NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.C.Chu Found 18 matches. 2024LU07 Chin.Phys.C 48, 044105 (2024) S.Luo, D.-M.Zhang, L.-J.Qi, X.Chen, P.-Ch.Chu, X.-H.Li α-particle preformation factors in heavy and superheavy nuclei RADIOACTIVITY 220,222,224,226,228,230,232Th, 222,224,226,228,230,232,234,236,238U, 230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 244,246,248,250,252,254,256Fm, 252,254,256No, 256,258Rf, 260Sg, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288Fl, 290,292Lv, 294Og(α); calculated T1/2 using the Two-Potential Approach (TPA); deduced preformation factors. Comparison with available data.
doi: 10.1088/1674-1137/ad21e9
2023CH40 Phys.Rev. C 108, 025808 (2023) P.-C.Chu, X.-H.Li, H.Liu, M.Ju, Y.Zhou Properties of isospin asymmetric quark matter in quark stars
doi: 10.1103/PhysRevC.108.025808
2023LU06 Eur.Phys.J. A 59, 125 (2023) S.Luo, L.-J.Qi, D.-M.Zhang, B.He, P.-C.Chu, X.-H.Li An improved empirical formula of α decay half-lives for superheavy nuclei RADIOACTIVITY 234,236,238Cm, 242Cm, 246Cm, 238Cf, 242Cf, 246Cf, 250Cf, 254Cf, 246Fm, 250Fm, 254Fm, 252No, 256No, 258Rf, 266Hs, 270Hs, 282Ds, 286Fl, 290Lv, 294Og(α); calculated T1/2; deduced formula. Comparison with available data.
doi: 10.1140/epja/s10050-023-01040-5
2023QI06 Phys.Rev. C 108, 014325 (2023) L.-J.Qi, D.-M.Zhang, S.Luo, G.-Q.Zhang, P.-C.Chu, X.-J.Wu, X.-H.Li Cluster radioactivity preformation probability of trans-lead nuclei in the NpNn scheme RADIOACTIVITY 221Fr, 221,222,223,224,226Ra, 223Ac(14C);228Th(20O);231Pa(23F);230Th, 231Pa, 232,233,234U(24Ne);233U(25Ne);234U(26Ne);234U, 236,238Pu(28Mg), 238Pu(30Mg);238Pu(32Si);242Cm(34Si); calculated cluster preformation probability. Comparison of results obtained with unified fission model (model dependent approach), cluster formation model (microscopic approach) and Wei model (analytical formula).
doi: 10.1103/PhysRevC.108.014325
2023QI07 Eur.Phys.J. A 59, 255 (2023) L.-J.Qi, D.-M.Zhang, S.Luo, X.-H.Li, B.He, P.C.Chu Cluster radioactivity half-lives of trans-lead nuclei with a statistical physical preformation factor RADIOACTIVITY 221Fr, 221,222,223Ra, 223Ac, 224,226Ra(14C), 228Th(20O), 230Th(24Ne), 231Pa(23F), 231Pa, 232,233U(24Ne), 233U(25Ne), 234U(24Ne), 236Pu(26Ne), 238Pu(28Mg); calculated T1/2 using the cluster preformation probability in statistical physical way and Wentzel-Kramers-Brillouin (WKB) theory. Comparison with available data.
doi: 10.1140/epja/s10050-023-01162-w
2022CH21 Phys.Rev. C 105, 045806 (2022) P.-C.Chu, Y.-N.Wang, X.-H.Li, H.Liu, J.-W.Zhang Strange quark matter at finite temperature under magnetic fields with a quasiparticle model
doi: 10.1103/PhysRevC.105.045806
2022CH48 Chin.Phys.C 46, 104104 (2022) J.-H.Cheng, Z.Zhang, X.-J.Wu, P.-C.Chu, X.-H.Li Systematic study of proton radioactivity half-lives based on the relationship between Skyrme-Hartree-Fock and the macroscopic quantities of nuclear matter RADIOACTIVITY 144,145,146,147Tm, 150,151Lu, 156,157Ta, 159,160,161Re, 164,165,166,167Ir, 170,171Au, 176,177Tl(p); calculated the spherical proton radioactivity using the relationship between Skyrme parameters and the macroscopic quantities of nuclear matter. Comparison with available data.
