Intro Physics II

Report 1 Downloads 230 Views
Administrivia

Intro Physics II Physics 11b Lecture 20

!

HW #9 due tomorrow (4/26)

!

Final Exam !

Thurs. May 15, 9:15, Science Center C

E & M in Free Space EM Waves Light Crisis!

What We Did Last Time

E and B in Free Space r

!

Displacement current !

!

!

Draw connections between electrostatic summary and magnetism summary ! Induction ! Displacement Current

Gauss’ Law

r r B ⋅ da = 0

No monopoles

ClosedSurface

Last piece, demanded by Ampere’s Law

Maxwell Equations (complete)

r

∫∫ E ⋅ da = 0

∫∫r

ClosedSurf ace

r dΦ B E ⋅ dl = − ∫ dt ClosedPath r r dΦ E B ⋅ d l = µ 0ε 0 dt ∫

Closed Path

r r F( )

r r r r r E( ) B( )

Energy conservation (Kirchoff) + Faraday’s Law Ampere’s Law + Displacement Current Lorenz Force Law

Q=I=0 Simple Form

How particles respond to fields

1

Hmmm…

ANY E and B in Free Space !We will now show a very curious fact; if ! !

!Line integral of E around rectangle in xy plane

Ey=E0sin(kx-ωt) Bz=B0sin(kx-ωt)

!

Ey=E0sin(kx-ωt) !Bz=B0sin(kx-ωt) !

! !

Flux of B through loop

!

Displacement sez

!

These fields satisfy our equations of E & M !

Bdy-(B+dB)∆y=-dB∆y

!

dΦE/dt=(dE/dt)dx∆y !

Even in free space No sources necessary

B B+dB

-dB∆y=µ0ε0(dE/dt)dx∆y

∆y

− µ 0ε 0

dE dB = dt dx

dx

ANY E and B in Free Space

Putting it all together

!Line integral of B around rectangle in xz plane !

Flux of E through loop

!

Faraday sez

dΦB/dt=(dB/dt)dx∆z !

dx

∆z E

(E+dE)∆z-E∆z=dE∆z

!

!

E+dE



dE∆z= −(dB/dt)dx∆z

dE

=−

dB



∂ ∂E

=

∂E ∂B = ∂x ∂t

∂ ∂B ∂ ∂E

=−

− µ 0ε 0

∂ ∂B

∂ ∂B

∂ ∂E

= − µ 0ε 0 −

2

2

∂ E2

=µε

0 0

∂ E 2

∂E ∂B = ∂t ∂x

1 0 0

∂ ∂B ∂ ∂E = ∂ ∂ ∂ ∂t 2

2

∂ B2

=µε

0 0

∂ B 2

2

Hmmm…

The Velocity k E0sin(kx-ωt)=µ0ε0ω2 E0sin(kx-ωt) !Only works if ω2/k2=1/µ0ε0 !sin(kx-wt)=sin[k(x-w/kt)] ! 2

!

   1 sin  k  x − t  µ 0ε 0    

!

Ey=E0sin(kx-ωt) !Bz=B0sin(kx-ωt)

Exactly the same happens for B !

!

∂2E ∂2E = µ 0ε 0 2 2 ∂t ∂x

∂2B ∂2B µ ε = 0 0 ∂x 2 ∂t 2

Recognize form of sin as a traveling wave from 11a!

What is value of 1/Sqrt(µ0ε0)? !

   1 sin  k  x − t  µ 0ε 0     !

Traveling wave

!

Ey=E0sin(kx-ωt) !Bz=B0sin(kx-ωt)

!

=3x108 m /s

!

This is the speed of light

!

E, B fields propagate through free space (no charges) at speed of light

!

!

Velocity

ε0=8.85x10-12 C2/(Nm2) µ0=4π x 10 -7 Tm/A

They ARE light

Conditions Velocity with respect to what? You can measure all the properties on earth !Or the sun !

!

Traveling wave with speed c

sin[k (x − ct )]

!

!

You get the same number (laws of physics are the same)

But you get same speed of light

!

!

Even though earth is Moving wrt the sun

Light should have the same speed regardless = !Speed of light seems internally inconsistent! !

! !

Least of our problems Let this guy take care of it

B and E perpendicular to one another !Each perpendicular to direction of motion !ExB is positive direction of motion !B/E=1/c !

