Sólitons latentes, cordas negras, membranas negras e equações de estado em modelos de Kaluza-Klein

Neste trabalho investigamos soluções solitônicas em modelos de Kaluza-Klein com um número arbitrário de espaços internos toroidais, que descrevem o campo gravitacional de um objeto massivo compacto. Cada toro d_i-dimensional possui um fator de escala independente C_i, i = 1, ..., N, que é caracterizado pelo parâmetro ᵞi. Destacamos a solução fisicamente interessante correspondente à massa puntual. Para a solução geral obtemos equações de estado nos espaços externo e interno. Estas equações demonstram que a massa pontual solitônica possui equações de estado tipo poeira em todos os espaços. Obtemos também os parâmetros pósnewtonianos que nos possibilitam encontrar as fórmulas da precessão do periélio, do desvio da luz e do atraso no tempo de ecos de radar. Além disso, os experimentos gravitacionais levam a uma forte limitação nos parâmetros do modelo: T = ƩNi=1 diYi = −(2, 1±2, 3)×10⁻⁵. A solução para massa pontual com Y1 = . . . = YN = (1+ƩNi=1 di)⁻¹ contradiz esta restrição. A imposição T = 0 satisfaz essa limitação experimental e define uma nova classe de soluções que são indistinguíveis para a relatividade geral. Chamamos estas soluções de sólitons latentes. Cordas negras e membranas negras com Yi = 0 pertencem a esta classe. Além disso, a condição de estabilidade dos espaços internos destaca cordas/membranas negras de sólitons latentes, conduzindo exclusivamente para as equações de estado de corda/membrana negra p_i = −ε/2, i = 1, . . . ,N, nos espaços internos e ao número de dimensões externas d₀ = 3. As investigações do fluido perfeito multidimensional estático e esfericamente simétrico com equação de estado tipo poeira no espaço externo confirmam os resultados acima.

Desenvolvimento de algoritmo para modelagem e simulação de sistemas por grafos de ligação

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Efeitos da equação de estado em hidrodinâmica relativística através de alguns observáveis

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

A new approach on the stability analysis in ELKO cosmology

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Equação de Estado para o Universo Primordial

Pós-graduação em Física - IFT

Energia escura e formação de estruturas em larga escala

Pós-graduação em Física - IFT

Entropy, complexity and disequilibrium in compact stars

We used the statistical measurements of information entropy, disequilibrium and complexity to infer a hierarchy of equations of state for two types of compact stars from the broad class of neutron stars, namely, with hadronic composition and with strange quark composition. Our results show that, since order costs energy. Nature would favor the exotic strange stars even though the question of how to form the strange stars cannot be answered within this approach. (C) 2012 Elsevier B.V. All rights reserved.

Mejora y optimización de un código de simulación hidrodinámico con transporte de radiación para el estudio de sistemas en condiciones de alta densidad de energía

