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NSR database version of April 26, 2024.

Search: Author = J.M.Pearson

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2023SH20      Phys.Rev. C 108, 025805 (2023)

N.N.Shchechilin, N.Chamel, J.M.Pearson

Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. IV. Role of the symmetry energy in pasta phases

doi: 10.1103/PhysRevC.108.025805
Citations: PlumX Metrics

2022PE01      Phys.Rev. C 105, 015803 (2022)

J.M.Pearson, N.Chamel

Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. III. Inclusion of microscopic corrections to pasta phases

doi: 10.1103/PhysRevC.105.015803
Citations: PlumX Metrics

2021PE06      Phys.Rev. C 103, 034328 (2021)

J.M.Pearson

Reflating the nucleus: The pachydermous droplet model

NUCLEAR STRUCTURE A=10-260; calculated rms radii as function of mass number using leptodermous droplet model (LDM) and pachydermous droplet model (PDM); deduced that the tendency of the standard droplet model (DM) to lead to excessive squeezing of nuclei can be rectified by going beyond the leptodermous picture and attributing to the DM a surface skin of finite thickness.

doi: 10.1103/PhysRevC.103.034328
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2020PE01      Phys.Rev. C 101, 015802 (2020)

J.M.Pearson, N.Chamel, A.Y.Potekhin

Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. II. Pasta phases in semiclassical approximation

doi: 10.1103/PhysRevC.101.015802
Citations: PlumX Metrics

2019MU10      Phys.Rev. C 99, 055805 (2019)

Y.D.Mutafchieva, N.Chamel, Zh.K.Stoyanov, J.M.Pearson, L.M.Mihailov

Role of Landau-Rabi quantization of electron motion on the crust of magnetars within the nuclear energy density functional theory

doi: 10.1103/PhysRevC.99.055805
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2016GO10      Phys.Rev. C 93, 034337 (2016)

S.Goriely, N.Chamel, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XVI. Inclusion of self-energy effects in pairing

ATOMIC MASSES N=8-240; calculated masses for 6884 nuclei using new family of three Hartree-Fock-Bogoliubov (HFB) mass models HFB-30, HFB-31, and HFB-32, and respective interactions, BSk30, BSk31, and BSk32, respectively. New feature of a purely phenomenological pairing term that depends on the density gradient. Best fit to the database of 2353 experimental nuclear masses from AME-2012, and to rms charge-radius data. Relevance to neutron superfluidity in the inner crust of neutron stars.

doi: 10.1103/PhysRevC.93.034337
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2015AU02      At.Data Nucl.Data Tables 103-104, 1 (2015); See 2014PF01

G.Audi, K.Blaum, M.Block, G.Bollen, S.Goriely, J.C.Hardy, F.Herfurth, F.G.Kondev, H.-J.Kluge, D.Lunney, J.M.Pearson, G.Savard, K.S.Sharma, M.Wang, Y.H.Zhang

Comment on "Atomic mass compilation 2012" by B. Pfeiffer, K. Venkataramaniah, U. Czok, C. Scheidenberger

COMPILATION ⁴⁵Cr, ⁴⁷Ar, ⁶⁵As, ⁷³Ge, ¹⁰⁰Sn, ²⁸⁶Nh; compiled experimental atomic masses; deduced differences with work of B. Pfeiffer et al.

doi: 10.1016/j.adt.2014.05.003
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2015CH21      Acta Phys.Pol. B46, 349 (2015)

N.Chamel, J.M.Pearson, A.F.Fantina, C.Ducoin, S.Goriely, A.Pastore

Brussels-Montreal Nuclear Energy Density Functionals, from Atomic Masses to Neutron Stars

doi: 10.5506/APhysPolB.46.349
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2015PE02      Phys.Rev. C 91, 018801 (2015)

J.M.Pearson, N.Chamel, A.Pastore, S.Goriely

Role of proton pairing in a semimicroscopic treatment of the inner crust of neutron stars

doi: 10.1103/PhysRevC.91.018801
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2014PE04      Eur.Phys.J. A 50, 43 (2014)

J.M.Pearson, N.Chamel, A.F.Fantina, S.Goriely

Symmetry energy: nuclear masses and neutron stars

NUCLEAR STRUCTURE Z=10-110; calculated neutron drip line, mass excess, 2n separation energy using HFB nuclear mass models with generalized Skyrme forces.

doi: 10.1140/epja/i2014-14043-8
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2013GO11      Phys.Rev. C 88, 024308 (2013)

S.Goriely, N.Chamel, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XIII. The 2012 atomic mass evaluation and the symmetry coefficient

ATOMIC MASSES Z=8-110, N=8-250; calculated masses of 8509 nuclei using five Hartree-Fock-Bogoliubov (HFB) mass models using unconventional Skyrme forces; fitted to the evaluated masses in AME-2012; deduced rms deviations from AME-2012 data, symmetry coefficients, charge radii, neutron skin thickness, shell gaps for Z=50, 82, N=28, 50, 82, 126 nuclei. Comparison with experimental data. Relevance of the mass models to a unified treatment of outer and inner crusts and cores of neutron stars.

doi: 10.1103/PhysRevC.88.024308
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2013GO18      Phys.Rev. C 88, 061302 (2013)

S.Goriely, N.Chamel, J.M.Pearson

Hartree-Fock-Bogoliubov nuclear mass model with 0.50 MeV accuracy based on standard forms of Skyrme and pairing functionals

ATOMIC MASSES Z>7, N>7; calculated masses for 2353 nuclei using Hartree-Fock-Bogoliubov nuclear mass model with Skyrme force BSk27*, and the pairing parameters. Comparison with evaluated mass data in AME-12.

