NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = D.Hirata Found 37 matches. 2011CA02 Few-Body Systems 49, 85 (2011) Static and Covariant Meson-Exchange Interactions in Nuclear Matter
doi: 10.1007/s00601-010-0189-2
2008SC03 Phys.Rev.Lett. 100, 112501 (2008) J.P.Schiffer, S.J.Freeman, J.A.Clark, C.Deibel, C.R.Fitzpatrick, S.Gros, A.Heinz, D.Hirata, C.L.Jiang, B.P.Kay, A.Parikh, P.D.Parker, K.E.Rehm, A.C.C.Villari, V.Werner, C.Wrede Nuclear Structure Relevant to Neutrinoless Double β Decay: 76Ge and 76Se NUCLEAR REACTIONS 74,76Ge, 76,78Se(d, p), E=15 MeV; 76Ge, 76Se(p, d), E=23 MeV; 74,76Ge, 76,78Se(3He, α), E=26 MeV; 74,76Ge, 76,78Se(α, 3He), E=40 MeV; measured reaction products energy spectra, cross sections. Deduced summed spectroscopic strengths, neutron vacancies.
doi: 10.1103/PhysRevLett.100.112501
2007FR10 Phys.Rev. C 75, 051301 (2007) S.J.Freeman, J.P.Schiffer, A.C.C.Villari, J.A.Clark, C.Deibel, S.Gros, A.Heinz, D.Hirata, C.L.Jiang, B.P.Kay, A.Parikh, P.D.Parker, J.Qian, K.E.Rehm, X.D.Tang, V.Werner, C.Wrede Pair correlations in nuclei involved in neutrinoless double Β decay: 76Ge and 76Se NUCLEAR REACTIONS 74,76Ge, 76,78Se(p, t), E=23 MeV; measured yields, cross sections and angular distributions. Compared results to DWBA calculations.
doi: 10.1103/PhysRevC.75.051301
2006BA23 J.Phys.(London) G32, 655 (2006) E.Baldini-Neto, B.V.Carlson, D.Hirata Self-consistent Dirac quasi-particle blocking approximation applied to the α-decay scheme of the superheavy element 287115 NUCLEAR STRUCTURE 63,64,65,66,67,68Ga, 65,66,67,68,69,70Ge, 67,68,69,70,71,72As, 69,70,71,72,73Se, 72,73,74,75Br; calculated binding energies, radii, β2. 287,288Mc, 283,284Nh, 279,280Rg, 275,276Mt, 271,272Bh, 268Db; calculated binding energies, β2, level energies and configurations.Dirac-Hartree-Bogoliubov formalism. RADIOACTIVITY 287Mc, 283Nh, 279Rg, 275Mt(α); calculated Qα, T1/2. Dirac-Hartree-Bogoliubov formalism.
doi: 10.1088/0954-3899/32/5/005
2006KH08 Nucl.Phys. A780, 1 (2006) A.Khouaja, A.C.C.Villari, M.Benjelloun, D.Hirata, G.Auger, H.Savajols, W.Mittig, P.Roussel-Chomaz, N.A.Orr, M.G.Saint-Laurent, S.Pita, A.Gillibert, M.Chartier, C.E.Demonchy, L.Giot, D.Baiborodin, Y.Penionzhkevich, W.N.Catford, A.Lepine-Szily, Z.Dlouhy Reaction cross-section and reduced strong absorption radius measurements of neutron-rich nuclei in the vicinity of closed shells N = 20 and N = 28 NUCLEAR REACTIONS Si(17N, X), (18N, X), (19N, X), (20N, X), (21N, X), (22N, X), (19O, X), (20O, X), (21O, X), (22O, X), (23O, X), (24O, X), (21F, X), (22F, X), (23F, X), (24F, X), (25F, X), (26F, X), (27F, X), (23Ne, X), (24Ne, X), (25Ne, X), (26Ne, X), (27Ne, X), (28Ne, X), (29Ne, X), (30Ne, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (30Na, X), (31Na, X), (32Na, X), (33Na, X), (28Mg, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), (33Mg, X), (34Mg, X), (35Mg, X), (31Al, X), (32Al, X), (33Al, X), (34Al, X), (35Al, X), (36Al, X), (37Al, X), (38Al, X), (33Si, X), (34Si, X), (35Si, X), (36Si, X), (37Si, X), (38Si, X), (39Si, X), (40Si, X), (36P, X), (37P, X), (38P, X), (39P, X), (40P, X), (41P, X), (42P, X), (39S, X), (40S, X), (41S, X), (42S, X), (43S, X), (44S, X), (42Cl, X), (43Cl, X), (44Cl, X), (45Cl, X), (45Ar, X), (46Ar, X), E=30-65 MeV/nucleon; measured energy-integrated reaction σ. 17,18,19,20,21,22N, 19,20,21,22,23,24O, 21,22,23,24,25,26,27F, 23,24,25,26,27,28,29,30Ne, 26,27,28,29,30,31,32,33Na, 28,29,30,31,32,33,34,35Mg, 31,32,33,34,35,36,37,38Al, 33,34,35,36,37,38,39,40Si, 36,37,38,39,40,41,42P, 39,40,41,42,43,44S, 42,43,44,45Cl, 45,46Ar; deduced radii, isospin dependence. 35Mg, 44S; deduced possible halo structure or large deformation.
