NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = A.B.Balantekin Found 68 matches. 2023AN15 J.Phys.(London) G50, 120501 (2023) A.M.Ankowski, A.Ashkenazi, S.Bacca, J.L.Barrow, M.Betancourt, A.Bodek, M.E.Christy, L.Doria, S.Dytman, A.Friedland, O.Hen, C.J.Horowitz, N.Jachowicz, W.Ketchum, T.Lux, K.Mahn, C.Mariani, J.Newby, V.Pandey, A.Papadopoulou, E.Radicioni, F.Sanchez, C.Sfienti, J.M.Udias, L.Weinstein, L.Alvarez-Ruso, J.E.Amaro, C.A.Arguelles, A.B.Balantekin, S.Bolognesi, V.Brdar, P.Butti, S.Carey, Z.Djurcic, O.Dvornikov, S.Edayath, S.Gardiner, J.Isaacson, W.Jay, A.Klustova, K.S.McFarland, A.Nikolakopoulos, A.Norrick, S.Pastore, G.Paz, M.H.Reno, I.Ruiz Simo, J.E.Sobczyk, A.Sousa, N.Toro, Y.-D.Tsai, M.Wagman, J.G.Walsh, G.Yang Electron scattering and neutrino physics
doi: 10.1088/1361-6471/acef42
2023BA28 Eur.Phys.J. A 59, 186 (2023) A.B.Balantekin, M.J.Cervia, A.V.Patwardhan, E.Rrapaj, P.Siwach Quantum information and quantum simulation of neutrino physics
doi: 10.1140/epja/s10050-023-01092-7
2021CE01 Phys.Rev. C 104, 024305 (2021) M.J.Cervia, A.B.Balantekin, S.N.Coppersmith, C.W.Johnson, P.J.Love, C.Poole, K.Robbins, M.Saffman Lipkin model on a quantum computer
doi: 10.1103/PhysRevC.104.024305
2020BA26 Phys.Rev. C 101, 054605 (2020) A.B.Balantekin, for the PROSPECT Collaboration Nonfuel antineutrino contributions in the ORNL High Flux Isotope Reactor (HFIR) NUCLEAR REACTIONS Li, Be, B, Mg, Al, V, Cr, Mn, Fe, Ni, Cu, Se, Nb, Mo, Eu, Ta, Np, 238Np, 239Pu, 245,247Cm(n, γ), (n, X)6He/7Li/8Li/11B/25Mg/26Mg/27Mg/28Al/52V/51Cr/53Cr/54Cr/55Cr/56Mn/55Fe/56Fe/58Fe/59Fe/59Ni/64Cu/66Cu/79Se/81Se/94Nb/99Mo/152Eu/154Eu/182Ta, E=neutrons from ORNL High Flux Isotope Reactor]; calculated probability density function of antineutrino for nonfission candidates, electron anti-neutrino spectrum from β- decays of antineutrino candidates produced in neutron irradiation of non-fuel High Flux Isotope Reactor materials, and their relative contribution to total antineutrino flux. HFIR reactor modeling and simulation using MCNP code. Relevance to Precision Reactor Oscillation and Spectrum Measurement (PROSPECT) experiment.
