PHYSICS 272 Electric & Magnetic Interactions

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Presentation transcript:

PHYSICS 272 Electric & Magnetic Interactions Lecture 27 (last lecture) Electromagnetic Waves and Radiation [Chap 24]

A Few Reminders Final Exam: 12/13 Tuesday 3:20-5:20 STEW 183 Special accommodation students: Phys Rm 203 3:20pm Students with conflicts: contact me asap by email the plan is to have the exam at 8:30am on Wednesday the 14th Equation sheet will be provided/posted Exam will be 20 multiple choice questions There will be recitation and lab this week; the lab will be review with some final practice problems

Summary

There is a “kink” in the E-field and it travels out in all directions at the speed of light r = ct

At t = r/c, observer 2 detects a sideways (“transverse”) E-field The associated B-field points out of the page on the right, and into the page on the left.

. x 1. The direction of the field is opposite to qa Ordinary B-field . x B = 0 The derivation* is given in 24.11 1. The direction of the field is opposite to qa 2. The electric field falls off at a rate 1/r

Exercise a An electron is briefly accelerated in the direction shown. Draw the electric and magnetic vectors of radiative field. E B 1. The direction of the field is opposite to qa 2. The direction of propagation is given by Derivation is too complex for this course Kink in the electric field Much slower than 1/r2 – makes it possible to affect matter that is very far from the accelerated charges – that is why we see very distant stars. Quali 7

Exercise An electric field of 106 N/C acts on an electron for a short time. What is the magnitude of electric field observed 2 cm away? 2 cm E=106 N/C B Erad a 1. Acceleration a=F/m=qE/m=1.78.1017 m/s2 2. The direction of the field is opposite to qa 3. The magnitude: E=1.44.10-7 N/C 4. The direction of propagation is given by Derivation is too complex for this course Kink in the electric field Much slower than 1/r2 – makes it possible to affect matter that is very far from the accelerated charges – that is why we see very distant stars. Quali What is the magnitude of the Coulomb field at the same location? 8

Clicker Question 1 A narrow collimated pulse of radiation propagates in the -x direction. There is an electron at location A. What is the direction of the radiative electric field observed at location B? B A C B D e- 9

Clicker Question 1 A narrow collimated pulse of radiation propagates in the -x direction. There is an electron at location A. What is the direction of the radiative electric field observed at location B? B A C D e- B 10

Clicker Question 2 A proton is briefly accelerated as shown below. What is the direction of the radiative magnetic field that will be detected at location A? A A) into the page B) out of the page C) not enough information + 11

Clicker Question 2 A proton is briefly accelerated as shown below. What is the direction of the radiative magnetic field that will be detected at location A? A A) into the page B) out of the page C) not enough information + A 12

Sinusoidal Electromagnetic Radiation Acceleration: Sinusoidal E/M field 13

Sinusoidal E/M Radiation: Wavelength Instead of period can use wavelength: Freeze picture in time: Example of sinusoidal E/M radiation: atoms radio stations E/M noise from AC wires 14

Energy density in E & M fields:

In a time ∆t, a volume of E & M fields passes through the area A. The amount of energy is Define energy flux as J/sec/m2 Define the “Poynting vector” Its direction is the energy flow direction.

Electromagnetic Radiation Carries Momentum Einstein’s equation: For E&M radiation: Define momentum flux is 1/c times the energy flux given by the Poynting vector The units of momentum flux are the same as pressure in N/m2