Relevant bibliographies by topics / Modelos de bianchi

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  2. Dissertations / Theses
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Academic literature on the topic 'Modelos de bianchi'

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Published: 4 June 2021
Last updated: 7 February 2022

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Journal articles on the topic "Modelos de bianchi"

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Chirde, Dr Vilas R., and Vijay P. Kadam. "Bianchi Type Bulk Viscous String Cosmological Models in Modified Theory of Gravity." International Journal of Scientific Research 3, no. 5 (June 1, 2012): 85–90. http://dx.doi.org/10.15373/22778179/may2014/28.

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SZYDŁOWSKI, MAREK, and ADAM KRAWIEC. "BIANCHI COSMOLOGIES AS DYNAMICAL SYSTEMS WITHOUT THE CONSTRAINT." International Journal of Modern Physics A 15, no. 17 (July 10, 2000): 2771–91. http://dx.doi.org/10.1142/s0217751x00001269.

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The Bianchi class A cosmology is treated as a nonlinear dynamical system. In the new variables in which Hamiltonian constraint is solved algebraically, the Bianchi class A model assumes the form of autonomous dynamical system in ℝ4 with polynomial form of vector field. It is proposed that the dimension of minimum reduced phase spaces of unconstrained autonomous systems be treated as a measure of generality of solution. The behavior of these models is studied in terms of qualitative analysis of differential equations. It is shown that the more general Bianchi IX and Bianchi VIII models (called Mixmaster models) can be presented as four-dimensional. We argue that the reduced Mixmaster dynamical systems are chaotic in the same sense as the original ones. The Bianchi I and Bianchi II world models are described by one-dimensional and two-dimensional systems, respectively. We also study dynamics of Bianchi VI0 and Bianchi VII0 models as a three-dimensional dynamical system. For two-dimensional dynamical system, the phase portraits are constructed with the Poincaré sphere which allows the analysis of dynamics both in finite domain and at infinity. For the last class of models we find an invariant submanifold on which systems are analyzed in details.
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SPINDEL, PHILIPPE. "COSMOLOGICAL MODELS IN THE R2 THEORY OF GRAVITY." International Journal of Modern Physics D 03, no. 01 (March 1994): 273–76. http://dx.doi.org/10.1142/s0218271894000447.

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I summarize some results obtained in the framework of the R2 theory of gravity: the general Bianchi-I solution in arbitrary dimensions and the description of the asymptotic behaviour of generic Bianchi-IX models in 3+1 dimensions.
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DI PIETRO, ELISA, and JACQUES DEMARET. "SCALE FACTOR DUALITY IN STRING BIANCHI COSMOLOGIES." International Journal of Modern Physics D 08, no. 03 (June 1999): 349–61. http://dx.doi.org/10.1142/s0218271899000262.

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We apply the scale factor duality transformations introduced in the context of the effective string theory to the anisotropic Bianchi-type models. We find dual models for all the Bianchi-types [except for types VIII and IX] and construct for each of them its explicit form starting from the exact original solution of the field equations. It is emphasized that the dual Bianchi class B models require the loss of the initial homogeneity symmetry of the dilatonic scalar field.
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Rezaei-Aghdam, A. "Bianchi bialgebras and WZW models." Surveys in High Energy Physics 17, no. 1-4 (January 2002): 173–81. http://dx.doi.org/10.1080/0142241021000058109.

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Belinchón, J. A. "Scalar-Tensor Bianchi VI Models." Journal of Gravity 2013 (June 5, 2013): 1–11. http://dx.doi.org/10.1155/2013/491905.

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We study how may vary the gravitational and the cosmological “constants,” ( and ) in several scalar-tensor theories with Bianchi III, , and symmetries. By working under the hypothesis of self-similarity we find exact solutions for two different theoretical models, which are the Jordan-Brans-Dicke (JBD) with and the usual JBD model with potential (that mimics the behaviour of . We compare both theoretical models, and some physical and geometrical properties of the solutions are also discussed putting special emphasis on the study of the isotropization of the solutions.
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Fujiwara, Y., H. Ishihara, and H. Kodama. "Comments on closed Bianchi models." Classical and Quantum Gravity 10, no. 5 (May 1, 1993): 859–67. http://dx.doi.org/10.1088/0264-9381/10/5/006.

