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PHY 711 Fall 2014 -- Lecture 39 112/01/2014
PHY 711 Classical Mechanics and Mathematical Methods
10-10:50 AM MWF Olin 103
Plan for Lecture 39
1. Brief introduction to the physics of elastic continua (Chap. 13 of F & W)
2. Brief review of topics covered this semester
3. Course evaluation forms
PHY 711 Fall 2014 -- Lecture 39 412/01/2014
Brief introduction to elastic continua
reference deformation
r1 r1’
2 2
2 1 2
1 1 1 2
1 2 1 1
( ) (' '
' '
)
( )
ur r r r
r r r r r
r r
u rr
u
PHY 711 Fall 2014 -- Lecture 39 512/01/2014
Brief introduction to elastic continua
Deformation components:
1 1
2 2
i i i
j j j
ij ij
j j
i i
O
u uu u u
x x x x x
ò
V a b c ' ' ' 'V ba c (1 )' 1 TrV VV uò
TrdV d
V
uò
PHY 711 Fall 2014 -- Lecture 39 612/01/2014
Stress tensor3
1
:
Lame' coeffi
ˆ com
cient
ponent of
s :
or :
force acting on surface
Generalization of Hooke's
law, F
thij j
x
ii
j
jj ij
j
i
i
j
kx
uuT
x x
T dA i
T
u
n
Tr 2ij ij ò ò
2Note that: Tr = 3 Tr
3
1
23
32ij ij ij
T
T Tr T
ò
ò
bulk modulus=p
VK V
PHY 711 Fall 2014 -- Lecture 39 712/01/2014
Example -- hydrostatic pressure:
2 333
ij ij
ij ij ij
T dp
dp dp
K
p
VK V
ò
22 33
1 ij ij ijT Tr T
ò
1
Example -- uniaxial pressure: 0 otherwise
in terms of Young's modulus
9
3
zz zz
ij
dp ij zzT
K
T
E
E
K
ò
PHY 711 Fall 2014 -- Lecture 39 812/01/2014
Dynamical equations of elastic continuum
2
22
1
3K
t
uu u f
1/ 2
In the absence of external forces, this reduces
to two decoupled wave equations representing
longitudinal and transverse modes:
=
where 0 and 0
4
3 and
t
t
l t
l
l
Kc c
u uu
u u
1/ 2
PHY 711 Fall 2014 -- Lecture 39 9
Scattering theory:
12/01/2014
Brief review of topics covered in this course --
PHY 711 Fall 2014 -- Lecture 39 1012/01/2014
angleat
detector into scattered is that beamincident of Area
areaunit per particlesincident ofNumber
particle per target at particles detected ofNumber
section cross alDifferenti
d
d
bdbdb
min1/
2 20
Scattering angle equation for
central potential ( ):
12
(1 / )1
r
V r
b duV u
b uE
sin sin
d d b db b db
d d d d
PHY 711 Fall 2014 -- Lecture 39 1112/01/2014
Rotating reference frames
VωωVωV
ωVV
VωV
ωV
dt
d
dt
d
dt
d
dt
d
dt
d
dt
d
dt
d
dt
d
bodybodyinertial
bodybodyinertial
22
2
2
2
01e
02e
03e
Inertial frame Body frame
1e
2e
3e
ω
Centrifugal force
12/01/2014 PHY 711 Fall 2014 -- Lecture 39 12
Newton’s laws; Let r denote the position of particle of mass m:
rωωrωr
ωa
Fr
Fr
mdt
dm
dt
dm
dt
dm
dt
dm
dt
dm
bodyinertial
ext
body
ext
inertial
2 2
2
2
2
2
2
Coriolis force
rωωrωr
ωFrr
m
dt
dm
dt
dm
r
mGM
dt
dm
earth
e
earth
2 'ˆ22
2
Equation of motion on Earth’s surface
w
z (up)
x (south)
y (east)
q
PHY 711 Fall 2014 -- Lecture 39 1312/01/2014
Calculus of variation example for a pure integral functions
Find the function ( ) which extremizes ( ), ,
where ( ), , ( ), , .
Necessary condition: 0
f
i
x
x
dyy x I y x x
dx
dy dyI y x x f y x x dx
dx dx
I
, ,
Euler-Lagrange equations:
0 /dy
x x ydx
f d f
y dx dy dx
PHY 711 Fall 2014 -- Lecture 39 1412/01/2014
Application to particle dynamics
2
1
(time)
(generalized coordinate)
(Lagrangian)
(action)
Denote:
, ;t
t
x t
y q
f L
I S
dqq
dt
S L q q t dt
, ,
Euler-Lagrange equations:
0 /dq
t t qdt
L d L
q dt dq dt
PHY 711 Fall 2014 -- Lecture 39 1512/01/2014
The Lagrangian is given by:
( ), ,d
L t t T Udt
rr
Kinetic energy
Potential energy
0
0
Note: For a particle of charge , the potential function can have the form
, , ,
where , denotes non-electromagnetic field contributions and
,1 where , ,
q U
qU U t q t t
cU t
tt t
c
r r r A r
r
A rE r r
, ,t
t t
B r A r
PHY 711 Fall 2014 -- Lecture 39 1612/01/2014
Recipe for constructing the Hamiltonian and analyzing the equations of motion
q
H
dt
dp
p
H
dt
dq
ttptqHH
LpqH
q
Lp
ttqtqLL
:motion of equations canonical Analyze .5
,)(,)( :functionn Hamiltonia Form .4
:expressionn HamiltoniaConstruct .3
:momenta dgeneralize Compute .2
,)(,)( :function LagrangianConstruct 1.
