The document discusses Floquet theory applied to analyze the stability of internal gravity waves in a density-stratified fluid. It summarizes previous approaches to studying gravity wave instability, and outlines the author's thesis goal of using Floquet-Fourier computation to identify all physically unstable modes. This involves analyzing the Floquet exponents as a Riemann surface with complex wavenumber, to distinguish the two primary sheets corresponding to the physically relevant unstable solutions.
I. Antoniadis - "Introduction to Supersymmetry" 2/2SEENET-MTP
1) The Supersymmetric Standard Model (SSM) extends the particle content of the Standard Model by introducing supersymmetric partners for each particle, called sparticles. This includes gluinos, winos, binos, squarks, sleptons, and higgsinos as sparticle counterparts to gluons, W/Z bosons, photons, quarks, leptons, and Higgs bosons.
2) The SSM Lagrangian contains additional terms beyond the Standard Model including gauge interactions between fermions and gauginos, quartic scalar interactions, and a superpotential with Yukawa-like couplings.
3) Spontaneous supersymmetry breaking is required to make sparticles heavy enough to have evaded detection
I. Antoniadis - "Introduction to Supersymmetry" 1/2SEENET-MTP
Supersymmetry (SUSY) is a symmetry that relates bosonic and fermionic degrees of freedom. It extends the Poincaré algebra by including spinorial generators (supercharges) that transform bosonic fields into fermionic fields and vice versa. SUSY provides motivations like natural elementary scalars, gauge coupling unification, and a dark matter candidate. SUSY is formulated using superspace, which extends spacetime by Grassmann coordinates. Chiral and vector superfields contain the bosonic and fermionic components of supermultiplets and allow constructing SUSY invariant actions.
El 7 de noviembre de 2016, la Fundación Ramón Areces organizó el Simposio Internacional 'Solitón: un concepto con extraordinaria diversidad de aplicaciones inter, trans, y multidisciplinares. Desde el mundo macroscópico al nanoscópico'.
This document discusses the path integral formulation of quantum mechanics and its application to relativistic theories like general relativity. It introduces causal dynamical triangulations as an approach to quantizing gravity by defining a path integral over causal triangulations of spacetime geometries. This allows imposing global hyperbolicity and causality constraints to avoid issues like wormholes and baby universes. The approach aims to make quantum gravity computations possible using desktop computers by dynamically triangulating Lorentzian spacetimes.
Describes the mathematics of the Calculus of Variations.
For comments please contact me at solo.hermelin@gmail.com.
For more presentations on different subjects visit my website on http://www.solohermelin.com
Solution manual for introduction to nonlinear finite element analysis nam-h...Salehkhanovic
Solution Manual for Introduction to Nonlinear Finite Element Analysis
Author(s) : Nam-Ho Kim
This solution manual include all problems (Chapters 1 to 5) of textbook. There is one PDF for each of chapters.
Hello, I am Subhajit Pramanick. I and my friend, Sougata Dandapathak, both presented this ppt in our college seminar. It is basically based on the origin of calculus of variation. It consists of several topics like the history of it, the origin of it, who developed it, application of it, advantages and disadvantages etc. The main aim of this presentation is to increase our mathematical as well as physical conception on advanced classical mechanics. We hope you will all enjoy by reading this presentation. Thank you.
Solution of Fractional Order Stokes´ First EquationIJRES Journal
Fractional sine transform and Laplace transform are used for solving the Stokes` first problem with
ractional derivative, where the fractional derivative is defined in the Caputo sense of orderm1 m.
The solution of classical problem for Stokes` first problem has been obtained as limiting case.
I. Antoniadis - "Introduction to Supersymmetry" 2/2SEENET-MTP
1) The Supersymmetric Standard Model (SSM) extends the particle content of the Standard Model by introducing supersymmetric partners for each particle, called sparticles. This includes gluinos, winos, binos, squarks, sleptons, and higgsinos as sparticle counterparts to gluons, W/Z bosons, photons, quarks, leptons, and Higgs bosons.
2) The SSM Lagrangian contains additional terms beyond the Standard Model including gauge interactions between fermions and gauginos, quartic scalar interactions, and a superpotential with Yukawa-like couplings.
3) Spontaneous supersymmetry breaking is required to make sparticles heavy enough to have evaded detection
I. Antoniadis - "Introduction to Supersymmetry" 1/2SEENET-MTP
Supersymmetry (SUSY) is a symmetry that relates bosonic and fermionic degrees of freedom. It extends the Poincaré algebra by including spinorial generators (supercharges) that transform bosonic fields into fermionic fields and vice versa. SUSY provides motivations like natural elementary scalars, gauge coupling unification, and a dark matter candidate. SUSY is formulated using superspace, which extends spacetime by Grassmann coordinates. Chiral and vector superfields contain the bosonic and fermionic components of supermultiplets and allow constructing SUSY invariant actions.
El 7 de noviembre de 2016, la Fundación Ramón Areces organizó el Simposio Internacional 'Solitón: un concepto con extraordinaria diversidad de aplicaciones inter, trans, y multidisciplinares. Desde el mundo macroscópico al nanoscópico'.
This document discusses the path integral formulation of quantum mechanics and its application to relativistic theories like general relativity. It introduces causal dynamical triangulations as an approach to quantizing gravity by defining a path integral over causal triangulations of spacetime geometries. This allows imposing global hyperbolicity and causality constraints to avoid issues like wormholes and baby universes. The approach aims to make quantum gravity computations possible using desktop computers by dynamically triangulating Lorentzian spacetimes.
Describes the mathematics of the Calculus of Variations.
For comments please contact me at solo.hermelin@gmail.com.
