3G in the pf-shell valence space.
doi: 10.1103/PhysRevC.100.044308
At.Data Nucl.Data Tables 125, 1 (2019)
P.Moller, M.R.Mumpower, T.Kawano, W.D.Myers
Nuclear properties for astrophysical and radioactive-ion-beam applications (II)
NUCLEAR STRUCTURE Z=8-136; calculated the ground-state odd-proton and odd-neutron spins and parities, proton and neutron pairing gaps, one- and two-neutron separation energies, quantities related to β-delayed one- and two-neutron emission probabilities, average energy and average number of emitted neutrons, β-decay energy release and T1/2 with respect to Gamow-Teller decay with a phenomenological treatment of first-forbidden decays, one- and two-proton separation energies, and α-decay energy release and half-life.
doi: 10.1016/j.adt.2018.03.003
Phys.Rev.Lett. 122, 062502 (2019)
L.Neufcourt, Y.Cao, W.Nazarewicz, E.Olsen, F.Viens
Neutron Drip Line in the Ca Region from Bayesian Model Averaging
NUCLEAR STRUCTURE 50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82Ca, 52Cl, 53Ar, 49S; calculated one- and two-neutron separation energies, posterior probability of existence of neutron-rich nuclei in the Ca region.
doi: 10.1103/PhysRevLett.122.062502
Phys.Lett. B 788, 1 (2019)
G.Saxena, M.Kumawat, M.Kaushik, S.K.Jain, M.Aggarwal
Bubble structure in magic nuclei
NUCLEAR STRUCTURE 12,13,14,15,16,17,18,19,20,21,22,23,24O, 34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70Ca, 48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98Ni, 80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150Zr, 78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126Sn, 178,179,180,181,182,183,184,185,186,187,188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262Pb, 251Fr, 299Mc, 302Og, 22Si, 34Si, 46Ar, 56S, 58Ar, 184Ce, 347119, 292120, 341Nh; calculated charge and matter densities, single particle levels and depletion fraction (DF) across the periodic chart; deduced that the central depletion is correlated to shell structure and occurs due to unoccupancy in s-orbit (2s, 3s, 4s) and inversion of (2s, 1d) and (3s, 1h) states in nuclei upto Z less or equal to 82. Bubble effect in superheavy region is a signature of the interplay between the Coulomb and nn-interaction where the depletion fraction is found to increase with Z (Coulomb repulsion) and decrease with isospin.
doi: 10.1016/j.physletb.2018.08.076
Chin.Phys.C 43, 114101 (2019)
Y.-Z.Wang, X.-D.Su, C.Qi, J.-Z.Gu
Tensor force effect on the exotic structure of neutron-rich Ca isotopes*
NUCLEAR STRUCTURE 56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74Ca; calculated two neutron separation energy, radii, neutron density distributions using spherical Skyrme-Hartree-Fock-Bogoliubov (SHFB) approach.
doi: 10.1088/1674-1137/43/11/114101
Chin.Phys.C 43, 074103 (2019)
H.-L.Wei, Y.-D.Song, C.-W.Ma, Z.-H.Li, J.Su
Cross-section prediction for isotopes near neutron drip line in 70, 80Zn projectile fragmentation reactions
NUCLEAR REACTIONS 9Be(70Zn, X)59Ca/60Ca, E=345 MeV/nucleon; analyzed available data. 66,70Ca; deduced parameters, σ for production of very neutron rich calcium nuclei.
doi: 10.1088/1674-1137/43/7/074103
Phys.Rev. C 102, 064301 (2020)
A.C.Dassie, R.M.Id Betan
Estimate of the location of the neutron drip line for calcium isotopes from an exact Hamiltonian with continuum pair correlations
NUCLEAR STRUCTURE 41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73Ca; calculated binding energies, S(2n), Fermi level and pairing gaps of even Ca isotopes, energies of single-particle bound levels for odd Ca isotopes from A=41-73, occupation probabilities for 50,54,62,66Ca, for even Ca isotopes, binding energies of 51,53,55,57,59,61Ca; deduced one particle drip line at 57Ca, and the two neutron drip line at 60Ca or 66Ca, depending on the model used. Modified Richardson equations to solve the many-body system, with two isospin independent models, and an isospin dependent model. Comparison with available experimental data.
