References quoted in the ENSDF dataset: 76FE ADOPTED LEVELS

25 references found.

Clicking on a keynumber will list datasets that reference the given article.

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1999EN03

Phys.Rev. C60, 014302 (1999)

J.Engel, M.Bender, J.Dobaczewski, W.Nazarewicz, R.Surman

β Decay Rates of r-Process Waiting-Point Nuclei in a Self-Consistent Approach

RADIOACTIVITY ^76,78,80Zn, ⁸²Ge, ^{124,126,128,130}Cd, ^{68,70,72,74,76,78}Ni, ⁸²Ge, ⁸⁰Zn, ⁷⁸Ni, ⁷⁶Fe, ⁷⁴Cr, ⁷²Ti(β^-); calculated β-decay T_1/2 vs pairing strength. Self-consistent approach. Implications for nucleosynthesis discussed.

doi: 10.1103/PhysRevC.60.014302

2000IS13

Yad.Fiz. 63, No 10, 1828 (2000); Phys.Atomic Nuclei 63, 1740 (2000)

V.I.Isakov, K.A.Mezilev, Yu.N.Novikov, K.I.Erokhina, B.Fogelberg, H.Mach

Mass-Surface Predictions Near the Doubly Magic Nuclide ⁷⁸Ni

NUCLEAR STRUCTURE ^75,76,77,78Fe, ^76,77,78,79Co, ^77,78,79,80Ni, ^78,79,80,81Cu, ^79,80,81,82Zn; calculated one-, two-neutron separation energies, Qβ. Implications for astrophysical r-process discussed.

doi: 10.1134/1.1320143

2004MI54

Int.J.Mod.Phys. E13, 1209 (2004)

P.Mitra, G.Gangopadhyay

Deformation projected RMF calculation for Cr and Fe nuclei in the hybrid derivative coupling model

NUCLEAR STRUCTURE ^{44,46,48,50,52,54,56,58,60,62,64,66,68,70,72,74,76,78,80,82,84,86,88,90,92}Cr, ^{48,50,52,54,56,58,60,62,64,66,68,70,72,74,76,78,80,82,84,86,88,90,92,94,96}Fe; calculated binding energies, deformation. ^54,78,96Fe; calculated neutron single particle energies. Generalized hybrid derivative coupling model.

doi: 10.1142/S021830130400265X

2005NI02

Phys.Rev. C 71, 014308 (2005)

T.Niksic, T.Marketin, D.Vretenar, N.Paar, P.Ring

β-decay rates of r-process nuclei in the relativistic quasiparticle random phase approximation

NUCLEAR STRUCTURE ^{69,71,73,75,77,79}Cu, ⁷⁸Ni, ¹³²Sn; calculated neutron and proton single-particle energy levels. Relativistic quasiparticle RPA.

RADIOACTIVITY ^{64,66,68,70,74,76}Fe, ^{70,72,74,76,78}Ni, ^76,78,80,82Zn, ⁸²Ge, ⁷²Ti, ⁷⁴Cr, ^{122,124,126,128,130,132}Cd, ^{134,136,138,140,142}Sn, ^{136,138,140,142,144,146}Te(β^-); calculated T_1/2. Relativistic quasiparticle RPA, comparisons with data.

doi: 10.1103/PhysRevC.71.014308

2007MA09

Phys.Rev. C 75, 024304 (2007)

T.Marketin, D.Vretenar, P.Ring

Calculation of β-decay rates in a relativistic model with momentum-dependent self-energies

RADIOACTIVITY ^{64,66,68,70,72,74,76}Fe, ^{70,72,74,76,78}Ni, ^76,78,80,82Zn, ^{122,124,126,128,130,132}Cd, ^{134,136,138,140,142}Sn, ^{136,138,140,142,144,146}Te(β^-); calculated β-decay T_1/2. Relativistic proton-neutron quasiparticle RPA.

doi: 10.1103/PhysRevC.75.024304

2010SI11

Phys.Rev. C 81, 061303 (2010)

K.Sieja, F.Nowacki

Shell quenching in ⁷⁸Ni: A hint from the structure of neutron-rich copper isotopes

NUCLEAR STRUCTURE ^{69,71,73,75,77,79}Cu; calculated levels, J, π, neutron and proton orbital occupancies, magnetic moments, g factors. Large-scale shell model calculations using a realistic interaction derived from the CD-Bonn potential and ⁴⁸Ca core. ^{68,70,72,74,76,78}Fe; calculated proton effective single-particle energies. Comparison with experimental data.