For more presentations on different subjects visit my website on http://www.solohermelin.com
Solution manual for introduction to nonlinear finite element analysis nam-h...Salehkhanovic
Solution Manual for Introduction to Nonlinear Finite Element Analysis
Author(s) : Nam-Ho Kim
This solution manual include all problems (Chapters 1 to 5) of textbook. There is one PDF for each of chapters.
Hello, I am Subhajit Pramanick. I and my friend, Sougata Dandapathak, both presented this ppt in our college seminar. It is basically based on the origin of calculus of variation. It consists of several topics like the history of it, the origin of it, who developed it, application of it, advantages and disadvantages etc. The main aim of this presentation is to increase our mathematical as well as physical conception on advanced classical mechanics. We hope you will all enjoy by reading this presentation. Thank you.
Solution of Fractional Order Stokes´ First EquationIJRES Journal
Fractional sine transform and Laplace transform are used for solving the Stokes` first problem with
ractional derivative, where the fractional derivative is defined in the Caputo sense of orderm1 m.
The solution of classical problem for Stokes` first problem has been obtained as limiting case.
The one-dimensional heat equation describes heat flow along a rod. It can be solved using separation of variables. For a rod with insulated sides initially at uniform temperature u0 and ends suddenly cooled to 0°C:
1) The solution is a Fourier series involving eigenfunctions that satisfy the boundary conditions.
2) The temperature is the sum of the eigenfunctions weighted by Fourier coefficients involving u0.
3) As time increases, the temperature decreases towards the boundary values according to exponential decay governed by the eigenvalues.
Rotation in 3d Space: Euler Angles, Quaternions, Marix DescriptionsSolo Hermelin
Mathematics of rotation in 3d space, a lecture that I've prepared.
This presentation is at a Undergraduate in Science (Math, Physics, Engineering) level.
Please send comments and suggestions to solo.hermelin@gmail.com. Thanks!
Fore more presentations, please visit my website at
http://www.solohermelin.com/
The document summarizes the solution process for determining the deflection, bending moment, and stress of a simply supported beam subjected to an external forcing function. Natural frequencies are calculated as ωn = n^2π^2/L^2(EI/ρA). Mode shapes are sinusoidal functions of nπx/L. Forced response is determined using mode superposition, yielding a deflection proportional to sin(Ωt) and sin(ω1t) with spatial dependence of sin(πx/L). Bending moment and stress are derived from deflection and have the same functional forms.
Non-Hermitian noncommutative models in quantum optics and their superioritiesSanjib Dey
This document discusses non-Hermitian noncommutative models in quantum optics and their advantages over traditional models. Key points include:
- Noncommutative spaces violate Lorentz-Poincaré symmetry but Snyder's version deforms the symmetries to make the algebra compatible.
- Deformed oscillator algebras lead to q-deformed noncommutative spaces with a minimal length scale.
- Noncommutative coherent states exhibit both classical and nonclassical behavior such as squeezing and entanglement.
- The models provide an extra degree of freedom for squeezing and nonclassicality compared to ordinary systems.
Calculus of variations & solution manual russakJosé Pallo
This document discusses finding minima or maxima of functions of multiple variables. It presents necessary conditions for a point to be an unconstrained relative minimum of such a function: the first partial derivatives must be zero at that point, and the Hessian matrix must be positive semidefinite. These conditions come from applying the single-variable optimization conditions to variations of the function in different directions. The document also notes that satisfying these necessary conditions is sufficient for a relative minimum. Overall, the document outlines the basic theory and necessary/sufficient conditions for optimizing functions of multiple variables without constraints.
Differential geometry three dimensional spaceSolo Hermelin
This presentation describes the mathematics of curves and surfaces in a 3 dimensional (Euclidean) space.
The presentation is at an Undergraduate in Science (Math, Physics, Engineering) level.
Plee send comments and suggestions to improvements to solo.hermelin@gmail.com. Thanks/
More presentations can be found at my website http://www.solohermelin.com.
This document presents an overview of classical Feynman graphs for the Higgs boson. It expands the classical Higgs boson solution perturbatively up to third order in the coupling constant. In the 0th order of this expansion, the first few classical Feynman graphs are constructed. Specifically, it describes how there are five classical graphs looking at terms in the equations of motion involving the W and Z fields coupled to the 0th order Higgs field. It then provides an example of writing one such solution in coordinate space and transforming it to momentum space, depicting the vertex and propagator that would represent it.
This document discusses techniques for calculating electric potential, including:
1. Laplace's equation and its solutions in 1D, 2D, and 3D, including boundary conditions.
2. The method of images, which uses fictitious "image" charges to solve problems involving conductors. The classical image problem and induced surface charge on a conductor are examined.
3. Other techniques like multipole expansion, separation of variables, and numerical methods like relaxation are mentioned but not explained in detail.
This document discusses Fourier series and integrals. It begins by explaining Fourier series using sines, cosines, and exponentials to represent periodic functions. Square waves are given as examples that can be expressed as infinite combinations of sines. Any periodic function can be expressed as a Fourier series. Fourier series are then derived for specific examples, including a square wave, repeating ramp, and up-down train of delta functions. Cosine series are also discussed. The document concludes by deriving the Fourier series for the delta function.
This presentation is intended for undergraduate students in physics and engineering.
Please send comments to solo.hermelin@gmail.com.
For more presentations on different subjects please visit my homepage at http://www.solohermelin.com.
This presentation is in the Physics folder.
This presentation gives example of "Calculus of Variations" problems that can be solved analytical. "Calculus of Variations" presentation is prerequisite to this one.
