Brian Wecht, the TA, is away this week. I will substitute for his office hours (in my office 3314 Mayer Hall, discussion and PS session.
- Pl. give all regrade requests to me this week (only)
Physics 2D Lecture Slides Lecture 12: Jan 28 th 2004 Vivek Sharma - - PDF document
Brian Wecht, the TA, is away this week. I will substitute for his office hours (in my office 3314 Mayer Hall, discussion and PS session. Pl. give all regrade requests to me this week (only) Quiz 3 Will Cover Sections 2.1-2.5 Physics 2D
Brian Wecht, the TA, is away this week. I will substitute for his office hours (in my office 3314 Mayer Hall, discussion and PS session.
Light as bullets of “photons” Energy concentrated in photons Energy exchanged instantly Energy of EM Wave E= hf What Maxwell Saw of EM Waves What Einstein Saw of EM Waves
– Transfer all energy to electron – Energy gets used up to pay for Work Function Φ (Binding Energy)
I3 = 3I1 I2 = 2I1
I1= intensity
Light shining on metal cathode is made of photons Energy E, depends on frequency f , E = hf = h (c/λ) This QUANTUM of energy is used to knock off electron
electro s n
Light shining on metal cathode is made of photons Quantum of Energy E = hf = KE + ϕ ⇒ KE = hf - ϕ Shining Light With Constant Intensity f1 > f2 >f3
f1 f2 f3
No matter where you travel in the galaxy and beyond… ..no matter what experiment You do h : Planck’s constant is same NOBEL PRIZE FOR PLANCK
2 2
Light of Intensity I = 1.0 W/cm inc A Photoelectric Effect on An Iron Surfa ssume Fe reflects 96% of ligh ce: further on ident on ly 3% of 1.0cm surfa incident li ce of ght i i F t e s V µ
2
(a) Intensity available for Ph. El eff I =3
barely above thres ect (b) how m hold frequency for Ph any photo-electrons e . El effec mitted per t # s % 4% (1.0 W/c econd ? m )
λ µ × ×
8
9 34 2 9
Power = h f hc (250 10 )(1.2 10 / ) = (6.6 10 )(3.0 1 p 3% 4 / ) hoto % (1.0 W/c electro m n ) s m J s J s m s µ λ
− − −
= × × × × × × i
10
9 15 1
9
= (c) Current in Ammeter : i = (1.6 10 )(1.5 10 ) (d) Work Function = ( )( ) 2.4 10 h 4.14 1 1.5 10 f 1.1 10 = 4.5 eV C A s eV s
− −
× × = Φ = × × × × i
– ⇒
Useful for probing structure of sub-atomic Particles (and your teeth)
when electron passes near a positively charged target nucleus contained in target material, its deflected from its path because of its electrical attraction , experiences acceleration. Rules of E&M say that any charged particle will emit radiation when accelerated. This EM radiation “appears” as photons. Since photo carries energy and momentum, the electron must lose same amount. If all of electron’s energy is lost in just one single collision then
max min min
= hf
hc hc e V e V λ λ ∆ = = ∆
continuously
nuclear structure of target material and varies between materials
Molybdenum (Mo)
is too wide, need smaller slits
grating (Bragg)
– Interference – Diffraction
– Good Resolution λ<< ∆
properties (acts like photons)
– Showed that classical theory failed to explain the scattering effect of
– Watch the scattering of light off electron : measure time + wavelength of scattered X-ray
a surface with loosely bound electrons interaction of E field of EM wave with electron: F = eE
f = fincident
waves with fradiated= fincident
– At all scattering angles, ∆f & ∆λ must be zero
electron gets a “tan” : soaks in radiation
( ' ) (1 cos ) Scattered ' larger than incident λ λ λ θ λ ∆ = − ∝ −
How does one explain this startling anisotropy?
'
2 e e e
E+m ' p = p'cos +p cos p'sin -p sin Use these to e Energy Conservation: Momentum Conserv liminate electron deflection angle (n
: )
e
c E E θ φ θ φ = + =
e e e 2 2 2 2 4 2 e 2 2 e e 2
p 2 'cos p cos 'cos p sin 'sin Square and add Eliminate p & using E & E ( ') '
e e e e
p c m c E E m p p p E p pp p c φ θ φ θ θ = = − + + = = + − = − ⇒
( )
2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2
( ') ' 2 ' 2( ') ( ' ) ( 2 'cos ( ) E For light p= c ' ( ') 'cos E-E' 1 )(1 co ' ' ' 2 co (1 cos ) EE' s s )
e e e e
E E m c EE E E m c E E EE E mc p pp p E E E E E mc h E E c c c c m m c c θ θ θ θ λ λ θ ⇒ = ⇒ − + − = − ⇒ = − − ⇒ − + = + ⎡ ⎤ − + + ⎣ − + − − = − ⎦ ⎡ ⎤ − + ⎢ ⎥ ⎣ ⎦
2 e e e
E+m ' p = p'cos +p cos p'sin -p sin Use these to e Energy Conservation: Momentum Conserv liminate electron deflection angle (n
: )
e
c E E θ φ θ φ = + =
Plot scattered photon data, calculate slope and measure “h”
( ' ) ( )(1 cos )
e
h m c λ λ θ − = −
Energy Quantization is a UNIVERSAL characteristic