doi: 10.1088/1674-1137/ac7a99
2022LU11 Eur.Phys.J. A 58, 244 (2022) S.Luo, Y.-Y.Xu, D.-X.Zhu, B.He, P.-C.Chu, X.-H.Li Improved Geiger-Nuttall law for α-decay half-lives of heavy and superheavy nuclei RADIOACTIVITY 220,222,224,226,228,230,232Th, 222,224,226,228,230,232,234,236,238U, 230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 244,246,248,250,252,254,256Fm, 252,254,256No, 256,258Rf, 260Sg, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288Fl, 292Lv, 294Og, 221,223,225,227,229Th, 221,223,225,227,229,231Pa, 223,225,227,229,231,233U, 233,235,237Np, 229,231,233,235Pu, 245,247,249,251,253,255Es, 241,243,245,247,249,251,253,255,257Fm, 245,247,249,251,253,255,257Md, 251,253,255,257,259No, 224,226,228,230Pa, 224,226,228,230,232,234,236Np, 234,236,238,240,242Am, 234Bk, 240,242,244,246Es, 281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317Ts, 282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318Og, 284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319119, 287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320120(α); calculated T1/2. Comparison with available data.
doi: 10.1140/epja/s10050-022-00898-1
2022XU04 Eur.Phys.J. A 58, 16 (2022) Y.-Y.Xu, H.-M.Liu, D.-X.Zhu, X.Pan, Y.-T.Zou, X.-H.Li, P.-C.Chu An improved formula for the favored α decay half-lives RADIOACTIVITY 146,148Sm, 148,150,152Gd, 150,152,154Dy, 152,154,156Er, 154,156Yb, 156,158,160,162Hf, 174Hf, 158,160,162,164,166,168W, 180W, 162,164,166,168,170,172,174Os, 186Os, 166,168,170,172,174,176,178,180,182,184,186,188,190Pt, 170,172,174,176,178,180,182,184,186,188Hg, 178,180,182,184,186,188,190,192,194Pb, 210Pb, 186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218Po, 194,196,198,200,202,204,206,208,210,212,214,216,218,220,222Rn, 202,204,206,208,210,212,214,216,218,220,222,224,226Ra, 208,210,212,214,216,218,220,222,224,226,228,230,232Th, 218,220,222,224,226,228,230,232,234,236,238U, 230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 244,246Fm, 252,254,256No, 256,258Rf, 260Sg, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288Fl, 290,292Lv, 294Og, 105,107,109Te, 113I, 109,111Xe, 145Pm, 147Sm, 147Eu, 149,151Gd, 151,153Dy, 151,153Ho, 153,155Er, 153,155,157Tm, 155Yb, 155,157Lu, 157,159,161Hf, 157,159,161Ta, 159,161,163,165,167W, 159,161,163,165Re, 161,163,165,167,169,171,173Os, 165,167,169,171,173Ir, 177Ir, 165,167,169,171,173Pt, 177Pt, 181,183,185Pt, 171,173,175,177,179,181,183,185Au, 173,175Hg, 179Hg, 183Hg, 185Hg, 177,179,181Tl, 185,187,189,191Pb, 185,187,189,191,193,195,197Bi, 191,193,195,197,199,201Po, 205,207,209Po, 213,215,217,219Po, 187Po, 191,193,195,197,199,201,203,205,207,209,211,213,215,217,219At, 195,197,199,201,203,205,207,209Rn, 215,217Rn, 197,199,201,203,205,207,209,211,213,215,217,219Fr, 201,203,205Ra, 209,211Ra, 217Ra, 207,209,211,213,215,217,219,221Ac, 227Ac, 209,211,213Th, 219Th, 211,213,215,217,219,221,223,225,227,229,231Pa, 221U, 229U, 233U, 219Np, 223,225Np, 233Np, 231Pu, 235Pu, 239Pu, 233Cm, 239,241Cf, 245Cf, 253Cf, 241,243,245,247Es, 251,253,255Es, 241Fm, 247Fm, 251No, 253,255Lr, 259Lr, 261Rf, 257Db, 263Sg, 263,265Hs, 267Ds, 148Eu, 152,154Ho, 154,156Tm, 156,158Lu, 158Ta, 162,164Re, 164,166,168,170,172Ir, 170,172,174,176,178Au, 184Au, 188Bi, 196Bi, 192,194,196,198,200,202At, 214,216At, 256,258,260Rf, 260Sg, 262,264Hs, 268,270,272Hs, 266Ds, 270Ds, 276,278Ds, 270Cn, 280,282Cn, 284,286,288Fl, 288,290,292,294,296Lv, 294,296,298,300,302,304Og, 296,298,300,302,304,306,308120, 302,304,306,308,310,312122, 308,310,312,314,316,318124, 314,316,318,320,322,324,326126, 320,322,324,326,328,330,332128(α); calculated T1/2 using the modified Hatsukawa formula. Comparison with available data.