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Sklavenites, D. "Geodesic Bianchi type cosmological models." General Relativity and Gravitation 24, no. 1 (January 1992): 47–58. http://dx.doi.org/10.1007/bf00756873.

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Asano, Masako, Masayuki Tanimoto, and Noriaki Yoshino. "Supersymmetric Bianchi class A models." Physics Letters B 314, no. 3-4 (September 1993): 303–7. http://dx.doi.org/10.1016/0370-2693(93)91240-n.

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Panov, V. F., and O. V. Sandakova. "The Bianchi IX cosmological models." Russian Physics Journal 54, no. 3 (August 2011): 354–59. http://dx.doi.org/10.1007/s11182-011-9621-4.

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Dissertations / Theses on the topic "Modelos de bianchi"

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MATEUS, Dairo Antonio Cuellar. "Considerações Sobre a Anisotropia em Modelos Bianchi Tipo I." reponame:Repositório Institucional da UNIFEI, 2018. http://repositorio.unifei.edu.br/xmlui/handle/123456789/1149.

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Neste trabalho apresentamos uma introdução matemática ao estudo de modelos cosmológicos espacialmente homogêneos, em especial aos modelos Bianchi tipo I, que são espacialmente planos. Neste caso analisamos como a geometria espacial evolui sob certas condições da anisotropia. Ao fi nal analisamos a possibilidade destes modelos substituirem o modelo Robertson-Walker plano com constante cosmológica.
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Fay, Stéphane. "Cosmologies spatialement homogènes en théories tenseur-scalaires." Phd thesis, Université Paris-Diderot - Paris VII, 2004. http://tel.archives-ouvertes.fr/tel-00008063.

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Cette thèse étudie les modèles cosmologiques homogènes mais anisotropes en théories tenseur-scalaire. Son but est de déterminer les propriétés que doivent avoir ces théories afin que ces modèles possèdent asymptotiquement les caractéristiques dynamiques de notre Univers actuel ou apportent une réponse à certains de ses problèmes comme ceux de la constante cosmologique. La première partie de la thèse est consacrée à une introduction historique et à une justification physique des théories tenseur-scalaires de la gravitation et des modèles cosmologiques anisotropes. La seconde partie détaille les notions mathématiques nécessaires à la compréhension de cette thèse, à savoir la classification des cosmologies anisotropes et l'écriture des équations de champs dans le formalisme Lagrangien et Hamiltonien. La troisième partie est composée d'une série de sept articles montrant comment l'on peut parvenir à contraindre les théories tenseur-scalaires à l'aide de solutions exactes, en exigeant que l'Univers possède certains comportements dynamiques (expansion, inflation, etc), soit dépourvu de singularité ou possède une symétrie de Noether. Dans la quatrième partie, le processus d'isotropisation des modèles anisotropes est étudié en détail pour de nombreuses classes de théories tenseur-scalaires. Des contraintes nécessaires à l'isotropisation, les comportements asymptotiques des fonctions métriques et du potentiel au voisinage de cet état sont déterminés et le phénomène de quintessence analysé. Un lien entre les champs scalaires quintessents qui pourraient peupler notre Univers et la matière noire dans les galaxies (1 article) est montré. Les six articles à l'origine de ce chapitre sont reproduits dans la sixième partie qui tient lieu d'appendice. Nous concluons dans la cinquième partie.
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Cheng, A. D. Y. "Supersymmetric quantum Bianchi models." Thesis, University of Cambridge, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.597576.

