18 résultats avec le mot-clé: 'crystallization inner crust neutron star influence shell effects'
Equilibrium value of the proton number Z as a function of baryon density in the inner crust at zero temperature for the BSk22 (panel a), BSk24 (panel b), BSk25 (panel c), and
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A multicomponent approach was developed at a finite temperature using a compressible liquid-drop description of the ions with an improved energy functional based on recent
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L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des
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We computed the finite-temperature composition of the outer crust of non-accreting unmagnetized NSs, both in the OCP approximation and in the MCP, thus including a distribution
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Emmanuelle Dorla, Anne Gauvin-Bialecki, Zoé Deuscher, Agathe Allibert, Isabelle Grondin, Jean-Philippe Deguine, Philippe Laurent.. To cite
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This key word indicates that one wants to modify the reference with the sequence numbers described in the concept l_ord of the listis type.. /NUME_MODE
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The advantages of THERMIT are that it contains the sophis- ticated two-fluid, two-phase flow model as well as an advanced numerical solution technique. Consequently,
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Specifically, we introduce pairing correlations both in the cluster and homogeneous matter component of the NSE model in the local BCS approximation and study the effect of the
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Older age, more recent splenectomy, hemo-lymphopathy and receiving the previous years’ doses of influenza vaccine are associated with receiving influenza vaccination during the
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Le mouvement est impossible, car avant d’arriver à destina- tion, ce qui se meut doit d’abord arriver au milieu, et ainsi de suite ad infinitum.. (paradoxe de Zénon )
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L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des
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This first comparison shows that the single particle wave functions of unbound neutrons are qualitatively well reproduced by the W-S approximation inside the nuclear clusters.. The
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D. PHONON DISPERSION AND TRANS- VERSE MODE SOFTENING IN RbFeCl3.. For wave vectors in the hexagonal plane the transverse phonons polarized along Z are found to have very
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In order to estimate the spurious shell effects due to the unbound neutrons, we simulate an homogeneous gas of neutron matter in W-S cell by removing all the proton states.
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On utilise pour tester notre syst`eme d’isolation une source de r´ef´erence qui ´emet un son d’intensit´e 100dB.. 1) D´eterminer l’intensit´e du son apr`es att´enuation par
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Treatments consisted of a Live Control with seawater (2SLC, seen in last row), Killed Control with nitrate & nitrite addition in seawater (2SKCN32, not photographed),
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The observed steady decrease in neutron star temperature provides strong support for the hypothesis that the crust was substantially heated during the 2010 accretion outburst and
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En utilisant les paramètres empiriques de SLy4, nous avons montré que la différence relative avec l’équation d’état de Douchin et Haensel est inférieure à 10% dans la
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