0000000000338406

AUTHOR

Jérôme Margueron

showing 6 related works from this author

Continued fraction approximation for the nuclear matter response function

2008

A continued fraction approximation is used to calculate the Random Phase Approximation (RPA) response function of nuclear matter. The convergence of the approximation is assessed by comparing it with the numerically exact response function obtained with a typical effective finite-range interaction used in nuclear physics. It is shown that just the first order term of the expansion can give reliable results at densities up to the saturation density value.

PhysicsNuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear Theory010308 nuclear & particles physicsFísicaFOS: Physical sciencesFunction (mathematics)Nuclear matter01 natural sciencesTerm (time)Nuclear Theory (nucl-th)Approximation errorQuantum electrodynamics21.30.-x 21.60.Jz 21.65.-f0103 physical sciencesConvergence (routing)Fraction (mathematics)010306 general physicsSaturation (chemistry)Random phase approximation
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Effects of spin-orbit interaction on nuclear response and neutrino mean free path

2006

PTH; The effects of the spin-orbit component of the particle-hole interaction on nuclear response functions and neutrino mean free path are examined. A complete treatment of the full Skyrme interaction in the case of symmetric nuclear matter and pure neutron matter is given. Numerical results for neutron matter are discussed. It is shown that the effects of the spin-orbit interaction remain small, even at momentum transfer larger than the Fermi momentum. The neutrino mean free paths are marginally affected.

Nuclear and High Energy PhysicsParticle physicsresponse functionsNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Mean free pathAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesAstrophysics01 natural sciences21.30.Fe 21.60.Jz 21.65.+f 26.60.+cNuclear Theory (nucl-th)Nuclear physicsMomentum[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesNeutronspin-orbit interaction010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Momentum transferFísicaSpin–orbit interactionNuclear matterNeutron starnuclear matterrandom phase approximationeffective Skyrme interactionsNeutrino
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Neutrino mean free path and in-medium nuclear interaction

2002

Neutrinos produced during the collapse of a massive star are trapped in a nuclear medium (the proto-neutron star). Typically, neutrino energies (10-100 MeV) are of the order of nuclear giant resonances energies. Hence, neutrino propagation is modified by the possibility of coherent scattering on nucleons. We have compared the predictions of different nuclear interaction models. It turns out that their main discrepancies are related to the density dependence of the k-effective mass as well as to the onset of instabilities as density increases. This last point had led us to a systematic study of instabilities of infinite matter with effective Skyrme-type interactions. We have shown that for s…

PhysicsNuclear and High Energy PhysicsNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physicsMean free pathScatteringNuclear TheoryFísicaFOS: Physical sciencesStar (graph theory)01 natural sciences7. Clean energyNuclear interactionNuclear physicsNuclear Theory (nucl-th)0103 physical sciencesNeutrino010306 general physicsNucleonNuclear Experiment
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Nuclear response functions in homogeneous matter with finite range effective interactions

2005

The question of nuclear response functions in a homogeneous medium is examined. A general method for calculating response functions in the random phase approximation (RPA) with exchange is presented. The method is applicable for finite-range nuclear interactions. Examples are shown in the case of symmetric nuclear matter described by a Gogny interaction. It is found that the convergence of the results with respect to the multipole truncation is quite fast. Various approximation schemes such as the Landau approximation, or the Landau approximation for the exchange terms only, are discussed in comparison with the exact results.

Nuclear and High Energy Physicsresponse functions[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryTruncationNuclear TheoryFOS: Physical sciencesFinite range21.30.Fe 21.60.Jz 21.65.+f 26.60.+c01 natural sciencesNuclear Theory (nucl-th)effective nuclear interactions0103 physical sciencesConvergence (routing)Statistical physics010306 general physicsPhysics010308 nuclear & particles physicsBorn–Huang approximationFísicaNuclear matter3. Good healthHomogeneousnuclear matterrandom phase approximationQuantum electrodynamicsRandom phase approximationMultipole expansion
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Nuclear liquid-gas phase transition and supernovae evolution

2004

It is shown that the large density fluctuations appearing at the onset of the first order nuclear liquid-gas phase transition can play an important role in the supernovae evolution. Due to these fluctuations, the neutrino gas may be trapped inside a thin layer of matter near the proto-neutron star surface. The resulting increase of pressure may induce strong particle ejection a few hundred milliseconds after the bounce of the collapse, contributing to the revival of the shock wave. The Hartree-Fock+RPA scheme, with a finite-range nucleon-nucleon effective interaction, is employed to estimate the effects of the neutrino trapping due to the strong density fluctuations, and to discuss qualitat…

Shock waveNuclear and High Energy PhysicsPhase transition97.60.Bw; 26.50.+x; 25.30.Pt; 21.60.JzNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]supernovaeAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesTrappingAstrophysics7. Clean energy01 natural sciencesNuclear Theory (nucl-th)Nuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsLiquid gasAstrophysics (astro-ph)FísicaneutrinosNuclear matterSupernovaphase transitionnuclear matterParticleNeutrino
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Instabilities of infinite matter with effective Skyrme-type interactions

2002

The stability of the equation of state predicted by Skyrme-type interactions is examined. We consider simultaneously symmetric nuclear matter and pure neutron matter. The stability is defined by the inequalities that the Landau parameters must satisfy simultaneously. A systematic study is carried out to define interaction parameter domains where the inequalities are fulfilled. It is found that there is always a critical density $\rho_{cr}$ beyond which the system becomes unstable. The results indicate in which parameter regions one can find effective forces to describe correctly finite nuclei and give at the same time a stable equation of state up to densities of 3-4 times the saturation de…

PhysicsNuclear and High Energy Physicsendocrine systemNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physicsEquation of state (cosmology)Nuclear TheoryFOS: Physical sciencesFísicaType (model theory)Flory–Huggins solution theoryNuclear matter01 natural sciencesStability (probability)Nuclear Theory (nucl-th)Quantum mechanics0103 physical sciencesSaturation (graph theory)Neutron010306 general physicsNuclear theoryhormones hormone substitutes and hormone antagonists
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