**References quoted in the ENSDF dataset: 49S ADOPTED LEVELS **

9 references found.

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

Z.Phys. A335, 117 (1990)

M.Lewitowicz, R.Anne, A.G.Artukh, D.Bazin, A.V.Belozyorov, P.Bricault, C.Detraz, D.Guillemaud-Mueller, J.C.Jacmart, E.Kashy, A.Latimier, S.M.Lukyanov, A.C.Mueller, Yu.E.Penionzhkevich, F.Pougheon, A.Richard, W.D.Schmidt-Ott, Y.Zhang

*First Observation of the Neutron-Rich Nuclei ^{42}Si, ^{45,46}P, ^{48}S, and ^{51}Cl from the Interaction of 44 MeV/u ^{48}Ca + ^{64}Ni*

NUCLEAR REACTIONS ^{64}Ni(^{48}Ca, X), E=44 MeV/nucleon; measured fragment spectra vs Z; deduced evidence for ^{42}Si, ^{45,46}P, ^{48}S, ^{51}Cl.

Phys.Rev. C 86, 024614 (2012)

W.Horiuchi, T.Inakura, T.Nakatsukasa, Y.Suzuki

*Glauber-model analysis of total reaction cross sections for Ne, Mg, Si, and S isotopes with Skyrme-Hartree-Fock densities*

NUCLEAR REACTIONS ^{12}C(^{17}Ne, X), (^{18}Ne, X), (^{19}Ne, X), (^{20}Ne, X), (^{21}Ne, X), (^{22}Ne, X), (^{23}Ne, X), (^{24}Ne, X), (^{25}Ne, X), (^{26}Ne, X), (^{27}Ne, X), (^{28}Ne, X), (^{29}Ne, X), (^{30}Ne, X), (^{31}Ne, X), (^{32}Ne, X), (^{33}Ne, X), (^{34}Ne, X), (^{20}Mg, X), (^{21}Mg, X), (^{22}Mg, X), (^{23}Mg, X), (^{24}Mg, X), (^{25}Mg, X), (^{26}Mg, X), (^{27}Mg, X), (^{28}Mg, X), (^{29}Mg, X), (^{30}Mg, X), (^{31}Mg, X), (^{32}Mg, X), (^{33}Mg, X), (^{34}Mg, X), (^{35}Mg, X), (^{36}Mg, X), (^{37}Mg, X), (^{38}Mg, X), (^{24}Si, X), (^{25}Si, X), (^{26}Si, X), (^{27}Si, X), (^{28}Si, X), (^{29}Si, X), (^{30}Si, X), (^{31}Si, X), (^{32}Si, X), (^{33}Si, X), (^{34}Si, X), (^{35}Si, X), (^{36}Si, X), (^{37}Si, X), (^{38}Si, X), (^{39}Si, X), (^{40}Si, X), (^{41}Si, X), (^{42}Si, X), (^{43}Si, X), (^{44}Si, X), (^{45}Si, X), (^{46}Si, X), (^{26}S, X), (^{27}S, X), (^{28}S, X), (^{29}S, X), (^{30}S, X), (^{31}S, X), (^{32}S, X), (^{33}S, X), (^{34}S, X), (^{35}S, X), (^{36}S, X), (^{37}S, X), (^{38}S, X), (^{39}S, X), (^{40}S, X), (^{41}S, X), (^{42}S, X), (^{43}S, X), (^{44}S, X), (^{45}S, X), (^{46}S, X), (^{47}S, X), (^{48}S, X), (^{49}S, X), (^{50}S, X), E=240 MeV/nucleon; ^{12}C(^{13}O, X), (^{14}O, X), (^{15}O, X), (^{16}O, X), (^{17}O, X), (^{18}O, X), (^{19}O, X), (^{20}O, X), (^{21}O, X), (^{22}O, X), (^{23}O, X), (^{24}O, X), (^{17}Ne, X), (^{18}Ne, X), (^{19}Ne, X), (^{20}Ne, X), (^{21}Ne, X), (^{22}Ne, X), (^{23}Ne, X), (^{24}Ne, X), (^{25}Ne, X), (^{26}Ne, X), (^{27}Ne, X), (^{28}Ne, X), (^{29}Ne, X), (^{30}Ne, X), (^{31}Ne, X), (^{32}Ne, X), (^{33}Ne, X), (^{34}Ne, X), (^{20}Mg, X), (^{21}Mg, X), (^{22}Mg, X), (^{23}Mg, X), (^{24}Mg, X), (^{25}Mg, X), (^{26}Mg, X), (^{27}Mg, X), (^{28}Mg, X), (^{29}Mg, X), (^{30}Mg, X), (^{31}Mg, X), (^{32}Mg, X), (^{33}Mg, X), (^{34}Mg, X), (^{35}Mg, X), (^{36}Mg, X), (^{37}Mg, X), (^{38}Mg, X), E=1000 MeV/nucleon; calculated total reaction σ. Glauber model for high-energy nucleus-nucleus collisions with SkM* interaction. Comparison with experimental data. Role of nuclear deformation in determining the matter radius.

NUCLEAR STRUCTURE ^{20,21,22,23,24,25,26,27,28,29,30,31,32,33,34}Ne, ^{22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38}Mg, ^{24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39,40,41,42,43,44,45,46}Si, ^{26,27,28,29,30,31,32,33,34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50}S; calculated point matter, neutron and proton radii, neutron Fermi energy for Ne isotopes, quadrupole deformation parameter. Skyrme-Hartree-Fock calculation SkM* and SLy4 interactions.

doi: 10.1103/PhysRevC.86.024614

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 ^{60}Ca and Implications For the Stability of ^{70}Ca*

NUCLEAR REACTIONS ^{9}Be(^{70}Zn, X)^{47}P/^{49}S/^{52}Cl/^{54}Ar/^{57}K/^{59}Ca/^{60}Ca/^{62}Sc, E=345 MeV/nucleon; measured reaction products. ^{59}K; 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 97, 054321 (2018); Erratum Phys.Rev. C 109, 029904 (2024)

S.Yoshida, Y.Utsuno, N.Shimizu, T.Otsuka

*Systematic shell-model study of β-decay properties and Gamow-Teller strength distributions in A ≈ 40 neutron-rich nuclei*

RADIOACTIVITY ^{39,40}S, ^{40}P, ^{41}Cl(β^{-}); calculated logft values and compared with experimental data. ^{35,36,37,38,39,40,41,42,43,44,45,46,47}Al, ^{36,37,38,39,40,41,42,43,44,45,46,47,48}Si, ^{37,38,39,40,41,42,43,44,45,46,47,48,49}P, ^{38,39,40,41,42,43,44,45,46,47,48,49,50}S, ^{39,40,41,42,43,44,45,46,47,48,49,50,51}Cl, ^{40,41,42,43,44,45,46,47,48,49,50,51,52}Ar(β^{-})(β^{-}n); calculated β-decay T_{1/2}, β-delayed neutron emission probabilities (Pn), Gamow-Teller (GT) strength distributions, and location of the Gamow-Teller giant resonances using large-scale shell-model with and without first-forbidden (FF) transitions included. Comparison with experimental values from the ENSDF database, and with other theoretical predictions.

doi: 10.1103/PhysRevC.97.054321

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

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 ^{50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82}Ca, ^{52}Cl, ^{53}Ar, ^{49}S; 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

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, 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 ^{140,162}Sn; 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. ^{89}Br, ^{138}I; 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

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.