Literatura científica selecionada sobre o tema "Mouvement chaotique"
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Artigos de revistas sobre o assunto "Mouvement chaotique"
Zinguer, Ilana. "Le langage chaotique". L’Annuaire théâtral, n.º 42 (5 de maio de 2010): 51–64. http://dx.doi.org/10.7202/041688ar.
Texto completo da fonteCOLLOREC, L., e D. JUVE. "MOUVEMENT CHAOTIQUE D'UN ENSEMBLE DE TOURBILLONS ET ÉMISSION ACOUSTIQUE ASSOCIÉE". Le Journal de Physique IV 02, n.º C1 (abril de 1992): C1–561—C1–564. http://dx.doi.org/10.1051/jp4:19921121.
Texto completo da fonteLaxenaire, Michel. "Les circuits de l’identification en groupe : à propos du «déterminisme chaotique»". Revue de psychothérapie psychanalytique de groupe 35, n.º 1 (2000): 63–72. http://dx.doi.org/10.3406/rppg.2000.1507.
Texto completo da fonteLandowski, Eric. "Une sémiotique à refaire?" Galáxia (São Paulo) 13, n.º 26 (dezembro de 2013): 10–32. http://dx.doi.org/10.1590/s1982-25532013000300002.
Texto completo da fonteBensussan, Gérard. "ROSENZWEIG, SCHELLING ET L’HISTOIRE: QUELQUES APERÇUS". História Revista 21, n.º 2 (9 de outubro de 2016): 4. http://dx.doi.org/10.5216/hr.v21i2.43381.
Texto completo da fonteRenier, Janine. "Crises systémiques : Effondrement ? Ou méta-morphose vers la grande transition ?" Acta Europeana Systemica 8 (10 de julho de 2020): 285–300. http://dx.doi.org/10.14428/aes.v8i1.56463.
Texto completo da fonteANTAR, Monia. "Autosimilarité et mémoire longue : Les rendements des indices boursiers tunisiens sont-ils chaotiques ?" Journal of Academic Finance 7, n.º 2 (17 de novembro de 2016): 1–32. http://dx.doi.org/10.59051/joaf.v7i2.60.
Texto completo da fonteChassay, Jean-François. "Les petites apocalypses de John Cassavetes". Cinémas 13, n.º 3 (28 de julho de 2004): 79–94. http://dx.doi.org/10.7202/008708ar.
Texto completo da fonteMoussaoui, Abderrahmane. "Violence extrême". Anthropen, 2020. http://dx.doi.org/10.17184/eac.anthropen.134.
Texto completo da fonteTeses / dissertações sobre o assunto "Mouvement chaotique"
GUEROUACHE, MOHAMED SALAH. "Etude numerique de l'instabilite de benard-karman derriere un cylindre fixe ou en mouvement periodique. Dynamique de l'ecoulement et advection chaotique". Nantes, 2000. http://www.theses.fr/2000NANT2048.
Texto completo da fonteHoang, Hoai-Nam. "Long term stability and diffusion in the solar system". Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO002.
Texto completo da fonteBecause the Solar System is chaotic, the orbital evolution of the Earth's orbit beyond 60 Myr cannot be reliably predicted. On the other hand, Earth's orbital variations control insolation which leads to long-term climate change, and were thus imprinted in the geological records. The recovery of this astronomical forcing in geological data has revolutionized the determination of the geological time scales. Taking into account the chaotic uncertainty of the astronomical forcing is necessary for a complete astronomical calibration of geological records. To address this problem, we obtain, benchmark and illustrate the application of probability density functions of the secular frequencies using kernel density estimation, whose uncertainty determined by the moving block bootstrap method.Apart from being chaotic, the inner planets of the Solar System can also be unstable. Despite the lack of apparent constraints that bound the chaotic dynamics, the probability of instability is remarkably low in 5 billion years, especially considering it is 1000 times longer than the Lyapunov time of the system. We attempt to resolve the paradox in this thesis by studying the destabilization in its total complexity of a high dimensional system. As a first step, we provide an exhaustive statistical analysis of instability up to 100 Gyr from a hierarchy of secular models at different degrees in eccentricities and inclinations. We find that the Hamiltonian truncated at degree 4, despite its comprehensiveness, is overly stable and not sufficient to reproduce the instability statistics. This is due to the unexpectedly significant contribution of the terms at degree 6 to the frontier of instability. As a second step, we show that the dynamics of the inner planets over its chaotic timescale is slow-fast with a wide separation of timescales. The first evidence is found in its Lyapunov spectrum, where a hierarchy of characteristic exponents spans two orders of magnitude. The smallest Lyapunov exponents can be related to the slow variables, which vary on a timescale much longer than the Lyapunov time. Concretely, from a systematic analysis of the leading secular resonances, we demonstrate three quasi-symmetries, which define three quasi-integral of motion. By a novel utilization of a traditional statistical method - principal component analysis, we confirm that these quasi-integrals are among the slowest degrees of freedom of the chaotic dynamics. The quasi-integrals constrain the long-term chaotic diffusion of the orbits, thereby slowing down the system in their pathway towards planetary collision
Vialar, Thierry. "Dynamiques non linéaires chaotiques en finance et économie /". Paris : Économica, 2005. http://catalogue.bnf.fr/ark:/12148/cb399130739.
Texto completo da fonteDella, Penna Gabriella. "Méthodes perturbatives et numériques pour l'étude des mouvements réguliers et chaotiques avec application à la mécanique céleste". Nice, 2001. http://www.theses.fr/2001NICE5611.
Texto completo da fonteHamdi, Tarek. "Calcul stochastique commutatif et non-commutatif : théorie et application". Thesis, Besançon, 2013. http://www.theses.fr/2013BESA2015/document.
Texto completo da fonteMy PhD work is composed of two parts, the first part is dedicated to the discrete-time stochastic analysis for obtuse random walks as to the second part, it is linked to free probability. In the first part, we present a construction of the stochastic integral of predictable square-integrable processes and the associated multiple stochastic integrals ofsymmetric functions on Nn (n_1), with respect to a normal martingale.[...] In a second step, we revisited thedescription of the marginal distribution of the Brownian motion on the large-size complex linear group. Precisely, let (Z(d)t )t_0 be a Brownian motion on GL(d,C) and consider nt the limit as d !¥ of the distribution of (Z(d)t/d)⋆Z(d)t/d with respect to E×tr
Renaud, Jean-François. "Calcul de Malliavin, processus de Lévy et applications en finance : quelques contributions". Thèse, 2007. http://hdl.handle.net/1866/18144.
Texto completo da fonteCapítulos de livros sobre o assunto "Mouvement chaotique"
"CHAP. XIII. Les opinions sur l'origine du monde sont au nombre de trois: celle des théologiens orthodoxes, qui admettent la création ex nihilo; celle de Platon et d'autres philosophes anciens, qui admettent l'éternité de la matière chaotique; celle d'Aristote et de tous les péripatéticiens, qui admettent l'éternité du mouvement et du temps". In Dalalat al Hairin, editado por Salomon Munk, 104–14. Piscataway, NJ, USA: Gorgias Press, 2010. http://dx.doi.org/10.31826/9781463225346-016.
Texto completo da fonte