Lagrangian to terms of second order LL2 section 65.

Slides:



Advertisements
Similar presentations
Relativistic mechanics
Advertisements

EMLAB 1 Solution of Maxwell’s eqs for simple cases.
Larmor Formula: radiation from non-relativistic particles
Feb 25, RETARDED POTENTIALS At point r =(x,y,z), integrate over charges at positions r’ (7) (8) where [ρ]  evaluate ρ at retarded time: Similar.
EEE340Lecture : Electromagnetic Boundary Conditions E 1t =E 2t, always. B 1n =B 2n, always. For PEC, the conductor side H 2 =0, E 2 =0. (7.66b)
The Klein Gordon equation (1926) Scalar field (J=0) :
Symmetries and conservation laws
Part 2.  Review…  Solve the following system by elimination:  x + 2y = 1 5x – 4y = -23  (2)x + (2)2y = 2(1)  2x + 4y = 2 5x – 4y = -23  7x = -21.
Reference Book is. NEWTON’S LAW OF UNIVERSAL GRAVITATION Before 1687, clear under- standing of the forces causing plants and moon motions was not available.
Central Force Motion Chapter 8
A PPLIED M ECHANICS Lecture 02 Slovak University of Technology Faculty of Material Science and Technology in Trnava.
Advanced EM Master in Physics Electromagnetism and special relativity We have nearly finished our program on special relativity… And then we.
Advanced EM - Master in Physics Magnetic potential and field of a SOLENOID Infinite length N spires/cm Current I Radius R The problem -for.
Absorption and Emission of Radiation:
For s=1 for EM-waves total energy density:  # of photons wave number vector: the Klein-Gordon equation:
Geometrical Optics LL2 Section 53. Local propagation vector is perpendicular to wave surface Looks like a plane wave if amplitude and direction are ~constant.
BH Astrophys Ch6.6. The Maxwell equations – how charges produce fields Total of 8 equations, but only 6 independent variables (3 components each for E,B)
Action function of the electromagnetic field Section 27.
The System of Equations of Interacting Electromagnetic, Scalar Gravitational and Spinor Fields Anatoliy N. SERDYUKOV Francisk Skorina Gomel State University.
Four-potential of a field Section 16. For a given field, the action is the sum of two terms S = S m + S mf – Free-particle term – Particle-field interaction.
The forces on a conductor Section 5. A conductor in an electric field experiences forces.
“Significance of Electromagnetic Potentials in the Quantum Theory”
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.
Characteristic vibrations of the field. LL2 section 52.
O Aim of the lecture  Gauss’ Law: Flux More mathematical descriptions Generalised field distributions o Main learning outcomes  familiarity with  Electric.
Advanced EM - Master in Physics Poynting’s theorem Momentum conservation Just as we arrived to the Poynting theorem – which represents the.
Phy 303: Classical Mechanics (2) Chapter 3 Lagrangian and Hamiltonian Mechanics.
POSITION AND COORDINATES l to specify a position, need: reference point (“origin”) O, distance from origin direction from origin (to define direction,
Work and Energy. Scalar (Dot) Product When two vectors are multiplied together a scalar is the result:
Module 10Energy1 Module 10 Energy We start this module by looking at another collision in our two inertial frames. Last time we considered a perfectly.
Constant magnetic field LL2 section 43. Electrons in atoms and circuits all perform finite motion. This creates magnetic fields that are constant when.
The Lagrangian to terms of second order LL2 section 65.
EXPRESSIONS This is what expressions are…. By Shayde.
Ch. 8: Summary So Far We’re doing the “2 body”, conservative central force problem! 2 bodies (m 1 & m 2 ) with a central force directed along the line.
For s=1 for EM-waves total energy density:  # of photons wave number vector: the Klein-Gordon equation:
ELECTROMAGNETIC PARTICLE: MASS, SPIN, CHARGE, AND MAGNETIC MOMENT Alexander A. Chernitskii.
1 Electric Potential Reading: Chapter 29 Chapter 29.
Four dimensional current vector Section 28. For convenience, we often consider a distribution of point charges to be a continuous distribution of charge.
Constant Electromagnetic Field Section 19. Constant fields E and H are independent of time t.  and A can be chosen time independent, too.
The wave equation LL2 Section 46. In vacuum,  = 0 and j = 0. These have non-trivial solutions. Thus, electromagnetic fields can exist without charges.
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.
Chapter 1. The principle of relativity Section 1. Velocity of propagation of interaction.
EMLAB 1 Chapter 1. Vector analysis. EMLAB 2 Mathematics -Glossary Scalar : a quantity defined by one number (eg. Temperature, mass, density, voltage,...
Equations of motion of a charge in a field Section 17.
The retarded potentials LL2 Section 62. Potentials for arbitrarily moving charges 2 nd pair of Maxwell’s equations (30.2) in 4-D.
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)
Canonical Quantization
MAT Classical Mechanics
Ionization losses by fast particles in matter, non-relativistic case
Maxwell’s Equations in Terms of Potentials
System of charges in an external field
Spectral resolution of the retarded potentials
Section C: Impulse & Momentum
Virial Theorem LL2 Section 34.
Lecture 20.
Warm-up September 14, 2017 Change to a decimal: 87% 7%
Electromagnetic field tensor
Hamiltonian Mechanics
Dipole Radiation LL2 Section 67.
Lienard-Wiechert Potentials
Quantum One.
Quantum Two.
What is the GROUND STATE?
General theory of scattering in isotropic media
Field of a system of charges at large distances
Chapter 29 Electric Potential Reading: Chapter 29.
Physics 319 Classical Mechanics
Physics 319 Classical Mechanics
Relativistic Quantum Mechanics
Physics 451/551 Theoretical Mechanics
Presentation transcript:

Lagrangian to terms of second order LL2 section 65

Classical mechanics: instantaneous interactions. – In Lagrangian L depends on q and dq/dt for all particles at the same time t. – Field is just a mathematical convenience

Relativistic mechanics: finite velocity of propagation. – Field is independent system – Lagrangian for interaction of particles must include degrees of freedom for the field

If v<<c, we seek the Lagrangian to order (v/c) 2 – Electromagnetic radiation appears only in the next (3 rd ) approximation.

Zeroth approximation (no powers of v/c, classical) Exact Lagrangian for a particle e a in given fields At the position of potentials are determined from positions and motions of all other charges Retarded potentials

If v << c for all charges, then  changes little during time R/c Expandin powers of R/c All terms evaluated at R/c = 0, i.e. at the present time t, Total charge of system = constant Second term is zero

Scalar potential to second order in 1/c The expression for A already contains a factor 1/c. Then A gets multiplied again by 1/c in the Lagrangian. Keep only the 1 st term in the expansion. Evaluated at present time t Substitute these potentials in the Lagrangian to find approximate L to order (v/c) 2.

Single point charge R(t) = |r – r 0 (t)| is time dependent We can get rid of this by gauge transform

Gauge transform Let Now the extra term appears in A’ Lorentz condition is not satisfied. Neither is

With respect to field point coordinates What is this?

For multiple charges, sum their contributions, e.g.

Lagrangian for charge e a using and ignoring constant mc 2 Compare to zeroth order Lagrangian Exact Approximate to 2 nd order in v/c

Small corrections Mechanics, volume 1, equation (40.7): For small changes to L and H, the additions are equal in magnitude, but opposite in sign.