doi: 10.1103/PhysRevC.102.064301
Phys.Rev. C 102, 034302 (2020)
J.G.Li, B.S.Hu, Q.Wu, Y.Gao, S.J.Dai, F.R.Xu
Neutron-rich calcium isotopes within realistic Gamow shell model calculations with continuum coupling
NUCLEAR STRUCTURE 49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72Ca; calculated binding energies, S(n), S(2n), neutron effective single-particle energies (ESPE), energies of the first 2+ states in even-A nuclei. 51,52,53,54,55,56,57,58Ca; calculated levels, J, π. 51,53,55,57Ca; calculated energies and widths of the first 5/2+ and 9/2+ resonance states. Realistic Gamow shell model based on high-precision CD-Bonn potential. Comparison with experimental data. 57Ca; predicted as the heaviest odd-A bound Ca isotope. 70Ca; predicted as the dripline nucleus. Calculations support shell closures at 52Ca, 54Ca, and possibly at 70Ca, and a weakening of shell closure at 60Ca.
doi: 10.1103/PhysRevC.102.034302
Phys.Rev. C 101, 014318 (2020)
V.Soma, P.Navratil, F.Raimondi, C.Barbieri, T.Duguet
Novel chiral Hamiltonian and observables in light and medium-mass nuclei
NUCLEAR STRUCTURE 3H, 3,4,6,8He, 6,7,9Li, 7,8,9,10Be, 10,11B, 12,13,14C, 14N, 14,16O, 36Ca, 68Ni; calculated ground-state energies. 6,7,9Li, 8,9Be, 10,11B, 12,13C; calculated levels, J, π. 12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28O, 34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,70Ca, 48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78Ni; calculated total binding energies, S(2n), rms charge radii. 16O, 40Ca, 58Ni; calculated charge density distribution. 47,49,53,55Ca, 53K, 55Sc; calculated levels, J, π populated in one-neutron removal and addition from and to 48Ca and 54Ca. 37,39,41,43,45,47,49,51,53,55K; calculated energies of the first excited states. 16O, 36Ca, 56Ni; calculated binding energies. 18O, 52Ca, 64Ni; calculated rms charge radii. 39K, 49,53Ca; calculated one-nucleon separation energies. 16,22,24O, 36,40,48,52,54,60Ca, 48,56,68Ni; calculated binding energy per particle for doubly closed-shell nuclei. State-of-the-art no-core shell model and self-consistent Green's function approaches with NN+3N(lnl) interaction, and with comparisons made with NNLOsat and NN+3N(400) interactions, and with experimental data.
doi: 10.1103/PhysRevC.101.014318
Phys.Rev. C 101, 014620 (2020)
S.Tagami, M.Tanaka, M.Takechi, M.Fukuda, M.Yahiro
Chiral g-matrix folding-model approach to reaction cross sections for scattering of Ca isotopes on a C target
NUCLEAR STRUCTURE 40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,62,64Ca; calculated β and γ deformation parameters, even and odd driplines, binding energies, charge, proton, neutron and matter radii, neutron skin for the ground states using Gogny-D1S Hartree-Fock-Bogoliubov (GHFB) theory with and without the angular momentum projection (AMP). Comparison with experimental data.
NUCLEAR REACTIONS 12C(40Ca, X), (41Ca, X), (42Ca, X), (43Ca, X), (44Ca, X), (45Ca, X), (46Ca, X), (47Ca, X), (48Ca, X), (49Ca, X), (50Ca, X), (51Ca, X), (52Ca, X), (53Ca, X), (54Ca, X), (55Ca, X), (56Ca, X), (57Ca, X), (58Ca, X), (59Ca, X), (60Ca, X), (62Ca, X), (64Ca, X), E=280, 250.7 MeV; calculated reaction σ(E) using chiral g-matrix double-folding model (DFM), and compared with GHFB+AMP density, and available experimental data. 9Be, 12C, 27Al(12C, X), E=30-400 MeV; calculated reaction σ(E) using chiral g-matrix double-folding model (DFM). Comparison with results from t-matrix DFM densities, and experimental data.