doi: 10.1103/PhysRevC.101.054605
2019AS01 Nucl.Instrum.Methods Phys.Res. A922, 287 (2019) J.Ashenfelter, A.B.Balantekin, C.Baldenegro, H.R.Band, C.D.Bass, D.E.Bergeron, D.Berish, L.J.Bignell, N.S.Bowden, J.Boyle, J.Bricco, J.P.Brodsky, C.D.Bryan, A.B.Telles, J.J.Cherwinka, T.Classen, K.Commeford, A.J.Conant, A.A.Cox, D.Davee, D.Dean, G.Deichert, M.V.Diwan, M.J.Dolinski, A.Erickson, M.Febbraro, B.T.Foust, J.K.Gaison, A.Galindo-Uribarri, C.E.Gilbert, K.E.Gilje, A.Glenn, B.W.Goddard, B.T.Hackett, K.Han, S.Hans, A.B.Hansell, K.M.Heeger, B.Heffron, J.Insler, D.E.Jaffe, X.Ji, D.C.Jones, K.Koehler, O.Kyzylova, C.E.Lane, T.J.Langford, J.LaRosa, B.R.Littlejohn, F.Lopez, X.Lu, D.A.Martinez Caicedo, J.T.Matta, R.D.McKeown, M.P.Mendenhall, H.J.Miller, J.M.Minock, P.E.Mueller, H.P.Mumm, J.Napolitano, R.Neilson, J.A.Nikkel, D.Norcini, S.Nour, D.A.Pushin, X.Qian, E.Romero-Romero, R.Rosero, D.Sarenac, B.S.Seilhan, R.Sharma, P.T.Surukuchi, C.Trinh, M.A.Tyra, R.L.Varner, B.Viren, J.M.Wagner, W.Wang, B.White, C.White, J.Wilhelmi, T.Wise, H.Yao, M.Yeh, Y.-R.Yen, A.Zhang, C.Zhang, X.Zhang, M.Zhao The PROSPECT reactor antineutrino experiment
doi: 10.1016/j.nima.2018.12.079
2019KA42 Prog.Part.Nucl.Phys. 107, 109 (2019) T.Kajino, W.Aoki, A.B.Balantekin, R.Diehl, M.A.Famiano, G.J.Mathews Current status of r-process nucleosynthesis
doi: 10.1016/j.ppnp.2019.02.008
2019SU21 J.Phys.(London) G46, 075103 (2019) T.Suzuki, A.B.Balantekin, T.Kajino, S.Chiba Neutrino-13C cross sections at supernova neutrino energies NUCLEAR REACTIONS 13C(ν, E), (ν, ν), E<50 MeV; calculated σ. Comparison with available data.
doi: 10.1088/1361-6471/ab1c11
2018BA26 Acta Phys.Pol. B49, 221 (2018) Facets of Neutrino-Nucleus Interactions
doi: 10.5506/APhysPolB.49.221
2018HA15 Phys.Rev. C 97, 034623 (2018) K.Hagino, A.B.Balantekin, N.W.Lwin, E.Shwe Zin Thein Origin of a maximum of the astrophysical S factor in heavy-ion fusion reactions at deep subbarrier energies NUCLEAR REACTIONS 64Ni(64Ni, X), E(cm)=83-97 MeV; 64Ni(28Si, X), E(cm)=43-53 MeV; calculated fusion σ(E), astrophysical S factor, first derivative of astrophysical S factor using method of two-potential fit to fusion cross sections at deep subbarrier energies. Comparison with experimental data.
doi: 10.1103/PhysRevC.97.034623
2016BA62 Eur.Phys.J. A 52, 341 (2016) Reactor antineutrinos and nuclear physics
doi: 10.1140/epja/i2016-16341-5
2016FA05 Phys.Rev. C 93, 045804 (2016) M.A.Famiano, A.B.Balantekin, T.Kajino Low-lying resonances and relativistic screening in Big Bang nucleosynthesis NUCLEAR REACTIONS 7Be(3He, γ)10C*, E=0.2-2 MeV; calculated integrand of thermonuclear reaction rate (TRR) for energy-dependent width, effects of relativistic electron screening, integrand of the reaction rate for a narrow resonance, ratio of screened to bare TRR for the nonresonant component of the TRR only, thermonuclear reaction rates for several resonances for possible 10C+γ, 9B+p and 2α+2p particle-decay channels in the 10C compound nucleus; deduced destruction of 7Be during the Big Bang nucleosynthesis.