doi: 10.1016/j.nuclphysa.2006.07.042
2005KH15 Eur.Phys.J. A 25, Supplement 1, 223 (2005) A.Khouaja, A.C.C.Villari, M.Benjelloun, G.Auger, D.Baiborodin, W.Catford, M.Chartier, C.E.Demonchy, Z.Dlouhy, A.Gillibert, L.Giot, D.Hirata, A.Lepine-Szily, W.Mittig, N.Orr, Y.Penionzhkevich, S.Pitae, P.Roussel-Chomaz, M.G.Saint-Laurent, H.Savajols Reaction cross-sections and reduced strong absorption radii of nuclei in the vicinity of closed shells N = 20 and N = 28 NUCLEAR STRUCTURE Z=5-28; A=12-46; analyzed reaction σ on Si target; deduced strong absorption radii. Secondary beams from 48Ca fragmentation, quadratic dependence on isospin observed.
doi: 10.1140/epjad/i2005-06-185-x
2005LE43 Eur.Phys.J. A 25, Supplement 1, 227 (2005) A.Lepine-Szily, G.F.Lima, A.C.C.Villari, W.Mittig, R.Lichtenthaler, M.Chartier, N.A.Orr, J.C.Angelique, G.Audi, J.M.Casandjian, A.Cunsolo, C.Donzaud, A.Foti, A.Gillibert, D.Hirata, M.Lewitowicz, S.Lukyanov, M.MacCormick, D.J.Morrissey, A.N.Ostrowski, B.M.Sherrill, C.Stephan, T.Suomijarvi, L.Tassan-Got, D.J.Vieira, J.M.Wouters Anomalous behaviour of matter radii of proton-rich Ga, Ge, As, Se and Br nuclei NUCLEAR STRUCTURE 63,64,65,66,67,68Ga, 65,66,67,68,69,70Ge, 67,68,69,70,71,72As, 69,70,71,72,73,74,75,76,77,78,79,80Se, 72,73,74,75Br; analyzed reaction σ on Si target; deduced matter radii. Secondary beams from 78Kr fragmentation. Glauber model analysis.
doi: 10.1140/epjad/i2005-06-115-0
2004BA21 Braz.J.Phys. 34, 855 (2004) E.Baldini-Neto, B.V.Carlson, D.Hirata Dirac-Hartree-Bogoliubov Approximation for Finite Nuclei with Blocking NUCLEAR STRUCTURE O, Ni, Ca, Sn; calculated mass defects. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data. RADIOACTIVITY 277Cn, 273Ds, 269Hs, 265Sg, 261Rf, 257No, 253Fm, 249Cf(α); calculated Qα. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data.
doi: 10.1590/s0103-97332004000500039
2004BB21 Braz.J.Phys. 34, 855 (2004) E.Baldini-Neto, B.V.Carlson, D.Hirata Dirac-Hartree-Bogoliubov Approximation for Finite Nuclei with Blocking NUCLEAR STRUCTURE O, Ni, Ca, Sn; calculated mass defects. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data. RADIOACTIVITY 277Cn, 273Ds, 269Hs, 265Sg, 261Rf, 257No, 253Fm, 249Cf(α); calculated Qα. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data.