Se presentan las mejoras introducidas en un código de transporte de radiación acoplada a la hidrodinámica llamado ARWEN para el estudio de sistemas en el rango de física de alta densidad de energía (High Energy Density Physics). Los desarrollos introducidos se basan en las siguientes áreas: ít>,~ Ecuaciones de estado: se desarrolla una nueva metodología mediante la cual es posible ajustar los resultados de un modelo simple de ecuaciones de estado como QEOS a datos experimentales y resultados de AIMD. Esta metodología tiene carácter general para poder ser aplicada en gran cantidad de materuales de interés y amplia la flexibilidad de ajuste de los métodos de los que ha partido como base este trabajo. En segundo lugar, se ha desarrollado una librería para la gestión de tablas de datos de ecuaciones de estado que también incluye la gestión de tablas con datos de opacidades y de ionización. Esta nueva librería extiende las capacidades de la anterior al tener llamadas más específicas que aceleran los cálculos, y posibilidad de uso de varias tablas a la vez. Solver de difusión: se ha desarrollado un nuevo paquete para resolver la ecuación de difusión que se aplicará a la conducción de calor dentro del plasma. El método anterior no podía ser ejecutado en paralelo y producía resultados dependientes de la resolución de la malla, mientras que este método es paralelizable y además obtiene una solución con mejor convergencia, lo que supone una solución que no depende del refinamiento del mallado. Revisión del paquete de radiación: en primer lugar se ha realizado una revisión de la implementación del modelo de radiación descubriendo varios errores que han sido depurados. También se ha incluido la nueva librería de gestión de tablas de opacidades que permiten la obtención de las propiedades ópticas del plasma en multigrupos de energía. Por otra parte se ha extendido el cálculo de los coeficientes de transporte al esquema multimaterial que ha introducido David Portillo García en el paquete hidrodinámico del código de simulación. Por último se ha revisado el esquema de resolución del transporte y se ha modificado para hacerlo paralelizable. • Se ha implementado un paquete de trazado de rayos para deposición láser que extiende la utilidad del anterior al ser en 3D y poder utilizar entonces diferentes configuraciones. • Una vez realizadas todas estas tareas se ha aplicado el código ARWEN al estudio de la astrofísica de laboratorio simulando los experimentos llevados a cabo en la instalación PALS por Chantal Stehlé acerca de ondas de choque radiativas. Se han comparado los resultados experimentales frente a las predicciones del código ARWEN obteniéndose una gran concordancia en la velocidad de la onda de choque generada y en las dimensiones del precursor. El código de simulación sobre el que se ha trabajado, junto con los desarrollos aportados por otros investigadores durante la realización de esta tesis, ha permitido participar en colaboraciones con laboratorios de Francia o Japón y se han producido resultados científicos publicados basados en el trabajo descrito en esta tesis. ABSTRACT Improvements in radiation hydrodynamic code ARWEN for the study of systems in the range of physics high energy density (High Energy Density Physics) are presented. The developments introduced are based on the following áreas: • Equations of state: a new methodology was developed to adjust the results of a simple Equation of State model like QEOS to experimental data and results of AIMD. This methodology can be applied to a large amount of materials and it increases the flexibility and range of the previous methods used as basis for this work. Also a new computer library has been developed to manage data tables of thermodynamic properties as well as includes the management of opacity and ionization data tables. This new library extends the capabilities of the previous one with more specific routines, and the possibility of using múltiple tables for several materials. • Diffusion solver: a new package has been developed to solve the diffusion equation applied to the heat conduction of the plasma. The previous method is not parallelizable and it produced mesh dependent results, while this new package can be executed in parallel and achieves a more converged solution that does not depend on the refinement of the mesh. • Radiation package: the check of the radiation model rose several bugs in the implementation that had been removed. The new computer library for EOS managing includes capabilities to store opacity tables for multigroups of energy. Moreover the transport coefficients calculations have been extended for the new multimaterial hydrodynamic package developed by David Portillo García. Also the solving methodology for the transport equation has been modified to make the code run in parallel. • A new ray tracing package has been introduced to extend the previous one to 3D. Once all these tasks has been implemented, the ARWEN code has been applied to study laboratory astrophysics systems. Simulations have been done in order to reproduce the results of the experiments carried out in PALS facility by Chantal Stehlé in radiative shock production. Experimental results are in cióse agreement to the ARWEN estimations of the speed of the shock wave and the length of the precursor. The simulation code used in this thesis, including the work done in ARWEN by other colleagues at the time of this research, allowed the collaboration with other research institution in France and Japan and some of the results presented in this thesis have been published in scientific journals.

A windows program for the derivation of steady-state equations in enzyme systems

Despite the number of computer-assisted methods described for the derivation of steady-state equations of enzyme systems, most of them are focused on strict steady-state conditions or are not able to solve complex reaction mechanisms. Moreover, many of them are based on computer programs that are either not readily available or have limitations. We present here a computer program called WinStes, which derives equations for both strict steady-state systems and those with the assumption of rapid equilibrium, for branched or unbranched mechanisms, containing both reversible and irreversible conversion steps. It solves reaction mechanisms involving up to 255 enzyme species, connected by up to 255 conversion steps. The program provides all the advantages of the Windows programs, such as a user-friendly graphical interface, and has a short computation time. WinStes is available free of charge on request from the authors. (c) 2006 Elsevier Inc. All rights reserved.

Brief note on the variation of constants formula for fuzzy differential equations

This note gives a theory of state transition matrices for linear systems of fuzzy differential equations. This is used to give a fuzzy version of the classical variation of constants formula. A simple example of a time-independent control system is used to illustrate the methods. While similar problems to the crisp case arise for time-dependent systems, in time-independent cases the calculations are elementary solutions of eigenvalue-eigenvector problems. In particular, for nonnegative or nonpositive matrices, the problems at each level set, can easily be solved in MATLAB to give the level sets of the fuzzy solution. (C) 2002 Elsevier Science B.V. All rights reserved.