doi: 10.1103/PhysRevC.81.061303

2012BE44

Phys.Atomic Nuclei 75, 1350 (2012); Yad.Fiz. 75, 1425 (2012)

O.V.Bespalova, T.A.Ermakova, A.A.Klimochkina, E.A.Romanovsky, T.I.Spasskaya

Dispersive optical potential from an analysis of neutron single-particle energies in the Ti, Cr, and Fe isotopes featuring 20 to 50 neutrons

NUCLEAR STRUCTURE ^{42,44,46,48,50,72}Ti, ^{44,46,48,50,52,54,74}Cr, ^{46,48,50,52,54,66,76}Fe; calculated single-particle energies. Shell model, GXPF1 interaction.

doi: 10.1134/S106377881211004X

2013ZH05

Phys.Rev. C 87, 025803 (2013)

Q.Zhi, E.Caurier, J.J.Cuenca-Garcia, K.Langanke, G.Martinez-Pinedo, K.Sieja

Shell-model half-lives including first-forbidden contributions for r-process waiting-point nuclei

RADIOACTIVITY ^129,131In, ²⁰⁵Au, ^205,206Hg, ^206,207Tl(β^-); calculated logft, first-forbidden shape factors. ⁷⁴Cr, ⁷⁵Mn, ⁷⁶Fe, ⁷⁷Co, ⁷⁸Ni, ⁷⁹Cu, ⁸⁰Zn, ⁸¹Ga, ⁸²Ge, ¹²⁴Mo, ¹²⁵Tc, ¹²⁶Ru, ¹²⁷Rh, ¹²⁸Pd, ¹²⁹Ag, ¹³⁰Cd, ¹³¹In, ¹⁹²Dy, ¹⁹³Ho, ¹⁹⁴Er, ¹⁹⁵Tm, ¹⁹⁶Yb, ¹⁹⁷Lu, ¹⁹⁸Hf, ¹⁹⁹Ta(β^-), (β^-n); calculated Q(β) values, T_1/2, beta-delayed neutron emission probabilities, first-forbidden transition components, partial decay rates for N=50, Z=24-32; N=82, Z=42-49; N=126, Z=66-73 r-process waiting-point nuclei. Large-scale shell-model calculations. Comparison with other model calculations, and with experimental data.

doi: 10.1103/PhysRevC.87.025803

2014SE19

Phys.Rev. C 90, 044320 (2014)

A.P.Severyukhin, V.V.Voronov, I.N.Borzov, N.N.Arsenyev, Nguyen Van Giai

Influence of 2p-2h configurations on β-decay rates

RADIOACTIVITY ⁷⁶Fe, ^{70,72,74,76,78,80}Ni, ⁸⁰Zn, ⁸²Ge, ⁸⁴Se(β^-); calculated half-lives, GamowTeller (G-T) strength distributions. Calculations based on phonon-phonon coupling in a microscopic model based on Skyrme-type interaction. Comparison with experimental results.

NUCLEAR STRUCTURE ⁷⁶Fe, ^{70,72,74,76,78,80}Ni, ⁸⁰Zn, ⁸²Ge, ⁸⁴Se, ⁸⁶Kr; calculated energies and B(E2) of first 2+ states based on QRPA and finite rank separable approximation (FRSA), with and without tensor interaction. Comparison with experimental results.

doi: 10.1103/PhysRevC.90.044320

2015WU04

Phys.Rev. C 92, 024306 (2015)

Z.-Y.Wu, C.Qi, R.Wyss, H.-L.Liu

Global calculations of microscopic energies and nuclear deformations: Isospin dependence of the spin-orbit coupling

NUCLEAR STRUCTURE A=16-375, N=8-270; ^{24,26,28,30,32,34,36,38,40,42,44}Si, ^{44,46,48,50,52,54,56,58,60,62,64,66,68,70,72,74,76}Cr, ^{48,50,52,54,56,58,60,62,64,66,68,70,72,74,76,78,80,82}Fe, ^{62,64,66,68,70,72,74,76,78,80,82,84,86,88,90,92,94,96,98,100,102,104}Ge, ^{66,68,70,72,74,76,78,80,82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116}Se, ^{70,72,74,76,78,80,82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118}Kr, ^{78,80,82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124}Zr, ^{82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132}Mo, ^{86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138}Ru, ^{172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264}Hg, ^{178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264,266}Pb; calculated microscopic binding energies and ground-state nuclear deformations β₂, γ and β₄ for 1850 even-even nuclei. Macroscopic-microscopic framework using three Woods-Saxon parametrizations with different isospin dependencies. Comparison with results of other macroscopic-microscopic mass models. Discussed isospin dependence of spin-orbital force.

