four equations (integral form) : gauss’s law gauss’s law for magnetism faraday’s law...
TRANSCRIPT
Four equations (integral form) :
Gauss’s law
Gauss’s law for magnetism
Faraday’s law
Ampere-Maxwell law
0
ˆ
insideqdAnE
dAnBdt
dldE ˆ
dt
dIldB elec
pathinside 0_0
+ Lorentz force BvqEqF
Maxwell’s Equations
0ˆ AnB
fT
f
/12
Acceleration:
tydt
yda sin2
max2
2
rc
aqEradiative 2
04
1
jsin4
12
2max
0
trc
qyEradiative
Sinusoidal E/M field
Sinusoidal Electromagnetic Radiation
According to particle theory of light: photons have energy and momentum
Classical E/M model of light: E/M radiation must carry energy and momentum
Energy and Momentum of E/M Radiation
A particle will experience electric force during a short time d/c:
qEFelec
p p 0 Felect qE d
c
What will happen to the ball?
It will oscillate
Energy was transferred from E/M field to the ball
mc
qEd
m
pKK
2
1
20
22Amount of energy in the pulse is ~ E2
Energy of E/M Radiation
mc
qEdK
2
12
Ball gained energy:
Pulse energy must decrease
)(J/m 32
0
20
1
2
1
2
1BE
Volume
Energy
E/M radiation: E=cB
200
20
2
0
20
11
2
11
2
1
2
1
cE
c
EE
Volume
Energy
2
0E
Energy of E/M Radiation
There is E/M energy stored in the pulse: )(J/m 320E
Volume
Energy
Pulse moves in space: there is energy flux
Units: J/(m2s) = W/m2
During t:
Energy 0E2 Act
2
0EctA
Energyflux
EBflux0
1
used: E=cB, 00=1/c2
Energy Flux
EBflux0
1
The direction of the E/M radiation was given by BE
Energy flux, the “Poynting vector”:
)1
0
2W/m (in BES
• S is the rate of energy flux in E/M radiation• It points in the direction of the E/M radiation
John HenryPoynting(1852-1914)
Energy Flux: The Poynting Vector
Intensity,
In the vicinity of the Earth, the energy density of radiation emitted by the sun is ~1400 W/m2. What is the approximate magnitude of the electric field in the sunlight?
Solution:EBflux
0
1
2
0Ec
N/C 7250
c
fluxE
Note: this is an average (rms) value
Exercise
A laser pointer emits ~5 mW of light power. What is the approximate magnitude of the electric field?
Solution:
1. Spot size: ~2 mm2. flux = (5.10-3 W)/(3.14.0.0012 m2)=1592 W/m2
3. Electric field:
N/C 7730
c
fluxE (rms value)
What if we focus it into 2 a micron spot?
Flux will increase 106 times, E will increase 103 times:
N/C 000,773E
Exercise
• E field starts motion• Moving charge in magnetic field:
BvqFmag
Fmag
What if there is negative charge?
BvqFmag
Fmag
‘Radiation pressure’: What is its magnitude?
Average speed: v/2
c
EvqB
vqFmag 22
12
)/(2
c
vqE
c
Evq
F
F
elec
mag
Momentum of E/M Radiation
Net momentum: in transverse direction: 0 in longitudinal direction: >0
Relativistic energy:
E2 pc 2 mc2 2
Quantum view: light consists of photons with zero mass: 22 pcE
Classical (Maxwell): it is also valid, i.e. momentum = energy/speed
BES
0
1
)N/m (in 2BEcc
S
0
1
Momentum flux:
Momentum Flux
Units of Pressure
What is the magnitude of the electric field due to sunlight near the Earth (1400 W/m2)? What is the force due to sunlight on a sail with the area 1 km2 at this location?Solution:
If reflective surface?2N/m 6103.9
Total force on the sail: N 3.9F
Exercise: Solar Sail
Atmospheric pressure is ~ 105 N/m2
|𝑆|= 1𝜇0
𝐸𝐵= 1𝜇0
𝐸 𝐸𝑐= 𝐸2
𝜇0𝑐725 N/C
If absorbed, pressure =N/m2
Electric fields are not blocked by matter: how can E decrease?
Re-radiation: Scattering
Positive charge
Why there is no light going through a cardboard?
Electric fields are not blocked by matterElectrons and nucleus in cardboard reradiate lightBehind the cardboard reradiated E/M field cancels original field
Cardboard
In transparent media, the superposition can result in change of wavelength and speed of wavefront
Index of refraction of medium,
Depends upon wavelengthand properties of medium
Refraction: Bending of Light
Rays perpendicular to wavefront bend at surface
A ray bends as it goes from one transparent media to another
Refraction: Snell’s Law
𝜃1
𝜃2
𝜃𝑎𝑖𝑟=45 °
𝜃𝑤𝑎𝑡𝑒𝑟 ≈ ?33 °