doi: 10.1103/PhysRevC.93.045804
2013BA07 Acta Phys.Pol. B44, 249 (2013) An Outlook on Nuclear Physics
doi: 10.5506/APhysPolB.44.249
2013BA35 J.Phys.:Conf.Ser. 445, 012022 (2013) Neutrinos and rare isotopes
doi: 10.1088/1742-6596/445/1/012022
2012BA45 J.Phys.:Conf.Ser. 337, 012049 (2012) The Last Neutrino Mixing angle θ13
doi: 10.1088/1742-6596/337/1/012049
2012DA02 Phys.Rev. C 85, 044602 (2012) H.Dapo, I.Boztosun, G.Kocak, A.B.Balantekin Influence of long-range effects on low-energy cross sections of He and HeX: The lithium problem NUCLEAR REACTIONS 2H(α, γ)6Li, E<10 MeV; calculated cross section, dependence of σ on charge and mass for 2H(α, γ)6Li and 2H(αX, X)6Li. Optical model and DWBA analysis. Relevance to 6,7Li in big-bang nucleosynthesis. Comparison with experimental data.
doi: 10.1103/PhysRevC.85.044602
2012SU15 Phys.Rev. C 86, 015502 (2012) T.Suzuki, A.B.Balantekin, T.Kajino Neutrino capture on 13C NUCLEAR REACTIONS 12C(ν, e)12N, E=20-60 MeV; 13C(ν, e)13N, E=2-20 MeV; 13C(ν, ν'), E=2-20 MeV; calculated σ(E), B(GT), B(M1) using shell-model calculations. Comparison with experimental data. Discussed implications for the scintillation counter-based experiments to measure electron neutrinos from a core-collapse supernova.
doi: 10.1103/PhysRevC.86.015502
2011AD03 Rev.Mod.Phys. 83, 195 (2011) E.G.Adelberger, A.Garcia, R.G.H.Robertson, K.A.Snover, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, D.Bemmerer, A.Junghans, D.Bemmerer, A.Junghans, C.A.Bertulani, K.-W.Chen, H.Costantini, P.Prati, M.Couder, E.Uberseder, M.Wiescher, R.Cyburt, B.Davids, S.J.Freedman, M.Gai, D.Gazit, L.Gialanella, G.Imbriani, U.Greife, M.Hass, W.C.Haxton, T.Itahashi, K.Kubodera, K.Langanke, D.Leitner, M.Leitner, P.Vetter, L.Winslow, L.E.Marcucci, T.Motobayashi, A.Mukhamedzhanov, R.E.Tribble, F.M.Nunes, T.-S.Park, R.Schiavilla, E.C.Simpson, C.Spitaleri, F.Strieder, H.-P.Trautvetter, K.Suemmerer, S.Typel Solar fusion cross sections. II. The pp chain and CNO cycles NUCLEAR REACTIONS 2H(p, γ), 3He(3He, 2p), (α, γ), (p, e), 7Be, 12C, 14N, 15N, 17O(p, γ), 15N, 16,17,18O(p, α), E<3 MeV; analyzed and evaluated experimental data; deduced recommended values and uncertainties.
doi: 10.1103/RevModPhys.83.195
2011WA02 Phys.Rev. C 83, 018801 (2011) B.Wang, C.A.Bertulani, A.B.Balantekin Electron screening and its effects on big-bang nucleosynthesis
doi: 10.1103/PhysRevC.83.018801
2010BA49 Nucl.Phys. A844, 14c (2010) Neutrinos and symmetries
doi: 10.1016/j.nuclphysa.2010.05.007
2010KO07 Phys.Rev. C 81, 024615 (2010) G.Kocak, M.Karakoc, I.Boztosun, A.B.Balantekin Effects of α-cluster potentials for the 16O+16O fusion reaction and S factor NUCLEAR REACTIONS 16O(16O, 16O), E(cm)=2-15 MeV; analyzed σ and S-factors. 16O(16O, 16O), E(cm)=12.5, 14, 15.5, 20.5, 24.5, 29.5 MeV; analyzed σ(θ). Optical model using Woods-Saxon and α-α double folding α-cluster potentials for fusion reactions.
