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JAI NARAIN VYAS UNIVERSITY
JODHPUR ( RAJ. )
PHYSICS DEPARTMENT
ADVANCE QUANTUM MECHANICS
PRESENTEDBY –
RAMNIWAS JAKHAR
SUBMITTEDTO – DR. S. S.
MEENASIR
GREEN FUNCTION FOR
SCATTERING PROBLEM AND
LIPPMANN-SCHWINGER
EQUATION
• GREEN FUNCTION :-
In mathematical a Green function is the impulse
response of an inhomogeneous linear differential
operator, defined on a domain with specified
initial condition or boundary condition.
If differential operator is L(x) is linear, then one
can superpose them to find the solution.
u(x) = ʃ f(y) G(x , y) dy
Solution of Green function if differential operator
is L than –
L G(x , s) = δn
(s-x)
where- δ = Dirac delta function.
n = Dimension
In physics :- the Green function as used in physics is
usually defined with the opposite sign, that is –
L G(s , x) = δ(x-s)
If the operator is translation invariant that is, when
L has constant coefficient with x, the Green
function can be taken to be a convolution kernel,
that is –
G(x , s) = G(x-s)
In this case, Green function is the same as the
impulse of linear time invariant system theory.
• GREEN FUNCTION FOR SCATTERING PROBLEM:-
PROPERTY OF GREEN FUNCTION :-
𝛻2 + 𝐾2 G( r, r’)=𝑑3 (r, r’) --------(1)
Schrodinger equation
G( r,r’)=G(r-r’)
 LOWER TRANSFORMATION OF GREEN FUNCTION:-
G(r-r’)= 𝐺 𝑞 iq(r − r′)𝑑3
𝑞 -------(2)
Generate r to q state
𝑑3
𝑟 − 𝑟′
=
1
(2𝜋)3 𝑒𝑞(𝑟−𝑟′)
𝑑3
q
Eq (1),
(q+𝑘2 )G (q)𝑒𝑖𝑞(𝑟−𝑟′)𝑑3q=
1
(2𝜋)3 𝑒𝑖𝑞(𝑟−𝑟′) 𝑑3q
(-𝑞2
+𝑘2
) 𝐺(𝑞) 𝑒𝑖𝑞(𝑟−𝑟′)
𝑑3
q=
1
(2𝜋)3 𝑒𝑖𝑞(𝑟−𝑟′)
𝑑3
q
[(𝑞2 − 𝑘2)G(q)+
1
(2𝜋)3]𝑒𝑖𝑞(𝑟−𝑟′)𝑑3𝑞 = 0
