Lagrangian Theory. Several-body Systems

Similar documents
Physics 181. Particle Systems

12. The Hamilton-Jacobi Equation Michael Fowler

Physics 5153 Classical Mechanics. D Alembert s Principle and The Lagrangian-1

Physics 53. Rotational Motion 3. Sir, I have found you an argument, but I am not obliged to find you an understanding.

THE VIBRATIONS OF MOLECULES II THE CARBON DIOXIDE MOLECULE Student Instructions

PHYS 705: Classical Mechanics. Newtonian Mechanics

Physics 5153 Classical Mechanics. Principle of Virtual Work-1

Salmon: Lectures on partial differential equations. Consider the general linear, second-order PDE in the form. ,x 2

The Feynman path integral

Numerical Heat and Mass Transfer

CHAPTER 14 GENERAL PERTURBATION THEORY

Week3, Chapter 4. Position and Displacement. Motion in Two Dimensions. Instantaneous Velocity. Average Velocity

Lecture 12: Discrete Laplacian

PHYS 705: Classical Mechanics. Calculus of Variations II

1 Matrix representations of canonical matrices

Physics 106a, Caltech 11 October, Lecture 4: Constraints, Virtual Work, etc. Constraints

Lecture 20: Noether s Theorem

Linear Approximation with Regularization and Moving Least Squares

Spin-rotation coupling of the angularly accelerated rigid body

C/CS/Phy191 Problem Set 3 Solutions Out: Oct 1, 2008., where ( 00. ), so the overall state of the system is ) ( ( ( ( 00 ± 11 ), Φ ± = 1

So far: simple (planar) geometries

Molecular structure: Diatomic molecules in the rigid rotor and harmonic oscillator approximations Notes on Quantum Mechanics

ELASTIC WAVE PROPAGATION IN A CONTINUOUS MEDIUM

Physics 207: Lecture 20. Today s Agenda Homework for Monday

The classical spin-rotation coupling

11. Dynamics in Rotating Frames of Reference

Rigid body simulation

Introduction to Vapor/Liquid Equilibrium, part 2. Raoult s Law:

U.C. Berkeley CS294: Beyond Worst-Case Analysis Luca Trevisan September 5, 2017

Kernel Methods and SVMs Extension

Integrals and Invariants of Euler-Lagrange Equations

coordinates. Then, the position vectors are described by

10. Canonical Transformations Michael Fowler

Difference Equations

Physics 111: Mechanics Lecture 11

χ x B E (c) Figure 2.1.1: (a) a material particle in a body, (b) a place in space, (c) a configuration of the body

EPR Paradox and the Physical Meaning of an Experiment in Quantum Mechanics. Vesselin C. Noninski

LAGRANGIAN MECHANICS

STAT 309: MATHEMATICAL COMPUTATIONS I FALL 2018 LECTURE 16

Moments of Inertia. and reminds us of the analogous equation for linear momentum p= mv, which is of the form. The kinetic energy of the body is.

Week 9 Chapter 10 Section 1-5

Poisson brackets and canonical transformations

Spring 2002 Lecture #13

Lectures - Week 4 Matrix norms, Conditioning, Vector Spaces, Linear Independence, Spanning sets and Basis, Null space and Range of a Matrix

Chapter 5. Solution of System of Linear Equations. Module No. 6. Solution of Inconsistent and Ill Conditioned Systems

Chapter 3. r r. Position, Velocity, and Acceleration Revisited

The Multiple Classical Linear Regression Model (CLRM): Specification and Assumptions. 1. Introduction

MEASUREMENT OF MOMENT OF INERTIA

Lecture 10 Support Vector Machines II

Lagrange Multipliers. A Somewhat Silly Example. Monday, 25 September 2013

The non-negativity of probabilities and the collapse of state

where the sums are over the partcle labels. In general H = p2 2m + V s(r ) V j = V nt (jr, r j j) (5) where V s s the sngle-partcle potental and V nt

Canonical transformations

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force.