doi: 10.1103/PhysRevC.92.024306

2016NO12

Phys.Rev.Lett. 117, 272501 (2016)

F.Nowacki, A.Poves, E.Caurier, B.Bounthong

Shape Coexistence in ⁷⁸Ni as the Portal to the Fifth Island of Inversion

NUCLEAR STRUCTURE ⁷⁸Ni, ⁷⁶Fe, ⁷⁴Cr, ⁷²Ti, ⁷⁰Ca; calculated quadrupole correlation energies of the neutron intruder configurations, projected Energy Surfaces, B(E2), energy levels, J, π, average number of p-h excitations and occupancies of the neutron and proton orbits; deduced shape coexistence.

doi: 10.1103/PhysRevLett.117.272501

2016SH39

Phys.Rev. C 94, 055802 (2016)

T.Shafer, J.Engel, C.Frohlich, G.C.McLaughlin, M.Mumpower, R.Surman

β decay of deformed r-process nuclei near A=80 and A=160, including odd-A and odd-odd nuclei, with the Skyrme finite-amplitude method

RADIOACTIVITY ^{68,69,70,71,72}Cr, ^{71,72,73,74,75}Mn, ^{72,73,74,75,76}Fe, ^76,77Co, ^80,81Cu, ^84,85,86Zn, ^86,87Ga, ^{86,87,88,89,90,91,92}Ge, ^{89,90,91,92,93,94,95}As, ^{92,93,94,95,96,97,98}Se, ^{157,159,161,163,165,167}Cs, ^{163,165,167,169,171,173,175}La, ^{146,148,150,152,160,164,166,168,170,172,174,176}Ce, ^{152,154,156,164,166,172,174,176,178}Nd(β^-); calculated half-lives using proton-neutron finite-amplitude method (pn-FAM) with Skyrme energy-density functionals (EDFs) in the quasiparticle random-phase approximation (QRPA), after optimizing the nuclear interaction to best fit the measured half-lives in A=80 and A=160 regions. Deduced r-process abundances. Comparison with other theoretical calculations and experimental values.

doi: 10.1103/PhysRevC.94.055802

2017SU15

Phys.Rev. C 95, 051601 (2017)

T.Sumikama, S.Nishimura, H.Baba, F.Browne, P.Doornenbal, N.Fukuda, S.Franchoo, G.Gey, N.Inabe, T.Isobe, P.R.John, H.S.Jung, D.Kameda, T.Kubo, Z.Li, G.Lorusso, I.Matea, K.Matsui, P.Morfouace, D.Mengoni, D.R.Napoli, M.Niikura, H.Nishibata, A.Odahara, E.Sahin, H.Sakurai, P.-A.Soderstrom, G.I.Stefan, D.Suzuki, H.Suzuki, H.Takeda, R.Taniuchi, J.Taprogge, Zs.Vajta, H.Watanabe, V.Werner, J.Wu, Z.Y.Xu, A.Yagi, K.Yoshinaga

Observation of new neutron-rich Mn, Fe, Co, Ni, and Cu isotopes in the vicinity of ⁷⁸Ni

NUCLEAR REACTIONS ⁹Be(²³⁸U, X), E=345 MeV/nucleon; measured reaction products, Eγ, Iγ, Eβ, particle-identifications through energy loss, times of flight, and magnetic rigidities using BigRIPS separator and ZeroDegree spectrometer at RIBF-RIKEN facility; deduced A/Q production yields for ^{65,66,67,68,69,70}Cr, ^{68,69,70,71,72,73}Mn, ^{71,72,73,74,75,76}Fe, ^{73,74,75,76,77,78}Co, ^{76,77,78,79,80,81,82}Ni, and ^{79,80,81,82,83}Cu. ⁷³Mn, ⁷⁶Fe, ^77,78Co, ^80,81,82Ni, ⁸³Cu; deduced production σ for the new isotopes. Comparison with theoretical calculations using LISE++ code.

doi: 10.1103/PhysRevC.95.051601

2018AG06

Int.J.Mod.Phys. E27, 1850062 (2018)

M.Aggarwal, G.Saxena

Persistence of magicity in neutron-rich exotic ⁷⁸Ni in ground as well as excited states