𝑒𝑖𝑞(𝑟−𝑟′)
𝑑3
q≠0
(𝑞2
− 𝑘2
)G(q)+
1
(2𝜋)3 = 0
G(q)= -
1
(2𝜋)3
1
( 𝑞2−𝑘2)
--------(4)
By equation (2) and(4)
G(r-r’)= 𝐺(𝑞)𝑒𝑖𝑞(𝑟−𝑟′)𝑑3𝑞
G(r-r’)=-
1
(2𝜋)3
𝑒𝑖𝑞(𝑟−𝑟′)
(𝑞2−𝑘2)
𝑑3q
Value of green function
:𝑑3
q=𝑞2
dqsin𝜃𝑑𝜃d∅
G(r-r’)=-
1
(2𝜋)3 0
∞
0
𝜋
0
2𝜋 𝑒𝑖𝑞(𝑟−𝑟′)
(𝑞2−𝑘2)
𝑞2
𝑑𝑞sin𝜃𝑑𝜃𝑑∅
If ∞ = (𝑟 − 𝑟′
)
G(r-r’)= -
1
(2𝜋)2 0
∞
0
𝜋 𝑒𝑖𝑅𝑐𝑜𝑠𝜃
(𝑞2−𝑘2)
𝑞2
sin𝜃d𝜃d∅
= -
1
(2𝜋)2 0
𝜋
𝑒𝑖𝑅𝑐𝑜𝑠𝜃
𝑠𝑖𝑛𝜃𝑑𝜃 0
∞ 𝑞2𝑑𝑞
(𝑞2−𝑘2)
=(𝐼1 + 𝐼2)
𝐼1 =
0
𝜋
𝑒𝑖𝑅𝐶𝑂𝑆𝜃 sinθdθ
COS𝜃 = 𝑡
-SIN𝜃𝑑𝜃 = 𝑑𝑡
𝐼1 = − 1
−1
𝑒𝑖𝑅𝑞𝑡
dt
=
1
𝑖𝑞𝑅
(𝑒𝑖𝑞𝑟
− 𝑒−𝑖𝑞𝑅
)
G(r-r’)= -
1
(2𝜋)2 0
∞ 𝑞2
(𝑞2+𝑘2)𝑖𝑞𝑡
𝑒𝑖𝑞𝑅 − 𝑒−𝑖𝑞𝑅 𝑑𝑞
= -
1
(2𝜋)2 −∞
∞ 𝑞𝑒𝑖𝑞𝑡
(𝑞2−𝑘2)𝑖𝑞𝑅
𝑑𝑞
= -
1
4𝜋2 −∞
∞ 𝑞𝑒𝑖𝑞𝑅
(𝑞+𝑘)(𝑞−𝑘)
dq
In equation(5) we can define
q=±k Because value of
𝑞𝑒𝑖𝑞𝑡
(𝑞+𝑘)(𝑞−𝑘)
(i) become=∞
Can be solved by
𝑓 𝑧 𝑑𝑧 = 2𝜋𝑖(𝑠𝑢𝑚 𝑜𝑓 𝑟𝑒𝑠𝑖𝑑𝑢𝑒)
q ±𝑘 (solve)
Solve at q +k
cos
Residue=𝑠𝑖𝑛𝑧 +𝑎 (2-a)f(2)
=𝑠𝑖𝑛𝑧 −𝑎 (2-a)f(2)
(1) For q +k (2) For q -k
Residue=𝑠𝑖𝑛𝑞 𝑘 (q-k)
𝑞
(𝑞2−𝑘2)
𝑒𝑖𝑞𝑅
or
=𝑠𝑖𝑛𝑞 𝑘
𝑞−𝑘 𝑞𝑒𝑖𝑞𝑅
(𝑞+𝑘)(𝑞−𝑘)
=
𝑘
𝑘+𝑘
𝑒𝑖𝑞𝑅
Residue
𝑒𝑖𝑘𝑅
2
So,
I= 2𝜋𝑖 −
𝑒𝑖𝑘𝑅
2
=𝜋𝑖𝑒𝑖𝑘𝑅
G(r-r’)=
−1
4𝜋2𝑖𝑅
𝜋𝑖𝑒𝑖𝑘𝑅
= -
1
4𝜋𝑅
𝑒𝑖𝑘𝑅
G(r-r’)= -
1
4𝜋(𝑟−𝑟′)
𝑒𝑖𝑘(𝑟−𝑟′)
Residue=𝑠𝑖𝑛𝑞 𝑘
𝑞𝑒𝑖𝑞𝑅
(𝑞2−𝑘2)
Residue=-
−𝑘𝑒𝑖𝑞𝑅
−2𝐾
I=2𝜋𝑖
1
2
𝑒−𝑖𝑘𝑅
=𝜋𝑖𝑒−𝑖𝑘𝑅
G(r-r’)= -
1
2
𝜋𝑖𝑒−𝑖𝑘𝑅
=-
1
4𝜋𝑅
𝑒−𝑖𝑘𝑅
Or,
G(r-r’)= -
1
4𝜋(𝑟−𝑟′)
𝑒−𝑖𝑘(𝑟−𝑟′)
=
𝑒−𝑖𝑘𝑅
2
G(r-r’)= -
1
4𝜋(𝑟−𝑟′)
𝑒−𝑖𝑘(𝑟−𝑟′)
+ 𝑒𝑖𝑘(𝑟−𝑟′)
For scattering ,we want to study about outgoing wave. So we cross restarted green
function than,
G(r-r’)= -
1
4𝜋(𝑟−𝑟′)
𝑒𝑖𝑘(𝑟−𝑟′)
ψ = 𝜑𝑖𝑛 + 𝜑𝑠𝑐
𝜑𝑠𝑐 =
2𝜋
ħ2
ℎ(𝑟𝑟′)𝜑(𝑟′)𝑑3𝑟′
𝜑𝑠𝑐 =
2
ħ2
−
1
4𝜋 𝑟 − 𝑟′
𝑒𝑖𝑘 𝑟−𝑟′
𝜑(𝑟′
)𝑑3
(𝑟′
)
𝜑 = 𝑒𝑖𝑘𝑟
−
2𝜋ħ2
𝑒𝑖𝑘 𝑟−𝑟′
𝑟−𝑟′ 𝜑 𝑟 𝑑3
r’
General solution of scattering problem of green function.
