NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.Lin Found 10 matches. 2023GA21 J.Radioanal.Nucl.Chem. 332, 3037 (2023) X.Gao, P.Zhang, J.Li, W.Mao, Z.Guo, J.Li, Y.Zhang, J.Chen, L.Sheng, M.Lin Production of 99Mo via photoneutron reaction using a 50 MeV electron linear accelerator NUCLEAR REACTIONS 100Mo(γ, n), E<50 MeV; calculated yields using FLUKA program; deduced guidance on the size of W conversion and molybdenum targets, as well as the selection of molybdenum species.
doi: 10.1007/s10967-023-09003-2
2023LI02 Nucl.Instrum.Methods Phys.Res. A1047, 167783 (2023) X.Li, T.Jiao, W.Li, Q.Zheng, N.Ni, S.Zhao, S.Zhao, F.Cheng, L.Yang, H.Yu, X.Qin, K.Xiao, S.Li, M.Lin, S.Wang, Y.Liu Spectrum measurement of secondary neutron induced by 9Be (p, n) reaction in low-Earth orbit NUCLEAR REACTIONS 9Be(p, n), E not given; measured reaction products, En, In; deduced spectrum of secondary neutron in low-Earth orbit.
doi: 10.1016/j.nima.2022.167783
2023LI54 Appl.Radiat.Isot. 202, 111059 (2023) M.Lin, W.Tian, J.Wang, R.Gao, F.Fan, Z.Qin, S.Cao, Z.Ran Optimization of target system for the production of 99Mo via 100Mo(γ, n)99Mo reaction NUCLEAR REACTIONS 100Mo(γ, n), E<50 MeV; measured reaction products, Eγ, Iγ; deduced yields. Comparison with the Geant4 simulation. The Electron Accelerator Research Center (EARC) at Institute of Modern Physics.
doi: 10.1016/j.apradiso.2023.111059
2022LI07 Phys.Rev. C 105, L021305 (2022) Evolution of collectivity and neutron-proton interactions NUCLEAR STRUCTURE Z=28-82, N=50-82; Z=50-82, N=82-126; analyzed energies of first 2+, 4+ states, integrated neutron-proton interactions Vnp; deduced correlation between the evolution of collective motions and Vnp.
doi: 10.1103/PhysRevC.105.L021305
2022SH45 Phys.Rev. C 106, L061304 (2022) R.Shou, X.Yin, C.Ma, M.Q.Lin, Y.M.Zhao Simple corrections in theoretical models of atomic masses and nuclear charge radii ATOMIC MASSES Z=29-110; N=20-160; A=49-270; analyzed systematic root mean square deviations of mass excesses, S(n), and S(p) between their experimental values from AME2020, and theoretical values from Hartree-Fock-Bogoliubov (HFB31), relativistic mean field (RMF), Duflo-Zuker (DZ), and Weizsaker-Skyrme (WS4+RBF) models using strong and specific correlations of these deviations, and deducing Pearson correlation coefficients for 3258 neutron- and proton-rich nuclei listed in the Supplemental Material of the paper. NUCLEAR STRUCTURE Z=29-59; Z=61-64; Z=66; Z=68-76; Z=78, 79; Z=81-84; Z=86-88; Z=90, 92, 95, 96; analyzed systematic root mean square deviations of charge radii between their experimental values taken from 2021Li25 (Atomic Data and Nuclear Data Tables 140, 101440 (2021)), and theoretical values from Hartree-Fock-Bogoliubov (HFB31), relativistic mean field (RMF), relativistic continuum Hartree-Bogoliubov (RCHB), and Weizsaker-Skyrme (WS*) models using strong and specific correlations of these deviations, and deducing Pearson correlation coefficients for neutron- and proton-rich nuclei listed in the Supplemental Material of the paper.