doi: 10.1590/S0103-97332004000500039
2004BE10 Int.J.Mod.Phys. E13, 79 (2004) J.F.Berger, D.Hirata, M.Girod, J.Decharge Structure of superheavy nuclei with the Gogny force NUCLEAR STRUCTURE Z=84-116; calculated Qα. Pb, Po, Rn, Ra, Th, U; calculated deformation energies. 213Bi, 217At, 221Fr, 225Ac, 229Pa, 233Np, 237Am, 241Bk, 245Es; calculated single-quasiparticle level energies. Hartree-Fock-Bogoliubov approach, Gogny force.
doi: 10.1142/S021830130400176X
2004LI29 Nucl.Phys. A735, 303 (2004) G.F.Lima, A.Lepine-Szily, A.C.C.Villari, W.Mittig, R.Lichtenthaler, M.Chartier, N.A.Orr, J.C.Angelique, G.Audi, E.Baldini-Neto, B.V.Carlson, J.M.Casandjian, A.Cunsolo, C.Donzaud, A.Foti, A.Gillibert, D.Hirata, M.Lewitowicz, S.Lukyanov, M.MacCormick, D.J.Morrissey, A.N.Ostrowski, B.M.Sherrill, C.Stephan, T.Suomijarvi, L.Tassan-Got, D.J.Vieira, J.M.Wouters Reaction cross section and matter radius measurements of proton-rich Ga, Ge, As, Se and Br nuclides NUCLEAR REACTIONS Si(63Ga, X), (64Ga, X), (65Ga, X), (66Ga, X), (67Ga, X), (68Ga, X), (65Ge, X), (66Ge, X), (67Ge, X), (68Ge, X), (69Ge, X), (70Ge, X), (67As, X), (68As, X), (69As, X), (70As, X), (71As, X), (72As, X), (69Se, X), (70Se, X), (71Se, X), (72Se, X), (73Se, X), (72Br, X), (73Br, X), (74Br, X), (75Br, X), E ≈ 50-60 MeV/nucleon; measured reaction σ. 63,64,65,66,67,68Ga, 65,66,67,68,69,70Ge, 67,68,69,70,71,72As, 69,70,71,72,73Se, 72,73,74,75Br; deduced matter radii. Glauber model analysis.
doi: 10.1016/j.nuclphysa.2004.01.125
2003BE67 Acta Phys.Pol. B34, 1909 (2003) Microscopic description of superheavy nuclei with the Gogny effective interaction NUCLEAR STRUCTURE 270Hs; calculated single-particle energies. 260No, 268Rf, 266Sg, 276,280,284Hs, 288Ds, 294Cn, 298Fl, 306118, 318,326122, 326,332124, 318126, 340128; calculated deformation energies. Z=102-126; calculated Qα, α-decay T1/2. 289,287Fl, 277,283,285Cn, 273,281Ds, 269,277Hs, 265Sg, 261Rf, 257No, 253Fm; calculated levels, J, π, Qα. Gogny effective interaction.
2002DE29 Nucl.Phys. A706, 295 (2002) A.de Vismes, P.Roussel-Chomaz, W.Mittig, A.Pakou, N.Alamanos, J.-C.Angelique, F.Auger, J.Barrette, E.Bauge, A.V.Belozyorov, C.Borcea, F.Carstoiu, W.N.Catford, M.-D.Cortina-Gil, J.-P.Delaroche, Z.Dlouhy, A.Gillibert, M.Girod, D.Hirata, V.Lapoux, A.Lepine-Szily, S.M.Lukyanov, F.Marie, A.Musumarra, F.de Oliveira, N.A.Orr, S.Ottini-Hustache, Y.E.Penionzhkevich, F.Sarazin, H.Savajols, N.Skobelev Proton Reaction Cross-Section Measurements on Stable and Neutron-Rich Nuclei as a Probe of the Nucleon-Nucleus Interaction NUCLEAR REACTIONS 1H(α, X), (6He, X), (7Li, X), (8Li, X), (9Li, X), (9Be, X), (10Be, X), (11Be, X), (21F, X), (22F, X), (23F, X), (24F, X), (23Ne, X), (24Ne, X), (25Ne, X), (26Ne, X), (25Na, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), E ≈ 35-81 MeV/nucleon; measured reaction σ. Comparison with model predictions.