doi: 10.1103/PhysRevC.88.061302
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2012CH45      Phys.Rev. C 86, 055804 (2012)

N.Chamel, R.L.Pavlov, L.M.Mihailov, Ch.J.Velchev, Zh.K.Stoyanov, Y.D.Mutafchieva, M.D.Ivanovich, J.M.Pearson, S.Goriely

Properties of the outer crust of strongly magnetized neutron stars from Hartree-Fock-Bogoliubov atomic mass models

doi: 10.1103/PhysRevC.86.055804
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2012PE09      Phys.Rev. C 85, 065803 (2012)

J.M.Pearson, N.Chamel, S.Goriely, C.Ducoin

Inner crust of neutron stars with mass-fitted Skyrme functionals

doi: 10.1103/PhysRevC.85.065803
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2011CH61      Phys.Rev. C 84, 062802 (2011)

N.Chamel, A.F.Fantina, J.M.Pearson, S.Goriely

Masses of neutron stars and nuclei

doi: 10.1103/PhysRevC.84.062802
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2011GO36      J.Korean Phys.Soc. 59, 2100s (2011)

S.Goriely, N.Chamel, J.M.Pearson

HFB Mass Models for Nucleosynthesis Applications

COMPILATION Z≈8-120; calculated Q, mass surfaces using various NN forces, neutron capture rates, abundances.

doi: 10.3938/jkps.59.2100
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2011PE16      Phys.Rev. C 83, 065810 (2011)

J.M.Pearson, S.Goriely, N.Chamel

Properties of the outer crust of neutron stars from Hartree-Fock-Bogoliubov mass models

doi: 10.1103/PhysRevC.83.065810
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2010CH11      Phys.Rev. C 81, 045804 (2010)

N.Chamel, S.Goriely, J.M.Pearson, M.Onsi

Unified description of neutron superfluidity in the neutron-star crust with analogy to anisotropic multiband BCS superconductors

doi: 10.1103/PhysRevC.81.045804
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2010GO23      Phys.Rev. C 82, 035804 (2010)

S.Goriely, N.Chamel, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII. Stiffness and stability of neutron-star matter

ATOMIC MASSES Z=8-110, N=8-250; calculated masses for 8509 nuclei using three new Hartree-Fock-Bogoliubov (HFB) mass models, HFB-19, HFB-20, and HFB-21 with unconventional Skyrme forces. ²⁰⁸Pb; calculated isoscalar and isovector effective masses as a function of the radial position, and single-particle proton levels.

doi: 10.1103/PhysRevC.82.035804
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2010PE10      Phys.Rev. C 82, 037301 (2010)

J.M.Pearson, N.Chamel, S.Goriely

Breathing-mode measurements in Sn isotopes and isospin dependence of nuclear incompressibility

NUCLEAR STRUCTURE ^{112,114,116,118,120,122,124}Sn; analyzed energies of breathing mode isoscalar giant-monopole resonances (GMR) using a higher-order leptodermous expansion; deduced symmetry-incompressibility coefficient K_τ. Comparison with experimental data.

doi: 10.1103/PhysRevC.82.037301
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2009CH63      Phys.Rev. C 80, 065804 (2009)

N.Chamel, S.Goriely, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI. Stabilizing neutron stars against a ferromagnetic collapse

doi: 10.1103/PhysRevC.80.065804
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2009GO11      Phys.Rev.Lett. 102, 152503 (2009)

S.Goriely, N.Chamel, J.M.Pearson

Skyrme-Hartree-Fock-Bogoliubov Nuclear Mass Formulas: Crossing the 0.6 MeV Accuracy Threshold with Microscopically Deduced Pairing

doi: 10.1103/PhysRevLett.102.152503
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2009GO41      Eur.Phys.J. A 42, 547 (2009)

S.Goriely, N.Chamel, J.M.Pearson

Recent breakthroughs in Skyrme-Hartree-Fock-Bogoliubov mass formulas

ATOMIC MASSES Z=8-110; calculated atomic masses. Comparison with data.

doi: 10.1140/epja/i2009-10784-7
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2008CH24      Nucl.Phys. A812, 72 (2008)

N.Chamel, S.Goriely, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. IX: Constraint of pairing force to ¹S₀ neutron-matter gap

NUCLEAR STRUCTURE Z=8-110; calculated S(n), Q(β), charge radii. Global fit to 2149 mass data. Compared Skyrme-Hartree-Fock-Bogoliubov mass models when constraining the contact pairing force.

doi: 10.1016/j.nuclphysa.2008.08.015
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2008GO05      Phys.Rev. C 77, 031301 (2008)

S.Goriely, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. VIII. Role of Coulomb exchange

NUCLEAR STRUCTURE N>7; Z=8-110; calculated fission barriers, S(n), Q(β), charge radii, mirror nuclei differences. Global fit to 2149 mass data. Compared Skyrme-Hartree-Fock-Bogoliubov mass models when the Coulomb-exchange term is ignored.

doi: 10.1103/PhysRevC.77.031301
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2008ON01      Phys.Rev. C 77, 065805 (2008), Publishers note Phys.Rev. C 78, 059902 (2008)

M.Onsi, A.K.Dutta, H.Chatri, S.Goriely, N.Chamel, J.M.Pearson

Semi-classical equation of state and specific-heat expressions with proton shell corrections for the inner crust of a neutron star

doi: 10.1103/PhysRevC.77.065805
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2007GO18      Phys.Rev. C 75, 064312 (2007)

S.Goriely, M.Samyn, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. VII. Simultaneous fits to masses and fission barriers

