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Artykuły w czasopismach na temat "Ondes de trou noir"
Ricard, Antoine. "Trou noir". Mémoires N° 75, nr 2 (3.06.2019): 2. http://dx.doi.org/10.3917/mem.075.0002.
Pełny tekst źródłaMoulier-Boutang, Yann. "L'Europe trou noir". Multitudes 11, nr 1 (2003): 5. http://dx.doi.org/10.3917/mult.011.0005.
Pełny tekst źródłaKorinman, Michel. "Le syndrome du trou noir". Outre-Terre N° 48, nr 3 (2016): 9. http://dx.doi.org/10.3917/oute1.048.0009.
Pełny tekst źródłaCombes, Françoise. "Première image d’un trou noir". Reflets de la physique, nr 64 (styczeń 2020): 23–25. http://dx.doi.org/10.1051/refdp/202064023.
Pełny tekst źródłaMey, Jacob L. "Le trou noir de l'âme". Journal of Pragmatics 14, nr 3 (czerwiec 1990): 431–38. http://dx.doi.org/10.1016/0378-2166(90)90099-y.
Pełny tekst źródłaChesnel, Sandrine. "La Normandie, trou noir ferroviaire". Pour l'Éco N° 53, nr 6 (31.07.2023): 26–27. http://dx.doi.org/10.3917/poec.053.0026.
Pełny tekst źródłaLaurent, Éric. "Le trou noir des vanités". La Cause freudienne N° 61, nr 3 (18.11.2005): 8–14. http://dx.doi.org/10.3917/lcdd.061.0008.
Pełny tekst źródłaFollet, Marianne. "Sortir du trou noir de l’histoire". Canal Psy, nr 117/118 (1.07.2016): 15–22. http://dx.doi.org/10.35562/canalpsy.1968.
Pełny tekst źródłaGoldberg, Henri. "Caroline Alexander, Ciel avec trou noir". Témoigner. Entre histoire et mémoire, nr 119 (31.12.2014): 206–7. http://dx.doi.org/10.4000/temoigner.1657.
Pełny tekst źródłaSchaffer, Jonathan, Max Kistler i Philippe De Brabanter. "Le trou noir de la causalité". Philosophie 89, nr 2 (2006): 40. http://dx.doi.org/10.3917/philo.089.0040.
Pełny tekst źródłaRozprawy doktorskie na temat "Ondes de trou noir"
Ritter, Patxi. "Ondes gravitationnelles et calcul de la force propre pour un astre compact en mouvement autour d'un trou noir super-massif". Thesis, Orléans, 2013. http://www.theses.fr/2013ORLE2038/document.
Pełny tekst źródłaThis thesis focuses on modelling the gravitational waves and the relativistic motion associated to Extreme Mass Ratio Inspiral (EMRI) systems. These systems consist of a stellar mass compact object gravitationally captured by a super-massive black hole. In black hole perturbation theory, we further develop a numerical method which computes waveforms generated by a point mass particle orbiting a Schwarzschild black hole. The Regge-Wheeler-Zerilli wave equation is solved in time domain. The gauge invariant solution is related to the polarisation modes, the energy and the angular momentum carried by the gravitational waves. In reaction to the energy and the moment lost, the trajectory is modified all along. In the MiSaTaQuWa formalism, we compute the self-force acting upon a point particle which is initially at rest, and then falling into a Schwarzschild black hole. We show how this quantity is defined in the Regge-Wheeler gauge by using the mode-sum regularisation technique. We take into account the self-force effect on the motion of the particle by using an iterative and osculating orbit method conceived herein. We quantify the orbital deviation with respect to the geodesic motion, but also the perturbed wave forms and the associated radiated energy
Ritter, Patxi. "Ondes gravitationnelles et calcul de la force propre pour un astre compact en mouvement autour d'un trou noir supermassif". Phd thesis, Université d'Orléans, 2013. http://tel.archives-ouvertes.fr/tel-00920959.
Pełny tekst źródłaGrandclément, Philippe. "Étude numérique de binaires d'étoiles à neutrons et de trous noirs". Paris 7, 2001. http://www.theses.fr/2001PA077200.
Pełny tekst źródłaGrosjean, Daniel. "Aspects de la recherche de coalescences binaires avec le détecteur Virgo". Phd thesis, Chambéry, 2007. http://tel.archives-ouvertes.fr/tel-00184887.
