Variational Principles and Lagrange’s Equations

Slides:



Advertisements
Similar presentations
Sect. 8.2: Cyclic Coordinates & Conservation Theorems
Advertisements

Sect. 1.6: Simple Applications of the Lagrangian Formulation
Conservative vs. Non-conservative Forces
Physics 430: Lecture 17 Examples of Lagrange’s Equations
Vector integrals Line integrals Surface integrals Volume integrals Integral theorems The divergence theorem Green’s theorem in the plane Stoke’s theorem.
Hamiltonian Formalism
Physics 430: Lecture 16 Lagrange’s Equations with Constraints
Gauge Invariance and Conserved Quantities
Lagrangian and Hamiltonian Dynamics
VECTOR CALCULUS Fundamental Theorem for Line Integrals In this section, we will learn about: The Fundamental Theorem for line integrals and.
Mechanics of Rigid Bodies
Theoretical Mechanics - PHY6200 Chapter 6 Introduction to the calculus of variations Prof. Claude A Pruneau, Physics and Astronomy Department Wayne State.
Linear Momentum and Collisions
Classical Mechanics Describes the relationship between the motion of objects in our everyday world and the forces acting on them Conditions when Classical.
Relative Velocity Two observers moving relative to each other generally do not agree on the outcome of an experiment However, the observations seen by.
Stanford University Department of Aeronautics and Astronautics Introduction to Symmetry Analysis Brian Cantwell Department of Aeronautics and Astronautics.
Kinetics of Particles:
STATIC EQUILIBRIUM [4] Calkin, M. G. “Lagrangian and Hamiltonian Mechanics”, World Scientific, Singapore, 1996, ISBN Consider an object having.
Relativistic Classical Mechanics. XIX century crisis in physics: some facts Maxwell: equations of electromagnetism are not invariant under Galilean transformations.
Central Force Motion Chapter 8
Revision Previous lecture was about Generating Function Approach Derivation of Conservation Laws via Lagrangian via Hamiltonian.
Kinetic Energy, Work, Power, and Potential Energy
Dr. Wang Xingbo Fall , 2005 Mathematical & Mechanical Method in Mechanical Engineering.
A PPLIED M ECHANICS Lecture 02 Slovak University of Technology Faculty of Material Science and Technology in Trnava.
Physics 430: Lecture 15 Lagrange’s Equations
Energy Transformations and Conservation of Mechanical Energy 8
The Two-Body Problem. The two-body problem The two-body problem: two point objects in 3D interacting with each other (closed system) Interaction between.
Vector Calculus 13. The Fundamental Theorem for Line Integrals 13.3.
Chapter 3: Central Forces Introduction Interested in the “2 body” problem! Start out generally, but eventually restrict to motion of 2 bodies interacting.
Energy Transformations and Conservation of Mechanical Energy 8.01 W05D2.
Motion & Force: DYNAMICS
Final review Help sessions scheduled for Dec. 8 and 9, 6:30 pm in MPHY 213 Your hand-written notes allowed No numbers, unless you want a problem with numbers.
In the Hamiltonian Formulation, the generalized coordinate q k & the generalized momentum p k are called Canonically Conjugate quantities. Hamilton’s.
Ch 2. The Schrödinger Equation (S.E)
D’Alembert’s Principle the sum of the work done by
Sect. 1.3: Constraints Discussion up to now  All mechanics is reduced to solving a set of simultaneous, coupled, 2 nd order differential eqtns which.
Exam 2 Review 8.02 W08D1. Announcements Test Two Next Week Thursday Oct 27 7:30-9:30 Section Room Assignments on Announcements Page Test Two Topics: Circular.
Chapter 4 The Laws of Motion. Classical Mechanics Describes the relationship between the motion of objects in our everyday world and the forces acting.
Sect. 7.9: Lagrangian Formulation of Relativity (input from Marion!) We now see, in principal at least, how to generalize Newton’s 2 nd Law Equations.
Introduction. The textbook “Classical Mechanics” (3rd Edition) By H. Goldstein, C. P. Poole, J. L. Safko Addison Wesley, ISBN: Herbert Goldstein.
Chapter 13 Gravitation Newton’s Law of Gravitation Here m 1 and m 2 are the masses of the particles, r is the distance between them, and G is the.
Phy 303: Classical Mechanics (2) Chapter 3 Lagrangian and Hamiltonian Mechanics.
Ch. 4, Motion & Force: DYNAMICS
The Hamiltonian method
Monday, Apr. 4, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #16 Monday, Apr. 4, 2005 Dr. Jae Yu Symmetries Why do we care about the symmetry?
Canonical Equations of Motion -- Hamiltonian Dynamics
Advanced Computer Graphics Spring 2014 K. H. Ko School of Mechatronics Gwangju Institute of Science and Technology.
The state of a system of n particles & subject to m constraints connecting some of the 3n rectangular coordinates is completely specified by s = 3n –
The Lagrangian Equation INTERMEDIATE MECHANICS WESLEY QUEEN.
Sect. 2.6: Conservation Theorems & Symmetry Properties Lagrange Method: A method to get the eqtns of motion. Solving them = math! n degrees of freedom.
Equivalence of Lagrange’s & Newton’s Equations Section 7.6 The Lagrangian & the Newtonian formulations of mechanics are 100% equivalent! –As we know,
The Lagrangian Equation INTERMEDIATE MECHANICS WESLEY QUEEN.
Ch. 2: Variational Principles & Lagrange’s Eqtns Sect. 2.1: Hamilton’s Principle Our derivation of Lagrange’s Eqtns from D’Alembert’s Principle: Used.
Chapter 3 Postulates of Quantum Mechanics. Questions QM answers 1) How is the state of a system described mathematically? (In CM – via generalized coordinates.
Syllabus Note : Attendance is important because the theory and questions will be explained in the class. II ntroduction. LL agrange’s Equation. SS.
Introduction to Lagrangian and Hamiltonian Mechanics
Test 2 review Test: 7 pm in 203 MPHY
Classical Mechanics Lagrangian Mechanics.
Canonical Quantization
Mathematical & Mechanical Method in Mechanical Engineering
Kinetics of Particles: Newton’s Second Law
Theoretical Mechanics: Lagrangian dynamics
Hamiltonian Mechanics
Relativistic Classical Mechanics
Continuous Systems and Fields
Introduction.
Physics 319 Classical Mechanics
Introduction.
Presentation transcript:

Variational Principles and Lagrange’s Equations

Definitions Lagrangian density: Lagrangian: Action: How to find the special value for action corresponding to observable ? Joseph Louis Lagrange/ Giuseppe Luigi Lagrangia (1736 – 1813)

Variational principle Maupertuis: Least Action Principle Hamilton: Hamilton’s Variational Principle Feynman: Quantum-Mechanical Path Integral Approach Pierre-Louis Moreau de Maupertuis (1698 – 1759) Sir William Rowan Hamilton (1805 – 1865) Richard Phillips Feynman (1918 – 1988)

Functionals Functional: given any function f(x), produces a number S Action is a functional: Examples of finding special values of functionals using variational approach: shortest distance between two points on a plane; the brachistochrone problem; minimum surface of revolution; etc.

Shortest distance between two points on a plane An element of length on a plane is Total length of any curve going between points 1 and 2 is The condition that the curve is the shortest path is that the functional I takes its minimum value

The brachistochrone problem Find a curve joining two points, along which a particle falling from rest under the influence of gravity travels from the highest to the lowest point in the least time Brachistochrone solution: the value of the functional t [y(x)] takes its minimum value

Calculus of variations Consider a functional of the following type What function y(x) yields a stationary value (minimum, maximum, or saddle) of J ?

Calculus of variations Assume that function y0(x) yields a stationary value and consider all possible functions in the form:

Calculus of variations In this case our functional becomes a function of α: Stationary value condition:

Stationary value 1 2 3

Stationary value 1 2 3 u dv u v v du

Stationary value 1 2 3

Stationary value 1 2 3

Stationary value arbitrary Trivial … 

Stationary value arbitrary Nontrivial !!! 

