Scattering by free charges

Slides:



Advertisements
Similar presentations
NASSP Self-study Review 0f Electrodynamics
Advertisements

Chapter 1 Electromagnetic Fields
Interaction of Electromagnetic Radiation with Matter
Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley. Chapter 35. Electromagnetic Fields and Waves To understand a laser beam,
Two questions: (1) How to find the force, F on the electric charge, Q excreted by the field E and/or B? (2) How fields E and/or B can be created? Gauss’s.
Now that we have determined the solutions to the differential equation describing the oscillations of the electric and magnetic fields with respect to.
Lecture 13 Electromagnetic Waves Ch. 33 Cartoon Opening Demo Topics –Electromagnetic waves –Traveling E/M wave - Induced electric and induced magnetic.
Chapter 23 Electromagnetic Waves. Formed from an electric field and magnetic field orthonormal to each other, propagating at the speed of light (in a.
Larmor Formula: radiation from non-relativistic particles
March 4, 2011 Turn in HW 5; Pick up HW 6 Today: Finish R&L Chapter 3 Next: Special Relativity.
p.1067 Ch 34 Electromagnetic Waves 34.1 Displacement Current and the General Form of Ampere’s Law I d =  0 d  E /dt B·ds =  0 (I + I d ) 
Physics 1402: Lecture 26 Today’s Agenda Announcements: Midterm 2: NOT Nov. 6 –About Monday Nov. 16 … Homework 07: due Friday this weekHomework 07: due.
Prof. Reinisch, EEAS / Simple Collision Parameters (1) There are many different types of collisions taking place in a gas. They can be grouped.
EEE340Lecture 351 This is “Poyntings theorem” The Poynting vector (watts/m 2 ) instantaneous If we assume that then (8-83) (8-92)
Physics for Scientists and Engineers II, Summer Semester Lecture 21: July 13 th 2009 Physics for Scientists and Engineers II.
Feb. 2, 2011 Rosseland Mean Absorption Poynting Vector Plane EM Waves The Radiation Spectrum: Fourier Transforms.
Chapter 33 Electromagnetic Waves
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
5. Simplified Transport Equations We want to derive two fundamental transport properties, diffusion and viscosity. Unable to handle the 13-moment system.
March 2, 2011 Fill in derivation from last lecture Polarization of Thomson Scattering No class Friday, March 11.
The Electromagnetic Field. Maxwell Equations Constitutive Equations.
Electromagnetic Waves. Maxwell’s Rainbow: The scale is open-ended; the wavelengths/frequencies of electromagnetic waves have no inherent upper or lower.
Four equations (integral form) : Gauss’s law Gauss’s law for magnetism Faraday’s law Ampere-Maxwell law + Lorentz force Maxwell’s Equations.
 Somnath Bharadwaj and Pratik Khastgir, Department of Physics and Meteorology, IIT Kharagpur, India Electromagnetic.
Time variation Combining electrostatics and magnetostatics: (1) .E =  /  o where  =  f +  b (2) .B = 0“no magnetic monopoles” (3)  x E = 0 “conservative”
电磁振荡和电磁波 Chapter 16 Electromagnetic Oscillation and Waves.
Consider a time dependent electric field E(t) acting on a metal. Take the case when the wavelength of the field is large compared to the electron mean.
Electromagnetic wave equations: dielectric without dispersion Section 75.
Advanced EM - Master in Physics Let us now investigate the next term in the series expansion. Multipole expansion of radiation fields: the.
Light and Matter Tim Freegarde School of Physics & Astronomy University of Southampton Classical electrodynamics.
Electromagnetic Waves
1 Chapter 3 Electromagnetic Theory, Photons and Light September 5,8 Electromagnetic waves 3.1 Basic laws of electromagnetic theory Lights are electromagnetic.
Chapter 33 Electromagnetic Waves. 33.2: Maxwell’s Rainbow: As the figure shows, we now know a wide spectrum (or range) of electromagnetic waves: Maxwell’s.
Chapter 34 (continued) The Laws of Electromagnetism Maxwell’s Equations Displacement Current Electromagnetic Radiation.
1 Lecture D32 : Damped Free Vibration Spring-Dashpot-Mass System Spring Force k > 0 Dashpot c > 0 Newton’s Second Law (Define) Natural Frequency and Period.
1 30 Outline Maxwell’s Equations and the Displacement Current Electromagnetic Waves Polarization.
Physics 1202: Lecture 18 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Nonlinear Optics Lab. Hanyang Univ. Chapter 6. Time-Dependent Schrodinger Equation 6.1 Introduction Energy can be imparted or taken from a quantum system.
Heinrich Rudolf Hertz 1857 – 1894 The first person generated and received the EM waves 1887 His experiment shows that the EM waves follow the wave.
Lecture 38 Radiation Energy Density EM Wave: Equal partitions: Intensity:
Chapter 11 Radiation 11.1 Dipole Radiation 11.2 Point Charges.
Elements of electromagnetic field theory and guided waves
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.
1Electromagnetic Waves.  Administrative ◦ Quiz Today ◦ Review Exam Grades ◦ Review Exam  Begin Chapter 23 – Electromagnetic Waves  No 10:30 Office.
Dipole radiation during collisions LL2 Section 68.
1 30 Outline Maxwell’s Equations and the Displacement Current Electromagnetic Waves Polarization.
04/10/2015PHY 712 Spring Lecture 301 PHY 712 Electrodynamics 9-9:50 AM MWF Olin 103 Plan for Lecture 30: Finish reading Chap. 14 – Radiation from.
Chapter 1 Electromagnetic Fields
Two questions: (1) How to find the force, F on the electric charge, Q excreted by the field E and/or B? (2) How fields E and/or B can be created?
Electromagnetic Waves
Electromagnetic Waves
E or B? It Depends on Your Perspective
Polarized Microscope Q.1 What does it mean for the light to be “Polarized” ? Natural sunlight and almost every other form of artificial illumination transmits.
Review of basic EM concepts
Lecture 14 : Electromagnetic Waves
Dipole Radiation LL2 Section 67.
The equations so far..... Gauss’ Law for E Fields
ENE 325 Electromagnetic Fields and Waves
Surface Impedance of Metals
ECE699 – 004 Sensor Device Technology
Chapter 3 Electromagnetic Theory, Photons and Light
General theory of scattering in isotropic media
Is charge moving?.
Review of basic EM concepts
Two questions: (1) How to find the force, F on the electric charge, Q excreted by the field E and/or B? (2) How fields E and/or B can be created?
Maxwell’s Equations (so far)
PHY 712 Electrodynamics 9-9:50 AM MWF Olin 105 Plan for Lecture 23:
Chapter 33 Electromagnetic Waves
Electromagnetic Waves
Presentation transcript:

Scattering by free charges LL2 section 78

Incident electromagnetic wave System of charges Scattered wave Energy flux density S

Effective scattering cross section Energy radiated by system into do per second = Poynting vector Units Energy per second = area Energy per area per second Total scattering cross section

Consider a free charge at rest Incident plane monochromatic linearly-polarized wave Assume that the velocity acquired by e is v << c The force on the charge is Small. Neglect.

Neglect the effect of displacement. Put the origin at the center of the charge’s vibrations. The field acting on the charge is the same as that at the origin r = 0:

Equation of motion Dipole moment Dipole radiation formula is valid since v << c The frequency of oscillations is the same as the driving frequency. The frequencies of scattered and incident waves are the same.

Total cross section using = Thomson formula

For unpolarized light, we need to average over all initial polarization directions. Let e be a unit vector in the direction of E.

After averaging, we need a tensor with these properties that does not depend on e. This is it:

Maximum for forward and back scattering Half as much for orthogonal scattering. Because there is no radiation along the direction of the electron’s oscillation.

Scattering imparts a force on the electron Average energy density in the incident wave = <W> Average energy flux density (energy/area-time) = c <W> Average energy lost to scattering per unit time = c <W> s Average momentum in the incident wave = <W> /c Average momentum per unit time lost to scattering = <W> s

Vibrations of charge driven by eE are usually small. Velocities of charges are also small, v ~0. Then total radiated momentum dP = 0 by (73.2). All of the momentum lost by the incident wave is absrobed by the charge. Average force on the charge Second order in the field since W ~ E2 Direction of incident wave Instantaneous force = eE is 1st order in the field.

Radiation damping force on the charge (75.10)