Pełny tekst źródłaLa sensibilité actuelle du détecteur a été atteinte après une période de mise en route de l'interféromètre marquée par différentes campagnes de prises de données. L'analyse dans le contexte d'une recherche de systèmes binaires d'étoiles à neutrons des données recueillies depuis août 2005 s'est concentrée sur la notion de qualité de données et a conduit à développer des méthodes d'exclusion d'événements liés à un fonctionnement anormalement bruyant de l'interféromètre. La compréhension de ces sources de bruit a parfois permis d'en améliorer le fonctionnement.
La méthode d'analyse utilisée pour la recherche de systèmes binaires d'étoiles à neutrons peut s'avérer mal adaptée au cas de systèmes binaires plus massifs comportant un ou deux trous noirs. Après avoir clarifié ce point, nous envisageons dans le contexte du détecteur Virgo fonctionnant à sensibilité nominale différentes solutions pour une recherche performante de tels systèmes. Il s'agit d'une part de l'utilisation d'une famille de calques de détection, dont on confirme les performances. D'autre part, on s'intéresse à l'utilisation de calques spécifiquement adaptés à la description de l'évolution de systèmes binaires de trous noirs. Certains aspects techniques nécessaires à la mise en oeuvre d'une recherche utilisant ces solutions sont discutés.
Enfin, le dernier aspect de la recherche de systèmes binaires abordé concerne l'analyse en réseau des données recueillies par les différents détecteurs mondiaux. En utilisant des données simulées, on montre que la définition d'un nouveau temps de référence pour les événements de coalescences permet d'améliorer la précision de reconstruction de la position des sources binaires.
Xiang, Shuyang. "Sur la dynamique des fluides dans le domaine de communication extérieur d'un espace-temps de Schwarzschild". Thesis, Paris 6, 2017. http://www.theses.fr/2017PA066179/document.
Pełny tekst źródłaThis thesis is devoted to fluid dynamics evolving in the domain of outer communication of a Schwarzschild black hole. In the first chapter, we formulate the initial value problem of the relativistic Euler model within a class of weak solutions with bounded variation, possibly containing shock waves. We then introduce a version of the random choice method founded on the global steady state solutions and the generalized Riemann problem and we establish a global-in-time existence theory for the initial value problem within the proposed class of weakly regular fluid flows. In the second chapter, we consider the relativistic Burgers model. We have introduced a version of the total variation which is decreasing with respect to time in the Cauchy problem. We also use the generalized characteristics to prove the nonlinear stability of a piecewise steady state solution. In the third chapter, we present some numerical methods based on the Schwarzschild geometry and study numerically the nonlinear stability of steady state solutions and the asymptotic behavior of a general solutions. The proposed schemes provide a numerical tool capable to preserve exactly the equilibria and allow us to analyse the evolution of fluids with the geometry effects
Bacon, Philippe. "Graphes d'ondelettes pour la recherche d'ondes gravitationnelles : application aux binaires excentriques de trous noirs". Thesis, Sorbonne Paris Cité, 2018. http://www.theses.fr/2018USPCC113/document.
Pełny tekst źródłaIn december 2015 the LIGO detectors have first detected a gravitational wave emitted by a pair of coalescing black holes 1.3 billion years ago. Many more observations have been realised since then and heralded gravitational waves as a new messenger in astronomy. The latest detection is the merge of two neutron stars whose electromagnetic counterpart has been followed up by many observatories around the globe. These direct observations have been made possible by the developpement of advanced data analysis techniques. With them the weak gravitational wave inprint in detectors may be recovered. The realised work during this thesis aims at developping an existing gravitational wave detection method which relies on minimal assumptions of the targeted signal. It more precisely consists in introducing an information on the signal phase depending on the astrophysical context. The first part is dedicated to a presentation of the method. The second one presents the results obtained when applying the method to the search of stellar mass binary black holes in simulated Gaussian noise data. The study is repeated in real instrumental data collected during the first run of LIGO. Finally, the third part presents the method applied in the search for eccentric binary black holes. Their orbit exhibits a deviation from the quasi-circular orbit case considered so far and thus complicates the signal morphology. This third analysis establishes first results with the proposed method in the case of a poorly modeled signal
Leng, Julien. "Controlling flexural waves using subwavelength perfect absorbers : application to Acoustic Black Holes". Thesis, Le Mans, 2019. http://www.theses.fr/2019LEMA1027/document.
