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This article was downloaded by: [Indian Instiute of Technology Mandi]On: 23 July 2014, At: 06:06Publisher: Taylor & FrancisInforma Ltd Registered in England and Wales Registered Number: 1072954 Registered office: Mortimer House,37-41 Mortimer Street, London W1T 3JH, UK
Molecular Physics: An International Journal at theInterface Between Chemistry and PhysicsPublication details, including instructions for authors and subscription information:http://www.tandfonline.com/loi/tmph20
Multi-channel scattering problems: an analyticallysolvable modelDiwaker a & Aniruddha Chakraborty aa School of Basic Sciences , Indian Institute of Technology Mandi , Mandi , Himachal Pradesh175001 , IndiaAccepted author version posted online: 16 Mar 2012.Published online: 27 Apr 2012.
To cite this article: Diwaker & Aniruddha Chakraborty (2012) Multi-channel scattering problems: an analytically solvablemodel, Molecular Physics: An International Journal at the Interface Between Chemistry and Physics, 110:18, 2257-2267, DOI:10.1080/00268976.2012.674569
To link to this article: http://dx.doi.org/10.1080/00268976.2012.674569
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Molecular PhysicsVol. 110, No. 18, September 2012, 2257–2267
RESEARCH ARTICLE
Multi-channel scattering problems: an analytically solvable model
Diwaker and Aniruddha Chakraborty*
School of Basic Sciences, Indian Institute of Technology Mandi, Mandi, Himachal Pradesh 175001, India
(Received 29 January 2012; final version received 2 March 2012)
We have proposed a general method for finding an exact analytical solution for the multi-channel scatteringproblem in the presence of a delta function coupling. Our solution is quite general and is valid for any set ofpotentials, if the uncoupled diabatic potential has an exact solution. We have also discussed a few examples,where our method can easily be applied.
Keywords: quantum mechanics; scattering; multi-channel; two state; analytical model; Green’s function
1. Introduction
Nonadiabatic transition due to potential curve crossing
is one of the most important mechanisms to effectivelyinduce electronic transitions in collisions [1–14]. This is
a very interdisciplinary concept and appears in various
fields of physics, chemistry and even in biology
[2,3,5,7,15]. The theory of non-adiabatic transitions
dates back to 1932, when the pioneering works for
curve-crossing and non-crossing were published byLandau [16], Zener [17], Stuckelberg [18] along with
Rosen and Zener [19] respectively. Two categories in
general can be classified be classified for finding an
exact analytical solution of the curve crossing problem.
The first is that an exact analytical solution can be
obtained for the whole region of the variable (say x
here, see in the next section). For example, Osherovand Voronin solved the case where two diabatic
potentials are constant with exponential coupling
[20]. Zhu solved the case where two diabatic potentials
are exponential with exponential coupling [21]. In our
earlier publications we have reported analytical solu-
tion in those cases where two or more arbitrarypotentials are coupled by Dirac Delta interactions
[15,22–26]. The second is that an exact analytical
solution is only possible for the asymptotic region.
Then, physical quantities such as eigenvalues, scatter-
ing matrices can still be solved in an exact analytical
form, providing that the connection problem of theasymptotic solution is known. The Stokes phenom-
enon [27] of the asymptotic solution of the ordinary
differential equation provides a powerful tool to deal
with these kinds of problems [28–30]. Generalizing thereal variable to the complex variable and tracing theasymptotic solution around the complex plane, theconnection matrix which connects the asymptoticsolution in the complex plane can be expressed interms of Stokes constants. Recent work by Zhu andNakamura [30] found an exact analytical solution ofthe Stokes constants for the second-order ordinarydifferential equation with the coefficient function asthe fourth-order polynomial. In this way, exactanalytical solutions of scattering matrices wereobtained for the two state linear curve crossingproblem with constant coupling [31]. In this paper weconsider the case of two or more arbitrary diabaticpotentials with Dirac Delta couplings. The Dirac Deltacoupling model has the advantage that it can be exactlysolved [15,22–24] if the uncoupled diabatic potentialhas an exact solution.
2. Our model
We consider two diabatic curves, crossing each other.There is a coupling between the two curves, whichcauses transitions from one curve to another. Thistransition would occur in the vicinity of the crossingpoint. In particular, it will occur in a narrow range ofx, given by
V1ðxÞ � V2ðxÞ ’ V12ðxcÞ, ð1Þ
where x denotes the nuclear coordinate and xc is thecrossing point. V1 and V2 are determined by the shape
*Corresponding author. Email: [email protected]
ISSN 0026–8976 print/ISSN 1362–3028 online
� 2012 Taylor & Francis
http://dx.doi.org/10.1080/00268976.2012.674569
http://www.tandfonline.com
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of the diabatic curves and V12 represents the couplingbetween them. Therefore it is interesting to analyse amodel where coupling is localized in space near xc.Thus we put
V12ðxÞ ¼ K0�ðx� xcÞ, ð2Þ
where K0 is a constant.