doi: 10.1016/S0375-9474(02)00753-4
2000CA47 Phys.Rev. C62, 054310 (2000) Dirac-Hartree-Bogoliubov Approximation for Finite Nuclei NUCLEAR STRUCTURE Sn, Kr, Sr; calculated even isotopes two-neutron separation energies, binding energies. Sn; calculated even isotopes neutron radii. Sn, Ni, S, Kr, Sr; calculated even isotopes neutron pair gap parameter. 44S, 46Ar, 100Sr; calculated binding energy vs deformation. Dirac-Hartree-Bogoliubov approximation.
doi: 10.1103/PhysRevC.62.054310
1999AI02 Phys.Rev. C60, 034614 (1999) N.Aissaoui, N.Added, N.Carlin, G.M.Crawley, S.Danczyk, J.Finck, M.M.de Moura, D.Hirata, D.J.Morrissey, S.J.Sanders, J.Stasko, M.Steiner, A.A.P.Suaide, E.M.Szanto, A.Szanto de Toledo, M.Thoennessen, J.A.Winger Strong Absorption Radii from Reaction Cross Section Measurements for Neutron-Rich Nuclei NUCLEAR REACTIONS Si(30Al, X), (31Al, X), (32Al, X), (33Al, X), (32Si, X), (33Si, X), (34Si, X), (35Si, X), (36Si, X), (34P, X), (35P, X), (36P, X), (37P, X), (38P, X), (39P, X), (36S, X), (37S, X), (38S, X), (39S, X), (40S, X), (41S, X), (39Cl, X), (40Cl, X), (41Cl, X), (42Cl, X), (43Cl, X), (44Cl, X), (41Ar, X), (42Ar, X), (43Ar, X), (44Ar, X), (45Ar, X), (46Ar, X), (44K, X), (45K, X), (46K, X), (47K, X), (48K, X), (46Ca, X), (47Ca, X), (48Ca, X), (49Ca, X), (50Ca, X), (49Sc, X), (50Sc, X), (51Sc, X), (52Sc, X), (53Ti, X), (54Ti, X), E ≈ 38-80 MeV/nucleon; measured mean energy-integrated reaction σ. 30,31,32,33Al, 32,33,34,35,36Si, 34,35,36,37,38,39P, 36,37,38,39,40,41S, 39,40,41,42,43,44Cl, 41,42,43,44,45,46Ar, 44,45,46,47,48K, 46,47,48,49,50Ca, 49,50,51,52Sc, 53,54Ti deduced strong absorption radii. Secondary beams from 55Mn fragmentation.
doi: 10.1103/PhysRevC.60.034614
1998SU06 Nucl.Phys. A630, 402c (1998) T.Suzuki, H.Geissel, O.Bochkarev, L.Chulkov, M.Golovkov, N.Fukunishi, D.Hirata, H.Irnich, Z.Janas, H.Keller, T.Kobayashi, G.Kraus, G.Munzenberg, S.Neumaier, F.Nickel, A.Ozawa, A.Piechaczeck, E.Roeckl, W.Schwab, K.Summerer, K.Yoshida, I.Tanihata Neutron Skin of Na Isotopes and an Application to the EOS NUCLEAR STRUCTURE Na; analyzed mass radii; deduced neutron skin features. Implications for equation of state.
doi: 10.1016/S0375-9474(97)00778-1
1998SU07 Nucl.Phys. A630, 661 (1998) T.Suzuki, H.Geissel, O.Bochkarev, L.Chulkov, M.Golovkov, N.Fukunishi, D.Hirata, H.Irnich, Z.Janas, H.Keller, T.Kobayashi, G.Kraus, G.Munzenberg, S.Neumaier, F.Nickel, A.Ozawa, A.Piechaczeck, E.Roeckl, W.Schwab, K.Summerer, K.Yoshida, I.Tanihata Nuclear Radii of Na and Mg Isotopes NUCLEAR REACTIONS C(20Na, X), (21Na, X), (22Na, X), (23Na, X), (25Na, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (30Na, X), (31Na, X), (32Na, X), (20Mg, X), (22Mg, X), (23Mg, X), (24Mg, X), (25Mg, X), (27Mg, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), (33Mg, X), E=950 MeV/nucleon; measured interaction σ. 20,21,22,23,25,26,27,28,29,30,31,32Na, 20,22,23,24,27,29,30,31,32Mg deduced rms radii, neutron, proton skin features. Shell model calculations.