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This thesis is about the quantum cosmology of supergravity theories, in particular N = 1 supergravity. In chapter 2, the Bianchi-IX model in N = 1 supergravity with a cosmological constant is investigated. This example is also restricted to the case of the k = +1 Friedmann universe. In chapter 3, the most general solution of the Lorentz constraints is found. Using this solution, N = 1 supergravity in the diagonal Bianchi-IX model is studied. The Hamilton-Jacobi equation is derived and completely solved. The Hartie-Hawking and wormhole actions are both found among the solutions. In chapter 4, the relation between the Chern-Simons functional and the no-boundary proposal is considered. The exponential of the Chern-Simons functional is the first known exact solution of quantum general relativity with a cosmological constant, being defined in the Ashtekar variables. However, it has turned out to be possible to show that the Chern-Simons functional and the no-boundary proposal are not related to each other in general relativity and N = 1 supergravity by considering perturbations around the k = +1 Friedmann universe. In chapter 5, the canonical formulation of N = 1 supergravity coupled to supermatter is presented. The supersymmetry and gauge constraints are derived. This model is then studied in the k = +1 Friedmann universe. It is found there are solutions in the case of a scalar multiplet. However, no non-trivial solution exists for a Yang-Mills multiplet, and it is explained why there is no physical state. Chapter 6 describes a brief investigation of the quantum cosmology of N = 2 and N = 4 supergravity theories. The thesis ends with concluding remarks and an indication of directions of future development.
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Friedrichsen, James Edward. "Quantization of Bianchi type cosmological models /." Full text (PDF) from UMI/Dissertation Abstracts International, 2000. http://wwwlib.umi.com/cr/utexas/fullcit?p3004268.

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Matsas, George Emanuel Avraam [UNESP]. "Estudo do universo primitivo no modelo bianchi IX." Universidade Estadual Paulista (UNESP), 1988. http://hdl.handle.net/11449/132638.

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Matsas, George Emanuel Avraam. "Estudo do universo primitivo no modelo bianchi IX /." São Paulo : [s.n.], 1988. http://hdl.handle.net/11449/132638.

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Yearsley, J. M. "Anisotropic cosmologies and the role of matter." Thesis, University of Sussex, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.259719.

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Hervik, Sigbjørn. "Mathematical cosmology : Bianchi models, asymptotics and extra dimensions." Thesis, University of Cambridge, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.616093.

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Nunes, Thiago Crisóstomo Carlos. "Relevância da dimensionalidade no modelo de Bianconi-Barabási." PROGRAMA DE PÓS-GRADUAÇÃO EM FÍSICA, 2017. https://repositorio.ufrn.br/jspui/handle/123456789/25467.

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
Redes sem escala são bastante populares hoje em dia, uma vez que muitos sistemas estão bem representados por tais estruturas. Para estudar esses sistemas, foram propostos vários modelos. No entanto, a maioria deles não levam em conta a distância Euclidiana nó à nó, ou seja, a distância geográ ca. Em redes reais, a distância entre os sítios pode ser muito relevante, por exemplo, os casos em que se pretende minimizar custos. Neste cenário, estudamos o papel da dimensionalidade d no Modelo de Bianconi-Barabási com um crescimento e ligação preferencial envolvendo distâncias Euclidianas. A ligação preferencial neste modelo segue a regra Πi ∝ ηiki/rαA ij (1 ≤ i < j; αA ≥ 0), onde ηi caracteriza a qualidade do i-ésimo sítio e é escolhido aleatoriamente dentro do intervalo (0, 1]. Veri camos que a distribuição de grau P(k) para as dimensões d = 1, 2, 3, 4 são bem ajustadas por P(k) ∝ e −k/κ q , onde e −k/κ q é a função q-exponencial que surge naturalmente da Mecânica Estatística não-extensiva de Tsallis. Determinamos o índice q e κ como funções das quantidades αA e d e veri camos numericamente que ambos apresentam um comportamento universal em relação à variável αA/d. O mesmo comportamento também foi exibido pelo expoente dinâmico β que está associado a taxa que determinado sítio tem em receber ligações.
Scale-free networks are quite popular nowadays since many systems are well represented by such structures. In order to study these systems, several models were proposed. However, most of them do not take into account the node-to-node Euclidean distance, i.e., the geographical distance. In real networks, the distance between sites can be very relevant, e.g., those cases where it is intended to minimize costs. Within this scenario, we studied the role of dimensionality d in the Bianconi-Barabási model with a preferential attachment growth involving Euclidean distances. The preferential attachment in this model follows the rule Πi ∝ ηiki/rαA ij (1 ≤ i < j; αA ≥ 0), where ηi characterizes the tness of the i-th site and is randomly chosen within the (0, 1] interval. We veri ed that the degree distribution P(k) for dimensions d = 1, 2, 3, 4 are well tted by P(k) ∝ e −k/κ q , where e −k/κ q is the q-exponential function naturally emerging within nonextensive statistical mechanics. We determine the index q and κ as functions of the quantities αA and d, and numerically verify that both present a universal behavior with respect to the scaled variable αA/d. The same behavior also has been displayed by the dynamical β exponent which characterizes the steadily growing number of links of a given site.
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Pereyra, Pablo Hernán. "Soluções não-planas no modelo cosmológico Bianchi tipo V na teoria 5D-Espaço-Tempo-Massa." reponame:Biblioteca Digital de Teses e Dissertações da UFRGS, 1999. http://hdl.handle.net/10183/127585.

