198 Bibliographie Harrison, B. K., Thorne, K. S., Wakano, M., Wheeler, J. A., Gravitation Theory and Gravitational Col<strong>la</strong>pse, Gravitation Theory and Gravitational Col<strong>la</strong>pse, Chicago : University of Chicago Press, 177 pages (1965). Hartle, J. B., Slowly Rotating Re<strong>la</strong>tivistic Stars. I. Equations of Structure, ApJ , 150 : 1005–1029 (1967). Hawking, S. W., Ellis, G. F. R., The <strong>la</strong>rge scale structure of space-time, Cambridge Monographs on Mathematical Physics, London : Cambridge University Press, 391 pages (1973). Hoffberg, M., G<strong>la</strong>ssgold, A. E., Richardson, R. W., Ru<strong>de</strong>rman, M., Anisotropic Superfluidity in Neutron Star Matter, Physical Review Letters, 24 : 775–777 (1970). Horowitz, G. T., Perry, M. J., Gravitational energy cannot become negative, Physical Review Letters, 48 : 371–374 (1982). Hulse, R. A., Taylor, J. H., Discovery of a pulsar in a binary system, ApJ, Lett., 195 : L51–LL53 (1975). Isenberg, J. A., Waveless approximation theories of gravity, preprint (1977). Isenberg, J. A., Nester, J., Canonical analysis of re<strong>la</strong>tivistic field theories, Held, A. (ed.), General re<strong>la</strong>tivity and gravitation, Plenum Press, pages 23– (1980). Jezequel, F., Charikhi, M., Chesneaux, J.-M., Dynamical control of computations of multiple integrals, SCAN2002 conference, Paris (France), 23-27 september 2002 (2002). Jones, P. B., Bulk viscosity of neutron-star matter, Physical Review D, 64 : 084003, 7 pages (2001a). Jones, P. B., Comment on ”Gravitational Radiation Instability in Hot Young Neutron Stars”, Physical Review L., 86 : 1384 (2001b). Jordan, P., The present state of Dirac’s cosmological hypothesis, Z. Phys., 157 : 112– 121 (1959). Kaminker, A. D., Haensel, P., Yakovlev, D. G., Nucleon superfluidity vs. observations of cooling neutron stars, A&A, 373 : L17–LL20 (2001). Kaminker, A. D., Yakovlev, D. G., Gnedin, O. Y., Three types of cooling superfluid neutron stars : Theory and observations, A&A, 383 : 1076–1087 (2002). Karino, S., Yoshida, S., Eriguchi, Y., R-mo<strong>de</strong> oscil<strong>la</strong>tions of differentially and rapidly rotating Newtonian polytropic stars, Physical Review D, 64 : 24003 (2001). Kojima, Y., Equations governing the nonradial oscil<strong>la</strong>tions of a slowly rotating re<strong>la</strong>tivistic star, Physical Review D, 46 : 4289–4303 (1992). Kojima, Y., Quasi-toroidal oscil<strong>la</strong>tions in rotating re<strong>la</strong>tivistic stars, Mon. Not. of the Royal Astron. Soc., 293 : 49–52 (1998). Kojima, Y., Hosonuma, M., Approximate equation relevant to axial oscil<strong>la</strong>tions on slowly rotating re<strong>la</strong>tivistic stars, Physical Review D, 62 : 44006 (2000).
Bibliographie 199 Kokkotas, K. D., Pulsating Re<strong>la</strong>tivistic Stars, Re<strong>la</strong>tivistic Gravitation and Gravitational Radiation, pages 89–102 (1997). Kokkotas, K. D., Schmidt, B. G., Quasi-Normal Mo<strong>de</strong>s of Stars and B<strong>la</strong>ck Holes, Living Reviews in Re<strong>la</strong>tivity, 2, Article en ligne : http ://www.livingreviews.org/Articles/Volume2/1999-2kokkotas/ (1999). Krylov, V. I., Approximate calcu<strong>la</strong>tions of integrals, The Mac Mil<strong>la</strong>n Comapagny, New York, 357 pages (1962). Lamb, D. Q., Lattimer, J. M., Pethick, C. J., Ravenhall, D. G., Hot <strong>de</strong>nse matter and stel<strong>la</strong>r col<strong>la</strong>pse, Physical Review Letters, 41 : 1623–1626 (1978). Landau, L. D., Lifshitz, E. M., The c<strong>la</strong>ssical theory of fields, Course of theoretical physics, Pergamon International Library of Science, Technology, Engineering and Social Studies, Oxford : Pergamon Press, 4th rev. engl. ed., @ pages (1975). Landau, L. D., Lifshitz, E. M., Statistical physics. Pt.1, Pt.2 , Course of theoretical physics, Pergamon International Library of Science, Technology, Engineering and Social Studies, Oxford : Pergamon Press, 1980—c1980, 3rd rev. and en<strong>la</strong>rg. ed., 374 pages (1980). Langer, W. D., Cameron, A. G. W., Effects of Hyperons on the Vibrations of Neutron Stars, Astr. and Space Sci., 5 : 213 (1969). Large, M. I., Vaughan, A. E., Mills, B. Y., A pulsar supernova association, Nature, 220 : 340–341 (1968). Latour, J., Spiegel, E. A., Toomre, J., Zahn, J.-P., Stel<strong>la</strong>r convection theory. I - The ane<strong>la</strong>stic modal equations, ApJ , 207 : 233–243 (1976). Lattimer, J. M., Prakash, M., Pethick, C. J., Haensel, P., Direct URCA process in neutron stars, Physical Review Letters, 66 : 2701–2704 (1991). Lebach, D. E., Corey, B. E., Shapiro, I. I., Ratner, M. I., Webber, J. C., Rogers, A. E. E., Davis, J. L., Herring, T. A., Measurement of the So<strong>la</strong>r Gravitational Deflection of Radio Waves Using Very-Long-Baseline Interferometry, Physical Review Letters, 75 : 1439–1442 (1995). Lesieur, M., Turbulence in fluids, Martinus Nijhoff Publishers, 286 pages, Dordrecht (1987). Levenfish, K. P., Yakovlev, D. G., Van Horn, H. M., Ichimaru, S. (eds.), Strongly Coupled P<strong>la</strong>sma Physics, Univ. of Rochester Press (1993). Levenfish, K. P., Yakovlev, D. G., Suppression of neutrino energy losses in reactions of direct urca processes by superfluidity in neutron star nuclei, Astronomy Letters, 20 : 43–51 (1994b). Levenfish, K. P., Yakovlev, D. G., Specific heat of neutron star cores with superfluid nucleons, Astronomy Reports, 38 : 247–251 (1994a). Lindblom, L., Neutron Star Pulsations and Instabilities, Ferrari, V., Miller, J. C., Rezzo<strong>la</strong>, L. (eds.), Gravitational Waves : A Challenge to Theoretical Astrophysics, ICTP, pages 259–276 (2001).