doi: 10.1016/S0375-9474(97)00799-9
1998TO16 J.Phys.(London) G24, 1479 (1998) H.Toki, H.Shen, K.Sumiyoshi, D.Hirata, Y.Sugahara, I.Tanihata Relativistic Many-Body Theory for Unstable Nuclei and Astrophysics
doi: 10.1088/0954-3899/24/8/023
1997HI03 Nucl.Phys. A616, 438c (1997) D.Hirata, K.Sumiyoshi, I.Tanihata, Y.Sugahara, T.Tachibana, H.Toki A Systematic Study of Even-Even Nuclei Up to the Drip Lines within the Relativistic Mean Field Framework NUCLEAR STRUCTURE Z=8-120; 94,96,98,100,102Zr; calculated binding energy per particle; A ≈ 80-220; calculated relative r-process abundances. Relativistic mean field theory.
doi: 10.1016/S0375-9474(97)00115-2
1997LI15 Phys.Rev. C56, 250 (1997) I.Licot, N.Added, N.Carlin, G.M.Crawley, S.Danczyk, J.Finck, D.Hirata, H.Laurent, D.J.Morrissey, M.M.de Moura, H.R.Schelin, J.Stasko, M.Steiner, A.A.P.Suaide, A.Szanto de Toledo, E.M.Szanto, M.Thoennessen, J.A.Winger Reaction Cross Sections and Radii for f-p Shell Exotic Neutron-Rich Nuclei NUCLEAR REACTIONS, ICPND Si(41Ar, X), (42Ar, X), (43Ar, X), (44Ar, X), (45Ar, X), (46Ar, X), (44K, X), (45K, X), (46K, X), (47K, X), (48K, X), (49K, X), (46Ca, X), (47Ca, X), (48Ca, X), (49Ca, X), (50Ca, X), (51Ca, X), (49Sc, X), (50Sc, X), (51Sc, X), (52Sc, X), (53Sc, X), E=52-69 MeV/nucleon; measured reaction σ. 41,42,43,44,45,46Ar, 44,45,46,47,48,49K, 46,47,48,49,50,51Ca, 49,50,51,52,53Sc deduced strong absorption radii, neutron separation energies. Comparison to Glauber model, RMF theory.
doi: 10.1103/PhysRevC.56.250
1997SU04 Nucl.Phys. A616, 286c (1997) T.Suzuki, H.Geissel, O.Bochkarev, L.Chulkov, M.Golovkov, D.Hirata, H.Irnich, Z.Janas, H.Keller, T.Kobayashi, G.Kraus, G.Munzenberg, S.Neumaier, F.Nickel, A.Ozawa, A.Piechaczek, E.Roeckl, W.Schwab, K.Summerer, K.Yoshida, I.Tanihata Matter Radii of Na and Mg Isotopes NUCLEAR REACTIONS C(20Na, X), (21Na, X), (22Na, X), (23Na, X), (25Na, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (30Na, X), (31Na, X), (32Na, X), (20Mg, X), (22Mg, X), (23Mg, X), (24Mg, X), (25Mg, X), (27Mg, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), (33Mg, X), E=950 MeV/nucleon; measured interaction σ. 32,31,30,29,28,27,26,25,23,22,21,20Na, 20,22,23,24,27,29,30,31,32Mg deduced effective rms radii, nucleon skin thickness related features.
doi: 10.1016/S0375-9474(97)00099-7
1996HI12 Nucl.Phys. A609, 131 (1996) D.Hirata, K.Sumiyoshi, B.V.Carlson, H.Toki, I.Tanihata Triaxial Deformation of Unstable Nuclei in the Relativistic Mean-Field Theory NUCLEAR STRUCTURE 16O, 40Ca, 20,24Ne, 24Mg; calculated energy surfaces, nucleon, charge radii, proton deformation, quadrupole moment. 42,44,46,48,50,52,54,46S; calculated energy surfaces, binding energy per nucleon, nucleon radii, deformations. Relativistic mean field theory.
