Dissertations / Theses on the topic 'Instability'
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Trouvé, Arnaud. "Instabilités hydrodynamiques et instabilités de combustion de flammes turbulentes prémélangées." Châtenay-Malabry, Ecole centrale de Paris, 1989. http://www.theses.fr/1989ECAP0097.
Full textGryfe, Robert. "Colorectal cancer microsatellite instability." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/NQ59033.pdf.
Full textStrefford, Jon C. "P53 and chromosome instability." Thesis, Swansea University, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.639125.
Full textForeman, S. J. "Baroclinic instability and blocking." Thesis, University of Reading, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.354071.
Full textWood, R. A. "Instability of oceanic fronts." Thesis, University of Exeter, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.381309.
Full textWilliamson, David. "Haemoglobin mutation and instability." Thesis, Open University, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.315297.
Full textJomah, Adel M. "Instability in switching systems." Thesis, University of Bristol, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.322593.
Full textBUFFONI, SALETE SOUZA DE OLIVEIRA. "PARAMETRIC INSTABILITY OF COLUMNS." PONTIFÍCIA UNIVERSIDADE CATÓLICA DO RIO DE JANEIRO, 1998. http://www.maxwell.vrac.puc-rio.br/Busca_etds.php?strSecao=resultado&nrSeq=2132@1.
Full textUNIVERSIDADE FEDERAL DO PARÁ
O presente trabalho tem por objetivo desenvolver uma formulação e certas estratégias que permitam a análise da perda de estabilidade de colunas esbeltas submetidas a carregamento axial periódico, fenômeno este conhecido como ressonância paramétrica. Uma excitação é dita paramétrica quando aparece nas equações de movimento do sistema na forma de coeficientes variáveis com o tempo - geralmente periódicos - e não como uma não homogeneidade. A coluna é descrita pela formulação clássica de Navier. O presente trabalho trata a coluna considerando-se um e três graus de liberdade com ou sem não-linearidades. As equações de movimento são obtidas utilizando-se o princípio de Hamilton através do método de Ritz. A equação linear (equação de Mathieu) e a equação de Duffing com pequeno amortecimento, são resolvidas de forma aproximada pelo método das múltiplas escalas, revelando a possibilidade de instabilização da posição de equilíbrio em diversas regiões do espaço definido pelos parâmetros de controle. A mesma conclusão é mostrada utilizando-se procedimentos computacionais para a resolução dos sistemas de equações lineares e nãolineares, com ou sem imperfeição geométrica inicial, podendo-se obter assim, a resposta do sistema, planos fase, seções de Poincaré e diagramas de bifurcação. Mostra-se a partir dos resultados numéricos, que a coluna submetida a cargas axiais harmônicas, pode tanto apresentar soluções com o mesmo período da força excitadora, quanto oscilações subarmônicas e superarmônicas de diversas ordens, além de movimentos caóticos.
The main aim of the present work is to develop a formulation and some strategies for the instability analysis of slender columns under an axial harmonic force this phenomenon is known as parametric ressonance. An excitation is said to be parametric if it appears as timedependent - often periodic - coefficients in the equations governing the motion of the system,and not as an inhomogeneous term.The column is described by Navier classical formulation. The present work consider the column with one or three degrees of freedom with or without nonlinearities. The equations governing the motion are obtained by the Ritz method.The linear equation (Mathieu equation) and the Duffing equation with small damping are solved in an approximate way using multiple scales techniques, revealing the possibility of destabilizing the static equilibrium position in certain regions of the control space. A similar conclusion is obtained by employing numerical methods for the solution of linear and nonlinear equation systems with or without initial geometrical imperfections.This enables one to obtain time response, phase space, projections Poincaré sections and bifurcation diagrams. These numerical results show that the column with nonlinearities and loaded by a periodic longitudinal force can present various solutions with the same period as the forcing and subharmonic e superharmonic oscillations, as well as chaotic motions.
Hou, Hang-sheng. "Cavitation instability in solids." Thesis, Massachusetts Institute of Technology, 1990. http://hdl.handle.net/1721.1/13697.