NUCLEAR STRUCTURE Z > 7, N > 7; analyzed masses and fission barrier data using a new HFB mass model.

doi: 10.1103/PhysRevC.75.064312
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2006GO21      Nucl.Phys. A773, 279 (2006)

S.Goriely, M.Samyn, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas VI: Weakened pairing

NUCLEAR STRUCTURE Z=8-120; A=16-360; analysed atomic masses. Nuclear matter properties discussed. Skyrme-Hartree-Fock-Bogoliubov approach, comparison with data and earlier models.

doi: 10.1016/j.nuclphysa.2006.05.002
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2006PE41      Nucl.Phys. A777, 623 (2006)

J.M.Pearson, S.Goriely

Nuclear mass formulas for astrophysics

doi: 10.1016/j.nuclphysa.2004.06.005
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2005BU39      Phys.Rev. C 72, 057305 (2005)

F.Buchinger, J.M.Pearson

Charge radii in macroscopic-microscopic mass models

NUCLEAR STRUCTURE ^{108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125}Sn; calculated charge radii. Finite-range droplet model and finite-range liquid drop model compared with data.

doi: 10.1103/PhysRevC.72.057305
Citations: PlumX Metrics

2005GO07      Nucl.Phys. A750, 425 (2005)

S.Goriely, M.Samyn, J.M.Pearson, M.Onsi

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. IV: Neutron-matter constraint

doi: 10.1016/j.nuclphysa.2005.01.009
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2005GO32      Nucl.Phys. A758, 587c (2005)

S.Goriely, P.Demetriou, H.-Th.Janka, J.M.Pearson, M.Samyn

The r-process nucleosynthesis: a continued challenge for nuclear physics and astrophysics

doi: 10.1016/j.nuclphysa.2005.05.107
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2005GO39      Eur.Phys.J. A 25, Supplement 1, 71 (2005)

S.Goriely, M.Samyn, J.M.Pearson, E.Khan

Recent progress in mass predictions

NUCLEAR STRUCTURE Z=8-120; A=16-340; analyzed atomic masses. Nuclear matter properties discussed. Skyrme-Hartree-Fock-Bogoliubov approach, comparison with data.

doi: 10.1140/epjad/i2005-06-022-4
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2005PE17      Nucl.Phys. A758, 651c (2005)

J.M.Pearson, M.Onsi, S.Goriely, M.Samyn

Hartree-Fock-Bogoliubov mass formulas and the equation of state of neutron-star matter

doi: 10.1016/j.nuclphysa.2005.05.117
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2005SA56      Phys.Rev. C 72, 044316 (2005)

M.Samyn, S.Goriely, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. V. Extension to fission barriers

NUCLEAR STRUCTURE Z=80-130; A=198-314; calculated deformation and fission barrier parameters. Skyrme-Hartree-Fock-Bogoliubov approach, comparisons with data.

doi: 10.1103/PhysRevC.72.044316
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2004DU13      Phys.Rev. C 69, 052801 (2004)

A.K.Dutta, M.Onsi, J.M.Pearson

Proton-shell effects in neutron-star matter

doi: 10.1103/PhysRevC.69.052801
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2004SA55      Phys.Rev. C 70, 044309 (2004)

M.Samyn, S.Goriely, M.Bender, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. III. Role of particle-number projection

NUCLEAR STRUCTURE Z=8-120; calculated masses. ^230,231,233Th, ^{235,236,237,238,239}U, ^237,238Np, ^{235,237,238,239,240,241,243,244}Pu, ^{239,240,241,242,243,244}Am, ^{241,242,243,244,245}Cm, ²⁴⁴Bk; analyzed shape isomer energies. ³²S, ²⁰⁸Pb; calculated charge density distributions. Skyrme-Hartree-Fock-Bogoliubov mass formulas.

doi: 10.1103/PhysRevC.70.044309
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2003GO31      Phys.Rev. C 68, 054325 (2003)

S.Goriely, M.Samyn, M.Bender, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. II. Role of the effective mass

NUCLEAR STRUCTURE Z=8-120; calculated masses; deduced role of effective mass. ¹⁶O, ¹³²Sn, ²⁰⁸Pb; calculated single-particle energy levels. Skyrme-Hartree-Fock-Bogoliubov approach, comparisons with data.

doi: 10.1103/PhysRevC.68.054325
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2003LU10      Rev.Mod.Phys. 75, 1021 (2003)

D.Lunney, J.M.Pearson, C.Thibault

Recent trends in the determination of nuclear masses

doi: 10.1103/RevModPhys.75.1021
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2003SA26      Nucl.Phys. A725, 69 (2003)

M.Samyn, S.Goriely, J.M.Pearson

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas I: Role of density dependence in pairing force

doi: 10.1016/S0375-9474(03)01578-1
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2003SA34      Nucl.Phys. A718, 653c (2003)

M.Samyn, S.Goriely, J.M.Pearson

Nuclear Mass Predictions Within The Skyrme HFB Theory

NUCLEAR STRUCTURE A=2-270; calculated masses. Z=34-70; calculated shell gaps. Self-consistent Skyrme HFB approach.

doi: 10.1016/S0375-9474(03)00877-7
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2002GO26      Phys.Rev. C66, 024326 (2002)

S.Goriely, M.Samyn, P.H.Heenen, J.M.Pearson, F.Tondeur

Hartree-Fock mass formulas and extrapolation to new mass data

NUCLEAR STRUCTURE Z=8-120; analyzed masses, mass formulas; deduced parameters.