doi: 10.1103/PhysRevC.81.024615
2007BA01 J.Phys.(London) G34, 47 (2007) Neutrino-neutrino interactions and flavour mixing in dense matter
doi: 10.1088/0954-3899/34/1/004
2007BA45 Phys.Rev. C 75, 064304 (2007) A.B.Balantekin, J.H.de Jesus, Y.Pehlivan Spectra and symmetry in nuclear pairing NUCLEAR STRUCTURE Ni; calculated excitation energy spectra by applying the Bethe ansatz technique to the nuclear pairing problem with orbit dependent coupling constants and degenerate single particle levels.
doi: 10.1103/PhysRevC.75.064304
2007BA72 Phys.Rev. C 76, 051001 (2007) Solutions of nuclear pairing
doi: 10.1103/PhysRevC.76.051001
2007MI13 Phys.Rev. C 75, 045802 (2007) F.Minato, K.Hagino, N.Takigawa, A.B.Balantekin, Ph.Chomaz Effect of electronic environment on neutrino-nucleus reactions at r-process sites NUCLEAR REACTIONS 56Fe, 208Pb(ν, e), E not given; calculated σ(E), electron screening and Pauli blocking effects.
doi: 10.1103/PhysRevC.75.045802
2005BA09 New Journal of Physics 7, 51 (2005) Neutrino mixing and nucleosynthesis in core-collapse supernovae
doi: 10.1088/1367-2630/7/1/051
2005BA26 Int.J.Mod.Phys. E14, 39 (2005) Neutrino physics and nuclear axial two-body interactions
doi: 10.1142/S0218301305002758
2005BA27 Int.J.Mod.Phys. E14, 47 (2005) A.B.Balantekin, T.Dereli, Y.Pehlivan Exactly solvable pairing model using an extension of the Richardson-Gaudin approach
doi: 10.1142/S021830130500276X
2005HA22 Phys.Rev. C 71, 044612 (2005) K.Hagino, T.Takehi, A.B.Balantekin, N.Takigawa Surface diffuseness anomaly in heavy-ion potentials for large-angle quasielastic scattering NUCLEAR REACTIONS 154Sm(16O, X), E(cm) ≈ 35-70 MeV; calculated quasielastic scattering σ, dependence on surface diffuseness parameter. Comparison with data.
doi: 10.1103/PhysRevC.71.044612
2005SA58 Astrophys.J. 634, 534 (2005) T.Sasaqui, T.Kajino, A.B.Balantekin Supernova neutrino effects on r-process nucleosynthesis in black hole formation
doi: 10.1086/491730
2004BA75 Prog.Theor.Phys.(Kyoto), Suppl. 154, 465 (2004) FUSION03, Concluding Remarks
doi: 10.1143/PTPS.154.465
2003BA87 J.Phys.(London) G29, 2513 (2003) Supernova neutrino-nucleus astrophysics
doi: 10.1088/0954-3899/29/11/007
2003BB01 Phys.Rev. C 68, 055801 (2003) Constraints on axial two-body currents from solar neutrino data
doi: 10.1103/PhysRevC.68.055801
2003HA35 Phys.Rev. C 68, 048801 (2003) K.Hagino, M.S.Hussein, A.B.Balantekin Role of virtual break-up of projectile in astrophysical fusion reactions NUCLEAR REACTIONS 3He(d, p), 7Li(p, α), E(cm)=0-100 keV; calculated virtual Coulomb breakup contribution.