Full textMiller, Ronald Lindsay. "Topics in shear instability." Thesis, Massachusetts Institute of Technology, 1990. http://hdl.handle.net/1721.1/54962.
Full textIncludes bibliographical references.
by Ronald Lindsay Miller.
Viscous destabilization of stratified shear flow -- Organization of rainfall by an unstable jet aloft.
Ph.D.
Andreoni, Federica. "SSB and genetic instability." Thesis, University of Edinburgh, 2009. http://hdl.handle.net/1842/3993.
Full textLai, Chi-hsuan. "Neutrino electron plasma instability /." Digital version accessible at:, 1999. http://wwwlib.umi.com/cr/utexas/main.
Full textPieri, Alexandre. "Turbulence barocline : effets couplés de rotation, stratification et cisaillement." Phd thesis, Ecole Centrale de Lyon, 2012. http://tel.archives-ouvertes.fr/tel-00781602.
Full textWang, Chen. "Novel software tool for microsatellite instability classification and landscape of microsatellite instability in osteosarcoma." Miami University / OhioLINK, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=miami1554829925088174.
Full textSchaefer, Rodrigo Gonçalves. "Global instability in Hamiltonian systems." Doctoral thesis, Universitat Politècnica de Catalunya, 2018. http://hdl.handle.net/10803/620741.
Full textAls Capítols 1 i 2 d'aquesta tesi es prova que per a una pertorbació no trivial depenent de dos harmònics qualsevol d'un pèndol i un rotor, hi ha inestabilitat global. La demostració es basa en el mètode geomètric i s'ha elaborat a través de computació concreta de diversos scattering maps. Es realitza una descripció completa dels diferents tipus de scattering map. La demostració del sistema general es divideix en dos casos. El primer és estudiat al Capítol 1, on es presenta una demostració per la funció de pertorbació més simple. A més a més, s'han observat algunes òrbites de difusió molt especials, anomenades "highways", i s'ha pogut fer estimacions sobre el temps de difusió d'aquestes òrbites. El segon cas és tractat al Capítol 2, en el que es completa la demostració de l'existència de difusió. Al Capítol 2, també s'estableix l'existència de "piecewise smooth global scattering maps". Al Capítol 3, es considera un Hamiltonià similar amb 3 graus de llibertat. S'ha provat la difusió utilitzant una combinació d'scattering maps i dinàmica interna amb camins de difusió concrets. Finalment, es comparen els resultats obtinguts en aquest cas amb els obtinguts al Capítol 1. Per a acabar, es comenten alguns problemes pertanyents a l'àmbit de la tesi, que seria interessant estudiar en futurs treballs
Kreider, Rose M. "Interracial marriage and marital instability." Click to view the dissertation via Digital dissertation consortium, 1999.
Find full textRoss, Julius. "Instability of polarised algebraic varieties." Thesis, Imperial College London, 2006. http://hdl.handle.net/10044/1/1250.
Full textKim, Han Soo. "Aerodynamic instability of inclined cables." Thesis, University of Ottawa (Canada), 2001. http://hdl.handle.net/10393/8976.
Full textMurray, John. "Instability in the human genome." Thesis, University of Leicester, 1998. http://hdl.handle.net/2381/30309.
Full textColeman, Mark Giles. "Genomic instability in colorectal carcinoma." Thesis, University of Leicester, 2001. http://hdl.handle.net/2381/29371.
Full textSalmeron, Raquel. "Magnetorotational Instability in Protostellar Discs." Physics, 2005. http://hdl.handle.net/2123/919.