Pełny tekst źródłaThe vibration control adapted to light structures is a scientific and technological challenge due toincreasingly stringent economic and ecological standards. Meanwhile, recent studies in audible acoustics havefocused on broadband wave absorption at low frequencies by means of subwavelength perfect absorbers. Suchmetamaterials can totally absorb the energy of an incident wave. The generalisation of this method for applicationsin elastodynamics could be of great interest for the vibration control of light structures.This thesis aims at adapting the perfect absorption problem for flexural waves in 1D and 2D systems with localresonators using the critical coupling condition. A study of 1D systems with simple geometries is first proposed. Thisprovides methods to design simple resonators for an effective absorption of flexural waves. The 1D systems thenbecome more complex by studying the critical coupling of 1D Acoustic Black Holes (ABH). The ABH effect is theninterpreted using the concept of critical coupling, and key features for future optimisation procedures of ABHs arepresented. The critical coupling condition is then extended to 2D systems. The perfect absorption by the firstaxisymmetric mode of a circular resonator inserted in a thin plate is analysed. Multiple scattering by an array ofcircular resonators inserted in an infinite or semi-infinite 2D thin plate, called metaplate, is also considered to getclose to practical applications. Through this thesis, analytical models, numerical simulations and experiments areshown to validate the physical behaviour of the systems presented
Aoudia, Sofiane. "Capture des étoiles par les trous noirs et ondes gravitationnelles". Nice, 2008. http://www.theses.fr/2008NICE4103.
Pełny tekst źródłaSiellez, Karelle. "Les systèmes binaires compacts comme sources de multimessagers : taux, distribution, émissions". Thesis, Nice, 2015. http://www.theses.fr/2015NICE4055.
Pełny tekst źródłaThe coalescence of compact binaries (two neutron stars or a neutron star and a black hole) emits gravitational waves and are thought to produce a short Gamma-Ray Burst (sGRB). With the second generation of gravitational waves detector, the detection in coincidence of both electromagnetic and gravitational emission will open a new window in astrophysics; the multimessenger area. It will allow the understanding of this phenomena, their progenitor and central engine. The goal of this thesis was to made an estimation of the coincident rate for different instruments, using two different method. The first one was based on the oberservations. Thus, I selected a sample of 31 sGRBs of known redshift based on specific criteria. After studying the spectral, temporal and host properties, I derived the isotropic local rate corrected from all known biases. This result was then applied to different satellites and gravitational detectors. After that I simulated this population to confirm this coincident rate with the Monte Carlo simulations. The difference between the two results is explained by a low-redshift population that can't be reproduce by the simulations, and was underestimated before. After tested different parameters for the model, I conclude that this non reproducible population of faint sGRBs at low redshift might be due to an other sort of progenitor. This thesis shows the feasibility of a coincident detection and the observational strategy that should be adopted. The understanding of our sample of sGRB is crucial in the preparation of this coincident detection
Foucaud, Simon. "Propagation d'ondes dans un guide inhomogène : application à la cochlée". Thesis, Toulouse, ISAE, 2012. http://www.theses.fr/2012ESAE0027/document.
Pełny tekst źródłaThe cochlea is the organ of hearing for humans and mammals. It is often modelled as an inhomogeneous waveguide. A travelling wave propagates along the fluid structure coupled waveguide. The mechanical impedance of the structure is varying and provides a frequency place relation. The asymptotic method Wentzel-Kramers-Brillouin allows to solve for the basilar membrane vibration. The evanescents modes are taken into account to provide a better representation compared to the numerical models. As a second step, the finite elements method is used to solve for the transversal modes while the WKB Approximation deals with the longitudinal propagation. The first flexural mode of the basilar membrane is shown. The second propagative mode reveals a shearing motion of the tectorial membrane which can help stimulating the hair cells. An over-size artificial cochlea is designed and built. Thanks to an acoustic black hole, used as a anechoic end, travelling waves are observed on this device. Reflected waves are attenuated and the interferences with incident waves reduced. Mode coupling could be applied not only to evanescent modes but also to propagatives ones. Perspectives for the adaptation of the WKB method to fluid structure inhomogeneous waveguides, and particularly to the immersed acoustic black hole, seem to be very promising
Książki na temat "Ondes de trou noir"
Vergnon, Gilles, i Yves Santamaria. Le syndrome de 1940: Un trou noir mémoriel? Paris: Riveneuve éditions, 2015.
