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 11: Jan 27 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 is This Friday Physics 2D Lecture Slides
4 4
Radianc c c 8 2 Radiancy y is Radiatio R( ) = u( ) = kT n intensity per u k nit interval T 4 4 c π π λ λ λ λ λ =
i Light of intensity I, wavelength λ and frequency ν incident on a photo-cathode Measure characteristics of current in the circuit as a fn of I, f, λ
– From current i seen in ammeter
– By applying retarding potential on electron moving towards Collector plate
Stopping voltage VS is a measure of the Max kinetic energy of the electron
f1 f2 f3
I
– f0 is characteristic of that metal
– E field and electrical force seen by the “charged subatomic oscillators” Larger
more Kinetic Energy KE !! The intensity of light shining rules !
– How much time ? Lets calculate it classically.
size of atom in cathode metal
minimum amount of radiation before its stripped off
– Binding energy = 2.3 eV= “Work Function” – Electron confined in Na atom, size ≅ 0.1nm ..how long before ejection ?
– Average Power Delivered PAV = I . A, A= πr2 ≅ 3.1 x 10-20 m2 – If all energy absorbed then ∆E = PAV . ∆T ⇒ ∆T = ∆E / PAV – Classical Physics predicts Measurable delay even by the primitive clocks of 1900 – But in experiment, the effect was observed to be instantaneous !!
19 2 20 2
− −
2 x 2 4 3
hc kT hc kT
λ λ
4
4
h c kT h h c h c kT kT c k c kT T h
λ λ λ λ λ
− − −