One Dimension Again. Chapter Fourteen

Snce h( q^; q) = hq ~ and h( p^ ; p) = hp, one can wrte ~ h hq hp = hq ~hp ~ (7) the uncertanty relaton for an arbtrary state. The states that mnmze t

n α j x j = 0 j=1 has a nontrivial solution. Here A is the n k matrix whose jth column is the vector for all t j=0

Quantum Mechanics I Problem set No.1

Workshop: Approximating energies and wave functions Quantum aspects of physical chemistry

U.C. Berkeley CS294: Spectral Methods and Expanders Handout 8 Luca Trevisan February 17, 2016

Temperature. Chapter Heat Engine

Tensor Analysis. For orthogonal curvilinear coordinates, ˆ ˆ (98) Expanding the derivative, we have, ˆ. h q. . h q h q

10-701/ Machine Learning, Fall 2005 Homework 3

How Differential Equations Arise. Newton s Second Law of Motion

Section 8.3 Polar Form of Complex Numbers

Mathematical Preparations

3.1 Expectation of Functions of Several Random Variables. )' be a k-dimensional discrete or continuous random vector, with joint PMF p (, E X E X1 E X

Some Comments on Accelerating Convergence of Iterative Sequences Using Direct Inversion of the Iterative Subspace (DIIS)

Integrals and Invariants of

9 Derivation of Rate Equations from Single-Cell Conductance (Hodgkin-Huxley-like) Equations

2.3 Nilpotent endomorphisms

APPENDIX A Some Linear Algebra

Global Sensitivity. Tuesday 20 th February, 2018

1 Derivation of Rate Equations from Single-Cell Conductance (Hodgkin-Huxley-like) Equations

Linear Momentum. Center of Mass.

Chapter Twelve. Integration. We now turn our attention to the idea of an integral in dimensions higher than one. Consider a real-valued function f : D

The exponential map of GL(N)

Georgia Tech PHYS 6124 Mathematical Methods of Physics I

r i r j 3. (2) Gm j m i r i (r i r j ) r i r j 3. (3)

Mechanics Physics 151

Week 11: Chapter 11. The Vector Product. The Vector Product Defined. The Vector Product and Torque. More About the Vector Product

NEWTON S LAWS. These laws only apply when viewed from an inertial coordinate system (unaccelerated system).

More metrics on cartesian products

CME 302: NUMERICAL LINEAR ALGEBRA FALL 2005/06 LECTURE 13

CSci 6974 and ECSE 6966 Math. Tech. for Vision, Graphics and Robotics Lecture 21, April 17, 2006 Estimating A Plane Homography

Applied Nuclear Physics (Fall 2004) Lecture 23 (12/3/04) Nuclear Reactions: Energetics and Compound Nucleus

2E Pattern Recognition Solutions to Introduction to Pattern Recognition, Chapter 2: Bayesian pattern classification

First Law: A body at rest remains at rest, a body in motion continues to move at constant velocity, unless acted upon by an external force.

Classical Mechanics Virtual Work & d Alembert s Principle

MEV442 Introduction to Robotics Module 2. Dr. Santhakumar Mohan Assistant Professor Mechanical Engineering National Institute of Technology Calicut

Iterative General Dynamic Model for Serial-Link Manipulators

Classical Field Theory

4. Laws of Dynamics: Hamilton s Principle and Noether's Theorem

6. Hamilton s Equations

Solution of Linear System of Equations and Matrix Inversion Gauss Seidel Iteration Method

Three views of mechanics

PY2101 Classical Mechanics Dr. Síle Nic Chormaic, Room 215 D Kane Bldg

8.592J: Solutions for Assignment 7 Spring 2005

The equation of motion of a dynamical system is given by a set of differential equations. That is (1)

APPROXIMATE PRICES OF BASKET AND ASIAN OPTIONS DUPONT OLIVIER. Premia 14

Transcription:

