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NSR database version of April 27, 2024.

Search: Author = P.Donati

Found 11 matches.

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2005DO06      J.Phys.(London) G31, 295 (2005)

P.Donati, G.Gori, F.Barranco, R.A.Broglia, E.Vigezzi

Effective pairing interaction induced by polarization effects in deformed nuclei

NUCLEAR STRUCTURE ^{146,148,150,152,154}Sm; calculated neutron pairing gap, single-particle levels, B(E2). ^156,158,160Gd, ^160,162,164Dy, ^166,168,170Er; calculated pairing gaps. Effective pairing interaction induced by polarization effects.

doi: 10.1088/0954-3899/31/5/002
Citations: PlumX Metrics

2004DO10      Nucl.Phys. A742, 363 (2004)

P.Donati, P.M.Pizzochero

Fully consistent semi-classical treatment of vortex-nucleus interaction in rotating neutron stars

doi: 10.1016/j.nuclphysa.2004.07.002
Citations: PlumX Metrics

2000BO23      Acta Phys.Pol. B31, 335 (2000)

P.F.Bortignon, G.Colo, P.Donati, R.A.Broglia

Description of Nuclear Excitations Beyond the Mean Field

2000DO07      Phys.Rev.Lett. 84, 4317 (2000)

P.Donati, T.Dossing, Y.R.Shimizu, S.Mizutori, P.F.Bortignon, R.A.Broglia

Effective Nucleon Mass in Deformed Nuclei

NUCLEAR STRUCTURE ¹⁶⁸Yb; calculated nucleon effective mass vs rotational frequency. ¹⁶⁹Yb; calculated quadrupole RPA response functions.

doi: 10.1103/PhysRevLett.84.4317
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2000SH36      Phys.Rev.Lett. 85, 2260 (2000)

Y.R.Shimizu, P.Donati, R.A.Broglia

Response Function Technique for Calculating the Random-Phase Approximation Correlation Energy

NUCLEAR STRUCTURE ¹⁶⁴Er; calculated rotational bands pairing gap, RPA correlation energy. Response function technique.

doi: 10.1103/PhysRevLett.85.2260
Citations: PlumX Metrics

1999DO08      Nucl.Phys. A649, 25c (1999)

P.Donati, T.Dossing, Y.R.Shimizu, P.F.Bortignon, R.A.Broglia

Self-Energy of Single-Particle States in Deformed, Rapidly Rotating Nuclei

doi: 10.1016/S0375-9474(99)00034-2
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1999DO12      Nucl.Phys. A653, 27 (1999)

P.Donati, T.Dossing, Y.R.Shimizu, P.F.Bortignon, R.A.Broglia

A Complex Integration Technique to Remove Spurious States Associated with Spontaneously Broken Symmetries in RPA Calculations

NUCLEAR STRUCTURE ¹⁶⁸Yb; calculated RPA response functions. Method for removal of spurious states.

doi: 10.1016/S0375-9474(99)00155-4
Citations: PlumX Metrics

1999DO15      Nucl.Phys. A653, 225 (1999)

P.Donati, T.Dossing, Y.R.Shimizu, P.F.Bortignon, R.A.Broglia

Nucleon-Phonon Coupling in Hot, Rapidly Rotating Nuclei (I)

doi: 10.1016/S0375-9474(99)00242-0
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1996DO08      Z.Phys. A354, 249 (1996)

P.Donati, P.F.Bortignon, R.A.Broglia

Temperature Dependence of the Damping Width of Single-Particle States in Hot Nuclei

NUCLEAR STRUCTURE ⁹⁸Mo, ⁶⁴Zn; calculated single-particle states damping width vs temperature. Hot nuclei.

doi: 10.1007/s002180050041
Citations: PlumX Metrics

1996DO17      Phys.Lett. 383B, 15 (1996)

P.Donati, N.Giovanardi, P.F.Bortignon, R.A.Broglia

Damping of Nuclear Motion in Hot Nuclei

NUCLEAR STRUCTURE ¹²⁰Sn; calculated GDR damping width; deduced temperature dependence related features.

doi: 10.1016/0370-2693(96)00568-0
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1994DO14      Phys.Rev.Lett. 72, 2835 (1994)

P.Donati, P.M.Pizzochero, P.F.Bortignon, R.A.Broglia

Temperature Dependence of the Nucleon Effect Mass and the Physics of Stellar Collapse

NUCLEAR STRUCTURE ⁹⁸Mo, ⁶⁴Zn, ⁶⁴Ni; calculated nucleon effective mass vs temperature; deduced consequences on level density parameter symmetry energy, stellar collapse implications. Dynamic mean field.

doi: 10.1103/PhysRevLett.72.2835
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