• Lippmann-Schwinger Equation :-
: Whenever large no. of component of
scattered particles are appreciable then we
use lippmann-schwinger equation. It give an
integral solution of scattering problem.
: By Green function, we analyze the partial
wave or particle scattering and it useful for
lower energy particle scattering.
: But Lippmann-Schwinger equation is useful
for higher energy scattering particles.
to find lippmann-schwinger equation we use
Helm-Holtz operator which is known as –
( 2 + K2 )
and we use the Green function –
2G(r , r’) = - 4πδ3[r - r’]
by solving these we can write Helm-Holtz
operator in form of Green function –
Ѱ(r) Ѱin + Ѱsc
r→ꚙ
by these equations we got a solution -
( 2 + K2 ) Ѱ(r) = 2μ/ћ2 { μ(r’) Ѱ(r’) }
this is not a unique solution.
For unique solution we use Ѱ(r) in form of Ѱ0(r), r
and r’.
where - r = stationary vector / constant
r’ = variable vector
( both are position vector )
therefore we found a unique solution –
( 2 + K2 ) Ѱ(r) = eiK.r + (2μ/ћ2) ʃ d3r’ δ3(r-r’) g(r’)
Ѱ(r’)
This equation is known as Lippmann-Schwinger
equation.
THANK YOU

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Ram-niwas Quantum.pptx.pptx

  • 1. JAI NARAIN VYAS UNIVERSITY JODHPUR ( RAJ. ) PHYSICS DEPARTMENT ADVANCE QUANTUM MECHANICS PRESENTEDBY – RAMNIWAS JAKHAR SUBMITTEDTO – DR. S. S. MEENASIR
  • 2. GREEN FUNCTION FOR SCATTERING PROBLEM AND LIPPMANN-SCHWINGER EQUATION
  • 3. • GREEN FUNCTION :- In mathematical a Green function is the impulse response of an inhomogeneous linear differential operator, defined on a domain with specified initial condition or boundary condition. If differential operator is L(x) is linear, then one can superpose them to find the solution. u(x) = ʃ f(y) G(x , y) dy Solution of Green function if differential operator is L than – L G(x , s) = δn (s-x)
  • 4. where- δ = Dirac delta function. n = Dimension In physics :- the Green function as used in physics is usually defined with the opposite sign, that is – L G(s , x) = δ(x-s) If the operator is translation invariant that is, when L has constant coefficient with x, the Green function can be taken to be a convolution kernel, that is – G(x , s) = G(x-s) In this case, Green function is the same as the impulse of linear time invariant system theory.