Lagrangan Theory of Several-body Systems Ncholas Wheeler, Reed College Physcs Department November 995 Introducton. Let the N-tuple of 3-vectors {x (t) : =, 2,..., N} descrbe, relatve to an nertal frame, the confguraton of an N-partcle system at tme t. To descrbe the dynamcs of the system we would fnd t natural to ntroduce the Lagrangan L = 2 m ẋ ẋ U(x, x 2,..., x N ) () Suppose, however, we had elected to descrbe the partcles n terms of ther Cartesan relatonshp to a reference pont X(t) n arbtrarly prescrbed moton: x = X + r. We would then have L = 2 m (Ẋ + ṙ ) (Ẋ + ṙ ) U(X + r) = 2 MẊ Ẋ + Ẋ m ṙ + 2 m ṙ ṙ U(X + r) (2) n whch the dynamcal varables formerly {x, x 2,..., x N }, presently {r, r 2,..., r N } are stll (as before, and not at all surprsngly) N n number. The equatons of moton now read m r = m Ẍ U(X + r) ( =, 2,..., N) (3) n whch we nterpret the frst term on the rght to be a fcttous force term, an artfact of the crcumstance that the orgn of the X-centered r-frame s (except when Ẍ = 0) non-nertal. None of whch s n any respect problematc.

2 Lagrangan theory of several body systems Now wth an eye to the algebrac smplfcaton of (2) mpose upon the r-varables ths constrant: m r = 0 (4.) Equvalently, assocate X wth the center of mass of the N-partcle system: X = m x wth M = M m (4.2) Equaton (2) can now be notated L = 2 MẊ Ẋ + 2 m ṙ ṙ U(X + r) (5) (note the dsappearance of the cross-term), whch on ts face appears to refer to a system wth dynamcal varables {X, r, r 2,..., r N } more numerous that the varables of the system wth whch we started. And (5) gves rse to equatons of moton whch are not only more numerous than but also nconsstent wth equatons (3). What s gone wrong? In (4) we see that when we subjected the varables x to a cross-term-kllng constrant we effectvely promoted X to the status of a dynamcal varable; t s, accordng to (4.2), a varable a collectve varable whose t-dependence has now to be extracted from equatons of moton, and can no longer be sad to be arbtrarly prescrbed. But the Lagrangan (5) s heedless of ths crcumstance, and gves rse to equatons of moton the solutons of whch wll, n general, stand n volaton of (4.). To obtan correct results we mght, for example, ntroduce N N r N = m N m r and ṙ N = m N m ṙ nto (5) to obtan a Lagrangan of type L(Ẋ, ṙ,..., ṙ N, X, r,..., r N ), but such a procedure bears the formal blemsh of a dscrmnatory asymmetry not natural to the physcs of the stuaton. How to proceed more symmetrcally? In place of (5) wrte L = 2 MẊ Ẋ + 2 m ṙ ṙ U(X + r) g m r (6) where g s a Lagrange multpler whch wll be accorded the formal status of a supernumerary dynamcal varable. The resultng equatons of moton read MẌ = U (7.) m r = U gm ( =, 2,..., N) (7.2) 0 = m r (7.3)