ATOMIC MASSES Z=8-120; analyzed masses, mass formulas; deduced parameters.

doi: 10.1103/PhysRevC.66.024326
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2002ON01      Phys.Rev. C65, 047302 (2002)

M.Onsi, J.M.Pearson

Equation of State of Stellar Nuclear Matter and the Effective Nucleon Mass

doi: 10.1103/PhysRevC.65.047302
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2002PE19      Eur.Phys.J. A 15, 13 (2002)

J.M.Pearson, S.Goriely, M.Samyn

A Hartree-Fock nuclear mass formula

doi: 10.1140/epja/i2001-10215-y
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2002SA14      Nucl.Phys. A700, 142 (2002)

M.Samyn, S.Goriely, P.-H.Heenen, J.M.Pearson, F.Tondeur

A Hartree-Fock-Bogoliubov Mass Formula

NUCLEAR STRUCTURE Z=8-120; calculated masses, binding energies. Hartree-Fock-Bogoliubov method.

doi: 10.1016/S0375-9474(01)01316-1
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2001BU30      Phys.Rev. C64, 067303 (2001)

F.Buchinger, J.M.Pearson, S.Goriely

Nuclear Charge Radii in Modern Mass Formulas: An update

NUCLEAR STRUCTURE Z=11-95; calculated radii. Comparison with data, two mass formulas compared.

doi: 10.1103/PhysRevC.64.067303
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2001FA22      Nucl.Phys. A696, 396 (2001)

M.Farine, J.M.Pearson, F.Tondeur

Skyrme Force with Surface-Peaked Effective Mass

NUCLEAR STRUCTURE ⁸⁴Ni, ¹²²Zr, ¹⁹⁰Gd, ²⁶⁶Pb, ²⁷⁶U; calculated mass, neutron separation energy, Qβ. ¹⁶O, ⁹⁰Zr, ²⁰⁸Pb; calculated single-particle levels. Skyrme force with effective mass.

doi: 10.1016/S0375-9474(01)01136-8
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2001GO20      At.Data Nucl.Data Tables 77, 311 (2001)

S.Goriely, F.Tondeur, J.M.Pearson

A Hartree-Fock Nuclear Mass Table

ATOMIC MASSES Z=8-120; calculated masses, deformation parameters. Hartree-Fock-BCS approach, Skyrme force, pairing force, Wigner term.

NUCLEAR STRUCTURE Z=8-120; calculated masses, deformation parameters. Hartree-Fock-BCS approach, Skyrme force, pairing force, Wigner term.

doi: 10.1006/adnd.2000.0857
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2001MA04      Nucl.Phys. A679, 337 (2001)

A.Mamdouh, J.M.Pearson, M.Rayet, F.Tondeur

Fission Barriers of Neutron-Rich and Superheavy Nuclei Calculated with the ETFSI Method

NUCLEAR STRUCTURE Z=84-120; A=214-318; calculated fission barrier heights. Extended Thomas-Fermi plus Strutinsky integral method.

doi: 10.1016/S0375-9474(00)00358-4
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2001PE13      Phys.Rev. C64, 027301 (2001)

J.M.Pearson, S.Goriely

Isovector Effective Mass in the Skyrme-Hartree-Fock Method

NUCLEAR STRUCTURE ⁸⁴Ni, ¹²²Zr, ¹⁵⁴Sn, ¹⁹⁰Gd, ²⁶⁶Pb, ²⁷⁶U, ³⁰⁰Cm; calculated mass, neutron separation energies, Qβ, level densities. Skyrme-Hartree-Fock method.

doi: 10.1103/PhysRevC.64.027301
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2001PE15      Phys.Lett. 513B, 319 (2001)

J.M.Pearson

Skyrme Hartree-Fock Method and the Spin-Orbit Term of the Relativistic Mean Field

NUCLEAR STRUCTURE ^{114,116,118,120,122,124,126}Zr; calculated total energy. ⁸⁴Ni, ¹²²Zr, ¹⁵⁴Sn, ¹⁹⁰Gd, ²⁶⁶Pb, ²⁷⁶U, ³⁰⁰Cm; calculated masses, one-neutron separation energies, Qβ. ^40,60Ca, ^208,266Pb; calculated neutron spin-orbit field. ³⁶Ne, ³⁸Mg, ¹²⁴Zr; calculated neutron spin-orbit splitting. Comparison of Skyrme-Hartree-Fock and relativistic mean-field calculations.

doi: 10.1016/S0370-2693(01)00375-6
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2001PE26      Hyperfine Interactions 132, 59 (2001)

J.M.Pearson

The Quest for a Microscopic Nuclear Mass Formula

doi: 10.1023/A:1011973100463
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2000DU06      Phys.Rev. C61, 054303 (2000)

A.K.Dutta, J.M.Pearson, F.Tondeur

Triaxial Nuclei Calculated with the Extended Thomas-Fermi plus Strutinsky Integral (ETFSI) Method

NUCLEAR STRUCTURE ⁶²Zn, ⁷⁴Ge, ^{110,111,112,113,114,115,116,117,118}Zr, ¹³²Ba, ¹³⁴Ce, ¹³⁸Sm, ¹⁶⁸Er, ¹⁸⁶W, ^188,192Os, ²²²Ra, ²³³Th, ^236,262U, ²⁷¹Np, ²⁴⁰Pu, ²⁴⁴Cm, ²⁸⁷Bk, ²⁵²Cf, ^255,286Fm, ^259,292Rf, ²⁹⁴Hs, ^288,294Cn, ²⁹⁸Fl; calculated ground state energy shift due to triaxial deformation. ²³³Th, ^236,262U, ²⁴⁰Pu, ²⁴⁴Cm, ²⁸⁷Bk, ²⁵²Cf, ^255,286Fm, ²⁹²Rf, ²⁹⁴Hs, ^288,294Cn, ²⁹⁸Fl; calculated fission barrier energy shift due to triaxial deformation. Extended Thomas-Fermi plus Strutinsky integral method.