For comments please contact me at solo.hermelin@gmail.com.
For more presentations on different subjects visit my website at http://www.solohermelin.com.
The Euler-Mascheroni constant is calculated by three novel representations over these sets respectively: 1) Turán moments, 2) coefficients of Jensen polynomials for the Taylor series of the Riemann Xi function at s = 1/2 + i.t and 3) even coefficients of the Riemann Xi function around s = 1/2.
Presentation of the work on Prime Numbers.
intended for mathematics loving people.
Please send comments and suggestions for improvement to solo.hermelin@gmail.com.
More presentations can be found in my website at http://solohermelin.com.
This document provides an overview of calculus of variations, which generalizes the method of finding extrema of functions to functionals. It discusses how functionals take on extreme values when their path or curve satisfies certain necessary conditions, analogous to single-variable calculus. These necessary conditions are derived by applying the calculus of variations methodology to functionals dependent on a path and finding the Euler-Lagrange equation. Several examples from physics are described where extremizing a functional corresponds to minimizing time, length, or other physical quantities.
Describes the simulation model of the backlash effect in gear mechanisms. For undergraduate students in engineering. In the download process a lot of figures are missing.
I recommend to visit my website in the Simulation Folder for a better view of this presentation.
Please send comments to solo.hermelin@gmail.com.
For more presentations on different subjects visit my website at http://www.solohermelin.com.
The one-dimensional wave equation governs vibrations of an elastic string. It is solved by separating variables, yielding solutions of the form F(x)G(t) where F and G satisfy ordinary differential equations. Boundary conditions require F(x) to be sinusoidal, with wavelengths that are integer multiples of the string length. The general solution is a superposition of these sinusoidal modes, with coefficients determined by the initial conditions. Motions of strings with different initial displacements are expressed as solutions to the one-dimensional wave equation.
This document discusses the stress function approach for solving two-dimensional elasticity problems. It begins by presenting the general equations of elasticity, including stress-strain relationships, strain-displacement equations, and equilibrium equations. It then introduces the stress function method proposed by Airy, where a single function of space coordinates is assumed that satisfies all the elasticity equations. The key steps are: (1) choosing a stress function, (2) confirming it is biharmonic, (3) deriving stresses from its derivatives, (4) using boundary conditions to determine the function, (5) deriving strains, and (6) displacements. Examples of polynomial stress functions are also provided.
This document summarizes a paper that considers the Klein-Gordon scalar field in a two-dimensional Rindler spacetime. It writes a two-dimensional action for the Klein-Gordon scalar in this background and obtains the equation of motion. The equation of motion can be solved exactly in imaginary time, with the solution taking an oscillatory form with a frequency equal to an integer number.
First part of description of Matrix Calculus at Undergraduate in Science (Math, Physics, Engineering) level.
Please send comments and suggestions to solo.hermelin@gmail.com.
For more presentations please visit my website at
http://www.solohermelin.com.
Second-order Cosmological Perturbations Engendered by Point-like MassesMaxim Eingorn
R. Brilenkov and M. Eingorn, Second-order cosmological perturbations engendered by point-like masses, ApJ 845 (2017) 153: http://iopscience.iop.org/article/10.3847/1538-4357/aa81cd
In the ΛCDM framework, presenting nonrelativistic matter inhomogeneities as discrete massive particles, we develop the second‐order cosmological perturbation theory. Our approach relies on the weak gravitational field limit. The derived equations for the second‐order scalar, vector, and tensor metric corrections are suitable at arbitrary distances, including regions with nonlinear contrasts of the matter density. We thoroughly verify fulfillment of all Einstein equations, as well as self‐consistency of order assignments. In addition, we achieve logical positive results in the Minkowski background limit. Feasible investigations of the cosmological backreaction manifestations by means of relativistic simulations are also outlined.
The slides are designed for my guided study in MSc CUHK.
It is about the brief description on classical mechanics and quantum mechanics .
Some Slides I got from the slideshare clipboards for better illustration of the ideas in Physics. Thanks to slideshare, I make a milestone on presenting one of the prominent fields in modern physics.
All of material inside is un-licence, kindly use it for educational only but please do not to commercialize it.
Based on 'ilman nafi'an, hopefully this file beneficially for you.
Thank you.
The one-dimensional heat equation describes heat flow along a rod. It can be solved using separation of variables. For a rod with insulated sides initially at uniform temperature u0 and ends suddenly cooled to 0°C:
1) The solution is a Fourier series involving eigenfunctions that satisfy the boundary conditions.
2) The temperature is the sum of the eigenfunctions weighted by Fourier coefficients involving u0.
3) As time increases, the temperature decreases towards the boundary values according to exponential decay governed by the eigenvalues.
Rotation in 3d Space: Euler Angles, Quaternions, Marix DescriptionsSolo Hermelin
Mathematics of rotation in 3d space, a lecture that I've prepared.
This presentation is at a Undergraduate in Science (Math, Physics, Engineering) level.
Please send comments and suggestions to solo.hermelin@gmail.com. Thanks!
Fore more presentations, please visit my website at
http://www.solohermelin.com/
The document summarizes the solution process for determining the deflection, bending moment, and stress of a simply supported beam subjected to an external forcing function. Natural frequencies are calculated as ωn = n^2π^2/L^2(EI/ρA). Mode shapes are sinusoidal functions of nπx/L. Forced response is determined using mode superposition, yielding a deflection proportional to sin(Ωt) and sin(ω1t) with spatial dependence of sin(πx/L). Bending moment and stress are derived from deflection and have the same functional forms.