NUCLEAR STRUCTURE ⁷⁰Ca, ⁷²Ti, ⁷⁴Cr, ⁷⁶Fe, ⁷⁸Ni; calculated charge distribution along with radius, pairing energy contributions from protons and neutrons, neutron and proton single-particle energies for Ni isotopes, two-neutron shell gaps, level density parameter versus mass number A for Ni isotopes at different temperatures, entropy versus mass number A for Ni isotopes at different temperatures, rotational states. Comparison with available data.

doi: 10.1142/S0218301318500623

2018BH01

Phys.Rev. C 97, 024322 (2018)

M.Bhuyan, B.V.Carlson, S.K.Patra, S.-G.Zhou

Surface properties of neutron-rich exotic nuclei within relativistic mean field formalisms

NUCLEAR STRUCTURE ^{70,72,74,76,78,80,82,84,86}Fe, ^{72,74,76,78,80,82,84,86,88}Ni, ^{74,76,78,80,82,84,86,88,90}Zn, ^{76,78,80,82,84,86,88,90,92}Ge, ^{78,80,82,84,86,88,90,92,94}Se, ^{80,82,84,86,88,90,92,94,96}Kr; calculated binding energies, charge radii, and quadrupole deformation parameter β₂ for ground states, S(2n), total density distribution, symmetry energy and neutron pressure as function of neutron skin thickness. Calculations based on axially deformed self-consistent relativistic mean field for the nonlinear NL3* and density-dependent DD-ME1 interactions. Comparison with available experimental data.

doi: 10.1103/PhysRevC.97.024322

2018JI08

Phys.Rev. C 98, 064323 (2018)

P.Jiang, Z.M.Niu, Y.F.Niu, W.H.Long

Strutinsky shell correction energies in relativistic Hartree-Fock theory

NUCLEAR STRUCTURE ¹⁶O, ^{36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51}Ca, ⁷⁸Ni, ^100,132Sn, ^{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}Pb, ^{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}Og, ⁷⁵Mn, ⁷⁶Fe, ⁷⁷Co, ⁷⁸Ni, ⁷⁹Cu, ⁸⁰Zn, ⁸¹Ga, ⁸²Ge, ⁸³As, ⁸⁴Se, ⁸⁵Br, ⁸⁶Kr, ⁸⁷Rb, ⁸⁸Sr, ⁸⁹Y, ⁹⁰Zr, ⁹¹Nb, ⁹²Mo, ⁹³Tc, ⁹⁴Ru, ⁹⁵Rh, ⁹⁶Pd, ⁹⁷Ag, ⁹⁸Cd, ⁹⁹In, ¹⁰¹Sb, ¹⁰²Te, ¹⁰³I, ¹⁰⁴Xe, ¹⁰⁵Cs; calculated shell correction energies, radial density of ¹⁶O, ⁴⁰Ca, ²⁰⁸Pb, and single neutron spectra of ²⁰⁸Pb using relativistic Hartree-Fock (RHF) theory with the Strutinsky method.

doi: 10.1103/PhysRevC.98.064323

2019MO01

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 T_1/2 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

2021KO07

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.

doi: 10.1088/1674-1137/abddae

2021LI12

Phys.Rev. C 103, 024326 (2021)

E.Litvinova, C.Robin

Impact of complex many-body correlations on electron capture in thermally excited nuclei around ⁷⁸Ni

NUCLEAR STRUCTURE ^76,78,80Ni, ⁷⁶Fe, ⁸⁰Zn; calculated Gamow-Teller GT₊ spectra, electron capture rates as a function of temperature from T=0 to 2.0 MeV, and electron density using finite-temperature proton-neutron relativistic random phase approximation (FT-pnRRPA) and finite-temperature proton-neutron relativistic time blocking approximation (FT-pnRTBA). Comparison of electron capture rates to thermal quasiparticle random phase approximation (TQRPA) calculations. Discussed role of complex nuclear correlations in stellar electron capture process for the nuclei around ⁷⁸Ni

doi: 10.1103/PhysRevC.103.024326

2021MI17

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 T_1/2, β^--delayed neutron emission (BDNE) branching ratios (P_0n, P_1n, P_2n, P_3n, P_4n, P_5n, P_6n, P_7n, P_8n, P_9n, P_10n), 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 T_1/2, β^--delayed fission (BDF) branching ratios (P_0f, P_1f, P_2f, P_3f, P_4f, P_5f, P_6f, P_7f, P_8f, P_9f, P_10f), 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 P_0n to P_10n by pn-RQRPA+HFM and pn-RQRPA methods. ^{137,138,139,140,156,157,158,159,160,161,162}Sb; calculated isotope production ratios as a function of excitation energy. ^{123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156}Pd, ^{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}Ag, ^{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}Os, ^{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}Ir; calculated β-delayed one neutron branching ratio P_1n 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. ^{260,261,262,263,264,265,266,267,268,269,270,271,272,273,274,275,276,277,278,279,280,281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330}Fm; 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. ^{63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99}Ni, ^{120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,161,162,163,164,165,166,167,168,169,170}Sn; 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 P_α (%) 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