! !

Ey=E0sin(kx-ωt) Bz=B0sin(kx-ωt)

!

!

From

dE

=−

dB

ω is free parameter !

Can be anything

3

Energy in Light

Poynting Vector !We already know how to calculate

Add uB and uE

!

!

!What is energy transport per unit time per unit area? !Can show that it is

Energy density

r 1 r r S = (E × B ) µ0

1 1 B2 u = ε0E2 + 2 2 µ0 ! !

Ey=E0sin(kx-ωt) Bz=B0sin(kx-ωt)

!

!

Use B=E/c, 1/c2=µ0ε0

!

1 1 µ 0ε 0 E 2 = ε0E 2 u = ε0E 2 + 2 2 µ0

If charge is stationary for a long time, field gets established !Imagine it starts moving with velocity v !After time t, field lines far away (outside circle of size ct) still static !

Cannot send any message faster than speed of light

Nearby fields (inside circle) change !Field lines cannot end !

ct

Lines inside and outside of circle must be connected along the circle

“Kink” in fields is EM wave; moves out to large distances !Accelerated charges produce EM waves

!

P=

2

2q a

Visible Light !

!

!

!

~100 MHz Wavelength~3 m

Microwaves ! !

!

400-700 nm wavelength ! c=fλ=2πω/λ ! f=750 THz to 420 THz

Radio waves !

!

2

E RMS BRMS µ0

The Spectrum of Light

!

vt

!Vector tells you direction of transport !Time-average of sines

S=

How Do We Get Light? !

Ey=E0sin(kx-ωt) Bz=B0sin(kx-ωt)

~1 MHz Wavelength ~cm

X-rays !

Wavelengths ~pm ! “Picometers”

3

4

Energy in Two Waves !The energy in one wave is proportional to E02

!

If you have two waves !

!

!

E-fields superimpose

Interference Cartoon Waves of amplitude E propagate from sources 1 and 2

!

!

E’=E1+E2

! !

Energy adds

!

!

There is the problem of interference

U=U1+U2=E12+E12 ! Or? U=E’2=(E1+E2)2=E12+E22+2E1E2

!

!

Along solid lines ! ! !

!

! !

!

d

= sin θ !

E1=-E2 out of phase U α (E1+E2)2 = 0 “Destructive Interference”

Sunrise on Beebe Lake

Along solid lines !

λ

E1=E2; in phase U α (E1+E2)2 = 4E2 “Constructive interference”

Along dashed lines !

Interference Cartoon

U1 α E2 U2 α E2 U1+U2 α 2E2

! !

E1=E2; in phase U α (E1+E2)2 = 4A “Constructive interference”

Along dashed lines ! ! !

E1=-E2 out of phase U α (E1+E2)2 = 0 “Destructive Interference”

5

Waves !All the usual wave equations apply

Accelerating Charges P=

dE 2q 2a 2 = dt 3c 3

a=

v2 r

!Accelerating charge should radiate energy, as we saw !Suppose an electron orbits an atom !

Constantly radiates power and spirals inwards toward nucleus

!According to this, atoms are not stable!

Line Frequencies !When you heat atoms of various kinds ! !

Out comes light At a particular frequency

!Frequencies are continuous in E & M !

!

Integral and differential equations give CONTINUOUS equations

What causes this?

6

More on Energy

Blackbody Radiation

!Suppose you shine colored lights on a metal !

!

Summary !

E & M Waves

!

Light Crises! ! ! ! !

P=

Ultraviolet Catastrophe !

Thermodynamics is able to predict spectrum from blackbody radiation !

!

Recall StefanBoltzmann only gives total energy

Spectrum is totally wrong at high frequency (UV)!

∂2E ∂2E = µ 0ε 0 2 2 ∂t ∂ 2 B ∂x ∂ 2B = µ 0ε 0 2 2 ∂x ∂t 2

!

Blue light: electrons are ejected from metal surface ! Binding energy is overcome Red light: no electrons emitted ! Binding energy never overcome ! No matter HOW MUCH energy is in the E-fields

!

2

2q a 3

r 1 r r S = (E × B ) sin[k (x − ct )] µ 0

Atomic Stability Emission lines Photoelectric effect Blackbody radiation

7