doi: 10.1103/PhysRevC.101.014620
Phys.Rev. C 102, 034322 (2020)
Q.Zhao, P.Zhao, J.Meng
Impact of tensor forces on spin-orbit splittings in neutron-proton drops
NUCLEAR STRUCTURE 40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69Ca; calculated spin-orbit splittings of single-particle states 1p and 1d orbitals in neutron-proton drops. N=8-50; calculated spin-orbit splittings of single-neutron states 1p, 1d, 1f and 2p as a function of the neutron number for neutron drops and neutron-proton drops with Z=1. Hartree-Fock (RHF) theory with the p-N coupling strength optimized to the relativistic Brueckner-Hartree-Fock (RBHF) results for neutron drops. Systematic study of the impact of tensor-force in neutron-proton drops.
doi: 10.1103/PhysRevC.102.034322
Chin.Phys.C 45, 030001 (2021)
F.G.Kondev, M.Wang, W.J.Huang, S.Naimi, G.Audi
The NUBASE2020 evaluation of nuclear physics properties
COMPILATION A=1-295; compiled, evaluated nuclear structure and decay data.
Phys.Rev. C 104, 014315 (2021)
Y.Liu, C.Su, J.Liu, P.Danielewicz, C.Xu, Z.Ren
Improved naive Bayesian probability classifier in predictions of nuclear mass
ATOMIC MASSES Z=8-118, N=8-170; analyzed masses of 3245 nuclei using an improved naive Bayesian probability (iNBP) method, with classifications tables generated from determination of residuals between theoretical masses from FRDM, HFB and RMF models and the experimental values in AME2016; predicted by iNBP method nuclear masses of the nuclei added in AME2016, as compared to those in AME2003. 48,49,50,51,52,53,54,55,56,57,58,59,60,62,64,66,68,70Ca; calculated binding energies using FRDM, HBF, and RMF methods with modifications by iNBP method, and compared with available experimental values from AME2016.
doi: 10.1103/PhysRevC.104.014315
Phys.Rev. C 104, L051302 (2021)
A.Magilligan, B.A.Brown, S.R.Stroberg
Data-driven configuration-interaction Hamiltonian extrapolation to 60Ca
NUCLEAR STRUCTURE 46,47,48,49,50,51,52,53,54,55,56,57,58,59,60Ca; calculated levels, J, π, S(2n); comparison of the two-body matrix elements (TBME) between the UFP-CA and the initial IMSRG interaction; deduced likely doubly magic nature of 60Ca at a level similar to that of 68Ni. State-of-the-art in-medium similarity renormalization group (IMSRG) interaction, with universal fp shell interaction for calcium isotopes (UFP-CA). Comparison with experimental data.
doi: 10.1103/PhysRevC.104.L051302
Phys.Rev. C 104, 044321 (2021)
F.Minato, T.Marketin, N.Paar
β-delayed neutron-emission and fission calculations within relativistic quasiparticle random-phase approximation and a statistical model
RADIOACTIVITY Z=8-110, N=11-209, A=19-318(β-), (β-n); calculated T1/2, β--delayed neutron emission (BDNE) branching ratios (P0n, P1n, P2n, P3n, P4n, P5n, P6n, P7n, P8n, P9n, P10n), mean number of delayed neutrons per beta-decay, and average delayed neutron kinetic energy, total beta-delayed fission and α emission branching ratios for four fission barrier height models (ETFSI, FRDM, SBM, HFB-14). Z=93-110, N=184-200, A=224-318; calculated T1/2, β--delayed fission (BDF) branching ratios (P0f, P1f, P2f, P3f, P4f, P5f, P6f, P7f, P8f, P9f, P10f), total beta-delayed fission and beta-delayed neutron emission branching ratios for four fission barrier height models 140,162Sn; calculated β strength functions, β--delayed neutron branching ratios from P0n to P10n by pn-RQRPA+HFM and pn-RQRPA methods. 137,138,139,140,156,157,158,159,160,161,162Sb; calculated isotope production ratios as a function of excitation energy. 123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156Pd, 120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159Ag, 200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250Os, 200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255Ir; calculated β-delayed one neutron branching ratio P1n by pn-RQRPA+HFM, pn-RQRPA, and FRDM+QRPA+HFM methods, and compared with available experimental data. 89Br, 138I; calculated β-delayed neutron spectrum by pn-RQRPA+HFM method, and compared with experimental spectra. 260,261,262,263,264,265,266,267,268,269,270,271,272,273,274,275,276,277,278,279,280,281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330Fm; calculated fission barrier heights for HFB-14, FRDM, ETFSI and SBM models, mean numbers and mean energies of emitted β-delayed neutrons by pn-RQRPA+HFM and pn-RQRPA methods. 63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99Ni, 120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,161,162,163,164,165,166,167,168,169,170Sn; calculated mean numbers and mean energies of emitted β-delayed neutrons by pn-RQRPA+HFM and pn-RQRPA methods. Z=70-110, N=120-190; calculated β--delayed α branching ratios Pα (%) for FRDM fission barrier data. Fully self-consistent covariant density-functional theory (CDFT), with the ground states of all the nuclei calculated with the relativistic Hartree-Bogoliubov (RHB) model with the D3C* interaction, and relativistic proton-neutron quasiparticle random-phase approximation (pn-RQRPA) for β strength functions, with particle evaporations and fission from highly excited nuclear states estimated by Hauser-Feshbach statistical model (pn-RQRPA+HFM) for four fission barrier height models (ETFSI, FRDM, SBM, HFB-14). Detailed tables of numerical data for β-delayed neutron emission (BDNE), β-delayed fission (BDF) and β-delayed α-particle emission branching ratios are given in the Supplemental Material of the paper.