doi: 10.1103/PhysRevC.61.054303
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2000PE08      Nucl.Phys. A668, 163 (2000)

J.M.Pearson, R.C.Nayak

Nuclear-Matter Symmetry Coefficient and Nuclear Masses

NUCLEAR STRUCTURE ⁶⁰Ca, ¹⁰¹As, ¹³⁶Ru, ¹⁵³Sn, ¹⁸⁴Ce, ²⁰²Dy, ²¹⁸Ta, ²⁶⁶Pb, ²⁷⁴Th, ³⁰⁰Cf; calculated masses, neutron separation energies, Qβ; deduced constraint on nuclear matter symmetry coefficient. Extended Thomas-Fermi plus Strutinsky integral, several force parameterizations compared.

ATOMIC MASSES ⁶⁰Ca, ¹⁰¹As, ¹³⁶Ru, ¹⁵³Sn, ¹⁸⁴Ce, ²⁰²Dy, ²¹⁸Ta, ²⁶⁶Pb, ²⁷⁴Th, ³⁰⁰Cf; calculated masses, neutron separation energies, Qβ; deduced constraint on nuclear matter symmetry coefficient. Extended Thomas-Fermi plus Strutinsky integral, several force parameterizations compared.

doi: 10.1016/S0375-9474(99)00431-5
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2000TO06      Phys.Rev. C62, 024308 (2000)

F.Tondeur, S.Goriely, J.M.Pearson, M.Onsi

Towards a Hartree-Fock Mass Formula

doi: 10.1103/PhysRevC.62.024308
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1999PE22      Acta Phys.Hung.N.S. 10, 159 (1999)

J.M.Pearson, F.Tondeur, A.Mamdouh, M.Rayet

Nuclear Masses and Fission Barriers via the ETFSI Method

NUCLEAR STRUCTURE Z=92; calculated fission barriers for N ≈ 140-190. ETFSI method, Skyrme force.

1998MA86      Nucl.Phys. A644, 389 (1998); Erratum Nucl.Phys. A648, 282 (1999)

A.Mamdouh, J.M.Pearson, M.Rayet, F.Tondeur

Large-Scale Fission-Barrier Calculations with the ETFSI Method

NUCLEAR STRUCTURE Z=80-100; calculated fission barrier heights. Extended Thomas-Fermi plus Strutinsky Integral method. Astrophysical implications discussed.

doi: 10.1016/S0375-9474(98)00576-4
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1998NA21      Phys.Rev. C58, 878 (1998)

R.C.Nayak, J.M.Pearson

Spin-Orbit Field and Extrapolated Properties of Exotic Nuclei

NUCLEAR STRUCTURE ¹³²Sn, ^208,266Pb; calculated single-particle levels. ⁶⁰Ca, ¹¹⁸Kr, ¹³⁶Ru, ¹⁵⁴Sn, ¹⁸⁴Ce, ²⁰²Dy, ²²⁸W, ²⁶⁶Pb, ²⁷⁴Th, ³⁰⁰Cf; calculated masses, beta-decay energy, neutron separation energy. Several force parameter sets compared.

doi: 10.1103/PhysRevC.58.878
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1997BO24      Nucl.Phys. A621, 307c (1997)

I.N.Borzov, S.Goriely, J.M.Pearson

Microscopic Calculations of β-Decay Characteristics Near the A = 130 r-Process Peak

RADIOACTIVITY ^{125,126,127,128,129,130,131,132,133,134,135}Cd(β^-); calculated T_1/2. ^{114,115,116,117,118,119,120,121,122,123,124,125,126,127,128}Ru, ^{117,118,119,120,121,122,123,124,125,126,127,128,129,130,131}Rh, ^{118,119,120,121,122,123,124,125,126,127,128,129,130,131,132}Pd, ^{119,120,121,122,123,124,125,126,127,128,129,130,131,132,133}Ag, ^{125,126,127,128,129,130,131,132,133,134}Cd, ¹³¹In; calculated β-decay yield ratios for various models.

doi: 10.1016/S0375-9474(97)00260-1
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1997FA06      Nucl.Phys. A615, 135 (1997)

M.Farine, J.M.Pearson, F.Tondeur

Nuclear-Matter Incompressibility from Fits of Generalized Skyrme Force to Breathing-Mode Energies

NUCLEAR STRUCTURE ¹⁶O, ^40,48Ca, ⁹⁰Zr, ^{112,114,116,120,124,132}Sn, ¹⁴⁴Sm, ²⁰⁸Pb; calculated internal energy, rms charge radius. Breathing modes, generalized Skyrme forces.

doi: 10.1016/S0375-9474(96)00453-8
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1997ON01      Phys.Rev. C55, 3139 (1997)

M.Onsi, H.Przysiezniak, J.M.Pearson

Equation of State of Stellar Nuclear Matter in the Temperature-Dependent Extended Thomas-Fermi Formalism

doi: 10.1103/PhysRevC.55.3139
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1997ON02      Phys.Rev. C55, 3166 (1997)

M.Onsi, R.C.Nayak, J.M.Pearson, H.Freyer, W.Stocker

Skyrme Representation of a Relativistic Spin-Orbit Field

doi: 10.1103/PhysRevC.55.3166
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1996PE22      Phys.Lett. 387B, 455 (1996)