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Ecole doctorale de Physique de la r
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Table des matières Résumé v Abst
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TABLE DES MATIÈRES iii 4.5.2 Noise
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Résumé Résumé v Cette étude tr
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Abstract Abstract vii This study de
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Introduction Les sens dont l’a do
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Introduction 3 même, leurs observa
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Chapitre 1 Relativité générale e
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1.1 Relativité générale 1.1.1 Gr
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1.1 Relativité générale 9 La rel
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1.1.3 Tests et prédictions 1.1 Rel
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1.2 Ondes gravitationnelles 1.2.1 E
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y 1.2 Ondes gravitationnelles 15 x
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1.3 Sources d’ondes gravitationne
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1.3 Sources d’ondes gravitationne
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1.3 Sources d’ondes gravitationne
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1.4 Détection 23 Figure 1.6 - Sens
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¢¡ £ © ¥ ¢¡ £ © ¤ ¢¡ £
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Chapitre 2 Etoiles à neutrons Somm
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2.1 Naissance d’une étoile à ne
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2.1 Naissance d’une étoile à ne
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astre Terre Soleil naine blanche é
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2.2 Structure interne 35 Figure 2.4
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2.2 Structure interne 37 extensions
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2.2 Structure interne 39 Figure 2.5
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2.2 Structure interne 41 rigidité
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2.2 Structure interne 43 où = h/2
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2.2 Structure interne 45 à des fer
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2.2 Structure interne 47 Type de su
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2.3 Principes de l’évolution d
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2.3 Principes de l’évolution d
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est environ 0.7 fois la masse nue 1
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2.3 Principes de l’évolution d
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2.3 Principes de l’évolution d
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Log 10 (T/10 9 K) 0 -0.5 -1 -1.5 -2
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2.4 Superfluidité et écarts à l
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2.4 Superfluidité et écarts à l
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aboutit à 2.4 Superfluidité et é
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2.4 Superfluidité et écarts à l
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2.4 Superfluidité et écarts à l
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Résultats 2.4 Superfluidité et é
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2.4 Superfluidité et écarts à l
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2.4 Superfluidité et écarts à l
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Chapitre 3 Oscillations stellaires
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3.1 Modes d’une étoile à neutro
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3.1.2 Perturbations 3.1 Modes d’u
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Un mode propre vérifie donc 3.1 Mo
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3.1 Modes d’une étoile à neutro
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3.2 Oscillations d’une étoile re
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3.2 Oscillations d’une étoile re
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3.2 Oscillations d’une étoile re
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3.2 Oscillations d’une étoile re
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Ω c /Ω max 1.00 0.98 0.96 0.94
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3.3 Modes inertiels et r-modes 97 F
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P K /P 1.0 0.8 0.6 0.4 0.2 3.3 Mode
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3.3 Modes inertiels et r-modes 101
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Chapitre 4 Inertial modes in slowly
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4.1 Introduction 105 what is done w
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4.2 Equations and numbers 107 obvio
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4.2 Equations and numbers 109 tenso
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4.2 Equations and numbers 111 4.2.2
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or 4.2 Equations and numbers 113 Tv
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4.3 Mass conservation, boundary con
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4.4 Test and calibration of the cod
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4.4 Test and calibration of the cod
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Sp(V θ ) 1 4.4 Test and calibratio
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E(t) / E 0 1.15 1.1 1.05 1 4.4 Test
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Sp(S xx ) S xx 0.1 0 -0.1 4.4 Test
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V r Sp(V r ) 0.4 0.2 0 -0.2 -0.4 -0
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4.5.1 Modifications 4.5 Differentia
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Sp(V r ) V r 4 2 0 -2 4.5 Different
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4.6 Strong Cowling approximation in
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V θ Sp(V θ ) 10 5 0 -5 -10 4.6 St
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can be written 4.6 Strong Cowling a
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E Polar / E Total 0.05 0.04 0.03 0.
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S xx Sp(S xx ) 0.2 0.1 0 -0.1 4.6 S
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GW emission. 4.8 Acknowledgments 4.
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Chapitre 5 Modes inertiels dans des
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