A smple example: the one-dmensonal A 2 molecule 3 where =. These are N + 2 equatons of moton n as many varables. The last of these the g th Lagrange equaton of moton (7.3) s smply the constrant relaton (4.), and entals m r = 0. Addng equatons (7.2) together, and subtractng the result from (7.), we obtan The equatons of moton (7) reduce therefore to g = Ẍ (8) MẌ = U (9.) m { r + Ẍ} = U ( =, 2,..., N) (9.2) whch are attractvely symmetrc (no r has been dscrmnated aganst), but redundant: addng equatons (9.2) together gves back (9.). Equatons (9.2) are consstent wth (3), of whch they are a partcularzed nstance. It s nstructve to note also that the ntroducton of (8) nto (6) yelds a Lagrangan whch s dstnct from but (by Ẍ m r = d dt [Ẋ m r ] Ẋ m ṙ ) gauge equvalent to the Lagrangan of (2). A smple example: the one-dmensonal A 2 molecule. We look now to the Lagrangan theory of what mght be called a one-dmensonal A 2 molecule. The consttuent atoms resde at x and x 2 > x, and both have mass m. The molecule tself therefore has mass M = 2m. We assume the molecule to be bound together by a sprng of natural length a and strength k, and to move n an ambent potental U(x). In natural varables the Lagrangan reads L = 2 m(ẋ2 + ẋ 2 2) U(x ) U(x 2 ) 2 k[(x 2 x ) a] 2 (0) The varables ntutvely most natural to ths smple system are the external coordnate X = M (mx + mx 2 ) = 2 (x + x 2 ) and the nternal coordnate 2s = x 2 x, whch descrbes the nstantaneous length of the molecule. Immedately } x = X s x 2 = X + s () gvng L = m(ẋ2 + ṡ 2 ) U(X s) U(X + s) 2 k(2s a)2 (3) It becomes analytcally advantageous at ths pont to ntroduce the varable q = 2s a whch descrbes molecular length relatve to the rest length of the molecule;

4 Lagrangan theory of several body systems then s = 2 (a + q) and we have where K = 2k and We are led thus to wrte L = mẋ2 + 2 { 2 m q2 2 Kq2 } U(X, q) U(X, q) = U(X + s) + U(X s) = {U(X) + U (X)s + 2 U (X)s 2 +...} + {U(X) U (X)s + 2 U (X)s 2 +...} = 2U(X) + U (X)s 2 +... L = {mẋ2 2U(X)} + 2 { 2 m q2 2 Kq2 } U nteracton (X, q) (4) wth U nteracton (X, q) = 4 U (X)(a 2 + 2aq + q 2 ) +... = 2 au (X) q +... The operatve assumpton here s that the ambent potental changes lttle over the dmenson of the molecule. The strkng absence of a U (X)-term s an artfact of our assumpton that m = m 2 = m, and means that the nteracton s, n leadng approxmaton, tdal. In ths respect the physcs of A 2 molecules s dstnct from the physcs of AB molecules. Lookng now to the equatons of moton mẍ = U (X) 2 qau (X) (5.) m q + Kq = au (X) (5.2) we fnd t natural on physcal grounds to abandon the 2 nd term on the rght sde of (5.). Returnng wth X(t) a soluton of the equaton thus obtaned to (5.2), we have m q + Kq = F(t) wth F(t) = au (X(t)) (6) Evdently the tdal term on the rght sde of (5.2) serves n effect to force the nternal oscllaton of the molecule. The reader who was awatng the entry of relatve varables r and r 2 nto the preceedng dscusson wll have been struck by ther absence. Ther non-appearance can be attrbuted to the crcumstance that the asymmetry problem whch motvated our ntal dscusson does not arse n the case N = 2; t s non-dscrmnatory to speak of s = 2 (r 2 r ). In ths respect the physcs of A n molecules (n > 2) s margnally more nterestng. The physcs even of A 2 molecules becomes markedly more nterestng when we gve up the one-dmensonalty or our problem, for then the molecule can be expected to experence torques, and to tumble n ways responsve to the dervatve