Non-Hermitian noncommutative models in quantum optics and their superioritiesSanjib Dey
This document discusses non-Hermitian noncommutative models in quantum optics and their advantages over traditional models. Key points include:
- Noncommutative spaces violate Lorentz-Poincaré symmetry but Snyder's version deforms the symmetries to make the algebra compatible.
- Deformed oscillator algebras lead to q-deformed noncommutative spaces with a minimal length scale.
- Noncommutative coherent states exhibit both classical and nonclassical behavior such as squeezing and entanglement.
- The models provide an extra degree of freedom for squeezing and nonclassicality compared to ordinary systems.
Calculus of variations & solution manual russakJosé Pallo
This document discusses finding minima or maxima of functions of multiple variables. It presents necessary conditions for a point to be an unconstrained relative minimum of such a function: the first partial derivatives must be zero at that point, and the Hessian matrix must be positive semidefinite. These conditions come from applying the single-variable optimization conditions to variations of the function in different directions. The document also notes that satisfying these necessary conditions is sufficient for a relative minimum. Overall, the document outlines the basic theory and necessary/sufficient conditions for optimizing functions of multiple variables without constraints.
Differential geometry three dimensional spaceSolo Hermelin
This presentation describes the mathematics of curves and surfaces in a 3 dimensional (Euclidean) space.
The presentation is at an Undergraduate in Science (Math, Physics, Engineering) level.
Plee send comments and suggestions to improvements to solo.hermelin@gmail.com. Thanks/
More presentations can be found at my website http://www.solohermelin.com.
This document presents an overview of classical Feynman graphs for the Higgs boson. It expands the classical Higgs boson solution perturbatively up to third order in the coupling constant. In the 0th order of this expansion, the first few classical Feynman graphs are constructed. Specifically, it describes how there are five classical graphs looking at terms in the equations of motion involving the W and Z fields coupled to the 0th order Higgs field. It then provides an example of writing one such solution in coordinate space and transforming it to momentum space, depicting the vertex and propagator that would represent it.
This document discusses techniques for calculating electric potential, including:
1. Laplace's equation and its solutions in 1D, 2D, and 3D, including boundary conditions.
2. The method of images, which uses fictitious "image" charges to solve problems involving conductors. The classical image problem and induced surface charge on a conductor are examined.
3. Other techniques like multipole expansion, separation of variables, and numerical methods like relaxation are mentioned but not explained in detail.
This document discusses Fourier series and integrals. It begins by explaining Fourier series using sines, cosines, and exponentials to represent periodic functions. Square waves are given as examples that can be expressed as infinite combinations of sines. Any periodic function can be expressed as a Fourier series. Fourier series are then derived for specific examples, including a square wave, repeating ramp, and up-down train of delta functions. Cosine series are also discussed. The document concludes by deriving the Fourier series for the delta function.
This presentation is intended for undergraduate students in physics and engineering.
Please send comments to solo.hermelin@gmail.com.
For more presentations on different subjects please visit my homepage at http://www.solohermelin.com.
This presentation is in the Physics folder.
This presentation gives example of "Calculus of Variations" problems that can be solved analytical. "Calculus of Variations" presentation is prerequisite to this one.
For comments please contact me at solo.hermelin@gmail.com.
For more presentations on different subjects visit my website at http://www.solohermelin.com.
The Euler-Mascheroni constant is calculated by three novel representations over these sets respectively: 1) Turán moments, 2) coefficients of Jensen polynomials for the Taylor series of the Riemann Xi function at s = 1/2 + i.t and 3) even coefficients of the Riemann Xi function around s = 1/2.
Presentation of the work on Prime Numbers.
intended for mathematics loving people.
Please send comments and suggestions for improvement to solo.hermelin@gmail.com.
More presentations can be found in my website at http://solohermelin.com.
This document provides an overview of calculus of variations, which generalizes the method of finding extrema of functions to functionals. It discusses how functionals take on extreme values when their path or curve satisfies certain necessary conditions, analogous to single-variable calculus. These necessary conditions are derived by applying the calculus of variations methodology to functionals dependent on a path and finding the Euler-Lagrange equation. Several examples from physics are described where extremizing a functional corresponds to minimizing time, length, or other physical quantities.
Describes the simulation model of the backlash effect in gear mechanisms. For undergraduate students in engineering. In the download process a lot of figures are missing.
I recommend to visit my website in the Simulation Folder for a better view of this presentation.
Please send comments to solo.hermelin@gmail.com.
For more presentations on different subjects visit my website at http://www.solohermelin.com.
The one-dimensional wave equation governs vibrations of an elastic string. It is solved by separating variables, yielding solutions of the form F(x)G(t) where F and G satisfy ordinary differential equations. Boundary conditions require F(x) to be sinusoidal, with wavelengths that are integer multiples of the string length. The general solution is a superposition of these sinusoidal modes, with coefficients determined by the initial conditions. Motions of strings with different initial displacements are expressed as solutions to the one-dimensional wave equation.
This document discusses the stress function approach for solving two-dimensional elasticity problems. It begins by presenting the general equations of elasticity, including stress-strain relationships, strain-displacement equations, and equilibrium equations. It then introduces the stress function method proposed by Airy, where a single function of space coordinates is assumed that satisfies all the elasticity equations. The key steps are: (1) choosing a stress function, (2) confirming it is biharmonic, (3) deriving stresses from its derivatives, (4) using boundary conditions to determine the function, (5) deriving strains, and (6) displacements. Examples of polynomial stress functions are also provided.
This document summarizes a paper that considers the Klein-Gordon scalar field in a two-dimensional Rindler spacetime. It writes a two-dimensional action for the Klein-Gordon scalar in this background and obtains the equation of motion. The equation of motion can be solved exactly in imaginary time, with the solution taking an oscillatory form with a frequency equal to an integer number.