2021NA22

Nucl.Phys. A1015, 122278 (2021)

J.U.Nabi, T.Bayram, G.Daraz, A.Kabir, S.Senturk

The nuclear ground-state properties and stellar electron emission rates of ⁷⁶Fe, ⁷⁸Ni, ⁸⁰Zn, ¹²⁶Ru, ¹²⁸Pd and ¹³⁰Cd using RMF and pn-QRPA models

NUCLEAR STRUCTURE ⁷⁶Fe, ⁷⁸Ni, ⁸⁰Zn, ¹²⁶Ru, ¹²⁸Pd, ¹³⁰Cd; calculated nuclear ground state properties and weak transition rates using Relativistic Mean Field (RMF) model.

doi: 10.1016/j.nuclphysa.2021.122278

2021WA16

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.

doi: 10.1088/1674-1137/abddaf

2022QU03

Phys.Scr. 97, 085301 (2022)

N.T.T.Quyen, K.Y.Chae, N.K.Uyen, N.N.Duy

Beta-decay half-lives of the isotopes close to the neutron drip line and astrophysical implications

RADIOACTIVITY ^74,75,76Fe, ⁷⁸Co, ^81,82Ni, ^84,85Zn, ^86,87Ga, ^{86,87,88,89,90}Ge, ^{88,89,90,91,92}As, ⁹⁰Se, ^92,93,94,95Se, ^97,98Br, ^101,102Kr, ^{103,104,105,106}Rb, ¹⁰³Sr, ^106,107,108Sr, ^110,111Y, ^112,113,114Zr, ^116,117Nb, ¹¹⁹Mo, ¹²²Tc, ¹²⁵Ru, ^127,128Rh, ^130,131Pd, ¹³²Ag, ¹³⁴Cd, ¹³⁷In, ^138,139,140Sn, ^140,141,142Sb, ^{139,140,141,142,143,144,145}Te, ^{142,143,144,145,146,147}I, ^{147,148,149,150}Xe, ^150,151Cs, ^{150,151,152,153,154}Ba, ^{151,152,153,154,155,156,157}La(β^-); calculated T_1/2 via the FRDM+QRPA approach. Comparison with available data.

doi: 10.1088/1402-4896/ac7d16

2023LI18

Phys.Lett. B 840, 137893 (2023)

J.G.Li

Merging of the island of inversion at N=40 and N=50

NUCLEAR STRUCTURE ^{62,64,66,68,70,72,74,76}Cr, ^{64,66,68,70,72,74,76,78}Fe, ^{66,68,70,72,74,76,78,80}Ni; calculated energy levels, J, π, B(E2), effective single-particle energies (ESPEs), the probability of particle-hole excitation, and the average occupations in the N=40 and N=50 isotones using the realistic shell model; deduced merging of the island of inversion.

doi: 10.1016/j.physletb.2023.137893

2023LY04

Acta Phys.Pol. B54, 8-A3 (2023)

N.D.Ly, N.N.Duy, N.K.Uyen, L.H.Khiem

Beta-decay Half-life Uncertainty of the Extremely Neutron-rich Nuclei Due to Nuclear-mass Deviation

RADIOACTIVITY ^75,76Fe, ⁷⁸Co, ^80,81,82Ni, ^82,83Cu, ⁸⁵Zn, ⁸⁶Ge, ^89,90Ge, ^{88,89,90,91,92}As, ^{90,91,92,93,94,95}Se, ^96,97,98Br, ^101,102Kr, ^{103,104,105,106}Rb, ¹⁰³Sr, ^107,108Sr, ^110,111Y, ^112,113,114Zr, ^116,117Nb, ¹¹⁹Mo, ¹²²Tc, ¹²⁵Ru, ^127,128Rh, ^130,131Pd, ¹³²Ag, ¹³⁴Cd, ¹³⁷In, ^138,139,140Sn, ^141,142Sb, ^{140,141,142,143,144,145}Te, ^{142,143,144,145,146,147}I, ^{147,148,149,150}Xe, ^150,151Cs, ^152,153,154Ba, ^{151,152,153,154,155,156,157}La(β^-); calculated T_1/2. Comparison with available data.

doi: 10.5506/APhysPolB.54.8-A3