J.M.Pearson, R.C.Nayak, S.Goriely

Nuclear Mass Formula with Bogolyubov-Enchanced Shell-Quenching: Application to r-process

NUCLEAR STRUCTURE Z=55-80; calculated magic neutron gaps. N=55-90; calculated two-neutron separation energies. A=80-200; calculated abundances, masses from different models; deduced r-process implications. Mass formula with Bogolyubov-enhanced self-quenching.

doi: 10.1016/0370-2693(96)01071-4
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1995AB38      At.Data Nucl.Data Tables 61, 127 (1995)

Y.Aboussir, J.M.Pearson, A.K.Dutta, F.Tondeur

Nuclear Mass Formula via an Approximation to the Hartree-Fock Method

NUCLEAR STRUCTURE A=36-300; calculated masses, n-, p-separation, β-decay energies. Extended Thomas-Fermi, plus Strutinsky integral method.

doi: 10.1016/S0092-640X(95)90014-4
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1995NA17      Phys.Rev. C52, 2254 (1995)

R.C.Nayak, J.M.Pearson

Even-Odd Staggering of Pairing-Force Strength

NUCLEAR STRUCTURE Z=30-100; N=30-144; analyzed mass data; deduced fourth-order even-odd mass difference rms errors. A=80-235; analyzed Q(β) data; deduced rms errors. High speed Hartree-Fock approximation, Skyrme force.

doi: 10.1103/PhysRevC.52.2254
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1994BU06      Phys.Rev. C49, 1402 (1994)

F.Buchinger, J.E.Crawford, A.K.Dutta, J.M.Pearson, F.Tondeur

Nuclear Charge Radii in Modern Mass Formulas

NUCLEAR STRUCTURE ^{78,80,82,84,86,88,90,92,94,96,98,100}Sr; calculated β₂ deformation parameter. A=36-238; calculated absolute rms charge radii. Extended Thomas-Fermi, finite-range droplet models mass formula.

doi: 10.1103/PhysRevC.49.1402
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1994ON01      Phys.Rev. C50, 460 (1994)

M.Onsi, H.Przysiezniak, J.M.Pearson

Equation of State of Homogeneous Nuclear Matter and the Symmetry Coefficient

doi: 10.1103/PhysRevC.50.460
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1994ON02      Z.Phys. A348, 255 (1994)

M.Onsi, A.M.Chaara, J.M.Pearson

On the Fermi Functions I(-)(n+(1/2))

doi: 10.1007/BF01305881
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1994PE12      Phys.Rev. C50, 185 (1994)

J.M.Pearson, M.Farine

Relativistic Mean-Field Theory and a Density-Dependent Spin-Orbit Skyrme Force

doi: 10.1103/PhysRevC.50.185
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1994VO07      Phys.Lett. 324B, 279 (1994)

D.Von-Eiff, J.M.Pearson, W.Stocker, M.K.Weigel

Relativistic Semi-Classical Analysis of Nuclear Surface-Symmetry Properties

doi: 10.1016/0370-2693(94)90194-5
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1994VO11      Phys.Rev. C50, 831 (1994)

D.Von-Eiff, J.M.Pearson, W.Stocker, M.K.Weigel

Relativistic Hartree Calculations of Nuclear Compressional Properties

NUCLEAR STRUCTURE ⁹⁰Zr, ^{112,114,116,120,124}Sn, ¹⁴⁴Sm, ²⁰⁸Pb; calculated compressibilities, breathing mode energies. Relativistic Hartree theory.

doi: 10.1103/PhysRevC.50.831
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1992AB08      Nucl.Phys. A549, 155 (1992)

Y.Aboussir, J.M.Pearson, A.K.Dutta, F.Tondeur

Thomas-Fermi Approach to Nuclear-Mass Formula (IV). The ETFSI-1 Mass Formula

NUCLEAR STRUCTURE A=36-300; analyzed mass data; calculated equilibrium deformations, fission barriers; deduced Skyrme, δ-function pairing forces parameters. Hartree-Fock, BCS method, semi-classical approximations.

doi: 10.1016/0375-9474(92)90038-L
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1991PE03      Nucl.Phys. A528, 1 (1991)

J.M.Pearson, Y.Aboussir, A.K.Dutta, R.C.Nayak, M.Farine, F.Tondeur

Thomas-Fermi Approach to Nuclear Mass Formula (III). Force Fitting and Construction of Mass Table

NUCLEAR STRUCTURE A=100-260; calculated energies, equilibrium deformation parameters. ¹⁸⁶Os, ²¹⁰Po, ²⁴⁰Pu, ²⁵⁰Cm, ²⁶²U; calculated fission barriers. Thomas-Fermi approach to mass formula.

doi: 10.1016/0375-9474(91)90418-6
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1991PE15      Phys.Lett. 271B, 12 (1991)

J.M.Pearson

The Incompressibility of Nuclear Matter and the Breathing Mode

NUCLEAR STRUCTURE ^{112,114,116,120,124}Sn, ¹⁴⁴Sm, ²⁰⁸Pb; analyzed breathing mode; deduced unique nuclear matter incompressibility value nonderivability.

doi: 10.1016/0370-2693(91)91269-2
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1990NA21      Nucl.Phys. A516, 62 (1990)

R.C.Nayak, J.M.Pearson, M.Farine, P.Gleissl, M.Brack

Leptodermous Expansion of Finite-Nucleus Incompressibility

NUCLEAR STRUCTURE A ≤ 250; ¹⁶O, ^40,48Ca, ⁵⁶Ni, ⁹⁰Zr, ^112,132Sn, ¹⁴⁰Ce, ²⁰⁸Pb; calculated compressibility vs mass. Leptodermous expansion.