First part of description of Matrix Calculus at Undergraduate in Science (Math, Physics, Engineering) level.
Please send comments and suggestions to solo.hermelin@gmail.com.
For more presentations please visit my website at
http://www.solohermelin.com.
Second-order Cosmological Perturbations Engendered by Point-like MassesMaxim Eingorn
R. Brilenkov and M. Eingorn, Second-order cosmological perturbations engendered by point-like masses, ApJ 845 (2017) 153: http://iopscience.iop.org/article/10.3847/1538-4357/aa81cd
In the ΛCDM framework, presenting nonrelativistic matter inhomogeneities as discrete massive particles, we develop the second‐order cosmological perturbation theory. Our approach relies on the weak gravitational field limit. The derived equations for the second‐order scalar, vector, and tensor metric corrections are suitable at arbitrary distances, including regions with nonlinear contrasts of the matter density. We thoroughly verify fulfillment of all Einstein equations, as well as self‐consistency of order assignments. In addition, we achieve logical positive results in the Minkowski background limit. Feasible investigations of the cosmological backreaction manifestations by means of relativistic simulations are also outlined.
The slides are designed for my guided study in MSc CUHK.
It is about the brief description on classical mechanics and quantum mechanics .
Some Slides I got from the slideshare clipboards for better illustration of the ideas in Physics. Thanks to slideshare, I make a milestone on presenting one of the prominent fields in modern physics.
All of material inside is un-licence, kindly use it for educational only but please do not to commercialize it.
Based on 'ilman nafi'an, hopefully this file beneficially for you.
Thank you.
This document summarizes key concepts about the particle in a rigid one-dimensional box:
1. It finds the energy eigenstates and discusses the wave functions and their properties like orthogonality.
2. It calculates the probability and expected values for the particle's position and discusses the physical interpretation of the wave function and coefficients when expanding an arbitrary function in the eigenstates.
3. It addresses several questions about normalized wave functions, time-dependent wave functions, energy measurements, and the wave function after a measurement.
Solution to schrodinger equation with dirac comb potential slides
This document summarizes solving the Schrödinger equation for a Dirac comb potential. The potential is an infinite series of Dirac delta functions spaced periodically. Floquet theory is used to solve the time-independent Schrödinger equation for this potential. Boundary conditions are applied and the resulting equations are solved graphically. Allowed energy bands are determined and plotted versus wave vector for both attractive and repulsive delta function potentials.
Optimal multi-configuration approximation of an N-fermion wave functionjiang-min zhang
We propose a simple iterative algorithm to construct the optimal multi-configuration approximation of an N-fermion wave function. That is, M≥N single-particle orbitals are sought iteratively so that the projection of the given wave function in the CNM-dimensional configuration subspace is maximized. The algorithm has a monotonic convergence property and can be easily parallelized. The significance of the algorithm on the study of entanglement in a multi-fermion system and its implication on the multi-configuration time-dependent Hartree-Fock (MCTDHF) are discussed. The ground state and real-time dynamics of spinless fermions with nearest-neighbor interactions are studied using this algorithm, discussing several subtleties.
dynamical analysis of soil and structuresHaHoangJR
1. The document discusses various topics in dynamics and vibrations including earthquake engineering, blast engineering, wind engineering, dynamic foundation design, pile driving, offshore foundations, geophysical methods, and dynamic design of transportation systems.
2. It introduces basic principles of dynamics and vibrations including Newton's laws of motion. It describes discrete systems with a finite number of degrees of freedom and continuous systems with infinite degrees of freedom.
3. The analysis of a single degree of freedom system is presented, including deriving the equation of motion and discussing free and forced vibration problems. Solutions are provided for different damping conditions.
This document provides an overview of Newton's laws of motion and Kepler's laws of planetary motion from a lecture on astrodynamics. It introduces Newton's two-body equations, conservation of linear momentum, the two-body equation of relative motion, and expressions of these equations in rectangular and polar coordinates. Kepler's laws of equal areas swept out in equal times and the harmony of the world (periods squared are proportional to semi-major axes cubed) are also summarized. Methods for determining orbital elements like the eccentricity vector and parameter are presented.
This document summarizes research on quantum chaos, including the principle of uniform semiclassical condensation of Wigner functions, spectral statistics in mixed systems, and dynamical localization of chaotic eigenstates. It discusses how in the semiclassical limit, Wigner functions condense uniformly on classical invariant components. For mixed systems, the spectrum can be seen as a superposition of regular and chaotic level sequences. Localization effects can be observed if the Heisenberg time is shorter than the classical diffusion time. The document presents an analytical formula called BRB that describes the transition between Poisson and random matrix statistics. An example is given of applying this to analyze the level spacing distribution for a billiard system.
1) The document discusses the problem of a particle sliding off a moving hemisphere, with the goal of finding the angle at which the particle's horizontal velocity is maximum.
2) Conservation of momentum and energy equations are used to derive an expression for the particle's horizontal velocity in terms of the angle, which reaches a maximum at a certain angle.
3) Setting the derivative of this expression to zero results in a cubic equation that determines the maximum angle, which can be solved numerically for different ratios of particle to hemisphere mass.
1) The document discusses the problem of a particle sliding off a moving hemisphere, using conservation of momentum and energy equations to derive an expression for the particle's horizontal velocity vx as a function of the angle θ.
2) Setting the derivative of vx equal to zero yields a cubic equation that determines the angle θ at which vx is maximized, corresponding to the particle losing contact with the hemisphere.
