final_coverage

final_coverage - 
 Topics
for
Final
...

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Unformatted text preview: 
 Topics
for
Final
 Physics
13
 Fall,
2008
 
 All
information
covered
in
lecture
and
recitations
including:

 • 
 The
Zeeman
effect
–
but
I
will
only
ask
a
qualitative
question
for
a
 situation
where
l=0
and
only
spin
contributes
OR
where
we
will
ignore
 spin
and
have
l>0
only.


(Recitation
#8)
 
 
 Sections
9­1
through
9­3
are
excluded. 
 Section

 Topic
 9‐4
 9‐5
 9‐6
 11‐1
 11‐2
 11‐3
 11‐4
 11‐5
 11‐6
 11‐7
 Energy
Levels
and
Spectra
 of
Diatomic
Molecules
 Scattering,
Absorption
and
 Stimulated
Emission
 Lasers
and
Masers
 Composition
of
the
Nucleus
 Ground
State
Properties
 Radioactivity
 Alpha,
Beta,
and
Gamma
 Decay
 The
Nuclear
Force
 The
Shell
Model
 Nuclear
Reactions
 E x c lu d e d 
 
 
 
 
 
 
 
 
 X
 C ro ss
 s e c t io n s ,
 com pou nd
 n u c l e u s ,
 r e a c t io n s 
 w it h 
n e u t r o n s 
 
 
 
 
 M o re
 C o n s e r v a t io n 
 Law s
 T h e 
8 fo ld 
 w a y ,
J / p s i
 p u z z le 
 
 S u r fa c e 
a n d 
 a t m o s p h e r e ,
 in t e r io r ,
 a c t iv e 
s u n 
 C o n s t e lla t io n s ,
s t e l l a r 
 p o p u l a t io n s ,
 c la s s ific a t n 
o f
 s t a r s ,
 s t r u c t u r e 
o f
 t h e 
M ilk y 
 W ay
 X
 X
 X
 
 Q u a lit a t iv e ly 
 
 X
 
 
 
 
 
 
 
 
 Q u a n t it a t iv e ly 
 + Q u a lit a t iv e ly 
 X
 
 X
 X
 X
 X
 X
 X
 
 X
 11‐8
 11‐9
 12‐1
 12‐2
 12‐3
 12‐4
 12‐5
 13‐1
 Fission
and
Fusion
 Applications
 Basic
Concepts
 Fundamental
Interactions
 Conservation
Laws
 The
Standard
Model
 Beyond
the
SM
 The
Sun
 
 
 
 
 
 
 
 
 X
 X
 X
 X
 X
 X
 X
 X
 13‐2
 The
stars
 X
 
 13‐3
 13‐4
 13‐5
 13‐6

 Evolution
of
Stars
 Cataclysmic
Events
 Final
States
of
Stars
 Galaxies
 
 
 
 
 
 
 
 X
 13‐7
 13‐8
 
 Cosmology
and
Gravitation
 Cosmology
and
the
 Evolution
of
the
Universe
 
 
 
 X
 X
 
 ...
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This note was uploaded on 10/19/2009 for the course PHY 13 taught by Professor Garyr.goldstein during the Fall '04 term at Tufts.

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