doi: 10.1016/0375-9474(90)90049-R
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1987DU12      Pramana 29, 379 (1987)

A.K.Dutta, J.M.Pearson

Semi-Classical Smoothing in a Non-Monotonic Field

NUCLEAR STRUCTURE A=40-292; calculated system total energy. ²⁰⁸Pb; calculated protons smoothed energy. Semi-classical model.

doi: 10.1007/BF02845775
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1987PA24      Phys.Rev. C36, 1408 (1987)

G.Pantis, J.M.Pearson

Folding Model for Sub-Barrier Interaction between Alpha-Type Nuclei

NUCLEAR REACTIONS, ICPND ¹⁶O(¹²C, ¹²C), E(cm) ≤ 12 MeV; ¹²C(¹²C, ¹²C), E(cm) ≤ 8 MeV; ¹⁶O(¹⁶O, ¹⁶O), E(cm) ≤ 14 MeV; calculated σ(θ=90°), fusion σ, S-factor vs E. Folding model.

doi: 10.1103/PhysRevC.36.1408
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1987TO13      Nucl.Phys. A470, 93 (1987)

F.Tondeur, A.K.Dutta, J.M.Pearson, R.Behrman

Thomas-Fermi Approach to Nuclear Mass Formula (II). Deformed Nuclei and Fission Barriers

NUCLEAR STRUCTURE ¹⁶²Dy, ¹⁷⁴Yb, ¹⁸⁴W, ²³²Th, ²⁴⁰Pu, ²⁵²Cf, ²⁶²U; calculated deformed ground states, fission barriers, isomers. Skyrme-extended Thomas-Fermi method.

doi: 10.1016/0375-9474(87)90122-9
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1986DU05      Nucl.Phys. A454, 374 (1986)

A.K.Dutta, J.-P.Arcoragi, J.M.Pearson, R.H.Behrman, M.Farine

Droplet Models as Approximations to the Extended Thomas-Fermi Method

NUCLEAR STRUCTURE ^36,42,48,54Ca, ^40,46,52,58Ti, ^44,51,58,65Cr, ^48,55,62,69Fe, ^52,60,68,76Ni, ^56,64,72,80Zn, ^60,69,78,87Ge, ^64,73,82,91Ga, ^69,78,87,96Kr, ^{73,83,93,100,103}Sr, ^{143,151,159,167,175,183}Er, ^{148,156,164,172,182,188}Yb, ^{153,161,169,177,185,193}Yb, ^{158,166,174,182,190,198}W, ^{163,171,179,187,195,203}Os; calculated extended Thomas-Fermi energies; deduced higher-order surface symmetry role in droplet model.

doi: 10.1016/0375-9474(86)90275-7
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1986DU12      Nucl.Phys. A458, 77 (1986)

A.K.Dutta, J.-P.Arcoragi, J.M.Pearson, R.Behrman, F.Tondeur

Thomas-Fermi Approach to Nuclear Mass Formula. (I). Spherical Nuclei

NUCLEAR STRUCTURE Z=8-88, A=16-222; calculated masses, neutron separation, β-decay energies. Extended Thomas-Fermi method, shell effects.

doi: 10.1016/0375-9474(86)90283-6
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1984FO10      Phys.Rev. C30, 79 (1984)

J.L.Foster, Jr., S.E.Darden, M.C.Rozak, J.A.Ross, J.P.Martin, L.Lessard, S.Gales, G.Noury, J.M.Pearson, P.Depommier, M.C.Hermida, M.Ruiz

¹³⁰Te(p(pol), p₁) and ¹³⁰Te(p, p₁(pol)) Reactions on Analog Resonances

NUCLEAR REACTIONS ¹³⁰Te(polarized p, p), (polarized p, p'), E(cm)=10.1-10.7 MeV; measured σ(θ) vs E, analyzing power vs θ, E, polarization vs θ; deduced optical model parameters. ¹³¹I deduced IAR, J, π, configuaration. Coupled-channels analysis.

doi: 10.1103/PhysRevC.30.79
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetT0096.

1984TO05      Nucl.Phys. A420, 297 (1984)

F.Tondeur, M.Brack, M.Farine, J.M.Pearson

Static Nuclear Properties and the Parametrisation of Skyrme Forces

NUCLEAR STRUCTURE ¹⁶O, ^40,48Ca, ⁹⁰Zr, ²⁰⁸Pb; calculated binding energies, rms radii. ³²S, ⁵⁶Fe, ⁷²Ge, ¹⁰⁰Ru, ¹¹⁰Cd, ^118,132Sn, ¹³⁸Ba, ¹⁴⁶Gd; calculated binding energies. ²⁴⁰Pu; calculated fission barriers. Trial Skyrme forces.

doi: 10.1016/0375-9474(84)90444-5
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1983TO02      Nucl.Phys. A394, 462 (1983)

F.Tondeur, J.M.Pearson, M.Farine

The Anomalies of the Droplet Model

NUCLEAR STRUCTURE A ≈ 10-260; calculated surface stiffness vs mass. Droplet model.

doi: 10.1016/0375-9474(83)90118-5
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1982PE02      Nucl.Phys. A376, 501 (1982)

J.M.Pearson

Nuclear Radii: A critique of the droplet model

NUCLEAR STRUCTURE ³²S, ³⁶Ar, ^40,48Ca, ⁴⁴Ti, ⁵⁶Ni, ⁶⁴Ge, ⁹⁰Zr, ¹⁰⁴Pd, ^110,132Sn, ¹⁶⁰Dy, ^206,208Pb; calculated proton, neutron distributions. Droplet model.