doi: 10.1103/PhysRevC.106.L061304
2022ZO01 Phys.Rev. C 105, 034321 (2022) Y.Y.Zong, C.Ma, M.Q.Lin, Y.M.Zhao Mass relations of mirror nuclei for both bound and unbound systems ATOMIC MASSES 3He, 6,7Be, 8,9B, 8,9,10,11C, 11,12,13N, 11,12,13,14,15O, 14,15,16,17F, 14,15,16,17,18,19Ne, 17,18,19,20,21Na, 17,18,19,20,21,22,23Mg, 20,21,22,23,24,25Al, 21,22,23,24,25,26,27Si, 23,24,25,26,27,28,29P, 24,25,26,27,28,29,30,31S, 27,28,29,30,31,32,33Cl, 28,29,30,31,32,33,34,35Ar, 31,32,33,34,35,36,37K, 32,33,34,35,36,37,38,39Ca, 35,36,37,38,39,40,41Sc, 36,37,38,39,40,41,42,43Ti, 39,40,41,42,43,44,45V, 40,41,42,43,44,45,46,47Cr, 43,44,45,46,47,48,49Mn, 44,45,46,47,48,49,50,51Fe, 47,48,49,50,51,52,53Co, 48,49,50,51,52,53,54,55Ni, 50,51,52,53,54,55,56,57Cu, 52,53,54,55,56,57,58,59Zn, 54,55,56,57,58,59,60,61Ga, 56,57,58,59,60,61,62,63Ge, 60,61,62,63,64,65As, 62,63,64,65,66,67Se, 65,66,67,68,69Br, 67,68,69,70,71Kr, 70,71,72,73Rb, 71,72,73,74,75Sr, 74,75,76,77Y, 75,76,77,78,79Zr, 78,79,80,81Nb, 79,80,81,82,83Mo, 82,83,84,85Tc, 84,85,86,87Ru, 86,87,88,89Rh, 88,89,90,91Pd, 90,91,92,93Ag, 92,93,94,95Cd, 94,95,96,97In, 96,97,98,99Sn; calculated S(p), S(2p), mass excesses for proton-rich systems, both inside and outside the proton drip line, in terms of mass relations for mirror nuclei, based on Weizsacker mass formula. Comparison with available evaluated experimental data from AME2020, and deduced root-mean-square deviations (RMSD).
doi: 10.1103/PhysRevC.105.034321
2019YU03 Phys.Rev. C 100, 014314 (2019) H.C.Yu, M.Q.Lin, M.Bao, Y.M.Zhao, A.Arima Empirical formulas for nuclear separation energies NUCLEAR STRUCTURE 70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100Zn, 112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137Mo, 151,152,153,154,155,156,157,158,159,160,161,162,163,164,165,166,167,168,169,170,171,172,173,174,175,176,177,178,179,180,181,182,183,184,185,186Ba, 204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239W; calculated S(n) and S(p) using empirical formulas. Comparison with AME-2016 evaluation, and with other theoretical model predictions.
doi: 10.1103/PhysRevC.100.014314
2019ZO02 Phys.Rev. C 100, 054315 (2019) Y.Y.Zong, M.Q.Lin, M.Bao, Y.M.Zhao, A.Arima Mass relations of corresponding mirror nuclei ATOMIC MASSES 21Na, 22,23Mg, 23,24,25Al, 24,25,26,27Si, 26,27,28,29P, 28,29,30,31S, 30,31,32,33Cl, 32,33,34,35Ar, 34,35,36,37K, 36,37,38,39Ca, 38,39,40,41Sc, 40,41,42,43Ti, 42,43,44,45V, 44,45,46,47Cr, 46,47,48,49Mn, 48,49,50,51Fe, 50,51,52,53Co, 52,53,54,55Ni, 54,55,56,57Cu, 56,57,58,59Zn, 58,59,60,61Ga, 60,61,62,63Ge, 62,63,64,65As, 64,65,66,67Se, 66,67,68,69Br, 68,69,70,71Kr, 70,71,72,73Rb, 72,73,74,75Sr, 74,75,76,77Y, 76,77,78,79Zr, 79,80Nb, 81,83Mo, 83,85Tc, 85,86,87Ru, 87,88Rh, 89Pd; calculated mass excesses, S(n), S(p) using mass relations for corresponding mirror nuclei, and compared with AME2016 values; deduced regularities related to neutron-proton interactions, and to separation energies for mirror nuclei.
doi: 10.1103/PhysRevC.100.054315
2018LI05 Appl.Radiat.Isot. 133, 1 (2018) M.Lin, G.J.Waligorski, C.Gonzalez Lepera Production of curie quantities of 68Ga with a medical cyclotron via the 68Zn(p, n)68Ga reaction NUCLEAR REACTIONS 68Zn(p, n), E=16.5 MeV; measured reaction products; deduced yields. Chemical separation.
doi: 10.1016/j.apradiso.2017.12.010
1996IK02 Physica C263, 526 (1996) S.Ikeda, K.Kumagai, J.Jiang, M.S.Lin, C.C.Lai, H.C.Ku NMR Study of Quaternary Superconductors RT2B2C(R = Y, La, Th, and T = Ni, Pd, Pt) NUCLEAR MOMENTS 195Pt, 139La, 11B; measured NMR; deduced Knight shift, spin-lattice relaxation characteristics. Quaternary superconductors RT2B2C(R=Y, La, Th;T=Ni, Pd, Pt).
doi: 10.1016/0921-4534(96)00081-0
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