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Lienard Wierchert Potential

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Presentation on theme: "Lienard Wierchert Potential"— Presentation transcript:

1 Lienard Wierchert Potential
1 1 Plane Waves & Lienard Wierchert Potential Jeffrey Eldred Classical Mechanics and Electromagnetism June 2018 USPAS at MSU 1 1 1 1 1 1

2 2 2 Plane Waves 2 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 2 2 2 2 2 2

3 Maxwell’s Equations in a Vacuum
d'Alembertian: Full solution is a plane wave: E1 and E2 are complex, the relative phase determines the polarization. 3 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 3 3 3 3

4 Poynting Vector The E & B field are oriented normal to the direction of propagation: The Poynting vector describes the energy flow per unit area of the fields: And the time average of the Poynting vector for a plane wave: If E and H are complex, the time average can be written simply: 4 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 4 4 4 4

5 Lienard Wierchert Potentials:
5 5 Lienard Wierchert Potentials: Relativistic 5 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 5 5 5 5 5 5

6 Fields at the Speed of Light
The plane wave illustrates the speed at which electromagnetic information is propagated. The fields from a moving charge radiate outward at speed c. See Java Demo. 6 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 6 6 6 6

7 Retarded Time A point in space is affected by the E-fields originating from a source in the past, at a time called the retarded time. In the past, the position of the source will have changed and that will in turn impact the time that should be evaluated. 7 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 7 7 7 7

8 Retarded Time & Light Cone
8 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 8 8 8 8

9 Potentials for Retarded Time
9 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 9 9 9 9

10 10 10 Moving Point Charge 10 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 10 10 10 10 10 10

11 Solve by change of variables:
Moving Point Charge Solve by change of variables: 11 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 11 11 11 11

12 Moving Point Charge 12 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 12 12 12 12

13 Moving Point Charge Potentials
We have derived: A similar derivation shows that: 13 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 13 13 13 13

14 Alternate Derivation With some algebra, it can be shown: 14 14 14 14
Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 14 14 14 14

15 Lienard-Wierchert Potentials
By using the instantaneous velocity of the particle at tret, the expression we derived can be applied to any particle movement, not just straight line movement. 15 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 15 15 15 15

16 Fields from a Point Charge
16 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 16 16 16 16

17 Power Radiated from Accelerating Charge
Radiation in reference frame in which Beta is small: Integrate over Poynting for radiation: 17 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 17 17 17 17

18 Power Radiated from Accelerating Charge
Total power radiated: Linear acceleration: Circular acceleration: Can also be written 18 Classical Mechanics and Electromagnetism | June 2018 USPAS at MSU 11/24/2018 18 18 18 18


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