Full textWe investigate the linear growth and vertical structure of the magnetorotational instability (MRI) in weakly ionised, stratified accretion discs. The magnetic field is initially vertical and perturbations have vertical wavevectors only. Solutions are obtained at representative radial locations from the central protostar for different choices of the initial magnetic field strength, sources of ionisation, disc structure and configuration of the conductivity tensor. The MRI is active over a wide range of magnetic field strengths and fluid conditions in low conductivity discs. For the minimum-mass solar nebula model, incorporating cosmic ray and x-ray ionisation and assuming that charges are carried by ions and electrons only, perturbations grow at 1 AU for B < 8G. For a significant subset of these strengths (200mG < B < 5 G), the growth rate is of order the ideal MHD rate (0.75 Omega). Hall conductivity modifies the structure and growth rate of global unstable modes at 1 AU for all magnetic field strengths that support MRI. As a result, at this radius, modes obtained with a full conductivity tensor grow faster and are active over a more extended cross-section of the disc, than perturbations in the ambipolar diffusion limit. For relatively strong fields (e.g. B > 200 mG), ambipolar diffusion alters the envelope shapes of the unstable modes, which peak at an intermediate height, instead of being mostly flat as modes in the Hall limit are in this region of parameter space. Similarly, when cosmic rays are assumed to be excluded from the disc by the winds emitted by the magnetically active protostar, unstable modes grow at this radius for B < 2 G. For strong fields, perturbations exhibit a kink at the height where x-ray ionisation becomes active. Finally, for R = 5 AU (10 AU), unstable modes exist for B < 800 mG (B < 250 mG) and the maximum growth rate is close to the ideal-MHD rate for 20 mG < B < 500 mG (2 mG < B < 50 mG). Similarly, perturbations incorporating Hall conductivity have a higher wavenumber and grow faster than solutions in the ambipolar diffusion limit for B < 100 mG (B < 10 mG). Unstable modes grow even at the midplane for B > 100 mG (B ~ 1 mG), but for weaker fields, a small dead region exists. When a population of 0.1 um grains is assumed to be present, perturbations grow at 10 AU for B < 10 mG. We estimate that the figure for R = 1 AU would be of order 400 mG. We conclude that, despite the low magnetic coupling, the magnetic field is dynamically important for a large range of fluid conditions and field strengths in protostellar discs. An example of such magnetic activity is the generation of MRI unstable modes, which are supported at 1 AU for field strengths up to a few gauss. Hall diffusion largely determines the structure and growth rate of these perturbations for all studied radii. At radii of order 1 AU, in particular, it is crucial to incorporate the full conductivity tensor in the analysis of this instability, and more generally, in studies of the dynamics of astrophysical discs.
Rebentisch, Eric. "Preliminary Observations on Program Instability." Massachusetts Institute of Technology, 1996. http://hdl.handle.net/1721.1/7331.
Full textValkhoff, Nienke Jeltje Marjoke. "Stabilization by competing instability mechanisms." [S.l. : Amsterdam : s.n.] ; Universiteit van Amsterdam [Host], 2006. http://dare.uva.nl/document/37776.
Full textBrown, Cathleen N. Guskiewicz Kevin M. "Factors contributing to ankle instability." Chapel Hill, N.C. : University of North Carolina at Chapel Hill, 2006. http://dc.lib.unc.edu/u?/etd,272.
Full textTitle from electronic title page (viewed Oct. 10, 2007). "... in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Interdisciplinary Human Movement Science (School of Medicine)." Discipline: Human Movement Science; Department/School: Medicine.
Spotton, Brenda L. (Brenda Lynn). "A study of financial instability." Thesis, McGill University, 1993. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=41138.
Full textMitmaker, Elliot. "Microsatellite instability in thyroid neoplasia." Thesis, McGill University, 2007. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=101730.
Full textUsing laser capture microdissection, cells from both normal and tumor tissue were individually collected. PCR amplification of the DNA was then performed using six dinucleotide and two mononucleotide microsatellite markers.
Forty benign and malignant thyroid tumors were compared with their adjacent normal thyroid follicular tissue and were analyzed for MSI. 9/14 papillary thyroid carcinomas and 10/16 of follicular thyroid carcinomas demonstrated MSI at >30--40% of loci tested. For benign follicular adenomas, 9/10 demonstrated microsatellite stability or low-frequency MSI.
Microsatellite instability appears to play a role in thyroid pathogenesis as evidenced by the high frequency of MSI in malignant thyroid neoplasms. In addition our study showed a significant difference in MSI frequency between follicular adenomas and follicular carcinomas. More importantly, the technique of laser capture microdissection allows for more accurate selection of benign, malignant and normal DNA.
Gregory, Michael Peter Robert. "Farm income inequality and instability." Thesis, Imperial College London, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338982.
