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AN INTRODUCTION to LAGRANGIAN MECHANICS Alain
AN INTRODUCTION TO LAGRANGIAN MECHANICS Alain J. Brizard Department of Chemistry and Physics Saint Michael’s College, Colchester, VT 05439 July 7, 2007 i Preface The original purpose of the present lecture notes on Classical Mechanics was to sup- plement the standard undergraduate textbooks (such as Marion and Thorton’s Classical Dynamics of Particles and Systems) normally used for an intermediate course in Classi- cal Mechanics by inserting a more general and rigorous introduction to Lagrangian and Hamiltonian methods suitable for undergraduate physics students at sophomore and ju- nior levels. The outcome of this effort is that the lecture notes are now meant to provide a self-consistent introduction to Classical Mechanics without the need of any additional material. It is expected that students taking this course will have had a one-year calculus-based introductory physics course followed by a one-semester course in Modern Physics. Ideally, students should have completed their three-semester calculus sequence by the time they enroll in this course and, perhaps, have taken a course in ordinary differential equations. On the other hand, this course should be taken before a rigorous course in Quantum Mechanics in order to provide students with a sound historical perspective involving the connection between Classical Physics and Quantum Physics. Hence, the second semester of the sophomore year or the fall semester of the junior year provide a perfect niche for this course. The structure of the lecture notes presented here is based on achieving several goals. As a first goal, I originally wanted to model these notes after the wonderful monograph of Landau and Lifschitz on Mechanics, which is often thought to be too concise for most undergraduate students. -
Classical Mechanics
Classical Mechanics Hyoungsoon Choi Spring, 2014 Contents 1 Introduction4 1.1 Kinematics and Kinetics . .5 1.2 Kinematics: Watching Wallace and Gromit ............6 1.3 Inertia and Inertial Frame . .8 2 Newton's Laws of Motion 10 2.1 The First Law: The Law of Inertia . 10 2.2 The Second Law: The Equation of Motion . 11 2.3 The Third Law: The Law of Action and Reaction . 12 3 Laws of Conservation 14 3.1 Conservation of Momentum . 14 3.2 Conservation of Angular Momentum . 15 3.3 Conservation of Energy . 17 3.3.1 Kinetic energy . 17 3.3.2 Potential energy . 18 3.3.3 Mechanical energy conservation . 19 4 Solving Equation of Motions 20 4.1 Force-Free Motion . 21 4.2 Constant Force Motion . 22 4.2.1 Constant force motion in one dimension . 22 4.2.2 Constant force motion in two dimensions . 23 4.3 Varying Force Motion . 25 4.3.1 Drag force . 25 4.3.2 Harmonic oscillator . 29 5 Lagrangian Mechanics 30 5.1 Configuration Space . 30 5.2 Lagrangian Equations of Motion . 32 5.3 Generalized Coordinates . 34 5.4 Lagrangian Mechanics . 36 5.5 D'Alembert's Principle . 37 5.6 Conjugate Variables . 39 1 CONTENTS 2 6 Hamiltonian Mechanics 40 6.1 Legendre Transformation: From Lagrangian to Hamiltonian . 40 6.2 Hamilton's Equations . 41 6.3 Configuration Space and Phase Space . 43 6.4 Hamiltonian and Energy . 45 7 Central Force Motion 47 7.1 Conservation Laws in Central Force Field . 47 7.2 The Path Equation . -
Chapter 8 Relationship Between Rotational Speed and Magnetic
Chapter 8 Relationship Between Rotational Speed and Magnetic Fields 8.1 Introduction It is well-known that sunspots and other solar magnetic features rotate faster than the surface plasma (Howard & Harvey, 1970). The sidereal rotation speeds of weak magnetic features and plages (Howard, Gilman, & Gilman, 1984; Komm, Howard, & Harvey, 1993), individual sunspots (Howard, Gilman, & Gilman, 1984; Sivaraman, Gupta, & Howard, 1993) and sunspot groups (Howard, 1992) have been studied for many years by different research groups by use of different observatory data (see reviews of Howard 1996 and Beck 2000). Such studies are deemed as diagnostics of subsurface conditions based on the assumption that the faster rotation of magnetic features was caused by the faster-rotating plasma in the