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As teorias de gravitação invariante por escala propõem uma variação com relação ao tempo da constante gravitacional ou da massa dos objetos que constituem o universo. Desta forma a intensidade da interação gravitacional também se torna variável, modificando sensivelmente o comportamento do universo. Algumas teorias foram propostas no decorrer do século, porém, descartadas devido a problemas técnicos e de concordância com dados observacionais. trabalho a ser apresentado nesta dissertação está fundamentado em uma teoria de gravitação invariante por escala, a qual vem atualmente sendo desenvolvida e é denominada teoria penta-dimensional Espaço-Tempo-Massa. Tal teoria propõe a quantidade de massa de repouso como uma quantidade extensiva, de maneira a introduzi-la na métrica e torná-la variável. Diversos trabalhos foram realizados com esta teoria, incluindo alguns, o estudo de modelos cosmológicos. Investigaremos aqui a extensão do modelo cosmológico de Bianchi tipo V, que é um dos mais importantes modelos do universo. Duas métricas foram propostas e as soluções das equações de campo da teoria SD-Espaço-Tempo-Massa para tais métricas foram obtidas. Tais soluções correspondem a espaços não-planos. Um estudo sobre singularidades na métrica e na curvatura foi realizado para ambas as métricas, em adição, o tensor de energia-momento induzido foi obtido para as métricas e as suas propriedades investigadas. Através da análise do tensor de Kretschmann verificou-se a ausência de singularidades efetivas nos modelos 5D abordados, sugerindo uma distribuição finita de energia devido a inclusão da massa de repouso.
The scale invariant gravitational theories propose the time variation either in the gravitational constant or in the rest mass of the objects that constitute the universe. By this way the intensity of the gravitational interaction varies as well, changing accordingly the behavior of the universe. Several theories have been proposed in the literature, however most of them have been discharged due to drawbacks in thecnicalities or lack of agreement with observational data. The work conducted here takes into account a 5-dimensional theory called SpaceTime- Mass, which proposes that the rest mass be na extensible quantity that change with time. Severa! investigations have been done so far with this theory, some o f them including cosmological studies. Here we will investigate the 5D extension of the Bianchi type V cosmological model, which is one of the most important model of the universe. Two metrics are proposed and the solution of the corresponding 5D-Spae-Time-Mass field equations are found. Both solutions shown to be non-flat spaces. The singularity behavior of the metric and curvature were done, the induced energy-momentum tensor for both metrics were determined and their properties were investigated. Through the analysis of the Kretschmann tensor, it has been shown that there is no effective singularity in the space, which suggest that there is a finite distribution of energy due to the inclusion of the rest mass variable.
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Book chapters on the topic "Modelos de bianchi"

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Liebscher, Stefan. "Application: Cosmological Models of Bianchi Type, the Tumbling Universe." In Bifurcation without Parameters, 115–18. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10777-6_13.

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Krasiński, Andrzej. "The Ultimate Extension of the Bianchi Classification for Rotating Dust Models." In On Einstein’s Path, 283–98. New York, NY: Springer New York, 1999. http://dx.doi.org/10.1007/978-1-4612-1422-9_20.

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Burd, Adrian. "How Can You Tell if the Bianchi IX Models Are Chaotic?" In Deterministic Chaos in General Relativity, 345–54. Boston, MA: Springer US, 1994. http://dx.doi.org/10.1007/978-1-4757-9993-4_20.

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Wainwright, J. "Bianchi cosmologies: non–tilted class A models." In Dynamical Systems in Cosmology, 123–52. Cambridge University Press, 1997. http://dx.doi.org/10.1017/cbo9780511524660.008.