A less smple example: the one-dmensonal A 3 molecule 5 structure of U(X); I shall, however, resst the temptaton to enter nto an mmedate dscusson of the detals. A less smple example: the one-dmensonal A 3 molecule. We now assume partcles of dentcal mass m to resde at x, x 2 > x and x 3 > x 2 and to be bound by sprngs dentcal to those encountered n the prevous example. In natural varables the Lagrangan (compare (0)) reads L = 2 m(ẋ2 + ẋ 2 2 + ẋ 2 3) U(x ) U(x 2 ) U(x 3 ) 2 k{[(x 2 x ) a] 2 + [(x 3 x 2 ) a] 2 } (7) Drect appropraton of (6) gves rse for such a system to L = 2 MẊ2 + 2 m(ṙ2 + ṙ 2 2 + ṙ 2 3) U(X + r ) U(X + r 2 ) U(X + r 3 ) 2 k[(r 2 r ) a] 2 2 k[(r 3 r 2 ) a] 2 g m(r + r 2 + r 3 ) (8) where M = 3m s the mass of the A 3 molecule, and where X = 3 (x + x 2 + x 3 ) serves to locate ts center of mass. Equatons (9) acqure therefore ths partcularzed meanng: MẌ = U (X + r ) U (X + r 2 ) U (X + r 3 ) (9.) m( r + Ẍ) = U (X + r ) + k[(r 2 r ) a] m( r 2 + Ẍ) = U (X + r 2 ) k[(r 2 r ) a] + k[(r 3 r 2 ) a] (9.2) m( r 3 + Ẍ) = U (X + r 3 ) k[(r 3 r 2 ) a] Lookng frst to (9.), we observe that RHS of (9.) = 3U (X) m U (X) 3 mr 2m U (X) 3 mr 2 +... (20) The second term on the rght vanshes by defnton of the center of mass. It s nterestng n ths lght to notce that the sum encountered n the thrd term on the rght serves to defne the nstantaneous moment of nerta relatve to the center of mass (.e., the centered second moment of the molecular mass dstrbuton), and that the sums encountered n hgher-order terms defne nameless hgher moments of the mass dstrbuton. Upon the abandonment of all such neglgble terms, (9.) reduces to mẍ = U (X): the center of mass moves as a sngle atom would move n the ambent potental. Lookng now to (9.2), we are motvated by the structure of the sprng terms to ntroduce } q = (r 2 r ) a (2) q 2 = (r 3 r 2 ) a Inverson of q + a = r + r 2 q 2 + a = r 2 + r 3 0 = +r + r 2 + r 3

6 Lagrangan theory of several body systems gves r = 3 (2q + q 2 ) a r 2 = + 3 ( q q 2 ) r 3 = + 3 ( q + 2q 2 ) + a (22) and when we return wth (2) and (22) to (8) we by computaton obtan (compare (4)) L = 3{ 2 mẋ2 U(X)} + { 3 m( q2 + q q 2 + q 2 2) 2 k(q2 + q 2 2)} U nteracton (X, q, q 2 ) (23) where U nteracton (X, q, q 2 ) = 2m U (X) m [ 2 9 a2 + 2 9 a(q 2 q ) = 9 au (X) (q 2 q ) +... + 2 3 (q2 + q q 2 + q 2 2) ] +... To better emphasze the essentals of the stuaton as t now stands, I wrte L = L center of mass (Ẋ, X) + L nternal( q, q) + L nteracton (X, q) and assert (on the physcal grounds to whch I have already alluded, and to a more careful dscusson of whch I promse to return) that L nteracton (X, q) contrbutes essentally to the moton of the nternal varables q, but nessentally to the moton of X. We are led thus to the equatons of moton mẍ = U (X) (24.) { d } L = 0 ( =, 2) (24.2) dt q q where L = L nternal ( q, q) + L nteracton (X(t), q). I have refraned from wrtng out the detaled mplcatons of (24.2) because those equatons are not welladapted to analytcal treatment. To obtan more workable equatons we very The tedum of the computaton s much reduced f one wrtes r r 2 = G q q 2 and ṙ ṙ 2 = G q 2 q 2 wth G = 3 + 0 r 3 a ṙ 3 0 2 and notces that G T G = 6 3 9 3 6 2 for then (r 2 + r 2 2 + r 2 3) and (ṙ 2 + ṙ 2 2 + ṙ 2 3) become qute easy to evaluate.