doi: 10.1103/PhysRevC.68.048801
2002BB14 Prog.Theor.Phys.(Kyoto), Suppl. 146, 227 (2002) Overview of Neutrino-Nucleus Interactions
doi: 10.1143/PTPS.146.227
2002HA51 Phys.Rev. C 66, 055801 (2002) Radiation correction to astrophysical fusion reactions and the electron screening problem NUCLEAR REACTIONS 3He(d, p), E=5.88 MeV; 2H(3He, p), E=5.38 MeV; 6,7Li, 10,11B(p, α), E=11-19 MeV; 1H(6Li, α), (7Li, α), E=11-13 MeV; calculated enhancement factor due to electromagnetic environment. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.66.055801
1999MC02 Phys.Rev. C59, 2873 (1999) G.C.McLaughlin, J.M.Fetter, A.B.Balantekin, G.M.Fuller Active-Sterile Neutrino Transformation Solution for r-Process Nucleosynthesis
doi: 10.1103/PhysRevC.59.2873
1998AD12 Rev.Mod.Phys. 70, 1265 (1998) E.G.Adelberger, S.M.Austin, J.B.Bahcall, A.B.Balantekin, G.Bogaert, L.S.Brown, L.Buchmann, F.E.Cecil, A.E.Champagne, L.de Braeckeleer, C.A.Duba, S.R.Elliott, S.J.Freedom, M.Gai, G.Goldring, C.R.Gould, A.Gruzinov, W.C.Haxton, K.M.Heeger, E.Henley, C.W.Johnson, M.Kamionkowski, R.W.Kavanagh, S.E.Koonin, K.Kubodera, K.Langanke, T.Motobayashi, V.Pandharipande, P.Parker, R.G.H.Robertson, C.Rolfs, R.F.Sawyer, N.Shaviv, T.D.Shoppa, K.A.Snover, E.Swanson, R.E.Tribble, S.Turck-Chieze, J.F.Wilkerson Solar Fusion Cross Sections NUCLEAR REACTIONS 7Be, 12,13C, 15N, 16,17,18O(p, γ), 14,15N, 17,18O(p, α), 7Li(d, p), 3He(p, e+), (α, γ), (3He, 2p), 1H(p, e+), E=low; compiled, analyzed S-factor data, calculations; deduced implications for solar neutrino flux calculations.
doi: 10.1103/RevModPhys.70.1265
1998BA10 Rev.Mod.Phys. 70, 77 (1998) Quantum Tunneling in Nuclear Fusion
doi: 10.1103/RevModPhys.70.77
1998BA96 J.Phys.(London) G24, 2087 (1998) A.B.Balantekin, J.F.Beacom, M.A.Candido Ribeiro Green's Function for Nonlocal Potentials
doi: 10.1088/0954-3899/24/11/010
1997BA95 Nucl.Phys. A627, 324 (1997) A.B.Balantekin, C.A.Bertulani, M.S.Hussein Small Effects in Astrophysical Fusion Reactions NUCLEAR REACTIONS 2H, 3He(d, p), 2H(3He, p), 3He(3He, 2p), 6,7Li, 10,11B(p, α), 6Li(d, α), 1,2H(6Li, α), 1H(7Li, α), E not given; calculated reaction rates correction factors. Atomic screening, vacuum polarization, bremsstralung, atomic polarization effects discussed.
doi: 10.1016/S0375-9474(97)00589-7
1997HA41 Phys.Rev. C56, 2104 (1997) K.Hagino, N.Takigawa, A.B.Balantekin Fusion Barrier Distributions in Systems with Finite Excitation Energy
doi: 10.1103/PhysRevC.56.2104
1996BA57 Phys.Rev. C54, 1853 (1996) A.B.Balantekin, A.J.DeWeerd, S.Kuyucak Relations between Fusion Cross Sections and Average Angular Momenta NUCLEAR REACTIONS 154Sm(16O, X), E=55-70 MeV; analyzed fusion; deduced fusion σ moments, angular momentum averages relation.