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Hewitt, C. G., and J. Wainwright. "Bianchi cosmologies: non–tilted class B models." In Dynamical Systems in Cosmology, 153–69. Cambridge University Press, 1997. http://dx.doi.org/10.1017/cbo9780511524660.009.

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McKercher, Bob, and Bruce Prideaux. "The Political Economy of Tourism and Approaches to Forecasting." In Tourism Theories, Concepts and Models. Goodfellow Publishers, 2020. http://dx.doi.org/10.23912/9781911635352-4726.

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While there is a vast literature on issues related to political economy, tourism scholars have generally paid little attention to this area of research. This chapter discusses some of the underlying debates related to political economy to provide a window into the fundamental role that economic forces play in the operation, sustainability and profitability of the global tourism system. In the near future, the need to transition to a carbon-neutral production system (see Chapter 15), and the immense difficulties that will be faced in reining in our increasing use of diminishing resources, will generate considerable discussion on the merits of various production systems such as Neoliberalism, socialism, neo-Marxism and post-Keynesian. This chapter also considers a range of models used to forecast tourism activity, a task that is an important element in future tourism investment and planning activities. The current production system is firmly embedded in the market driven capitalist system of economic production and for this reason, the following dis- cussion will focus on capitalism. This chapter provides a neo-Marxist perspective to demonstrate a counter view to the predominate interpretation of capitalism through a neoliberal lens. Degrowth (see Chapter 15) also offers another vision for organizing a future economic system of production. Understanding how we arrived at our system of economic production is important and provides insights into the next stage of economic evolution, which will most likely to be based on a carbon-neutral economic production system. So what is the difference between political economy and economics? Political economy is concerned with the process of production and its impact on national income and wealth, and the conflicts, inequalities and problems that arise in trade, law and government (Bianchi, 2018; Williams, 2004). Scholars generally approach the study of political economy from perspectives that include Liberalism, Keynesianism, Marxism, Socialism and Neoliberalism (and the many sub-branches of these schools). Economics on the other hand is concerned with production, distribution and consumption of goods and services and leaves aside political and social considerations although as Bianchi (2018) observed, the distinction between political economy and economics has become blurred because of the political nature of significant areas of neoliberal thought.
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Socorro, J., Paulo A., Abraham Espinoza-Garcia, Luis O., and Priscila Romero. "Cosmological Bianchi Class A Models in Sáez-Ballester Theory." In Aspects of Today's Cosmology. InTech, 2011. http://dx.doi.org/10.5772/24088.

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Conference papers on the topic "Modelos de bianchi"

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Berköz, G., and Ö Sevinç. "Bianchi Models with Chaplygin Gas." In SIXTH INTERNATIONAL CONFERENCE OF THE BALKAN PHYSICAL UNION. AIP, 2007. http://dx.doi.org/10.1063/1.2733076.

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BRADLEY, M., and D. ERIKSSON. "ROTATING COSMOLOGICAL MODELS OF BIANCHI TYPE V." In Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF). World Scientific Publishing Company, 2006. http://dx.doi.org/10.1142/9789812704030_0246.

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Socorro, J., and Abraham Espinoza-García. "Bianchi class A models in Sàez-Ballester's theory." In IX WORKSHOP OF THE GRAVITATION AND MATHEMATICAL PHYSICS DIVISION OF THE MEXICAN PHYSICAL SOCIETY. AIP, 2012. http://dx.doi.org/10.1063/1.4748541.

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Amirhashchi, Hassan, Hishamuddin Zainuddin, Jumiah Hassan, Halimah Mohamed Kamari, A. K. Yahya, and Shah Alam. "Bianchi Type III String Cosmological Models for Perfect Fluid Distribution in General Relativity." In PROGRESS OF PHYSICS RESEARCH IN MALAYSIA: PERFIK2009. AIP, 2010. http://dx.doi.org/10.1063/1.3469655.

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Reports on the topic "Modelos de bianchi"

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Turner, M. S., and L. Widrow. Bianchi models and new inflation. Office of Scientific and Technical Information (OSTI), March 1986. http://dx.doi.org/10.2172/5801979.

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