doi: 10.1016/S0375-9474(96)00298-9
1996OB01 Nucl.Phys. A609, 74 (1996) M.M.Obuti, T.Kobayashi, D.Hirata, Y.Ogawa, A.Ozawa, K.Sugimoto, I.Tanihata, D.Olson, W.Christie, H.Wieman Interaction Cross Section and Interaction Radius of the 8B Nucleus NUCLEAR REACTIONS C(8B, X), E=790 MeV/nucleon; measured interaction σ. 8B deduced nucleon distribution rms radius, halo tail, separation energy relationship.
doi: 10.1016/0375-9474(96)00267-9
1995HI09 Nucl.Phys. A587, 787 (1995) S.Hirenzaki, P.Fernandez de Cordoba, N.Fukunishi, D.Hirata, H.Kitagawa, M.J.Vicente-Vacas (3He, t) Reactions on Unstable Nuclei at Intermediate Energies NUCLEAR REACTIONS 33,38,40,60,70Ca(3He, t), E=1.4-2 GeV; calculated σ(θ, E(t)); deduced neutron skin role. Target density distributions from relativistic mean field theory.
doi: 10.1016/0375-9474(94)00800-3
1995HI10 Nucl.Phys. A589, 239 (1995) Relativistic Mean-Field Theory on the Xenon, Cesium and Barium Isotopes NUCLEAR STRUCTURE 118,120,122,124,126,128,130,132,134,136,138,140,142,144,146,148Ba; calculated binding energies, radii. Relativistic mean field theory, Xe, Cs isotopes included.
doi: 10.1016/0375-9474(95)00035-Y
1995OZ01 Nucl.Phys. A583, 807c (1995) A.Ozawa, I.Tanihata, T.Kobayashi, D.Hirata, O.Yamakawa, K.Omata, N.Takahashi, T.Shimoda, K.Sugimoto, D.Olson, W.Christie, H.Wieman Interaction Cross-Sections and Radii of 11C and 12N and Effective Deformation Parameters in Light Mirror Nuclei NUCLEAR REACTIONS 9Be, C, 27Al(11C, X), (12N, X), E=670-740 MeV; measured interaction σ. 12N deduced effective rms radius, halo characteristics.
doi: 10.1016/0375-9474(94)00763-D
1995SU18 Phys.Rev.Lett. 75, 3241 (1995) T.Suzuki, H.Geissel, O.Bochkarev, L.Chulkov, M.Golovkov, D.Hirata, H.Irnich, Z.Janas, H.Keller, T.Kobayashi, G.Kraus, G.Munzenberg, S.Neumaier, F.Nickel, A.Ozawa, A.Piechaczek, E.Roeckl, W.Schwab, K.Summerer, K.Yoshida, I.Tanihata Neutron Skin of Na Isotopes Studied Via Their Interaction Cross Sections NUCLEAR REACTIONS C(20Na, X), (21Na, X), (22Na, X), (23Na, X), (25Na, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (30Na, X), (31Na, X), (32Na, X), E=950 MeV/nucleon; measured interaction σ. 20,21,22,23,25,26,27,28,29,30,31,32Na deduced effective rms radii, proton-neutron separation energy difference.
doi: 10.1103/PhysRevLett.75.3241
1995TA06 Nucl.Phys. A583, 769c (1995) Are All Nucleus Spherical at the Drip Line ( Question ) NUCLEAR STRUCTURE 14Be, 17Ne; calculated 2s1/2, 1d5/2, n-, p-orbital binding energy vs potential depth. 17Ne, 12,17N, 17F, 17O, 12C, 8,12,7B, 8,7Li; analyzed minor pairs radii; deduced spherical orbitals closure role in drip lines.
doi: 10.1016/0375-9474(94)00756-D
1995TO06 Nucl.Phys. A588, 357c (1995) H.Toki, D.Hirata, Y.Sugahara, K.Sumiyoshi, I.Tanihata Relativistic Many Body Approach for Unstable Nuclei and Supernova NUCLEAR STRUCTURE A=10-270; calculated binding energy per nucleon vs mass, proton, neutron radii for proton magic nuclei. Relativistic many body approach.
doi: 10.1016/0375-9474(95)00161-S
1994OZ02 Phys.Lett. 334B, 18 (1994) A.Ozawa, T.Kobayashi, H.Sato, D.Hirata, I.Tanihata, O.Yamakawa, K.Omata, K.Sugimoto, D.Olson, W.Christie, H.Wieman Interaction Cross Sections and Radii of the Mass Number A = 17 Isobar (17N, 17F, and 17Ne) NUCLEAR REACTIONS 9Be, C, 27Al(20Ne, X), (22Ne, X), (18O, X), E=620-750 MeV/nucleon; measured 17N, 17F, 17Ne interaction σ with 9Be, C, 27Al targets. 17N, 17F, 17Ne, 17B deduced charge, nucleon, matter distributions rms radii.