doi: 10.1140/epja/s10050-022-00666-1
2022ZH39 Chin.Phys.C 46, 044106 (2022) D.-X.Zhu, H.-M.Liu, Y.-Y.Xu, Y.-T.Zou, X.-J.Wu, P.-C.Chu, X.-H.Li Two-proton radioactivity within Coulomb and proximity potential model RADIOACTIVITY 19Mg, 45Fe, 48Ni, 54Zn, 67Kr(2p); calculated T1/2 using the Coulomb and proximity potential model (CPPM). Comparison with available data.
doi: 10.1088/1674-1137/ac45ef
2021CH52 Phys.Rev. C 104, 045805 (2021) P.-C.Chu, X.-H.Li, H.Liu, J.-W.Zhang Quark matter and quark stars within the quasiparticle model under magnetic fields
doi: 10.1103/PhysRevC.104.045805
2021CH57 Eur.Phys.J. A 57, 305 (2021) J.-L.Chen, X.-H.Li, X.-J.Wu, P.-C.Chu, B.He Systematic study on proton radioactivity of spherical proton emitters within two-potential approach RADIOACTIVITY 144,145,146,147Tm, 150,151Lu, 155,156,157Ta, 159,160,161Re, 164,165,166,167Ir, 170,171Au, 176,177Tl(p); calculated T1/2. Comparison with available data.
doi: 10.1140/epja/s10050-021-00618-1
2020CH12 Nucl.Phys. A997, 121717(2020) J.-Ha.Cheng, J.-L.Chen, J.-G.Deng, X.-H.Li, Z.Zhang, P.-C.Chu Systematic study of proton emission half-lives within the two-potential approach with Skyrme-Hartree-Fock
doi: 10.1016/j.nuclphysa.2020.121717
2020CH43 Eur.Phys.J. A 56, 273 (2020) J.-H.Cheng, X.Pan, Y.-T.Zou, X.-H.Li, Z.Zhang, P.-C.Chu Systematic study of proton radioactivity of spherical proton emitters with Skyrme interactions RADIOACTIVITY 144,145,146,147Tm, 150,151Lu, 155,156,157Ta, 159,160,161Re, 164,165,166,167Ir, 170,171Au, 176,177Tl(p); calculated T1/2. Comparison with experimental data.
doi: 10.1140/epja/s10050-020-00280-z
2019CH14 Phys.Rev. C 99, 035802 (2019) P.-C.Chu, Y.Zhou, X.Qi, X.-H.Li, Z.Zhang, Y.Zhou Isospin properties in quark matter and quark stars within isospin-dependent quark mass models
doi: 10.1103/PhysRevC.99.035802
2019CH27 Nucl.Phys. A987, 350 (2019) J.-H.Cheng, J.-L.Chen, J.G.Deng, X.-J.Wu, X.-H.Li, P.-C.Chu Systematic study of α decay half-lives based on Gamow-like model with a screened electrostatic barrier RADIOACTIVITY Z>51(α); calculated even-even nuclei T1/2 using modified Gamow-like model including centrifugal potential and electrostatic shielding with two parameters, radius constant r0 and a parameter for the screened electrostatic potential; Z=120; calculated T1/2 for 7 even-even nuclei and for some of their not yet synthesized α-decay chain. Halflives compared with those calculated using different approaches and with available data.
doi: 10.1016/j.nuclphysa.2019.05.002
2019CH45 Eur.Phys.J. A 55, 214 (2019) J.-L.Chen, J.-Y.Xu, J.-G.Deng, X.-H.Li, B.He, P.-C.Chu New Geiger-Nuttall law for proton radioactivity
doi: 10.1140/epja/i2019-12927-7
2018DE17 Phys.Rev. C 97, 044322 (2018) J.-G.Deng, J.-C.Zhao, P.-C.Chu, X.-H.Li Systematic study of α decay of nuclei around the Z=82, N=126 shell closures within the cluster-formation model and proximity potential 1977 formalism RADIOACTIVITY 189,190,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,210,212,213,214,215,216,218,219Po, 194,195,196,197,200,202,203,204,205,206,207,208,209,210,212,213,214,215,216,217,218,219,220,221,222Rn, 202,203,204,207,208,209,213,214,215,216,217,218,219,220Ra, 212,214,215,216,217,218,219,220,221Th, 216,217,218,221,222U, 186,188Hg, 187,188,189,190,191,192,194,210Pb, 190,192,194,209,210,212,213,214Bi, 192,197,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,223At, 199,200,201,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221Fr, 212,213,214,215,217,219,220,221,222Pa, 205,206,207,211,215,216,217,218,219,220Ac(α); calculated α-decay preformation factors using cluster-formation model (CFM) and T1/2 using proximity potential 1977 formalism (Prox.1977). Comparison with experimental data.
doi: 10.1103/PhysRevC.97.044322
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