Znajdź pełny tekst źródłaTustin, Frances. Le trou noir de la psyché: Barrières autistiques chez les névrosés. Paris: Seuil, 1989.
Znajdź pełny tekst źródłaMétaphysique de l'astre noir, ou, La métaphysique du trou du cul. Paris (France): Sens&Tonka, 2012.
Znajdź pełny tekst źródła1942-, Rees Martin J., red. Gravity's fatal attraction: Black holes in the universe. New York: Scientific American Library, 1996.
Znajdź pełny tekst źródłaRéparer sa route de vie. Outremont, Québec: Québecor, 2002.
Znajdź pełny tekst źródłaTrou Noir: Notion de Trou Noir. Independently Published, 2022.
Znajdź pełny tekst źródłaLenaars, Aurélien. Blanc Trou Noir. Independently Published, 2021.
Znajdź pełny tekst źródłaFoster, Alan Dean. Le Trou Noir. J'Ai Lu, 2006.
Znajdź pełny tekst źródłaBordé, Pascal. Qu'est-ce qu'un trou noir ? POMMIER, 2005.
Znajdź pełny tekst źródłaAbsorbé Par un Trou Noir. Independently Published, 2021.
Znajdź pełny tekst źródłaCzęści książek na temat "Ondes de trou noir"
Picouleau, E., M. Denis, P. Tas i J. Leveque. "Les hyperplasies atypiques isolées : trou noir du dépistage du cancer du sein?" W Cancer du sein : surdiagnostic, surtraitement, 266–67. Paris: Springer Paris, 2012. http://dx.doi.org/10.1007/978-2-8178-0249-7_64.
Pełny tekst źródłaSOL, Hélène. "Jets relativistes et mécanismes aux très hautes énergies". W Noyaux actifs de galaxie, 165–246. ISTE Group, 2023. http://dx.doi.org/10.51926/iste.9087.ch4.
Pełny tekst źródłaGranger, Bernard. "Dépression : le trou noir". W Troubles mentaux et psychothérapies, 42. Editions Sciences Humaines, 2016. http://dx.doi.org/10.3917/sh.marmi.2016.01.0042.
Pełny tekst źródłaMORRIS, Mark. "Le trou noir Galactique". W Noyaux actifs de galaxie, 67–104. ISTE Group, 2023. http://dx.doi.org/10.51926/iste.9087.ch2.
Pełny tekst źródła"Comment voir un trou noir ?" W Science, 42–43. EDP Sciences, 2023. http://dx.doi.org/10.1051/978-2-7598-3094-7.c015.
Pełny tekst źródłaCOLPI, Monica. "Trous noirs binaires dans l’univers des ondes gravitationnelles". W Noyaux actifs de galaxie, 295–322. ISTE Group, 2023. http://dx.doi.org/10.51926/iste.9087.ch6.
Pełny tekst źródłaLegendre, Caroline, i Joséphine Truffaut. "Chapitre 15. Traverser le trou noir". W Sexualités et transgressions, 159–65. Dunod, 2019. http://dx.doi.org/10.3917/dunod.couta.2019.01.0159.
Pełny tekst źródłaCOLLIN-ZAHN, Suzy. "Les noyaux actifs de galaxies : un combat entre accrétion et éjection". W Noyaux actifs de galaxie, 1–65. ISTE Group, 2023. http://dx.doi.org/10.51926/iste.9087.ch1.
Pełny tekst źródłaStrauss, Michael A. "5. La Voie lactée et son trou noir supermassif". W Passeport pour l'univers, 79–90. EDP Sciences, 2023. http://dx.doi.org/10.1051/978-2-7598-2929-3.c005.
Pełny tekst źródłaCOMBES, Françoise. "Co-évolution bulbestrous noirs, alimentation et feedback des AGN". W Noyaux actifs de galaxie, 247–94. ISTE Group, 2023. http://dx.doi.org/10.51926/iste.9087.ch5.
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