Modeling of non-isothermalvapor membrane separation with thermodynamic models and generalized mass transfer equations

A rigorous unit operation model is developed for vapor membrane separation. The new model is able to describe temperature, pressure, and concentration dependent permeation as wellreal fluid effects in vapor and gas separation with hydrocarbon selective rubbery polymeric membranes. The permeation through the membrane is described by a separate treatment of sorption and diffusion within the membrane. The chemical engineering thermodynamics is used to describe the equilibrium sorption of vapors and gases in rubbery membranes with equation of state models for polymeric systems. Also a new modification of the UNIFAC model is proposed for this purpose. Various thermodynamic models are extensively compared in order to verify the models' ability to predict and correlate experimental vapor-liquid equilibrium data. The penetrant transport through the selective layer of the membrane is described with the generalized Maxwell-Stefan equations, which are able to account for thebulk flux contribution as well as the diffusive coupling effect. A method is described to compute and correlate binary penetrant¿membrane diffusion coefficients from the experimental permeability coefficients at different temperatures and pressures. A fluid flow model for spiral-wound modules is derived from the conservation equation of mass, momentum, and energy. The conservation equations are presented in a discretized form by using the control volume approach. A combination of the permeation model and the fluid flow model yields the desired rigorous model for vapor membrane separation. The model is implemented into an inhouse process simulator and so vapor membrane separation may be evaluated as an integralpart of a process flowsheet.

Dehydration and volatilization non isothermic kinetic of the solid state aluminium 8-hydroxyquinolinate

Al(C9H6ON)3.2.5H2O was precipitated from the mixture of an aqueous solution of aluminium ion and an acid solution of 8-hydroxyquinoline, by increasing the pH value to 9.5 with ammonia aqueous solution. The TG curves in nitrogen atmosphere present mass losses due to dehydration, partial volatilisation (sublimation plus vaporisation) of the anhydrous compound followed by thermal decomposition with the formation of a mixture of carbonaceous and residues. The relation between sublimation and vaporisation depends on the heating rate used. The non isothermic integral isoconventional methods as linear equations of Ozawa-Flynn-Wall and Kissinger-Akahira-Sunose (KAS) were used to obtain the kinetic parameters from TG and DTA curves, respectively. Despite the fact that both dehydration and volatilisation reactions follow the linearity by using both methods, only for the volatilisation reaction the validity condition, 20<= E/RT<= 50, was verified.

The measurement of the optical absorption cross section of photosystem 1 and photosystem 2 from whole live cells of porphyridium cruentum, in light state 1 and light state 2

The optical cross section of PS I in whole cells of Porphyridium cruentum (UTEX 161), held in either state 1 or state 2, was determined by measuring the change in absorbance at 820nm, an indication of P700+; the X-section of PS2 was determined by measuring the variable fluorescence, (Fv-Fo)/Fo, from PS2. Both cross-sections were 7 determined by fitting Poisson distribution equations to the light saturation curves obtained with single turnover laser flashes which varied in intensity from zero to a level where maximum yield occurred. Flash wavelengths of 574nm, 626nm, and 668nm were used, energy absorbed by PBS, by PBS and chla, and by chla respectively. There were two populations of both PSi and PS2. A fraction of PSi is associated with PBS, and a fraction of PS2 is free from PBS. On the transition S1->S2, only with PBS-absorbed energy (574nm) did the average X-section of PSi increase (27%), and that of PS2 decrease (40%). The fraction of PSi associated with PBS decreased, from 0.65 to 0.35, and the Xsection of this associated PS 1 increased, from 135±65 A2 to 400±300A2. The cross section of PS2 associated with PBS decreased from 150±50 A2 to 85±45 A2, but the fraction of PS2 associated with PBS, approximately 0.75, did not change significantly. The increase in PSi cross section could not be completely accounted for by postulating that several PSi are associated with a single PBS and that in the transition to state2, fewer PSi share the same number of PBS, resulting in a larger X-section. It is postulated that small changes occur in the attachment of PS2 to PBS causing energy to be diverted to the attached PSi. These experiments support neither the mobile-PBS model of state transitions nor that of spillover. From cross section changes there was no evidence of energy transfer from PS2 to PSi with 668nm light. The decrease in PS2 fluorescence which occurred at this wavelength cannot be explained by energy transfer; another explanation must be sought. No explanation was found for an observed decrease in PSi yield at high flash intensities.

Dehydration and volatilization non isothermic kinetic of the solid state aluminium 8-hydroxyquinolinate

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

A steady-state model for heat pipes of circular or rectangular cross-sections

The objective of this paper is to present a generalized analytical-numerical model of the internal flow in heat pipes. The model formulation is based on two-dimensional formulation of the energy and momentum equations in the vapour and liquid regions and also in the metallic tube. The numerical solution of the model is obtained by using the descretization scheme LOAD and the SIMPLE numerical code. The flow fields, as well as the pressure fields, for different geometries were obtained and discussed. Copyright © 1996 Elsevier Science Ltd.