doi: 10.1103/PhysRevC.54.1853
1995HA15 Phys.Rev. C52, 286 (1995) K.Hagino, N.Takigawa, A.B.Balantekin, J.R.Bennett Path Integral Approach to No-Coriolis Approximation in Heavy-Ion Collisions
doi: 10.1103/PhysRevC.52.286
1994BA03 Phys.Rev. C49, 1079 (1994) A.B.Balantekin, J.R.Bennett, S.Kuyucak Systematic Study of Subbarrier Fusion in Rare-Earth Nuclei NUCLEAR REACTIONS, ICPND 144,148,154Sm(16O, X), E(cm)=50-66 MeV; 186W(16O, X), E(cm) ≈ 62-78 MeV; 194Pt, 192Os(16O, X), E(cm)=65-80 MeV; calculated fusion σ(E); deduced barrier distribution shape changes, shape-phase transitions connection. Interacting boson model for structure effects.
doi: 10.1103/PhysRevC.49.1079
1994BA16 Phys.Rev. C49, 1294 (1994) A.B.Balantekin, J.R.Bennett, S.Kuyucak Sub-Barrier Fusion in Generalized Boson Models NUCLEAR REACTIONS, ICPND 154Sm(16O, X), E(cm)=50-70 MeV; calculated fusion σ(E), barrier distributions, average angular momentum vs E. Generalized boson models, sub-barrier fusion.
doi: 10.1103/PhysRevC.49.1294
1994BA63 Phys.Lett. 335B, 295 (1994) A.B.Balantekin, J.R.Bennett, S.Kuyucak Effects of Nuclear Structure on Average Angular Momentum in Subbarrier Fusion NUCLEAR REACTIONS, ICPND 154,152,150,148Sm(16O, X), E(cm)=50-70 MeV; 192Os, 194Pt(16O, X), E=64-80 MeV; 192Os, 194Pt(40Ca, X), E=158-182 MeV; calculated fusion σ(E); deduced structure effects on average angular momentum.
doi: 10.1016/0370-2693(94)90353-0
1994BE23 Phys.Rev. C50, 1104 (1994) C.A.Bertulani, A.B.Balantekin, E.Ditzel Mott Scattering as a Probe of Long Range QCD Effects NUCLEAR REACTIONS Pb(Pb, X), E=873 MeV; calculated δ-electron spectrum, electron total binding energy in quasimolecule. Pb(Pb, Pb), E ≈ 850-1150 MeV; calculated Mott oscillations shifts; deduced atomic effects role in extracting color van der Waals force strength limits.
doi: 10.1103/PhysRevC.50.1104
1993BA38 Phys.Rev. C48, 1269 (1993) A.B.Balantekin, J.R.Bennett, S.Kuyucak Importance of Higher Order Coupling Effects in Sub-Barrier Fusion NUCLEAR REACTIONS, ICPND 154Sm(16O, X), E(cm) ≈ 50-70 MeV; calculated fusion σ(E); deduced higher order coupling effects role. Green's function technique, interacting boson model.
doi: 10.1103/PhysRevC.48.1269
1993BE36 Phys.Lett. 314B, 275 (1993) Molecular Bond Effects in the Fusion of Halo Nuclei NUCLEAR REACTIONS, ICPND 9Li(11Li, X), E(cm)=0.5-3 MeV; calculated σ(E); deduced molecular bond effects role. Halo nuclei.
doi: 10.1016/0370-2693(93)91235-F
1992BA54 Phys.Rev. C46, 2019 (1992) A.B.Balantekin, J.R.Bennett, A.J.DeWeerd, S.Kuyucak Subbarrier Fusion in the Interacting Boson Model NUCLEAR REACTIONS, ICPND 154Sm(16O, X), E=50-70 MeV; calculated σ(E), average angular momentum vs E, barrier distributions. Interacting boson model, comparison with geometrical model.