PHY 711 Fall 2014 -- Lecture 39 1712/01/2014
x
p
Notion of phase space – example for one-dimensional motion due to constant force
2
0 0
200 0 0 0
( )
,2
1
2( ) i
i i i i
px p F x
mp
p t p t x t x tm
pH x p F
m
F t F
PHY 711 Fall 2014 -- Lecture 39 1812/01/2014
Liouville’s Theorem (1838) The density of representative points in phase space corresponding to the motion of a system of particles remains constant during the motion.
0 : theoremsLiouville' toAccording
,)(,)( :space phasein particles ofdensity theDenote
dt
dD
t
Dp
p
Dq
q
D
dt
dD
ttptqDD
Importance of Liouville’s theorem to statistical mechanical analysis: In statistical mechanics, we need to evaluate the probability of various configurations of particles. The fact that the density of particles in phase space is constant in time, implies that each point in phase space is equally probable and that the time average of the evolution of a system can be determined by an average of the system over phase space volume.
PHY 711 Fall 2014 -- Lecture 39 1912/01/2014
223232
1212
233
222
211
2
1
2
1
2
1
2
1
2
1
xxkxxk
xmxmxmL
Example – linear molecule
1x2x
3x
m1 m2 m3
Analysis of small oscillations near equilibrium
PHY 711 Fall 2014 -- Lecture 39 2012/01/2014
m1 m2 m3
m1 m2 m3
m1 m2 m3
01
Om
k2
CO m
k
m
k 23
Normal modes of oscillation for linear molecule example--
PHY 711 Fall 2014 -- Lecture 39 2112/01/2014
Longitudinal waves as the continuum limit of a linear mass-spring system --
1ixix 1ix
m m m
0
2
10
2
2
1
2
1
iii
ii xxkxmVTL
2 11 iiii xxxkxm
22
2
11
2
2
2
),()(
:system thisof version continuum theimagine Now
xx
xxx
txtxtx
iii
iii
PHY 711 Fall 2014 -- Lecture 39 2212/01/2014
/
:equation Continuum
2 :equation Discrete
2
2
2
2
2
22
2
2
11
xxm
xk
t
xxk
tm
xxxkxm iiii
system parameter with units of (velocity)2=c2
2 22
2 2
Wave equation for longitudinal or
transverse displacement :
0
μ(x,t)
ct x
PHY 711 Fall 2014 -- Lecture 39 2312/01/2014
Solution methods for wave equations and generalizations1. D’Alembert’s method2. Fourier transforms3. Laplace transforms; contour integration4. Eigenfunction expansions5. Green’s functions6. Variational methods
PHY 711 Fall 2014 -- Lecture 39 2412/01/2014
r
w
22
2
1 1Kinetic energy:
2 2
1
2
1
2
inertial
p p p pp p
p p pp
p p p pp
d
dt
T m v m
m
m
rω r
ω r
ω r ω r
ω ω r r r ω
Physics of rigid bodies rotating about a fixed origin
ω I ω�
PHY 711 Fall 2014 -- Lecture 39 2512/01/2014
2
Matrix notation:
xx xy xz
yx yy yz ij p ij p pi pjp
zx zy zz
I I I
I I I I m r r r
I I I
I�
Moment of inertia tensor
1 1 2 2 3 3
1For general coordinate system:
2
For (body fixed) coordinate system that diagonalizes
ˆ ˆ moment of inertia tensor: 1,2,3
1ˆ ˆ ˆ
2
ij i jij
i i i
T I
I i
T I
I e e
ω e e e
�
2i i
i
PHY 711 Fall 2014 -- Lecture 39 2612/01/2014
03e
y
xy
x '2e
3e
3'2
03 ˆ ˆ ˆ ~ eeeω
3
2
1
ˆcos
ˆcossinsin
ˆsincossin ~
e
e
eω
Euler angles for describing angular velocity in terms of body fixed contributions --
PHY 711 Fall 2014 -- Lecture 39 2712/01/2014
Equations describing fluid physics
Newton-Euler equation of motion:
Continuity condition: 0
applied
p
t
t
vv v f
v
PHY 711 Fall 2014 -- Lecture 39 2812/01/2014
Solution of equations in the linear approximation – (linear sound waves)
1 0p
t t
v
v v f v
0
20 0
=0
Assume: 0
p p p p c
v fv
2
00
0 0
20
0 0 0 00
22 0 0
20
Linearized equations: 0
Let
0
ˆ
i tit
c
e e
kc
t
c
c
t
k kr r
vv
v v
k
v v
v
k k
PHY 711 Fall 2014 -- Lecture 39 2912/01/2014
Wave analysis in fluid physics beyond linear regime1. Non-linear effects in sound waves – shock
phenomena2. Application of Euler-Newton equations to surface
waves in water3. Korteweg-de Vries soliton analysis
PHY 711 Fall 2014 -- Lecture 39 3012/01/2014
Analysis of heat conduction
a
T1
b
c
2,,
p
th
p
T t qT
c
tt c
k
rr
T0
PHY 711 Fall 2014 -- Lecture 39 3112/01/2014
Newton-Euler equations for viscous fluids
2
Navier-Stokes equation
1 1 1
3
Continuity condition
0
pt
t
vv v f v
v
v