NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = V.Safoora Found 6 matches. 2018SA31 Eur.Phys.J. A 54, 80 (2018) Theoretical studies on the synthesis of SHE 290-302Og (Z=118) using 48Ca, 45Sc, 50Ti, 51V, 54Cr, 55Mn, 58Fe, 59Co and 64Ni induced reactions NUCLEAR REACTIONS 231Pa(59Co, xn), 232,233,234,235,236,238U(58Fe, xn), 235,236,237Np(55Mn, xn), 238,239,240,241,242,244Pu(54Cr, xn), 241,243Am(51V, xn), 242,243,244,245,246,247,248,250Cm(50Ti, xn), 247,249Bk(45Sc, xn), 249,250,251,252,253,254Cf(48Ca, xn), E*≈27-47 MeV; calculated Og capture, fusion, maximal ER value σ using PMPC (Phenomenological Model for Production Cross section); compared with data of Moller and of Warsaw groups; deduced mass and shell corrections.
doi: 10.1140/epja/i2018-12512-8
2017SA35 Phys.Rev. C 95, 064611 (2017) Predictions of probable projectile-target combinations for the synthesis of superheavy isotopes of Ts NUCLEAR REACTIONS 290Fl(7Li, X), 287Nh(10Be, X), 283Rg(14C, X), 281Rg(16C, X), 279Mt(20O, X), 275Mt(22O, X), 271Bh(26Ne, X), 267Db(30Mg, X), 263Lr(34Si, X), 261Lr(36Si, X), 257Md(40S, X), 255Md(42S, X), 254Fm(43Cl, X), 253Es(44Ar, X), 251Es(46Ar, X), 249Bk(48Ca, X), 247Bk(50Ca, X), 245Bk(52Ca, X), 244Cm(53Sc, X), 243Am(54Ti, X), 241Am(56Ti, X), 239Np(58Cr, X), 237Np(60Cr, X), 234U(63Mn, X), 233Pa(64Fe, X), 231Pa(66Fe, X), 230Th(67Co, X), 229Ac(68Ni, X), 227Ac(70Ni, X), 225Ac(72Ni, X), 224Ra(73Cu, X), 223Fr(74Zn, X), 222Ra(75Cu, X), 221Fr(76Zn, X), 220Rn(77Ga, X), 219Fr(78Zn, X), 218Rn(79Ga, X), 217At(80Ge, X), 215At(82Ge, X), 214Po(83As, X), 213Bi(84Se, X), 211Bi(86Se, X), 210Pb(87Br, X), 209Pb(88Br, X), 208Pb(89Br, X), 207Tl(90Kr, X), 206Hg(91Rb, X), 205Tl(92Kr, X), 204Hg(93Rb, X), 203Au(94Sr, X), 201Au(96Sr, X), 200Pt(97Y, X), 169Ho(128Sn, X), 167Ho(130Sn, X), 166Dy(131Sb, X), 165Tb(132Te, X), 164Dy(133Sb, X), 163Tb(134Te, X), 162Gd(135I, X), 161Eu(136Xe, X)297Ts*, E*=10, 30-40 MeV; calculated cold reaction valley plot of superheavy nucleus 297Ts, barrier heights, barrier radii, quasifission barriers, scattering potentials, evaporation residue cross sections for 1n-, 2n-, 3n-, 4n- and 5n-channels. 243Bk(48Ca, X)291Ts*, 244Bk(48Ca, X)292Ts*, 245Bk(48Ca, X)293Ts*, 246Bk(48Ca, X)294Ts*, 247Bk(48Ca, X)295Ts*, 248Bk(48Ca, X)296Ts*, 249Bk(48Ca, X)297Ts*, 250Bk(48Ca, X)298Ts*, 251Bk(48Ca, X)299Ts*, E*<50 MeV; calculated fission barriers, S(n), maximum value of the evaporation residue cross sections for 3n-, 4n- and 5n-channels. Calculations used Coulomb and proximity potential as the interaction barrier. Comparison with available experimental data.