doi: 10.1016/0370-2693(94)90585-1
1993HI11 Phys.Lett. 314B, 168 (1993) D.Hirata, H.Toki, I.Tanihata, P.Ring Systematic Study of Sr Isotopes in the Relativistic Mean Field Theory NUCLEAR STRUCTURE 78,80,82,84,86,88,90,92,94,98,100,79,81,83,85,87,89,91,93,95,97,99Sr; calculated binding energy per particle, isotope shifts. Relativistic mean field theory.
doi: 10.1016/0370-2693(93)90444-M
1993SU05 Nucl.Phys. A552, 437 (1993) K.Sumiyoshi, D.Hirata, H.Toki, H.Sagawa Comparison of the Relativistic Mean-Field Theory and the Skyrme Hartree-Fock Theory for Properties of Nuclei and Nuclear Matter NUCLEAR STRUCTURE 40,48Ca, 56,58,60,62Ni, 112,114,116,118,120,122,124Sn, 204,206,208Pb; calculated proton, neutron rms radii, binding energy per particle. 36,38,42,44,46,50Ca, 54,64,66,68Ni, 102,104,106,108,110,126,128,132,134Sn, 184,186,188,190,192,194,196,198,200,202,210,212Pb; calculated binding energy per particle. Relativistic mean field, Skyrme Hartree-Fock theories comparison.
doi: 10.1016/0375-9474(93)90277-5
1992BO06 Phys.Rev.Lett. 68, 1283 (1992) R.N.Boyd, I.Tanihata, N.Inabe, T.Kubo, T.Nakagawa, T.Suzuki, M.Yanokura, X.X.Bai, K.Kimura, S.Kubono, S.Shimoura, H.S.Xu, D.Hirata Measurement of the 8Li(α, n)11B Reaction Cross Section at Energies of Astrophysical Interest NUCLEAR REACTIONS, ICPND 4He(8Li, n), E(cm)=1-6 MeV; measured σ(E).
doi: 10.1103/PhysRevLett.68.1283
1992TA18 Phys.Lett. 289B, 261 (1992) I.Tanihata, D.Hirata, T.Kobayashi, S.Shimoura, K.Sugimoto, H.Toki Revelation of Thick Neutron Skins in Nuclei NUCLEAR STRUCTURE 4,6,8He; analyzed reaction data; deduced model parameters, point-nucleon rms radii, nucleon density distributions. Results on Na isotopes also presented. Relativitic mean field model.
doi: 10.1016/0370-2693(92)91216-V
1992TO07 Hyperfine Interactions 74, 113 (1992) Nuclear Properties Far from the Stability Line in the Relativistic Mean Field Theory NUCLEAR STRUCTURE N ≤ 175; calculated binding energy per particle, proton, neutron, charge rms radii. Relativistic mean field theory.
doi: 10.1007/BF02398621
1991HI10 Phys.Rev. C44, 1467 (1991) D.Hirata, H.Toki, T.Watabe, I.Tanihata, B.V.Carlson Relativistic Hartree Theory for Nuclei Far from the Stability Line NUCLEAR STRUCTURE 36,40,44,48,52,56,60,64,68,38,42,46,50,54,58,62,66,70Ca; calculated binding energy per particle, p, n, charge radii, single particle spectra. Relativistic Hartree theory.
doi: 10.1103/PhysRevC.44.1467
1991TO03 Nucl.Phys. A524, 633 (1991) H.Toki, Y.Sugahara, D.Hirata, B.V.Carlson, I.Tanihata Properties of Nuclei Far from the Stability Line in the Relativistic Hartree Theory NUCLEAR STRUCTURE 12C, 16O, 40Ca, 90Zr; calculated binding energy per particle, p, n charge rms radii. 36,38,40,42,44,46,48,50,52,54,56,58,60,62,64,66,68,70Ca; calculated binding energy per particle, p, n charge rms radii, density distributions. Relativistic Hartree theory.
doi: 10.1016/0375-9474(91)90266-9
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