3) For the special case where the particle and hemisphere masses are equal (ratio r = 1), the cubic equation can be solved to find θ ≈ 42.9 degrees.
Additional Mathematics form 4 (formula)Fatini Adnan
This document provides a summary of various math formulae for Form 4 students in Malaysia, including:
1. Functions, quadratic equations, and quadratic functions
2. Simultaneous equations, indices and logarithms, and coordinate geometry
3. Statistics, circular measures, and differentiation
It lists common formulae for topics like the quadratic formula, completing the square, differentiation rules, and measures of central tendency and dispersion. The document is intended as a study guide for students to review essential formulae.
This document provides a summary of various math formulae for Form 4 students in Malaysia, including:
1. Functions, quadratic equations, and quadratic functions
2. Simultaneous equations, indices and logarithms, and coordinate geometry
3. Statistics, circular measures, and differentiation
It lists common formulae for topics like the quadratic formula, completing the square, differentiation rules, and measures of central tendency and dispersion. The document is intended as a study guide for students to review essential formulae.
This document provides a summary of various math formulae for Form 4 students in Malaysia, including:
1. Functions, quadratic equations, and quadratic functions
2. Simultaneous equations, indices and logarithms, and coordinate geometry
3. Statistics, circular measures, and differentiation
It lists common formulae for topics like the quadratic formula, completing the square, differentiation rules, and measures of central tendency and dispersion. The document is intended as a study guide for students to review essential formulae.
The document summarizes research on magnetic monopoles in noncommutative spacetime. It begins by motivating noncommutative spacetime as a way to incorporate quantum gravitational effects. It then shows that attempting to quantize spacetime by imposing noncommutativity of coordinates leads to inconsistencies when trying to define a Wu-Yang magnetic monopole in this framework. Specifically, the potentials describing the monopole fail to simultaneously satisfy Maxwell's equations and transform correctly under gauge transformations when expanded to second order in the noncommutativity parameter. This suggests the Dirac quantization condition cannot be satisfied in noncommutative spacetime. Possible reasons for this failure and directions for future work are discussed.
The document discusses wave energy and interference. It defines standing waves as occurring when a traveling wave is reflected by a fixed boundary, resulting in the superposition of the original wave and reflected wave. Standing waves have nodes where the displacement is always zero, and antinodes where the displacement is at a maximum. The normal modes of a system are its allowed standing wave patterns, which are determined by the boundary conditions. For a string fixed at both ends, the normal modes are half-wavelengths that are integer multiples of the string length.
- The document provides the solution to problem 25.72 from the textbook, which asks to derive an expression for the total electric potential energy of a solid sphere with uniform charge density.
- The sphere is modeled as being built up of concentric spherical shells, with each shell carrying a small charge dq.
- The expression derived for the total potential energy is Ue = (3/5)kεQ2/R, where Q is the total charge on the sphere, R is the radius, and kε is the Coulomb's constant.
- The derivation involves integrating the electric potential energy dUe = Vdq over the volume of the sphere, where V is the potential and dq is the charge
This document discusses base excitation in vibration analysis and provides examples. It begins by introducing base excitation as an important class of vibration analysis that involves preventing vibrations from passing through a vibrating base into a structure. Examples of base excitation include vibrations in cars, satellites, and buildings during earthquakes. The document then provides mathematical models and equations to analyze single degree of freedom base excitation systems. Graphs of transmissibility ratios are presented and examples are worked through, such as calculating car vibration amplitude at different speeds. Rotating unbalance is also covered as another source of vibration excitation.
1. The graph of the equation y = x^2 - 1 can be viewed as a torus when considered with points at infinity and over the complex numbers.
2. Intersections of the graph with planes where x or y is set to a constant reveal curves hinting at the toric structure, such as ellipses or lemniscates.
3. When extended to projective space over the complex numbers, the graph can be seen topologically as a two-dimensional surface in four-dimensional space, matching the geometry of a torus.
This document provides an overview of second order ordinary differential equations (ODEs). It discusses the method of variation of parameters for finding particular solutions to inhomogeneous second order linear ODEs. It provides examples of applying this method, including a spring-mass system and an electric circuit. It also discusses applications of second order ODEs to modeling spring-mass systems and electric circuits.
1. Floquet Theory for Internal Gravity Waves
in a Density-Stratified Fluid
Yuanxun Bill Bao
Senior Supervisor: Professor David J. Muraki
August 3, 2012
2. Density-Stratified Fluid Dynamics
Density-Stratified Fluids
density of the fluid varies with altitude
stable stratification: heavy fluids below light fluids, internal waves
unstable stratification: heavy fluids above light fluids, convective dynamics
Buoyancy-Gravity Restoring Dynamics
uniform stable stratification: dρ/dz < 0 constant
vertical displacements ⇒ oscillatory motions
3. Internal Gravity Waves
evidence of internal gravity waves in the atmosphere
left: lenticular clouds near Mt. Ranier, Washington
right: uniform flow over a mountain ⇒ oscillatory wave motions
scientific significance of studying internal gravity waves
internal waves are known to be unstable
a major suspect of clear-air-turbulence
5. My Thesis Goal
Floquet-Fourier computation: over-counting of instability in wavenumber space
Lin’s DNS: two branches of disturbance Fourier modes
goal: to identify all physically unstable modes from Floquet-Fourier computation
6. My Thesis Goal
Floquet-Fourier computation: over-counting of instability in wavenumber space
Lin’s DNS: two branches of disturbance Fourier modes
goal: to identify all physically unstable modes from Floquet-Fourier computation
7. The Governing Equations
Boussinesq Equations in Vorticity-Buoyancy Form
· u = 0 ;
Dη
Dt
= −bx ;
Db
Dt
= −N2
w
incompressible, inviscid Boussinesq Fluid
Euler equations + weak density variation (the Boussinesq approximation)
Brunt-Vaisala frequency N: uniform stable stratification, N2 > 0
2D velocity: u(x, z, t) ; buoyancy: b(x, z, t)
streamfunction: u =
u
w
= − × ψ ˆy =
−ψz
ψx
vorticity: × u = η ˆy = 2ψ ˆy
8. Exact Plane Gravity Wave Solutions
+
z
y
x
−
buoyancy b
Dη
Dt
= −bx
−
+
+
buoyancy b
−
Db
Dt
= −N2
w
dynamics of buoyancy & vorticity ⇒ oscillatory wave motions
exact plane gravity wave solutions
ψ
b
η
=
−Ωd/K
N2
N2K/Ωd
2A sin(Kx + Mz − Ωdt)
primary wavenumbers: (K, M)
dispersion relation: Ω2
d(K, M) =
N2K2
K2 + M2
.