doi: 10.1103/PhysRevC.95.064611
2017SA53 Phys.Rev. C 96, 034610 (2017) Synthesis of 292-303119 superheavy elements using Ca- and Ti-induced reactions NUCLEAR REACTIONS 252,253,254,255Es(42Ca, 3n), (42Ca, 4n), (42Ca, 5n), (44Ca, 3n), (44Ca, 4n), (44Ca, 5n), (46Ca, 3n), (46Ca, 4n), (46Ca, 5n), (48Ca, 3n), (48Ca, 4n), (48Ca, 5n)294119*/295119*/296119*/297119*/298119*/299119*/300119*/301119*/302119*/303119*, E*=29.64-48.63 MeV; 246,247,248,249Bk(46Ti, 3n), (46Ti, 4n), (46Ti, 5n), (47Ti, 3n), (47Ti, 4n), (47Ti, 5n), (48Ti, 3n), (48Ti, 4n), (48Ti, 5n), (49Ti, 3n), (49Ti, 4n), (49Ti, 5n), (50Ti, 3n), (50Ti, 4n), (50Ti, 5n)292119*/293119*/294119*/295119*/296119*/297119*/298119*/299119*, E*=31.49-46.27 MeV; calculated maximum value of cross sections for evaporation residues (ERs) for Z=119 isotopes using Coulomb and proximity potentials, and compared to other theoretical calculations. 242Pu(48Ca, 3n), (48Ca, 4n), (48Ca, 5n)290Fl*, E*=40.2, 50 MeV; 244Pu(48Ca, 3n), (48Ca, 4n)292Fl*, E*=40.5, 42, 44 MeV; 243Am(48Ca, 3n), (48Ca, 4n)291Mc*, E*=35, 38.9, 39, 44 MeV; 248Cm(48Ca, 3n), (48Ca, 4n)296Lv*, E*=32.6, 35, 40.9 MeV; 249Bk(48Ca, 4n)297Ts*, E*=39, 43, 46 MeV; 249Cf(48Ca, 3n)297Og*, E*=34 MeV; calculated σ for capture, fusion, and ERs. Comparison with experimental data.
doi: 10.1103/PhysRevC.96.034610
2017SA67 J.Phys.(London) G44, 125105 (2017) 48Ca induced reactions for the synthesis of isotopes 284-292Fl NUCLEAR REACTIONS 236,237,238,239,240,241,242,243,244Pu(48Ca, X)284Fl/285Fl/286Fl/287Fl/288Fl/289Fl/290Fl/291Fl/292Fl, E(cm)=205-225 MeV; calculated σ. Comparison with experimental data.
doi: 10.1088/1361-6471/aa9097
2017SA72 Eur.Phys.J. A 53, 229 (2017) Studies on the synthesis of isotopes of superheavy element Lv (Z = 116)
doi: 10.1140/epja/i2017-12417-0
2016SA35 Phys.Rev. C 94, 024623 (2016) Systematic study of probable projectile-target combinations for the synthesis of the superheavy nucleus 302120 NUCLEAR REACTIONS 258No(44Ar, xn), 256No(46Ar, xn), E(cm)=185-230 MeV; 254Fm(48Ca, xn), 252Fm(50Ca, xn), 250Fm(52Ca, xn), E(cm)=200-250 MeV; 248Cf(54Ti, xn), 246Cf(56Ti, xn), E(cm)=215-265 MeV; 244Cm(58Cr, xn), 242Cm(60Cr, xn), E(cm)=235-280 MeV; 240Pu(62Fe, xn), 238Pu(64Fe, xn), 236Pu(66Fe, xn), E(cm)=245-295 MeV; 234U(68Ni, xn), 232U(70Ni, xn), 230U(72Ni, xn), E(cm)=260-310 MeV; 228Th(74Zn, xn), E(cm)=270-2320 MeV; 218Rn(84Se, xn), 216Rn(86Se, xn), E(cm)=290-330 MeV; 214Po(88Kr, xn), 212Po(90Kr, xn), E(cm)=300-345 MeV; 210Pb(92Sr, xn), 208Pb(94Sr, xn), 206Pb(96Sr, xn), 204Hg(98Zr, xn), E(cm)=310-365 MeV; calculated fusion σ(E), capture σ(E), evaporation σ(E) for x=2n, 3n, 4n and 5n channels. 248Cm(54Cr, xn), E(cm)=235-275 MeV; 244Pu(58Fe, xn), E(cm)=250-290 MeV; 238U(64Ni, xn), E(cm)=260-300 MeV; 249Cf(50Ti, xn), E(cm)=220-270 MeV; calculated fusion σ(E), capture σ(E), evaporation σ(E) for x=2n, 3n, 4n and 5n channels, and compared with available experimental data; deduced probable target-projectile combinations for 302120 from the cold reaction valleys. Wong, and Glas-Mosel models used for calculations. Relevance to the production of Z=120 superheavy element.
doi: 10.1103/PhysRevC.94.024623
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