interior where the magnetic features were anchored (Gilman & Foukal, 1979). By matching the sunspot surface speed with the solar interior rotational speed robustly derived by helioseismology (e.g., Thompson et al., 1996; Kosovichev et al., 1997; Howe et al., 2000a), several studies estimated the depth of sunspot roots for sunspots of different sizes and life spans (e.g., Hiremath, 2002; Sivaraman et al., 2003). Such studies are valuable for understanding the solar dynamo and origin of solar active regions. However, D’Silva & Howard (1994) proposed a different explanation, namely that effects of buoyancy 111 112 CHAPTER 8. ROTATIONAL SPEED AND MAGNETIC FIELDS and drag coupled with the Coriolis force during the emergence of active regions might lead to the faster rotational speed. Although many studies were done to infer the rotational speed of various solar magnetic features, the relationship between the rotational speed of the magnetic fea- tures and their magnetic strength has not yet been studied. -
Rotating Objects Tend to Keep Rotating While Non- Rotating Objects Tend to Remain Non-Rotating
12 Rotational Motion Rotating objects tend to keep rotating while non- rotating objects tend to remain non-rotating. 12 Rotational Motion In the absence of an external force, the momentum of an object remains unchanged— conservation of momentum. In this chapter we extend the law of momentum conservation to rotation. 12 Rotational Motion 12.1 Rotational Inertia The greater the rotational inertia, the more difficult it is to change the rotational speed of an object. 1 12 Rotational Motion 12.1 Rotational Inertia Newton’s first law, the law of inertia, applies to rotating objects. • An object rotating about an internal axis tends to keep rotating about that axis. • Rotating objects tend to keep rotating, while non- rotating objects tend to remain non-rotating. • The resistance of an object to changes in its rotational motion is called rotational inertia (sometimes moment of inertia). 12 Rotational Motion 12.1 Rotational Inertia Just as it takes a force to change the linear state of motion of an object, a torque is required to change the rotational state of motion of an object. In the absence of a net torque, a rotating object keeps rotating, while a non-rotating object stays non-rotating. 12 Rotational Motion 12.1 Rotational Inertia Rotational Inertia and Mass Like inertia in the linear sense, rotational inertia depends on mass, but unlike inertia, rotational inertia depends on the distribution of the mass. The greater the distance between an object’s mass concentration and the axis of rotation, the greater the rotational inertia. 2 12 Rotational Motion 12.1 Rotational Inertia Rotational inertia depends on the distance of mass from the axis of rotation. -
Branched Hamiltonians and Supersymmetry
Branched Hamiltonians and Supersymmetry Thomas Curtright, University of Miami Wigner 111 seminar, 12 November 2013 Some examples of branched Hamiltonians are explored, as recently advo- cated by Shapere and Wilczek. These are actually cases of switchback poten- tials, albeit in momentum space, as previously analyzed for quasi-Hamiltonian dynamical systems in a classical context. A basic model, with a pair of Hamiltonian branches related by supersymmetry, is considered as an inter- esting illustration, and as stimulation. “It is quite possible ... we may discover that in nature the relation of past and future is so intimate ... that no simple representation of a present may exist.” – R P Feynman Based on work with Cosmas Zachos, Argonne National Laboratory Introduction to the problem In quantum mechanics H = p2 + V (x) (1) is neither more nor less difficult than H = x2 + V (p) (2) by reason of x, p duality, i.e. the Fourier transform: ψ (x) φ (p) ⎫ ⎧ x ⎪ ⎪ +i∂/∂p ⎪ ⇐⇒ ⎪ ⎬⎪ ⎨⎪ i∂/∂x p − ⎪ ⎪ ⎪ ⎪ ⎭⎪ ⎩⎪ This equivalence of (1) and (2) is manifest in the QMPS formalism, as initiated by Wigner (1932), 1 2ipy/ f (x, p)= dy x + y ρ x y e− π | | − 1 = dk p + k ρ p k e2ixk/ π | | − where x and p are on an equal footing, and where even more general H (x, p) can be considered. See CZ to follow, and other talks at this conference. Or even better, in addition to the excellent books cited at the conclusion of Professor Schleich’s talk yesterday morning, please see our new book on the subject ... Even in classical Hamiltonian mechanics, (1) and (2) are equivalent under a classical canonical transformation on phase space: (x, p) (p, x) ⇐⇒ − But upon transitioning to Lagrangian mechanics, the equivalence between the two theories becomes obscure. -