doi: 10.1103/PhysRevC.104.044321
Chin.Phys.C 45, 030003 (2021)
M.Wang, W.J.Huang, F.G.Kondev, G.Audi, S.Naimi
The AME 2020 atomic mass evaluation (II). Tables, graphs and references
ATOMIC MASSES A=1-295; compiled, evaluated atomic masses, mass excess, β-, ββ and ββββ-decay, binding, neutron and proton separation energies, decay and reaction Q-value data.
Phys.Rev. C 107, 014603 (2023)
N.Tang, B.Li, J.-J.Li, F.-S.Zhang
Production of 61Ca, 63Sc, 65Ti, 68, 69V, 71Cr, 77Fe and 79Co in projectile fragmentation with radioactive ion beams at 1A GeV
NUCLEAR REACTIONS 9Be(69Cu, X)37Ar/38Ar/39Ar/40Ar/41Ar/42Ar/43Ar/44Ar/39K/40K/41K/42K/43K/44K/45K/46K/41Ca/42Ca/43Ca/44Ca/45Ca/46Ca/47Ca/43Sc/44Sc/45Sc/46Sc/47Sc/48Sc/49Sc/50Sc/45Ti/46Ti/47Ti/48Ti/49Ti/50Ti/51Ti/52Ti/48V/49V/50V/51V/52V/53V/54V/55V/50Cr/51Cr/52Cr/53Cr/54Cr/55Cr/56Cr/57Cr/53Mn/54Mn/55Mn/56Mn/57Mn/58Mn/59Mn, E=98.1 MeV/nucleon; calculated isotopes production σ. 9Be(81Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/49Sc/50Sc/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/52Ti/53Ti/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/56V/57V/58V/59V/60V/61V/62V/63V/64V/65V/56Cr/57Cr/58Cr/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/59Mn/60Mn/61Mn/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/62Fe/63Fe/64Fe/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/64Co/65Co/66Co/67Co/68Co/69Co/70Co/71Co/72Co/73Co, E=1 GeV/nucleon; 9Be(84Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/57Ca/58Ca/59Ca/60Ca/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/61Sc/53Ti/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/64Ti/57V/58V/59V/60V/61V/62V/63V/64V/65V/66V/58Cr/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/68Cr/69Cr/60Mn/61Mn/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/70Mn/71Mn/72Mn/64Fe/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/73Fe/74Fe/75Fe/66Co/67Co/68Co/69Co/70Co/71Co/72Co/73Co/74Co/75Co/76Co/77Co, E=1 GeV/nucleon; 9Be(86Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/57Ca/58Ca/59Ca/60Ca/61Ca/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/61Sc/62Sc/63Sc/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/64Ti/65Ti/57V/58V/59V/60V/61V/62V/63V/64V/65V/66V/67V/68V/69V/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/68Cr/69Cr/70Cr/71Cr/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/70Mn/71Mn/72Mn/73Mn/74Mn/75Mn/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/73Fe/74Fe/75Fe/76Fe/77Fe/67Co/68Co/69Co/70Co/71Co/72Co/73Co/74Co/75Co/76Co/77Co/78Co/79Co, E=1 GeV/nucleon; calculated isotopes production σ. Isospin-dependent Boltzmann-Langevin equation (IBLE) model. Comparison of model predictions with experimental data for 9Be(69Cu, X) reaction.
doi: 10.1103/PhysRevC.107.014603