  • 5. • GREEN FUNCTION FOR SCATTERING PROBLEM:- PROPERTY OF GREEN FUNCTION :- 𝛻2 + 𝐾2 G( r, r’)=𝑑3 (r, r’) --------(1) Schrodinger equation G( r,r’)=G(r-r’)  LOWER TRANSFORMATION OF GREEN FUNCTION:- G(r-r’)= 𝐺 𝑞 iq(r − r′)𝑑3 𝑞 -------(2) Generate r to q state 𝑑3 𝑟 − 𝑟′ = 1 (2𝜋)3 𝑒𝑞(𝑟−𝑟′) 𝑑3 q Eq (1), (q+𝑘2 )G (q)𝑒𝑖𝑞(𝑟−𝑟′)𝑑3q= 1 (2𝜋)3 𝑒𝑖𝑞(𝑟−𝑟′) 𝑑3q
  • 6. (-𝑞2 +𝑘2 ) 𝐺(𝑞) 𝑒𝑖𝑞(𝑟−𝑟′) 𝑑3 q= 1 (2𝜋)3 𝑒𝑖𝑞(𝑟−𝑟′) 𝑑3 q [(𝑞2 − 𝑘2)G(q)+ 1 (2𝜋)3]𝑒𝑖𝑞(𝑟−𝑟′)𝑑3𝑞 = 0 𝑒𝑖𝑞(𝑟−𝑟′) 𝑑3 q≠0 (𝑞2 − 𝑘2 )G(q)+ 1 (2𝜋)3 = 0 G(q)= - 1 (2𝜋)3 1 ( 𝑞2−𝑘2) --------(4) By equation (2) and(4) G(r-r’)= 𝐺(𝑞)𝑒𝑖𝑞(𝑟−𝑟′)𝑑3𝑞 G(r-r’)=- 1 (2𝜋)3 𝑒𝑖𝑞(𝑟−𝑟′) (𝑞2−𝑘2) 𝑑3q Value of green function
  • 7. :𝑑3 q=𝑞2 dqsin𝜃𝑑𝜃d∅ G(r-r’)=- 1 (2𝜋)3 0 ∞ 0 𝜋 0 2𝜋 𝑒𝑖𝑞(𝑟−𝑟′) (𝑞2−𝑘2) 𝑞2 𝑑𝑞sin𝜃𝑑𝜃𝑑∅ If ∞ = (𝑟 − 𝑟′ ) G(r-r’)= - 1 (2𝜋)2 0 ∞ 0 𝜋 𝑒𝑖𝑅𝑐𝑜𝑠𝜃 (𝑞2−𝑘2) 𝑞2 sin𝜃d𝜃d∅ = - 1 (2𝜋)2 0 𝜋 𝑒𝑖𝑅𝑐𝑜𝑠𝜃 𝑠𝑖𝑛𝜃𝑑𝜃 0 ∞ 𝑞2𝑑𝑞 (𝑞2−𝑘2) =(𝐼1 + 𝐼2) 𝐼1 = 0 𝜋 𝑒𝑖𝑅𝐶𝑂𝑆𝜃 sinθdθ COS𝜃 = 𝑡 -SIN𝜃𝑑𝜃 = 𝑑𝑡 𝐼1 = − 1 −1 𝑒𝑖𝑅𝑞𝑡 dt
  • 8. = 1 𝑖𝑞𝑅 (𝑒𝑖𝑞𝑟 − 𝑒−𝑖𝑞𝑅 ) G(r-r’)= - 1 (2𝜋)2 0 ∞ 𝑞2 (𝑞2+𝑘2)𝑖𝑞𝑡 𝑒𝑖𝑞𝑅 − 𝑒−𝑖𝑞𝑅 𝑑𝑞 = - 1 (2𝜋)2 −∞ ∞ 𝑞𝑒𝑖𝑞𝑡 (𝑞2−𝑘2)𝑖𝑞𝑅 𝑑𝑞 = - 1 4𝜋2 −∞ ∞ 𝑞𝑒𝑖𝑞𝑅 (𝑞+𝑘)(𝑞−𝑘) dq In equation(5) we can define q=±k Because value of 𝑞𝑒𝑖𝑞𝑡 (𝑞+𝑘)(𝑞−𝑘) (i) become=∞ Can be solved by 𝑓 𝑧 𝑑𝑧 = 2𝜋𝑖(𝑠𝑢𝑚 𝑜𝑓 𝑟𝑒𝑠𝑖𝑑𝑢𝑒) q ±𝑘 (solve) Solve at q +k cos
  • 9. Residue=𝑠𝑖𝑛𝑧 +𝑎 (2-a)f(2) =𝑠𝑖𝑛𝑧 −𝑎 (2-a)f(2) (1) For q +k (2) For q -k Residue=𝑠𝑖𝑛𝑞 𝑘 (q-k) 𝑞 (𝑞2−𝑘2) 𝑒𝑖𝑞𝑅 or =𝑠𝑖𝑛𝑞 𝑘 𝑞−𝑘 𝑞𝑒𝑖𝑞𝑅 (𝑞+𝑘)(𝑞−𝑘) = 𝑘 𝑘+𝑘 𝑒𝑖𝑞𝑅 Residue 𝑒𝑖𝑘𝑅 2 So, I= 2𝜋𝑖 − 𝑒𝑖𝑘𝑅 2 =𝜋𝑖𝑒𝑖𝑘𝑅 G(r-r’)= −1 4𝜋2𝑖𝑅 𝜋𝑖𝑒𝑖𝑘𝑅 = - 1 4𝜋𝑅 𝑒𝑖𝑘𝑅 G(r-r’)= - 1 4𝜋(𝑟−𝑟′) 𝑒𝑖𝑘(𝑟−𝑟′) Residue=𝑠𝑖𝑛𝑞 𝑘 𝑞𝑒𝑖𝑞𝑅 (𝑞2−𝑘2) Residue=- −𝑘𝑒𝑖𝑞𝑅 −2𝐾 I=2𝜋𝑖 1 2 𝑒−𝑖𝑘𝑅 =𝜋𝑖𝑒−𝑖𝑘𝑅 G(r-r’)= - 1 2 𝜋𝑖𝑒−𝑖𝑘𝑅 =- 1 4𝜋𝑅 𝑒−𝑖𝑘𝑅 Or, G(r-r’)= - 1 4𝜋(𝑟−𝑟′) 𝑒−𝑖𝑘(𝑟−𝑟′) = 𝑒−𝑖𝑘𝑅 2