Full textKandil, Mohamed Abdelhadi. "On rotor internal damping instability." Thesis, Imperial College London, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.421790.
Full textSethia, Krishna Kumar. "The pathophysiology of detrusor instability." Thesis, University of Oxford, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.235958.
Full textErwin, Patrick Seumas. "Palaeomagnetic investigations of volcano instability." Thesis, University of Oxford, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.249474.
Full textBhattacharya, S. "Pile instability during earthquake liquefaction." Thesis, University of Cambridge, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.596628.
Full textNguyen, Giang Huong. "Cancer, aging and genome instability." Thesis, University of Oxford, 2013. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.600238.
Full textGore, Whitney L. "AFFECTIVE INSTABILITY ACROSS DIAGNOSTIC MODELS." UKnowledge, 2015. http://uknowledge.uky.edu/psychology_etds/76.
Full textDixon, Richard Stuart. "Diagnostic studies of symmetric instability." Thesis, University of Reading, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.270255.
Full textElliott, Simon S. "Numerical studies of baroclinic instability." Thesis, University of Oxford, 1995. http://ora.ox.ac.uk/objects/uuid:eb0c26fe-b0f0-4f2b-aa3b-00428cdd2a57.
Full textGrimshaw, P. N. "Quantitative assessment of knee instability." Thesis, University of Salford, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.234593.
Full textLucey, Anthony Denis. "Hydroelastic instability of flexible surfaces." Thesis, University of Exeter, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.235966.
Full textKhumbah, Fidelis Morfaw. "Instability of three-dimensional frameworks." Thesis, University of Southampton, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.315305.
Full textGajo, Alessandro. "Instability phenomena in sand samples." Thesis, University of Bristol, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.399938.
Full textAndriotis, Andreas. "Fracture instability in nuclear graphite." Thesis, University of Bristol, 2018. http://hdl.handle.net/1983/8f4c72b9-6a8a-4c69-8ded-5425f847a148.
Full textWu, Xuesong. "Nonlinear instability of Stokes-layers." Thesis, Imperial College London, 1992. http://hdl.handle.net/10044/1/59202.
Full textDodgson, Emily. "Thermoconvective instability in porous media." Thesis, University of Bath, 2011. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.547618.
Full textAkl, Sherif Adel. "Wellbore instability mechanisms in clays." Thesis, Massachusetts Institute of Technology, 2010. http://hdl.handle.net/1721.1/64569.
Full text"February 2011." Cataloged from PDF version of thesis.
Includes bibliographical references (p. 331-341).
This dissertation investigates the stability of wellbores drilled in Ko-consolidated clays using non-linear finite element method (FEM) and effective stress soil models to characterize the behavior of clay and unconsolidated shale formations. Two constitutive models are used: Modified Cam Clay (MCC; Roscoe and Burland, 1968), and MIT-E3 (Whittle and Kavvadas, 1994). These soil models are incorporated in the commercial finite element program ABAQUS TM through user material subroutines (Hashash, 1992). The wellbores are modeled by a quasi-3D finite element model to approximate the far field stresses and plane strain boundary conditions. The constitutive models are calibrated to the behavior of Resedimented Boston Blue Clay (RBBC), an analog shale material which is Ko-consolidated to stress levels ranging from 0.15MPa to 10.0 MPa. The thesis comprises three major parts. Part one analyzes the short-term wellbore instability during drilling in low permeability formations. The part focuses on the relationship between the mud pressure inside the wellbore and the undrained shear deformations within the formations. The analyses predict critical mud pressure values necessary to maintain wellbore stability at different deviation angles and stress histories. The MIT-E3 model predicted higher deformations at reference mud pressure and estimated higher values of mud pressures than the underbalanced limit to prevent failure in highly deviated wellbores in NC clays. The second part validates the numerical analyses by comparing model predictions to results of an extensive program of model borehole tests. The lab experiments are performed on high pressure Thick- Walled Cylinder (TWC devices) using RBBC as analog testing material (Abdulhadi, 2009). The MIT-E3 predictions demonstrated a very good match with results from the experiments. The results from the analyses illustrated the effect of the device boundary conditions on specimen behavior and validated approximate analytical methods for interpreting TWC results. Part three studies the effects of consolidation on long-term wellbore stability. Non-linear coupled consolidation analyses are performed to simulate the post-drilling, time-dependent deformations and pore pressures around the wellbore. The analyses consider two different boundary conditions on seepage at the cavity. The analyses show that consolidation generates extensive volumetric strains around the wellbore and cavity deformations can aggravate stability conditions in highly deviated wellbores.
by Sherif Adel Akl.