A less smple example: the one-dmensonal A 3 molecule 7 much n the sprt of standard small oscllaton theory subject L nternal ( q, q) to some preparatory massagng. Wrtng T L nternal ( q, q) = 6 m q M q 2 wth M = ( q q 2 ) T 2 k q K q 2 2 2 ( q K = q 2 ) 0 0 we ntroduce new varables (wrte q = RQ wth R a rotaton matrx: R T R = I) to obtan T T Q L nternal ( Q, Q) = 6 m Q R Q T M R 2 Q 2 k Q R T K R 2 Q 2 ( Q Q 2 ) (25) and look to the smultaneous dagonalzaton of R T M R and R T K R. Ths, of course, s standard theory of small oscllatons methodology; the only unusual crcumstance s that here t s not be sprng matrx K but the mass matrx M whch comes to us n ntally non-dagonal form. Some prelmnary observatons: from det(m λi) = λ 2 4λ + 3 we conclude that the egenvalues of M can be descrbed λ = 2 ±, and that our assgnment, therefore, s to dscover the matrx cos ϕ sn ϕ R = sn ϕ cos ϕ such that R T M R = 0 0 3 Our assgnment (to say the same thng another way) s to dscover the ϕ such that ( 2 cos = 2 ϕ + 3 sn 2 ) ϕ 2 sn ϕ cos ϕ 2 2 sn ϕ cos ϕ sn 2 ϕ + 3 cos 2 ϕ Immedately ϕ = 45, gvng R = 2 (26) In any event qute apart from the detals of the argument whch led us to (26) we have only to nsert (26) nto (25) to obtan L nternal ( Q, Q) = 6 m( Q 2 + 3 Q 2 2) 2 k(q2 + Q 2 ) The modal moton of the free A 3 molecule can therefore be descrbed Q + ω 2 Q = 0 (27)

8 Lagrangan theory of several body systems wth ω = 3k/m ω 2 = k/m (28) For such a molecule (.e., for a one-dmensonal A 3 molecule n the total absence of an ambent potental) we have X(t) = X 0 + V 0 t q (t) = A cos(ω t + δ ) + A 2 cos(ω 2 t + δ 2 ) q 2 (t) = A cos(ω t + δ ) + A 2 cos(ω 2 t + δ 2 ) so (recall (22)) n natural varables we have the followng explct descrpton of the free moton latent n the Lagrangan (7): x (t) = X(t) 3 A cos(ω t + δ ) A 2 cos(ω 2 t + δ 2 ) x 2 (t) = X(t) + 2 3 A cos(ω t + δ ) x 3 (t) = X(t) 3 A cos(ω t + δ ) + A 2 cos(ω 2 t + δ 2 ) (29) These equatons make clear the sense n whch the fast mode (the mode under the control of A ) s a hp-swngng mode, and the slow mode (controlled by A 2 ) s a breather mode a dance n whch m 2 does not partcpate. So much for the free moton of the system. Now renstate the ambent potental U(x). The moton X(t) of the center of mass s now no longer unform, but accelerated as descrbed (n leadng approxmaton) by (24.). Of more partcular nterest s the fact that L nteracton = 9 au (X(t)) (q q 2 ) = F(t) Q where F(t) = 2 9 au (X(t)). The mplcaton s that tdal forces couple (n leadng approxmaton) only to the fast mode. Ths I fnd somewhat counterntutve, snce t s the slow breather mode of the A 3 molecule whch most resembles the soltary mode of the A 2 molecule a breather mode whch, as we know from prevous work, does respond to tdal forces. From L molecular ( Q, Q, t) = 6 m( Q 2 + 3 Q 2 2) 2 k(q2 + Q 2 ) + F(t) Q we obtan Q + ω 2 Q = 3 m F(t) Q 2 + ω 2 2Q 2 = 0 (30) whch gve back (27) n the absence of tdal forces. Moton of a struck A 3 molecule. In place of (7) we now have L = 2 m(ẋ2 + ẋ 2 2 + ẋ 2 3) 2 k{[(x 2 x ) a] 2 + [(x 3 x 2 ) a] 2 } x F (t) the nessental assumpton here beng that (snce objects are most commonly struck on ther exposed surfaces) t s the end-partcle m whch has been struck.