the klein gordon equation (1926) scalar field (j=0) :
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The Klein Gordon equation (1926)
Scalar field (J=0) : (x)
2
2
2 2 2
tE m m
2 2p
2( ) 0m
0 0( , ), ( , )A A A B B B
4 vector notation
0 0( , ), ( , )A A A B B B
contravariant
covariant
0 0. .A B A B A B A B A B
A g A A g A
( , )ct x x
4 vectors
( , ) ( , )c t c t
( , )Ep p
c
p i 22 2p p E p
Field theory of
2( ) 0m
Classical electrodynamics, motion of charge –e in EM potential0A (A , ) A
is obtained by the substitution : p p eA
Quantum mechanics : i i eA
The Klein Gordon equation becomes:
2 2 2( ) ( )m V where V ie A A e A
2 14 137e
em The smallness of the EM coupling, , means that it is sensible to
Make a “perturbation” expansion of V in powers of em
Scalar particle – satisfies KG equation
( )V ie A A
Physical interpretation of Quantum Mechanical equations
Schrödinger equation (S.E.)21
2 0t mi
2=
* *( . .) ( . .)i S E i S E continuity 0 eq. .t j
“probability current”
* *2 ( )im j
“probability density”
Physical interpretation of Quantum Mechanics
Schrödinger equation (S.E.)21
2 0t mi
2=
* *( . .) ( . .)i S E i S E continuity 0 eq. .t j
“probability current”
* *2 ( )im j
“probability density”
Klein Gordon equation
**( )t ti
* *( )
( , )
i
j
j
j
2
2
2
tm
2
Pauli and Weisskopf ( , ) EMj e j j
. 0 =t j
j
22E N
Negative energy?
iEtNe
Negative probability??
Want to solve :
Solution :
where
2 4( ) ( ' ) ( ' )Fm x x x x
Feynman propagator Dirac Delta function
2( )m V
4( ) ( ) ' ( ' ) ( ') ( ')Fx x d x x x V x x 2( ) 0m
and
44 ' ( ' ) ( ') ( )d x x x f x f x
Want to solve :
Solution :
where
2 4( ) ( ' ) ( ' )Fm x x x x
Feynman propagator Dirac Delta function
Simplest to solve for propagator in momentum space by taking Fourier transform
2 2
.( ' ) 2 4 .( ' ) 4 41 12 2
( ) ( ' ) ( ' ) ( ' ) ( ' )ip x x ip x xFe m x x d x x e x x d x x
2
2 2 12
( ) ( )Fp m p
2 2 2 4 2 2
.41 1 1 1(2 ) (2 )
( ) , ( )ip x
F Fp m i p m ip x d p e
2( )m V
4( ) ( ) ' ( ' ) ( ') ( ')Fx x d x x x V x x
2
1
(2 ) 2
1
(2 )
2
1
(2 )
2( ) 0m
and
4( ) ( ) ' ( ' ) ( ') ( ')Fx x d x x x V x x
The Born series
Since V(x) is small can solve this equation iteratively :
Interpretation :
'x
x
''x'''x
( ' )F x x
( ')V x
( ) ( )x x 4 ' ( ' ) ( ') ( ')Fd x x x V x x 4 4'' '' ' ( '' ) ( '') ( ''' '') ( ''') ( ''')F Fd x d x x x V x x x V x x ...
but what about negative energy eigenvalues
2 1/ 2( ) ???E m 2p
Feynman – Stuckelberg interpretation
( 0)E ( 0)E
iEte ( )( )i E te
time
space
Two different time orderings giving same observable event :
't t 't t
t
't
4 2 2
.( ' )41 1(2 )
( ' )ip x x
F p m ix x d p e
time
space
't t 't t
3
3
'
(2 ) 2
p
p
i t t id pi e
p.(x'-x)
(p0 integral most conveniently evaluated using contour integration via Cauchy’s theorem )
1/ 22 2p p m
4 2 2
.41 1(2 )
( )ip x
F p m ix d p e
1/ 22 22 2 2 2 20o pp m i p p m i p p m i i
0
4
( ' ).( ' )31
0(2 )0 0
( ' )ip t t
i p x x
F
p p
ex x d p e dp
p i p i
0 If '- 0, choose contour such that ( +ve)I It t p ip p 0 ( ' ) ( ' )Iip t t p t te e
}I
( ' ) 'pi t t
p
iI e t t
0 If '- 0, choose contour such that ( +ve)I It t p ip p 0 ( ' ) ( ' )Iip t t p t te e
( ' ) 'pi t t
p
iI e t t
3
4 2 2 3
.( ' ) ' .( ' )41 1(2 ) (2 ) 2
( ' ) p
p
ip x x i t t ip x xd pF p m ix x d p e i e
time
space
1 2t t 1 2t t
0
. 1
2
ip xp p Vf e
where are positive and negative energy solutions to free KG equation
3 * 3 *( ') ( ') ( ) ( ' ) ( ') ( ) ( ')F p pp px x i d p f x f x t t i d p f x f x t t
Scattering in Quantum Mechanics
Prepare state at t | ( ) |in t i
Time evolution (possibly scattering) | ( ) | ( )in int S t
Observe resulting system in state | ( ) |out t f
QM : probability amplitude :
( ) | ( ) ( ) | | ( )
| |out in out in
fi
t t t S t
f S i S
fi fi fiS iT
Theory confronts experiment - Cross sections and decay rates
S matrix for Klein Gordon scattering
3 *' 0lim ( )pt
d x f i x
' , ( ) | ( )p p out inS t t
*3 ' 4' , ( ) ' ( ') ( ') ( ') ...p p pp
S p p i d x f x V x f x
Relativistic probability density
4( ) ( ) ' ( ' ) ( ') ( ') ...Fx x d x x x V x x 3 * 3 *( ' ) ( ') ( ) ( ' ) ( ') ( ) ( ')F p pp p
x x i d p f x f x t t i d p f x f x t t
fiiT
4 4* *( ) ( )( () ) )() (fi pp p piT i d y i dV y ie A Af y f y f yyf y
4 fiji d y A
* *( ) ( ) ( ) ( )p p pf
pij ie f y f y f y f y
0
. 1
2
ip xp p Vf e
( ).( ) f ii p p x
f ie p p e
Feynman rules
( ' )ie p p
p 'p
,k
Feynman rule associated with Feynman diagram