Fermat's Principle and the Geometric Mechanics of Ray
Fermat’s Principle and the Geometric Mechanics of Ray Optics Summer School Lectures, Fields Institute, Toronto, July 2012 Darryl D Holm Imperial College London [email protected] http://www.ma.ic.ac.uk/~dholm/ Texts for the course include: Geometric Mechanics I: Dynamics and Symmetry, & II: Rotating, Translating and Rolling, by DD Holm, World Scientific: Imperial College Press, Singapore, Second edition (2011). ISBN 978-1-84816-195-5 and ISBN 978-1-84816-155-9. Geometric Mechanics and Symmetry: From Finite to Infinite Dimensions, by DD Holm,T Schmah and C Stoica. Oxford University Press, (2009). ISBN 978-0-19-921290-3 Introduction to Mechanics and Symmetry, by J. E. Marsden and T. S. Ratiu Texts in Applied Mathematics, Vol. 75. New York: Springer-Verlag (1994). 1 GeometricMechanicsofFermatRayOptics DDHolm FieldsInstitute,Toronto,July2012 2 Contents 1 Mathematical setting 5 2 Fermat’s principle 8 2.1 Three-dimensional eikonal equation . 10 2.2 Three-dimensional Huygens wave fronts . 17 2.3 Eikonal equation for axial ray optics . 23 2.4 The eikonal equation for mirages . 29 2.5 Paraxial optics and classical mechanics . 32 3 Lecture 2: Hamiltonian formulation of axial ray optics 34 3.1 Geometry, phase space and the ray path . 36 3.2 Legendre transformation . 39 4 Hamiltonian form of optical transmission 42 4.1 Translation-invariant media . 49 4.2 Axisymmetric, translation-invariant materials . 50 4.3 Hamiltonian optics in polar coordinates . 53 4.4 Geometric phase for Fermat’s principle . 56 4.5 Skewness . 58 4.6 Lagrange invariant: Poisson bracket relations . 63 GeometricMechanicsofFermatRayOptics DDHolm FieldsInstitute,Toronto,July2012 3 5 Axisymmetric invariant coordinates 69 6 Geometry of invariant coordinates 73 6.1 Flows of Hamiltonian vector fields . -
Analogy in William Rowan Hamilton's New Algebra
Technical Communication Quarterly ISSN: 1057-2252 (Print) 1542-7625 (Online) Journal homepage: https://www.tandfonline.com/loi/htcq20 Analogy in William Rowan Hamilton's New Algebra Joseph Little & Maritza M. Branker To cite this article: Joseph Little & Maritza M. Branker (2012) Analogy in William Rowan Hamilton's New Algebra, Technical Communication Quarterly, 21:4, 277-289, DOI: 10.1080/10572252.2012.673955 To link to this article: https://doi.org/10.1080/10572252.2012.673955 Accepted author version posted online: 16 Mar 2012. Published online: 16 Mar 2012. Submit your article to this journal Article views: 158 Citing articles: 1 View citing articles Full Terms & Conditions of access and use can be found at https://www.tandfonline.com/action/journalInformation?journalCode=htcq20 Technical Communication Quarterly, 21: 277–289, 2012 Copyright # Association of Teachers of Technical Writing ISSN: 1057-2252 print/1542-7625 online DOI: 10.1080/10572252.2012.673955 Analogy in William Rowan Hamilton’s New Algebra Joseph Little and Maritza M. Branker Niagara University This essay offers the first analysis of analogy in research-level mathematics, taking as its case the 1837 treatise of William Rowan Hamilton. Analogy spatialized Hamilton’s key concepts—knowl- edge and time—in culturally familiar ways, creating an effective landscape for thinking about the new algebra. It also structurally aligned his theory with the real number system so his objects and operations would behave customarily, thus encompassing the old algebra while systematically bringing into existence the new. Keywords: algebra, analogy, mathematics, William Rowan Hamilton INTRODUCTION Studies of analogy in technical discourse have made important strides in the 30 years since Lakoff and Johnson (1980) ushered in the cognitive linguistic turn. -
Leonhard Euler: His Life, the Man, and His Works∗