  • 10. G(r-r’)= - 1 4𝜋(𝑟−𝑟′) 𝑒−𝑖𝑘(𝑟−𝑟′) + 𝑒𝑖𝑘(𝑟−𝑟′) For scattering ,we want to study about outgoing wave. So we cross restarted green function than, G(r-r’)= - 1 4𝜋(𝑟−𝑟′) 𝑒𝑖𝑘(𝑟−𝑟′) ψ = 𝜑𝑖𝑛 + 𝜑𝑠𝑐 𝜑𝑠𝑐 = 2𝜋 ħ2 ℎ(𝑟𝑟′)𝜑(𝑟′)𝑑3𝑟′ 𝜑𝑠𝑐 = 2 ħ2 − 1 4𝜋 𝑟 − 𝑟′ 𝑒𝑖𝑘 𝑟−𝑟′ 𝜑(𝑟′ )𝑑3 (𝑟′ ) 𝜑 = 𝑒𝑖𝑘𝑟 − 2𝜋ħ2 𝑒𝑖𝑘 𝑟−𝑟′ 𝑟−𝑟′ 𝜑 𝑟 𝑑3 r’ General solution of scattering problem of green function.
  • 11. • Lippmann-Schwinger Equation :- : Whenever large no. of component of scattered particles are appreciable then we use lippmann-schwinger equation. It give an integral solution of scattering problem. : By Green function, we analyze the partial wave or particle scattering and it useful for lower energy particle scattering. : But Lippmann-Schwinger equation is useful for higher energy scattering particles.
  • 12. to find lippmann-schwinger equation we use Helm-Holtz operator which is known as – ( 2 + K2 ) and we use the Green function – 2G(r , r’) = - 4πδ3[r - r’] by solving these we can write Helm-Holtz operator in form of Green function – Ѱ(r) Ѱin + Ѱsc r→ꚙ by these equations we got a solution -
  • 13. ( 2 + K2 ) Ѱ(r) = 2μ/ћ2 { μ(r’) Ѱ(r’) } this is not a unique solution. For unique solution we use Ѱ(r) in form of Ѱ0(r), r and r’. where - r = stationary vector / constant r’ = variable vector ( both are position vector ) therefore we found a unique solution – ( 2 + K2 ) Ѱ(r) = eiK.r + (2μ/ћ2) ʃ d3r’ δ3(r-r’) g(r’) Ѱ(r’) This equation is known as Lippmann-Schwinger equation.