Larmor’s Theorem LL2 Section 45. System of charges, finite motion, external constant H-field Time average force Time average of time derivative of quantity.

Slides:



Advertisements
Similar presentations
Chapter 9 Momentum and Its Conservation
Advertisements

Sect 5.9: Precession of Systems of Charges in a Magnetic Field A brief discussion of something that is not rigid body motion. Uses a similar formalism.
Chapter 10 Rotational Motion
AS 4002 Star Formation & Plasma Astrophysics BACKGROUND: Maxwell’s Equations (mks) H (the magnetic field) and D (the electric displacement) to eliminate.
Angular Momentum (of a particle) O The angular momentum of a particle, about the reference point O, is defined as the vector product of the position, relative.
Larmor Formula: radiation from non-relativistic particles
Department of Physics and Applied Physics , F2010, Lecture 18 Physics I LECTURE 18 11/15/10.
Adiabatic Invariance. Slow Changes  A periodic system may have slow changes with time. Slow compared to periodSlow compared to period Phase space trajectory.
Mechanics of Rigid Bodies
Nuclear de-excitation Outline of approach… Source of radiation Propagation of radiation field Detection of radiation ?? nucleus.
Angular Momentum. Moments  The moment of a vector at a point is the wedge product.  This is applied to physical variables in rotating systems. Applied.
A B C D. Find currents through resistors Loop 1Loop 2Loop 3 Loop 4 I1I1 I2I2 I3I3 I5I5 I4I4 loop 1: loop 2: loop 3: nodes: Five independent equations.
Physics for Scientists and Engineers II, Summer Semester Lecture 11: June 15 th 2009 Physics for Scientists and Engineers II.
March 2, 2011 Fill in derivation from last lecture Polarization of Thomson Scattering No class Friday, March 11.
The Magnetic Field The force on a charge q moving with a velocity The magnitude of the force.
Symmetries and conservation laws
Dispersion of the permittivity Section 77. Polarization involves motion of charge against a restoring force. When the electromagnetic frequency approaches.
Central Force Motion Chapter 8
Electromagnetic wave equations: dielectric without dispersion Section 75.
Plasma in time-varying B-field. Particle acceleration Consider a plasma in a homogeneous magnetic field changing in time We then have: Using Stokes theorem:
PHY221 Ch19/20: Angular Momentum 1.Main Points: Definition Proof dL/dt=  Proof L=I  for a rigid body Conservation of L 2.Examples Person running and.
Energy momentum tensor of macroscopic bodies Section 35.
Magnetic Field.
Classical Mechanics 420 J. D. Gunton Lewis Lab 418
Motion in a constant uniform magnetic field Section 21.
Geometrical Optics LL2 Section 53. Local propagation vector is perpendicular to wave surface Looks like a plane wave if amplitude and direction are ~constant.
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.
The forces on a conductor Section 5. A conductor in an electric field experiences forces.
Lagrangian to terms of second order LL2 section 65.
The Spinning Top Chloe Elliott. Rigid Bodies Six degrees of freedom:  3 cartesian coordinates specifying position of centre of mass  3 angles specifying.
Sect. 1.2: Mechanics of a System of Particles Generalization to many (N) particle system: –Distinguish External & Internal Forces. –Newton’s 2 nd Law.
Ch. 21 Electric Forces & Fields
POSITION AND COORDINATES l to specify a position, need: reference point (“origin”) O, distance from origin direction from origin (to define direction,
CH Review -- how electric and magnetic fields are created Any charged particle creates an electric field at all points in space around it. A moving.
Constant magnetic field LL2 section 43. Electrons in atoms and circuits all perform finite motion. This creates magnetic fields that are constant when.
Motion of a conductor in a magnetic field Section 63.
Energy-momentum tensor of the electromagnetic field
Permittivity at high frequency Section 78. At high frequency, polarization processes cannot keep up. P = 0 D = E + 4  P = E How does  approach unity.
The Lagrangian to terms of second order LL2 section 65.
Chapter 1: Survey of Elementary Principles
Advanced Computer Graphics Spring 2014 K. H. Ko School of Mechatronics Gwangju Institute of Science and Technology.
P Spring 2002 L4Richard Kass Conservation Laws When something doesn’t happen there is usually a reason! Read: M&S Chapters 2, 4, and 5.1, That something.
Central Force Umiatin,M.Si. The aim : to evaluate characteristic of motion under central force field.
ELECTROMAGNETIC PARTICLE: MASS, SPIN, CHARGE, AND MAGNETIC MOMENT Alexander A. Chernitskii.
Magnetic Fields Chapter 29 Permanent Magnets & Magnetic Field Lines The Magnetic Force on Charges.
Constant Electromagnetic Field Section 19. Constant fields E and H are independent of time t.  and A can be chosen time independent, too.
Magnetism. Our most familiar experience of magnetism is through permanent magnets. These are made of materials which exhibit a property we call “ferromagnetism”
Particle Kinematics Direction of velocity vector is parallel to path Magnitude of velocity vector is distance traveled / time Inertial frame – non accelerating,
Equations of motion of a charge in a field Section 17.
Field of uniformly moving charge LL2 Section 38. Origins are the same at t = 0. Coordinates of the charge e K: (Vt, 0, 0) K’: (0, 0, 0)
Test 2 review Test: 7 pm in 203 MPHY
Charge in a constant uniform electric & magnetic field
Forces & Newton’s First Law
System of charges in an external field
Magnetic Dipoles and Angular Momenta
Ch 8 : Rotational Motion .
Lecture Rigid Body Dynamics.
Dipole Radiation LL2 Section 67.
الفصل 1: الحركة الدورانية Rotational Motion
Chapter 9 Momentum and Its Conservation
Chapter 6 Objectives Compare the momentum of different moving objects.
Forces & Newton’s First Law
Diatomic molecules
Canonical Quantization
Scattering by free charges
G. A. Krafft Jefferson Lab Old Dominion University Lecture 1
Chapter 28 Magnetic Fields
Physics 319 Classical Mechanics
Forces & Newton’s First Law
LECTURE 12 SPINS Source: D. Griffiths, Introduction to Quantum Mechanics (Prentice Hall, 2004) R. Scherrer, Quantum Mechanics An Accessible Introduction.
Presentation transcript:

Larmor’s Theorem LL2 Section 45

System of charges, finite motion, external constant H-field Time average force Time average of time derivative of quantity with finite variations

Time averaged torque Time average of time derivative of quantity with finite variations

Compare with electric dipole

Lagrangian for charge in a given electro-magnetic field Free particle term If no external electric field. Lagrangian for system of charges in an external constant uniform H-field For closed system Extra term due to external H- field,

(19.4) for uniform H-field Compare

Centrally symmetric electric field. System of charges, finite motion, v<<c, e.g. electrons of atom Transform to rotation reference frame Velocity in lab frame Velocity in rotating frame  r Suppose v’ = 0, Then v = -  x r -  x r

Lagrangian of system of charges in lab frame L =  ½ mv’ 2 - U U is a function of the distances from the e a to Q and of the distances between the e a. This function is unchanged by the transform to the rotating frame. Lagrangian of system of charges in rotating frame

Assume e/m is the same for all particles, e.g. electrons of an atom. And choose Neglect for small H

Lagrangian for closed system when v<<c Lagrangian for external constant uniform H-field - U

Larmor Theorem: System of charges Non-relativistic Same e/m, Finite motion Central E-field Weak H field, Coordinates not rotating No H-field, Coordinates rotating at  = eH/2mc = “Larmor frequency” These two problems have the same Lagrangian

For sufficiently weak H,  = eH/2mc << frequencies of finite motion of charges Then, average quantities describing the system over t << 2  /  = Larmor period Averaged quantities will vary slowly with time at frequency .

Time averaged angular momentum t If e/m is the same for all particles, m = eM/2mc (44.5) torque Larmor precession: and rotate around H Without changing |M|