SIAM REVIEW c 2008 Walter Gautschi Vol. 50, No. 1, pp. 3–33 Leonhard Euler: His Life, the Man, and His Works∗ Walter Gautschi† Abstract. On the occasion of the 300th anniversary (on April 15, 2007) of Euler’s birth, an attempt is made to bring Euler’s genius to the attention of a broad segment of the educated public. The three stations of his life—Basel, St. Petersburg, andBerlin—are sketchedandthe principal works identified in more or less chronological order. To convey a flavor of his work andits impact on modernscience, a few of Euler’s memorable contributions are selected anddiscussedinmore detail. Remarks on Euler’s personality, intellect, andcraftsmanship roundout the presentation. Key words. LeonhardEuler, sketch of Euler’s life, works, andpersonality AMS subject classification. 01A50 DOI. 10.1137/070702710 Seh ich die Werke der Meister an, So sehe ich, was sie getan; Betracht ich meine Siebensachen, Seh ich, was ich h¨att sollen machen. –Goethe, Weimar 1814/1815 1. Introduction. It is a virtually impossible task to do justice, in a short span of time and space, to the great genius of Leonhard Euler. All we can do, in this lecture, is to bring across some glimpses of Euler’s incredibly voluminous and diverse work, which today fills 74 massive volumes of the Opera omnia (with two more to come). Nine additional volumes of correspondence are planned and have already appeared in part, and about seven volumes of notebooks and diaries still await editing! We begin in section 2 with a brief outline of Euler’s life, going through the three stations of his life: Basel, St. -
Schrödinger's Argument.Pdf
SCHRÖDINGER’S TRAIN OF THOUGHT Nicholas Wheeler, Reed College Physics Department April 2006 Introduction. David Griffiths, in his Introduction to Quantum Mechanics (2nd edition, 2005), is content—at equation (1.1) on page 1—to pull (a typical instance of) the Schr¨odinger equation 2 2 i ∂Ψ = − ∂ Ψ + V Ψ ∂t 2m ∂x2 out of his hat, and then to proceed directly to book-length discussion of its interpretation and illustrative physical ramifications. I remarked when I wrote that equation on the blackboard for the first time that in a course of my own design I would feel an obligation to try to encapsulate the train of thought that led Schr¨odinger to his equation (1926), but that I was determined on this occasion to adhere rigorously to the text. Later, however, I was approached by several students who asked if I would consider interpolating an account of the historical events I had felt constrained to omit. That I attempt to do here. It seems to me a story from which useful lessons can still be drawn. 1. Prior events. Schr¨odinger cultivated soil that had been prepared by others. Planck was led to write E = hν by his successful attempt (1900) to use the then-recently-established principles of statistical mechanics to account for the spectral distribution of thermalized electromagnetic radiation. It was soon appreciated that Planck’s energy/frequency relation was relevant to the understanding of optical phenomena that take place far from thermal equilibrium (photoelectric effect: Einstein 1905; atomic radiation: Bohr 1913). By 1916 it had become clear to Einstein that, while light is in some contexts well described as a Maxwellian wave, in other contexts it is more usefully thought of as a massless particle, with energy E = hν and momentum p = h/λ. -
Hamilton's Principle in Continuum Mechanics
Hamilton’s Principle in Continuum Mechanics A. Bedford University of Texas at Austin This document contains the complete text of the monograph published in 1985 by Pitman Publishing, Ltd. Copyright by A. Bedford. 1 Contents Preface 4 1 Mechanics of Systems of Particles 8 1.1 The First Problem of the Calculus of Variations . 8 1.2 Conservative Systems . 12 1.2.1 Hamilton’s principle . 12 1.2.2 Constraints.......................... 15 1.3 Nonconservative Systems . 17 2 Foundations of Continuum Mechanics 20 2.1 Mathematical Preliminaries . 20 2.1.1 Inner Product Spaces . 20 2.1.2 Linear Transformations . 22 2.1.3 Functions, Continuity, and Differentiability . 24 2.1.4 Fields and the Divergence Theorem . 