Shortest distance between two points on a plane Straight line! 

The brachistochrone problem Scary! 

Recipe Best Fit 1. Bring together structure and fields 2. Relate this togetherness to the entire system 3. Make them fit best when the fields have observable dependencies: Structure Physical Laws Best Fit Structure Fields

Back to trajectories and Lagrangians How to find the special values for action corresponding to observable trajectories ? We look for a stationary action using variational principle

Recipe Best Fit 1. Bring together structure and fields 2. Relate this togetherness to the entire system 3. Make them fit best when the fields have observable dependencies: Structure Physical Laws Best Fit Structure Fields

Back to trajectories and Lagrangians For open systems, we cannot apply variational principle in a consistent way, since integration in not well defined for them We look for a stationary action using variational principle for closed systems:

Stationary value Nontrivial !!! 

Simplest non-trivial case Let’s start with the simplest non-trivial result of the variational calculus and see if it can yield observable trajectories

Stationary value Nontrivial !!! 

Euler- Lagrange equations These equations are called the Euler- Lagrange equations Joseph Louis Lagrange (1736 – 1813) Leonhard Euler (1707 – 1783)

Recipe Best Fit 1. Bring together structure and fields 2. Relate this togetherness to the entire system 3. Make them fit best when the fields have observable dependencies: Structure Physical Laws Best Fit Structure Fields

How to construct Lagrangians? Let us recall some kindergarten stuff On our – classical-mechanical – level, we know several types of fundamental interactions: Gravitational Electromagnetic That’s it

Gravitation For a particle in a gravitational field, the trajectory is described via 2nd Newton’s Law: This system can be approximated as closed The structure (symmetry) of the system is described by the gravitational potential Sir Isaac Newton (1643 – 1727)

Electromagnetic field For a charged particle in an electromagnetic field, the trajectory is described via 2nd Newton’s Law: This system can be approximated as closed The structure (symmetry) of the system is described by the scalar and vector potentials Really???

Electromagnetic field

Electromagnetic field

Electromagnetic field Lorentz force!  Hendrik Lorentz (1853-1928)

Kindergarten Thereby: In component form

How to construct Lagrangians? Kindergarten stuff: The “kindergarten equations” look very similar to the Euler-Lagrange equations! We may be on the right track! 

Gravitation

Gravitation

Electromagnetism

Bottom line We successfully demonstrated applicability of our recipe This approach works not just in classical mechanics only, but in all other fields of physics Structure Physical Laws Best Fit

Some philosophy de Maupertuis on the principle of least action (“Essai de cosmologie”, 1750): “In all the changes that take place in the universe, the sum of the products of each body multiplied by the distance it moves and by the speed with which it moves is the least that is possible.” How does an object know in advance what trajectory corresponds to a stationary action??? Answer: quantum-mechanical path integral approach Pierre-Louis Moreau de Maupertuis (1698 – 1759)

Some philosophy Feynman: “Is it true that the particle doesn't just "take the right path" but that it looks at all the other possible trajectories? ... The miracle of it all is, of course, that it does just that. ... It isn't that a particle takes the path of least action but that it smells all the paths in the neighborhood and chooses the one that has the least action ...” Richard Phillips Feynman (1918 – 1988)

Some philosophy Dyson: “In 1949, Dick Feynman told me about his "sum over histories" version of quantum mechanics. "The electron does anything it likes," he said. "It just goes in any direction at any speed, forward or backward in time, however it likes, and then you add up the amplitudes and it gives you the wave-function." I said to him, "You're crazy." But he wasn't.” Freeman John Dyson (born 1923)

Some philosophy Philosophical meaning of the Lagrangian formalism: structure of a system determines its observable behavior So, that's it? Why do we need all this? In addition to the deep philosophical meaning, Lagrangian formalism offers great many advantages compared to the Newtonian approach

Lagrangian approach: extra goodies It is scalar (Newtonian – vectorial) Allows introduction of configuration space and efficient description of systems with constrains Becomes relatively simpler as the mechanical system becomes more complex Applicable outside Newtonian mechanics Relates conservation laws with symmetries Scale invariance applications Gauge invariance applications

Simple example Projectile motion

Another example Another Lagrangian What is going on?!