10. Linear Stability Analysis
dimensionless exact plane wave + small disturbances
ψ
b
η
=
−Ω
1
1/Ω
2 sin(x + z − Ωt) +
˜ψ
˜b
˜η
: dimensionless amplitude & dimensionless frequency: Ω2
=
1
1 + δ2
linearized Boussinesq equations
δ2 ˜ψxx + ˜ψzz = ˜η
˜ηt + ˜bx − 2 J( Ω˜η + ˜ψ/Ω , sin(x + z − Ωt) ) = 0
˜bt − ˜ψx − 2 J( Ω˜b + ˜ψ , sin(x + z − Ωt) ) = 0
system of linear PDEs with non-constant, but periodic coefficients
analyzed by Floquet theory
classical textbook example: Mathieu equation (Chapter 3)
11. Floquet Theory: Mathieu Equation
Mathieu Equation:
d2u
dt2
+ k2
− 2 cos(t) u = 0
second-order linear ODE with periodic coefficients
Floquet theory: u = e−iωt
· p(t) = exponential part × co-periodic part
Floquet exponent ω(k; ): Im ω > 0 → instability
goal: to identify all unstable solutions in (k, )-space
12. Floquet Theory: Mathieu Equation
Mathieu Equation:
d2u
dt2
+ k2
− 2 cos(t) u = 0
Two perspectives:
perturbation analysis ⇒ two branches of Floquet exponent
away from resonances: ω(k; ) ∼ ±k
resonant instability at primary resonance k =
1
2
: ω(k; ) ∼ ±
1
2
+ i
Floquet-Fourier computation of ω(k; )
a Riemann surface interpretation of ω(k; ) with k ∈ C
13. Floquet-Fourier Computation
Mathieu equation in system form:
d
dt
u
v
= i
0 1
k2 − 2 cos(t) 0
u
v
Floquet-Fourier representation:
u
v
= e−iωt
·
∞
m=−∞
cme−imt
ω(k; ) as eigenvalues of Hill’s bi-infinite matrix:
...
...
... S0 M
M S1
...
...
...
2 × 2 real blocks: Sm and M
truncated Hill’s matrix: −N ≤ m ≤ N
real-coefficient characteristic polynomial
compute 4N + 2 eigenvalues: {ωn(k; )}
= 0, eigenvalues from Sn blocks: ωn(k; 0) = −n ± k & all real-valued
1, complex eigenvalues may arise from = 0 double eigenvalues
14. Floquet-Fourier Computation
−2 −1.5 −1 −0.5 0 0.5 1 1.5 2
−2
−1.5
−1
−0.5
0
0.5
1
1.5
2
k−axis
Reω
ε = 0.1 ωn(k; ): real • ; complex •
‘——’: ωn(k; 0) = −n ± k
‘——’: ω0(k; 0) = ± k
ωn(k; ) curves are close to ωn(k; 0)
two continuous curves close to ±k
the rest are shifted due to
u
v
= e−i(ω0+n)t
·
∞
m=−∞
cm+ne−imt
For each k, how many Floquet exponents are associated with the unstable solu-
tions of Mathieu equation? two or ∞? Both!
two is understood from perturbation analysis
∞ will be understood from the Riemann surface of ω(k; ) with k ∈ C
15. Floquet-Fourier Computation
−2 −1 0 1 2
−2
−1
0
1
2
k−axis
Reω
ε = 0.1 ωn(k; ): real • ; complex •
‘——’: ωn(k; 0) = −n ± k
‘——’: ω0(k; 0) = ± k
ωn(k; ) curves are close to ωn(k; 0)
two continuous curves close to ±k
the rest are shifted due to
u
v
= e−i(ω0+n)t
·
∞
m=−∞
cm+ne−imt
For each k, how many Floquet exponents are associated with the unstable solu-
tions of Mathieu equation? two or ∞? Both!
two is understood from perturbation analysis
∞ will be understood from the Riemann surface of ω(k; ) with k ∈ C
16. A Riemann Surface Interpretation of ω(k; )
−2 −1 0 1 2
−2
−1
0
1
2
k−axis
Reω
ε = 0.1
Floquet-Fourier computation with k ∈ C → the Riemann surface of ω(k; )
surface height: real ω ; surface colour: imag ω
layers of curves for k ∈ R become layers of sheets for k ∈ C
the two physical branches belong to two primary Riemann sheets
How to identify the two primary Riemann sheets?