25 2.2 Motion and Deformation . 27 2.3 The Comparison Motion . 32 2.4 The Fundamental Lemmas . 36 3 Mechanics of Continuous Media 39 3.1 The Classical Theories . 40 3.1.1 IdealFluids.......................... 40 3.1.2 ElasticSolids......................... 46 3.1.3 Inelastic Materials . 50 3.2 Theories with Microstructure . 54 3.2.1 Granular Solids . 54 3.2.2 Elastic Solids with Microstructure . 59 2 4 Mechanics of Mixtures 65 4.1 Motions and Comparison Motions of a Mixture . 66 4.1.1 Motions............................ 66 4.1.2 Comparison Fields . 68 4.2 Mixtures of Ideal Fluids . 71 4.2.1 Compressible Fluids . 71 4.2.2 Incompressible Fluids . 73 4.2.3 Fluids with Microinertia . 75 4.3 Mixture of an Ideal Fluid and an Elastic Solid . 83 4.4 A Theory of Mixtures with Microstructure . 86 5 Discontinuous Fields 91 5.1 Singular Surfaces . -
BRST APPROACH to HAMILTONIAN SYSTEMS Our Starting Point Is the Partition Function
BRST APPROACH TO HAMILTONIAN SYSTEMS A.K.Aringazin1, V.V.Arkhipov2, and A.S.Kudusov3 Department of Theoretical Physics Karaganda State University Karaganda 470074 Kazakstan Preprint KSU-DTP-10/96 Abstract BRST formulation of cohomological Hamiltonian mechanics is presented. In the path integral approach, we use the BRST gauge fixing procedure for the partition func- tion with trivial underlying Lagrangian to fix symplectic diffeomorphism invariance. Resulting Lagrangian is BRST and anti-BRST exact and the Liouvillian of classical mechanics is reproduced in the ghost-free sector. The theory can be thought of as a topological phase of Hamiltonian mechanics and is considered as one-dimensional cohomological field theory with the target space a symplectic manifold. Twisted (anti- )BRST symmetry is related to global N = 2 supersymmetry, which is identified with an exterior algebra. Landau-Ginzburg formulation of the associated d = 1, N = 2 model is presented and Slavnov identity is analyzed. We study deformations and per- turbations of the theory. Physical states of the theory and correlation functions of the BRST invariant observables are studied. This approach provides a powerful tool to investigate the properties of Hamiltonian systems. PACS number(s): 02.40.+m, 03.40.-t,03.65.Db, 11.10.Ef, 11.30.Pb. arXiv:hep-th/9811026v1 2 Nov 1998 [email protected] [email protected] [email protected] 1 1 INTRODUCTION Recently, path integral approach to classical mechanics has been developed by Gozzi, Reuter and Thacker in a series of papers[1]-[10]. They used a delta function constraint on phase space variables to satisfy Hamilton’s equation and a sort of Faddeev-Popov representation. -
Exploring Robotics Joel Kammet Supplemental Notes on Gear Ratios
CORC 3303 – Exploring Robotics Joel Kammet Supplemental notes on gear ratios, torque and speed Vocabulary SI (Système International d'Unités) – the metric system force torque axis moment arm acceleration gear ratio newton – Si unit of force meter – SI unit of distance newton-meter – SI unit of torque Torque Torque is a measure of the tendency of a force to rotate an object about some axis. A torque is meaningful only in relation to a particular axis, so we speak of the torque about the motor shaft, the torque about the axle, and so on. In order to produce torque, the force must act at some distance from the axis or pivot point. For example, a force applied at the end of a wrench handle to turn a nut around a screw located in the jaw at the other end of the wrench produces a torque about the screw. Similarly, a force applied at the circumference of a gear attached to an axle produces a torque about the axle. The perpendicular distance d from the line of force to the axis is called the moment arm. In the following diagram, the circle represents a gear of radius d. The dot in the center represents the axle (A). A force F is applied at the edge of the gear, tangentially. F d A Diagram 1 In this example, the radius of the gear is the moment arm. The force is acting along a tangent to the gear, so it is perpendicular to the radius. The amount of torque at A about the gear axle is defined as = F×d 1 We use the Greek letter Tau ( ) to represent torque.