doi: 10.1103/PhysRevC.46.2019
1991BA27 Phys.Rev. C44, 145 (1991) A.B.Balantekin, J.R.Bennett, N.Takigawa Description of Nuclear Structure Effects in Sub-Barrier Fusion by the Interacting Boson Model NUCLEAR REACTIONS, ICPND 154Sm(16O, X), E ≈ 54-69 MeV; 166Er(16O, X), E=58-83 MeV; calculated fusion σ(E). Interacting boson model.
doi: 10.1103/PhysRevC.44.145
1991TA12 Phys.Rev. C44, 477 (1991) N.Takigawa, F.Michel, A.B.Balantekin, G.Reidemeister Dynamic Polarization Potential Induced by the Coulomb Excitation of Deformed Heavy Ions: Geometric scattering approach NUCLEAR REACTIONS 184W(18O, 18O), E=90 MeV; calculated σ(θ). Geometric scattering theory, WKB approximation.
doi: 10.1103/PhysRevC.44.477
1991TA20 Phys.Lett. 262B, 199 (1991) N.Takigawa, F.Michel, A.B.Balantekin, G.Reidemeister A Geometric Approach to Strong Coupling Effects in Heavy-Ion Collisions. Deviation from the Fresnel Diffraction Pattern NUCLEAR REACTIONS 189W(18O, 18O), E=90 MeV; calculated σ(θ); deduced Coriolis coupling role. Geometric approach.
doi: 10.1016/0370-2693(91)91554-9
1989SC11 Phys.Rev. C39, 2419 (1989) H.A.Schmitt, P.Halse, A.B.Balantekin, B.R.Barrett Noncompact Orthosymplectic Supersymmetry in 61Ni and 62Ni NUCLEAR STRUCTURE 61,62Ni; calculated levels, B(λ); deduced supersymmetry classification scheme. Geometrical model, noncompact orthosymplectic supersymmetry.
doi: 10.1103/PhysRevC.39.2419
1988BA47 Phys.Rev. C38, 1392 (1988) A.B.Balantekin, B.R.Barrett, P.Halse β Vibrations in the O(6) Limit of the Proton-Neutron Interacting Boson Model NUCLEAR STRUCTURE 196Pt, 134Ba; calculated (β)-vibrational state energy. Proton-neutron interacting boson model, O(6) limit.
doi: 10.1103/PhysRevC.38.1392
1988SC06 J.Phys.(London) G14, 657 (1988) H.A.Schmitt, A.B.Balantekin, B.R.Barrett Comment on ' Application of Spinor Symmetry to 131,133Xe and 135Ba ' NUCLEAR STRUCTURE 131Xe; calculated B(λ). Spinor symmetry validity discussion.
doi: 10.1088/0305-4616/14/5/020
1987BA17 Phys.Rev. C35, 1878 (1987) Collective 2+ States in the U(5) Classical Limit of the Proton-Neutron Interacting Boson Model NUCLEAR STRUCTURE 140Ba; calculated symmetric, antisymmetric 2+ state energies. Interacting boson model.
doi: 10.1103/PhysRevC.35.1878
1986BA01 Phys.Rev. C33, 379 (1986) Determination of an Effective Radius from the Gamma-Ray Multiplicities in Fusion Reactions NUCLEAR REACTIONS, ICPND 12C(12C, 12C), E=4.5-6.5 MeV; 64Ni(64Ni, 64Ni), E=96-102 MeV; calculated σ(E), effective radius, <L> vs E. 154Sm(12C, X), (16O, X), E not given; analyzed fusion σ, γ multiplicity data; deduced effective radius. Inversion procedure.
doi: 10.1103/PhysRevC.33.379
1986BA55 Phys.Rev. C34, 1917 (1986) Bose-Fermi Symmetry Chain for the Description of Odd-Odd Nuclei NUCLEAR STRUCTURE 196,198Au; calculated levels. Bose-Fermi symmetry scheme.