Ph.D.
Tivey, Hannah S. E. "Physiological responses to genomic instability." Thesis, Cardiff University, 2010. http://orca.cf.ac.uk/54394/.
Full textBlakey, Caroline. "Anterior instability of the hip." Thesis, St George's, University of London, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.676894.
Full textTajik, Mohammad. "Banking instability : causes and remedies." Thesis, Brunel University, 2015. http://bura.brunel.ac.uk/handle/2438/10667.
Full textKordesch, Wendy E. C. "Middle Eocene greenhouse climate instability." Thesis, University of Southampton, 2016. https://eprints.soton.ac.uk/402327/.
Full textGadgil, Rujuta Yashodhan. "Instability at Trinucleotide Repeat DNAs." Wright State University / OhioLINK, 2016. http://rave.ohiolink.edu/etdc/view?acc_num=wright1472231204.
Full textSantos, Tapia Celia. "Understanding chromosomal instability-induced senescence." Doctoral thesis, Universitat de Barcelona, 2019. http://hdl.handle.net/10803/671915.
Full textLa aneuploidía, que se define como un número de cromosomas diferente al haploide, es una característica muy común en cáncer ya que se encuentra en alrededor de 68% de los tumores sólidos. Esta resulta en un desequilibrio metabólico que compromete la función celular induciendo estrés proteotóxico y afectando el crecimiento celular, dando lugar a así a una transformación maligna de estas células. Sin embargo, muchos de los mecanismos moleculares detrás de esta transformación generada por la aneuploidía son aún desconocidos. En este trabajo, usamos el epitelio del ala de Drosophila como tejido modelo para demostrar la contribución de la aneuploidía al crecimiento tumoral. Mediante la inhibición de genes del checkpoint del huso mitótico, inducimos inestabilidad cromosómica y aneuploidía que, tras bloquear la muerte celular, da lugar a un sobrecrecimiento tumoral. Cuando las células no tienen aún altos niveles de aneuploidía, activan bajos niveles de la quinasa c-Jun N-terminal (JNK) y activan la respuesta a daño en el DNA (DDR). Esto induce un arresto temporal en G1 que previene la acumulación de más daño. Sin embargo, debido a la inestabilidad cromosómica, estas células continúan proliferando y acumulan altos niveles de aneuploidía, delaminan del epitelio y adquieren un comportamiento senescente. Este depende de la activación de altos niveles de JNK y la DDR y tiene como consecuencia la secreción de distintos factores (SASP) y un arresto permanente en G2, entre otras características senescentes. Además, hemos podido identificar dos factores involucrados en el arresto, Tribbles and String, que podrían actuar en respuesta a JNK y a la DDR para hacer efectivo el arresto en G2. Finalmente, exploramos dos maneras distintas de afectar los tumores CIN aprovechando que sufren daño en el DNA: genéticamente (mediante la sobre-expresión de CycE/Dap) y químicamente (mediante el tratamiento con hidroxiurea), afectando ambas el crecimiento del tejido e inhibiendo la progresión tumoral.
Ismael, Mohanad. "Market imperfections and macroeconomic instability." Thesis, Evry-Val d'Essonne, 2011. http://www.theses.fr/2011EVRY0011/document.
Full textIn this thesis, we study the effect of market imperfection on macroeconomic stability in the standard Ramsey model and that of the Olg. In order to achieve this objective, we use the local analysis method pioneered by Grandmont, Pintus and De Vilder (1998). The imperfections used in this thesis are the consumption externalities, credit market imperfections, progressive labor-income taxation policy and the presence of transaction costs associated with capital accumulations