more understanding of how sheets are connected
17. A Riemann Surface Interpretation of ω(k; )
zoomed view near Re k = 1/2 shows Riemann sheet connection
branch points: end points of instability intervals
loop around the branch points ⇒
√
type
branch cuts coincide with instability intervals (McKean & Trubowitz 1975)
18. A Riemann Surface Interpretation of ω(k; )
zoomed view near Re k = 0 shows Riemann sheet connection
branch points: two on imaginary axis
loop around the branch points ⇒
√
type
branch cuts to ± i∞ give V-shaped sheets
19. A Riemann Surface Interpretation of ω(k; )
−1 −0.5 0 0.5 1
−i
√
2ǫ
i
√
2ǫ
real k
imagk
ε = 0.1
branch cuts: instability intervals & two cuts to ± i∞
two primary sheets: upward & downward V-shaped sheets
associated with the two physically-relevant Floquet exponents
the other sheets are integer-shifts of primary sheets
20. A Riemann Surface Interpretation of ω(k; )
−1 −0.5 0 0.5 1
−i
√
2ǫ
i
√
2ǫ
real k
imagk
ε = 0.1
branch cuts: instability intervals & two cuts to ± i∞
two primary sheets: upward & downward V-shaped sheets
associated with the two physically-relevant Floquet exponents
the other sheets are integer-shifts of primary sheets
21. Recap of Mathieu Equation
Floquet-Fourier: u
v
= e−iωt
·
N
m=−N
cne−imt
4N + 2 computed Floquet exponents ωn(k; )
perturbation analysis: ω(k; ) ∼ ±k
Riemann surface has two primary Riemann sheets (physically-relevant)
−2 −1 0 1 2
−2
−1
0
1
2
k−axis
Reω
ε = 0.1
23. Gravity Wave Stability Problem
four parameters of ω(k, m; , δ)
, δ = 1.7 (Lin)
wavevector, (k, m) ; k ∈ C with k − m = 2.5
over-counting of Floquet-Fourier computation
vertical & horizontal shifts → instability bands
−2 −1 0 1 2
−2
−1
0
1
2
k−axis, (k−m = 2.5)
realω
ε = 0.1, δ = 1.7
24. Gravity Wave Stability Problem
four parameters of ω(k, m; , δ)
, δ = 1.7 (Lin)
wavevector, (k, m) ; k ∈ C with k − m = 2.5
over-counting of Floquet-Fourier computation
vertical & horizontal shifts → instability bands
−2 −1 0 1 2
−2
−1
0
1
2
k−axis, (k−m = 2.5)
realω
ε = 0.1, δ = 1.7
physically-relevant Floquet exponents solves over-counting problem
25. Fixing the Gap along k − m = 1
−2 −1.5 −1 −0.5 0 0.5 1 1.5 2
−2
−1.5
−1
−0.5
0
0.5
1
1.5
real−k
δ = 1.7, ε = 0.1
realω
new feature: four-sheet collision (only two for Mathieu!)
physically corresponds to near-resonance of four fourier modes (section 5.3)
26. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.1, δ = 1.7
zoomed view near Re k = 0 with Riemann surface
27. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.1, δ = 1.7
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
ω−
(k,m;0)
ω−
(k+1,m+1;0)−Ω
ω+
(k,m;0)
ω+
(k−1,m−1;0)+Ω
k−axis
ω(k,m)
δ = 1.7, ε = 0
continuation algorithm for ω(k, m; = 0.1) starts from = 0 values
28. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.02, δ = 1.7
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
ω−
(k,m;0)
ω−
(k+1,m+1;0)−Ω
ω+
(k,m;0)
ω+
(k−1,m−1;0)+Ω
k−axis
ω(k,m)
δ = 1.7, ε = 0
continuation algorithm for ω(k, m; = 0.1) starts from = 0 values
= 0.02: shows = 0 limit incorrect
29. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.02, δ = 1.7
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0, δ = 1.7
continuation algorithm for ω(k, m; = 0.1) starts from = 0 values
= 0.02: suggests redefining = 0 branch values (continuous)
30. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.06, δ = 1.7
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0, δ = 1.7
continuation algorithm for ω(k, m; = 0.1) starts from = 0 values
= 0.06: instability bands are about to merge
31. Fixing the Gap along k − m = 1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.1, δ = 1.7
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0, δ = 1.7
continuation algorithm for ω(k, m; = 0.1) starts from = 0 values
= 0.1: the gap is fixed
32. Instabilities from Two Primary Sheets
stability diagram is a superposition of instabilities from the two primary sheets
both primary sheets are continuous in Re ω & Im ω
over-counting problem is solved by complex analysis!
33. In Closing: What I Have Learned
density-stratified fluid dynamics & internal gravity waves
linear stability analysis
the Mathieu equation, Floquet theory & Floquet-Fourier computation
perturbation analysis (near & away from resonance)
understanding the Riemann surface structure & computation
34. Four Sheets: = 0.1
−0.4 −0.2 0 0.2 0.4
−0.4
−0.2
0
0.2
0.4
sheet 4
sheet 2
sheet 1
sheet 3
real k
realω
ε = 0.1, δ = 1.7
−0.2 −0.1 0 0.1 0.2
−0.1
−0.05
0
0.05
0.1
sheet 1
real k
imagk
ε = 0.1
−0.2 −0.1 0 0.1 0.2
−0.1
−0.05
0
0.05
0.1
sheet 2
real k
imagk
ε = 0.1
−0.2 −0.1 0 0.1 0.2
−0.1
−0.05
0
0.05
0.1
sheet 3
real k
imagk
ε = 0.1
−0.2 −0.1 0 0.1 0.2
−0.1
−0.05
0
0.05
0.1
sheet 4
real k
imagk
ε = 0.1