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Title: ATOMIC PHYSICS


1
ATOMIC PHYSICS
2
History of Atomic Structure
  • Thompson Model
  • Plum Pudding Model
  • Rutherford Model
  • Nucleus
  • 99 mass of atom
  • Electrons surrounding nucleus
  • Take up most of space, negligible mass
  • Bohr Model
  • Electron orbital model
  • Electrons occupy discrete energy levels
  • Energy levels quantized
  • Modern Model
  • Electron cloud (region of high probability to
    find electron

3
Ernest Rutherford Bio
4
RUTHERFORD EXPERIMENT
SCREEN
Au FOIL
Pb SHIELD
ALPHA SOURCE
5
The Rutherford Experiment 1911
6
Rutherford ExperimentJ.J. Thompson Model
7
Rutherford ExperimentRutherford Model
Au atoms mostly vacant space!
charged nucleus contained most of matter,
occupied very little space.
- charges occupy most of the space, very little
matter
8
Balmer (1885)
H atom Emission Spectra
Balmer Equation
R Rydbergs Constant 6.84 x 105 m-1
n whole interger s gt 2
n 3,4,5,6
9
Niels Bohr Bio
10
Bohr Orbital Model
H atom energy level diagram
(eV)
ionization
0.00
-0.38
-0.54
-0.85
-1.51
-3.4
-13.6
11
Bohr Orbital Model
12
Bohrs Postulates
  • Radiationless energy states exist
  • During transition from one E state to another
  • Ef Ei E photon hf
  • Electron wavelength in stable orbit creates
    standing wave
  • nl 2pr
  • n 1,2,3,

13
e deBroglie l Standing Wave
n 4
4l 2pr4
e is ?
No radiation emitted
14
Bohrs Postulates (continued)
3. Electron in orbital is in a standing wave
nl 2pr
n 1,2,3,
l h
l h
p
mv
h
2pr

n
mv

mvr
15
Bohrs Postulates (continued)
3. Angular Momentum of electron orbits is
quantized

mvr

Angular Momentum
n 1,2,3,
16
Balmer Series
Hydrogen Emission Spectra
H atom energy levels
(eV)
e
e
e
e
17
Lyman Series
H atom energy levels
ALL PHOTONS ULTRAVIOLET
(eV)
e
e
e
e
18
Paschen Series
H atom energy levels
(eV)
ALL PHOTONS INFARED
e
e
e
19
H UltravioletAbsorption Spectra
H atom energy levels
ALL PHOTONS ULTRAVIOLET
(eV)
e
e
DE 13.06 ev
e
DE 12.75 ev
DE 12.09 ev
e
DE 10.2 ev
20
H Visible Absorption Spectra
Visible spectrum
H atom energy level diagram
(eV)
e
DE 3.02 ev
e
DE 2.86 ev
DE 2.55 ev
DE 1.89 ev
e
e
21
Visible Solar SpectrumShowing Prominent
Absorption Fraunhofer Lines
H
22
Bohr Orbital Model
H atom energy level diagram
(eV)
ionization
How did Bohr determine these energy values????
0.00
-0.38
-0.54
-0.85
-1.51
-3.4
-13.6
23
H atom
r 5.3 x 10-11 m
potential created by proton at r
e
Fe
p
V kq
27.2 V
r
TOTAL ENERGY OF ATOM
ETOTAL PEe KE
PEe qV (-1.6 x 10 19) ( 27.2 V)
PEe - 4.35 x 10 18 J
24
H atom (continued)
KE ½ mv2
V ?
Fe kq1q2
Fc mv2
Fe Fc
r
r2
Fe 8.22 x 10-8 N
V 2.18 x106 m/s 5 MILLION MPH
KE ½ mv2 2.2 x10-18 J
-2.2 x 10-18 J
ETOT PEe KE
ETOT -13.6 eV
25
H atom (cont.)
Fc Fe
kq2
mv2
r
r2
ETOTAL KE PEe
26
Bohr H atom
EARLIER
EARLIER
nh

mvr
mv2
kq2
2p
r
( )
nh
nh
2

v
kq2
m
2pmr
2pmr
r
r a n2
27
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28
H Energy Levels
29
Balmer Equation Derivation
Ep DE Ef - Ei
Ef - Ei

-
30
For Balmer Series
BALMER EQUATION
n 3,4,5,6
BOHRS EQUATION
nf 2
6.84 x 105 m-1
31
Balmer Equation Unit Check
1
(kg)
(Nm2/C2)2
(C4)

m
(m/s)
(J s)3
32
Hg Energy Levels
33
H Energy Level Diagram
34
SPONTANEOUS ABSORPTION
Ef
Ei
35
SPONTANEOUS EMISSION
Ei
Ef
36
STIMULATED EMISSION
Ei
COHERENT PHOTONS IN PHASE, SAME f
Ef
37
L. A. S. E. R.
by
of
ight
adiation
mplification
timulated
mmission
38
L.A.S.E.R.
Energy pump
39
LASER STIMULATED EMISSION
E3
E2
METASTABLE STATE
E1
POPULATION INVERSION
40
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41
ATOMIC PHYSICS
  • SAMPLE AP QUESTIONS

42
AP PHYSICS HOMEWORK 25

NAME _____________________________________ MO
DERN PHYSICS

DATE _________________ PERIOD
___________
43
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44
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45
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46
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47
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48
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49
AP PHYSICS HOMEWORK 25

NAME _____________________________________ MO
DERN PHYSICS

DATE _________________ PERIOD
___________
50
AP PHYSICS HOMEWORK 25

NAME _____________________________________ MO
DERN PHYSICS

DATE _________________ PERIOD
___________
51
AP PHYSICS HOMEWORK 25

NAME _____________________________________ MO
DERN PHYSICS

DATE _________________ PERIOD
___________
52
AP PHYSICS HOMEWORK 25

NAME _____________________________________ MO
DERN PHYSICS

DATE _________________ PERIOD
___________
53
Sample Prolem 2
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