doi: 10.1103/PhysRevC.34.1917
1986LE16 Phys.Rev.Lett. 57, 2916 (1986); Erratum Phys.Rev.Lett. 59, 1171 (1987) S.-J.Lee, J.Fink, A.B.Balantekin, M.R.Strayer, A.S.Umar, P.-G.Reinhard, J.A.Maruhn, W.Greiner Relativistic Hartree Calculations for Axially Deformed Nuclei NUCLEAR STRUCTURE 12C, 16O, 20Ne, 24Mg, 40,48Ca; calculated binding energies, quadrupole moments. Relativistic Hartree calculations.
doi: 10.1103/PhysRevLett.57.2916
1986LO04 Z.Phys. A323, 491 (1986) V.Lopac, S.Brant, V.Paar, O.W.B.Schult, H.Seyfarth, A.B.Balantekin Odd-Odd Nucleus 198Au as First Test of IBFFM (OTQM) NUCLEAR STRUCTURE 198Au; calculated levels. Interacting boson-fermion model, multipole-multipole, surface delta, spin-spin, spin-spin delta, tensor interactions.
1985BA31 Phys.Rev. C32, 288 (1985) Collective M1 States in the Classical Limit of the Neutron-Proton Interacting Boson Model NUCLEAR STRUCTURE 152,154,156Gd; calculated n-p antisymmetric M1 state vs Majorana term parameter. Interacting boson model.
doi: 10.1103/PhysRevC.32.288
1985WU03 Phys.Rev. C32, 1432 (1985) J.Q.Wu, G.Bertsch, A.B.Balantekin Channel Coupling Effects in Subbarrier Fusion of Oxygen with Oxygen NUCLEAR REACTIONS, ICPND 16,18O(16O, X), E(cm) ≈ 6.5-12 MeV; calculated fusion σ(E); deduced subbbarrier enhancement mechanism. Coupled-channels model.
doi: 10.1103/PhysRevC.32.1432
1983BA16 Phys.Rev. C27, 1761 (1983) A.B.Balantekin, I.Bars, R.Bijker, F.Iachello New Class of Supersymmetry in Nuclei NUCLEAR STRUCTURE 195Pt; calculated levels; deduced new supersymmetry classification.
doi: 10.1103/PhysRevC.27.1761
1983BA47 Phys.Lett. 129B, 153 (1983) A.B.Balantekin, B.R.Barrett, S.Levit Potential Energy Surfaces in the Classical Limit of the IBM-2 NUCLEAR STRUCTURE 168,170,172,174,176,178,180,182,184,186,188,190,192,194W; calculated neutron proton potential energy distribution; deduced stable minimum deformation parameters.
doi: 10.1016/0370-2693(83)90832-8
1983BA49 Phys.Rev. C28, 1565 (1983) A.B.Balantekin, S.E.Koonin, J.W.Negele Inversion Formula for the Internucleus Potential using Sub-Barrier Fusion Cross Sections NUCLEAR REACTIONS 13C(13C, X), 64Ni(64Ni, X), 40Ca(40Ca, X), E=sub-barrier; analyzed fusion σ; deduced ion-ion potential. Inversion formula.
doi: 10.1103/PhysRevC.28.1565
1981BA24 Phys.Rev.Lett. 47, 19 (1981) A.B.Balantekin, I.Bars, F.Iachello U(6/4) Dynamical Supersymmetry in Nuclei NUCLEAR STRUCTURE 190Os, 191Ir; calculated levels; deduced supersymmetry scheme. Group, U(6/4).
doi: 10.1103/PhysRevLett.47.19
1981BA47 Nucl.Phys. A370, 284 (1981) A.B.Balantekin, I.Bars, F.Iachello U(6/4) Supersymmetry in Nuclei NUCLEAR STRUCTURE 196Pt, 191,193Ir, 190,192Os; calculated levels; deduced supersymmetry scheme. 198,196Hg, 192,194,196Pt, 191,193Ir, 190,192Os; calculated B(E2); deduced supersymmetry scheme. Group, U(6/4).
doi: 10.1016/0375-9474(81)90078-6
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