Gauge invariance For the Lagrangians of the type And functions of the type Let’s introduce a transformation (gauge transformation):

Gauge invariance

Gauge invariance

Gauge invariance

Back to the question: How to construct Lagrangians? Ambiguity: different Lagrangians result in the same equations of motion How to select a Lagrangian appropriately? It is a matter of taste and art It is a question of symmetries of the physical system one wishes to describe Conventionally, and for expediency, for most applications in classical mechanics:

Cylindrically symmetric potential Motion in a potential that depends only on the distance to the z axis It is convenient to work in cylindrical coordinates Then

Cylindrically symmetric potential How to rewrite the equations of motion in cylindrical coordinates?

Generalized coordinates Instead of re-deriving the Euler-Lagrange equations explicitly for each problem (e.g. cylindrical coordinates), we introduce a concept of generalized coordinates Let us consider a set of coordinates Assume that the Euler-Lagrange equations hold for these variables Consider a new set of (generalized) coordinates

Generalized coordinates We can, in theory, invert these equations: Let us do some calculations:

Generalized coordinates The Euler-Lagrange equations are the same in generalized coordinates!!!

Generalized coordinates If the Euler-Lagrange equations are true for one set of coordinates, then they are also true for the other set

Cylindrically symmetric potential Radial force causes a change in radial momentum and a centripetal acceleration

Cylindrically symmetric potential Angular momentum relative to the z axis is a constant

Cylindrically symmetric potential Axial component of velocity does not change

Symmetries and conservation laws The most beautiful and useful illustration of the “structure vs observed behavior” philosophy is the link between symmetries and conservation laws Conjugate momentum for coordinate : If Lagrangian does not depend on a certain coordinate, this coordinate is called cyclic (ignorable) For cyclic coordinates, conjugate momenta are conserved

Symmetries and conservation laws For cyclic coordinates, conjugate momenta are conserved p = const p ≠ const

Cylindrically symmetric potential Cyclic coordinates: Rotational symmetry Translational symmetry Conjugate momenta:

Electromagnetism Conjugate momenta:

Noether’s theorem Relationship between Lagrangian symmetries and conserved quantities was formalized only in 1915 by Emmy Noether: “For each symmetry of the Lagrangian, there is a conserved quantity” Let the Lagrangian be invariant under the change of coordinates: α is a small parameter. This invariance has to hold to the first order in α Emmy Noether/ Amalie Nöther (1882 – 1935)

Noether’s theorem Invariance of the Lagrangian: Using the Euler-Lagrange equations

Example Motion in an x-y plane of a mass on a spring (zero equilibrium length): The Lagrangian is invariant (to the first order in α) under the following change of coordinates: Then, from Noether’s theorem it follows that

Example In polar coordinates: The conserved quantity: Angular momentum in the x-y plane is conserved

Example For the same problem, we can start with a Lagrangian expressed in polar coordinates: The Lagrangian is invariant (to any order in α) under the following change of coordinates: The conserved quantity from Noether’s theorem:

Back to trajectories and Lagrangians How to find the special values for action corresponding to observable trajectories ? We look for a stationary action using variational principle

Stationary value 1 2 3 u dv u v v du

More on symmetries Full time derivative of a Lagrangian: From the Euler-Lagrange equations: If

What is H? Let us expand the Lagrangian in powers of : Form calculus, for a homogeneous function f of degree n (Euler’s theorem) :

What is H? If the Lagrangian has a form: Then For electromagnetism:

Conservation of energy In the field formalism, the conservation of H is a part of Noether’s theorem

The brachistochrone problem Similarly to the “H-trick”: !!! Scary! 