doi: 10.1016/0375-9474(82)90127-0
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1979DR03      Nucl.Phys. A317, 300 (1979)

H.Driller, E.Blanke, H.Genz, A.Richter, G.Schrieder, J.M.Pearson

Test of Detailed Balance at Isolated Resonances in the Reactions ²⁷Al + p → ²⁴Mg + α and Time Reversibility

NUCLEAR REACTIONS ²⁷Al(p, α), E=1.35-1.46 MeV; Mg(α, p), E=3.38-3.52 MeV; measured σ(E); deduced detailed balance, time reversibility. ²⁸Si deduced isolated resonances.

doi: 10.1016/0375-9474(79)90484-6
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1979PE03      Nucl.Phys. A317, 447 (1979)

J.M.Pearson, B.Rouben, G.Saunier, F.Brut

Saturation Properties of Infinite Nuclear Matter via Hartree-Fock Calculations on Finite Nuclei

NUCLEAR STRUCTURE ¹⁶O, ²⁰⁸Pb; calculated static properties of finite spherical nuclei fits with three types of effective interactions equivalent; deduced different saturation densities for infinite nuclear matter.

doi: 10.1016/0375-9474(79)90491-3
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1977RO19      Phys.Lett. 70B, 6 (1977)

B.Rouben, F.Brut, J.M.Pearson, G.Saunier

Superheavy Hartree-Fock Calculations for Magic Numbers Z = 126 and 138

NUCLEAR STRUCTURE A > 200; calculated single particle spectra; deduced no magic number at Z=126, possible magic number at Z=138. Hartree-Fock calculations.

doi: 10.1016/0370-2693(77)90330-6
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1974SA04      Phys.Lett. 48B, 293 (1974)

G.Saunier, B.Rouben, J.M.Pearson

Bubbles and the Odd-State Force

NUCLEAR STRUCTURE ³⁶Ar; calculated levels, mass density.

doi: 10.1016/0370-2693(74)90593-0
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1972BO13      Nucl.Phys. A185, 593 (1972)

E.Boridy, J.M.Pearson

Spin-Orbit Force and Excitation of Unnatural-Parity States by α-Particles

NUCLEAR REACTIONS ¹⁶O(α, α'), E=40.5 MeV; analyzed σ(θ). Microscopic formalism, spin-orbit force.

doi: 10.1016/0375-9474(72)90034-6
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1972BO39      Nucl.Phys. A193, 113 (1972)

E.Boridy, J.M.Pearson

DWBA for Inelastic Nucleon Scattering with Velocity-Dependent Forces

NUCLEAR REACTIONS ¹⁶O, ⁵⁸Ni(p, p'), E=17-46, 17.7 MeV; calculated σ(θ). DWBA, microscopic formalism.

doi: 10.1016/0375-9474(72)90239-4
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1972RO39      Phys.Lett. 42B, 385 (1972)

B.Rouben, J.M.Pearson, G.Saunier

Hartree-Fock Calculation of Superheavy Magic Numbers

NUCLEAR STRUCTURE Z=114, 120; ²⁰⁸Pb; calculated single-particle spectra, binding energies. ¹⁶O, ^40,48Ca, ⁵⁶Ni, ⁹⁰Zr; calculated binding energies.

doi: 10.1016/0370-2693(72)90087-1
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1971BO28      Phys.Rev.Lett. 27, 203 (1971)

E.Boridy, J.M.Pearson

Excitation of Abnormal Parity States by α Particles Acting with Velocity-Dependent Central Forces

NUCLEAR REACTIONS ⁵⁸Ni(α, α'), E=18, 40 MeV; calculated σ. DWBA formalism, velocity-dependent central force.

doi: 10.1103/PhysRevLett.27.203
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1971QU01      Nucl.Phys. A164, 631 (1971)

N.Quang-Hoc, J.M.Pearson

Calculation of sd Shell Spectra in A = 18 Nuclei with Hartree-Fock Interactions

NUCLEAR STRUCTURE ¹⁸F, ¹⁸O; calculated levels. Hartree-Fock method.

doi: 10.1016/0375-9474(71)90784-6
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1963RO04      Bull.Am.Phys.Soc. 8, No.2, 130, W11 (1963)

B.L.Robinson, J.M.Pearson

Capture of M-Shell and High-Angular-Momentum Electrons

NUCLEAR STRUCTURE ¹³⁸La; measured not abstracted; deduced nuclear properties.

1960PE12      Nuclear Phys. 18, 91 (1960)

J.M.Pearson, M.A.Preston

The Electric Quadrupole Interaction in Beta Decay

NUCLEAR STRUCTURE ²³⁶Np, ¹⁷⁶Lu, ¹⁸⁰Ta; measured not abstracted; deduced nuclear properties.

doi: 10.1016/0029-5582(60)90389-8
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1960PE21      Can.J.Phys. 38, 148 (1960)

J.M.Pearson

The Nuclear Matrix Element Ratio in the 0-→0+ Beta Transition of Pr¹⁴⁴

NUCLEAR STRUCTURE ¹⁴⁴Pr; measured not abstracted; deduced nuclear properties.

doi: 10.1139/p60-014
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1960PR11      Phys.Rev. 119, 305 (1960)

M.A.Preston, G.H.Keech, J.M.Pearson

Beta-Decay Theory and the Spectrum of Rb⁸⁷

NUCLEAR STRUCTURE ⁸⁷Rb; measured not abstracted; deduced nuclear properties.

doi: 10.1103/PhysRev.119.305
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