The brachistochrone problem Change of variables: Parametric solution (cycloid)

Scale invariance For Lagrangians of the following form: And homogeneous L0 of degree k Introducing scale and time transformations Then

Scale invariance Therefore, after transformations If Then The Euler-Lagrange equations after transformations The same!

Scale invariance So, the Euler-Lagrange equations after transformations are the same if Free fall Let us recall

Scale invariance So, the Euler-Lagrange equations after transformations are the same if Mass on a spring Let us recall

Scale invariance So, the Euler-Lagrange equations after transformations are the same if Kepler’s problem Let us recall 3rd Kepler’s law Johannes Kepler (1571-1630)

How about open systems? For some systems we can neglect their interaction with the outside world and formulate their behavior in terms of Lagrangian formalism For some systems we can not do it Approach: to describe the system without “leaks” and “feeds” and then add them to the description of the system

How about open systems? For open systems, we first describe the system without “leaks” and “feeds” After that we add “leaks” and “feeds” to the description of the system Q: Non-conservative generalized forces

Generalized forces Forces 1: Conservative (Potential) 2: Non-conservative

Richard Phillips Feynman (1918 – 1988) Generalized forces In principle, there is no need to introduce generalized forces for a closed system fully described by a Lagrangian Feynman: “…The principle of least action only works for conservative systems — where all forces can be gotten from a potential function. … On a microscopic level — on the deepest level of physics — there are no non-conservative forces. Non-conservative forces, like friction, appear only because we neglect microscopic complications — there are just too many particles to analyze.” So, introduction of non-conservative forces is a result of the open-system approach

Degrees of freedom The number of degrees of freedom is the number of independent coordinates that must be specified in order to define uniquely the state of the system For a system of N free particle there are 3N degrees of freedom (3N coordinates) N

N k Constraints We can imposed k constraints on the system The number of degrees of freedom is reduced to 3N – k = s It is convenient to think of the remaining s independent coordinates as the coordinates of a single point in an s-dimensional space: configuration space N k

Types of constraints Holonomic (integrable) constraints can be expressed in the form: Nonholonomic constraints cannot be expressed in this form Rheonomous constraints – contain time dependence explicitly Scleronomous constraints – do not contain time dependence explicitly

Analysis of systems with holonomic constraints Elimination of variables using constraints equations Use of independent generalized coordinates Lagrange’s multiplier method

Double 2D pendulum An example of a holonomic scleronomous constraint The trajectories of the system are very complex Lagrangian approach produces equation of motion We need 2 independent generalized coordinates (N = 2, k = 2 + 2, s = 3 N – k = 2)

Double 2D pendulum Relative to the pivot, the Cartesian coordinates Taking the time derivative, and then squaring Lagrangian in Cartesian coordinates:

Double 2D pendulum Lagrangian in new coordinates: The equations of motion:

Double 2D pendulum Special case The equations of motion: More fun at: http://www.mathstat.dal.ca/~selinger/lagrange/doublependulum.html

Lagrange’s multiplier method Used when constraint reactions are the object of interest Instead of considering 3N - k variables and equations, this method deals with 3N + k variables As a results, we obtain 3N trajectories and k constraint reactions Lagrange’s multiplier method can be applied to some nonholonomic constraints

Lagrange’s multiplier method Let us explicitly incorporate constraints into the structure of our system For observable trajectories So

Lagrange’s multiplier method - constraint reactions Now we have 3N + k equations for and

Application to a nonholonomic case A particle on a smooth hemisphere One nonholonomic constraint: While the particle remains on the sphere, the constraint is holonomic And the reaction from the surface is not zero

Application to a nonholonomic case Constraint equation in cylindrical coordinates: New Lagrangian in cylindrical coordinates: Equations of motion

Application to a nonholonomic case Constraint equation in cylindrical coordinates: New Lagrangian in cylindrical coordinates: Equations of motion

Application to a nonholonomic case Constraint equation in cylindrical coordinates: New Lagrangian in cylindrical coordinates: Equations of motion Trivial

Application to a nonholonomic case Constraint reaction:

Application to a nonholonomic case Constraint reaction: Reaction disappears when The particle becomes airborne