3. Formulation of multi-channel scattering problems
3.1. Two channel scattering problems
We start with a particle moving on any of the twodiabatic curves and the problem is to calculate theprobability of the particle to be still on that diabaticcurve after a time t. We write the probability amplitudefor the particle as
CðxÞ ¼ 1ðxÞ 2ðxÞ
� �, ð3Þ
where 1(x) and 2(x) are the probability amplitudesfor the two states. The Hamiltonian is given by
H ¼H11ðxÞ V12ðxÞV21ðxÞ H22ðxÞ
� �, ð4Þ
where H11(x), H22(x) and V12(x) are defined by
H11ðxÞ ¼ ��h2
2m
@2
@x2þ V1ðxÞ,
H22ðxÞ ¼ ��h2
2m
@2
@x2þ V2ðxÞ,
V12ðxÞ ¼ V21ðxÞ ¼ K0�ðx� xcÞ: ð5Þ
The above V1(x) and V2(x) are determined by theshape of that diabatic curve. V12(x) is a couplingfunction which we assume to be a Dirac delta function.The time-independent Schrodinger equation is writenin the matrix form
H11ðxÞ V12ðxÞ
V21ðxÞ H22ðxÞ
� � 1ðxÞ
2ðxÞ
� �¼ E
1ðxÞ
2ðxÞ
� �: ð6Þ
This is equivalent to
H11ðxÞ 1ðxÞ þ K0�ðx� xcÞ 2ðxÞ ¼ E 1ðxÞ,
K0�ðx� xcÞ 1ðxÞ þH22ðxÞ 2ðxÞ ¼ E 2ðxÞ:ð7Þ
Integrating the above two equations from xc� � toxcþ � (where �! 0) we get the following twoboundary conditions
��h2
2m
d 1ðxÞ
dx
� �xcþ�xc��
þK0 2ðxcÞ ¼ 0,
��h2
2m
d 2ðxÞ
dx
� �xcþ�xc��
þK0 1ðxcÞ ¼ 0: ð8Þ
Also we have two more boundary conditions
1ðxc � �Þ ¼ 1ðxc þ �Þ,
2ðxc � �Þ ¼ 2ðxc þ �Þ: ð9Þ
Using the above four boundary conditions one can
derive the transition probability from one diabatic
potential to the other.
3.2. Three channel scattering problems
Here we start with a particle moving on any of the
three diabatic curves and the problem is to calculate
the probability that the particle will still be in that
diabatic curve after a time t. We write the probability
amplitude for the particle as
CðxÞ ¼
1ðxÞ
2ðxÞ
3ðxÞ
0B@
1CA, ð10Þ
where 1(x), 2(x) and 3(x) are the probability
amplitudes for the three states. The Hamiltonian
matrix of this system is given by
H ¼
H11ðxÞ V12ðxÞ V13ðxÞ
V21ðxÞ H22ðxÞ 0
V31ðxÞ 0 H33ðxÞ
0B@
1CA, ð11Þ
where H11(x), H22(x), H33(x), V12(x), V21(x), V31(x)
and V13(x) are defined by
H11ðxÞ ¼ ��h2
2m
@2
@x2þ V1ðxÞ,
H22ðxÞ ¼ ��h2
2m
@2
@x2þ V2ðxÞ,
H33ðxÞ ¼ ��h2
2m
@2
@x2þ V3ðxÞ,
V12ðxÞ ¼ V21ðxÞ ¼ K2�ðx� x2Þ,
V13ðxÞ ¼ V31ðxÞ ¼ K3�ðx� x3Þ: ð12Þ
In the above equations V1(x), V2(x) and V3(x) are
determined by the shape of the diabatic curve. The
time-independent Schrodinger equation for this pro-
blem is given by
H11ðxÞ K2�ðx� x2Þ K3�ðx� x3Þ
K2�ðx� x2Þ H22ðxÞ 0
K3�ðx� x3Þ 0 H33ðxÞ
0B@
1CA
1ðxÞ
2ðxÞ
3ðxÞ
0B@
1CA
¼ E
1ðxÞ
2ðxÞ
3ðxÞ
0B@
1CA: ð13Þ
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This matrix representation is equivalent to the
following three equations
H11ðxÞ 1ðxÞ þ K2�ðx� x2Þ 2ðxÞ
þ K3�ðx� x3Þ 3ðxÞ ¼ E 1ðxÞ,
K2�ðx� x2Þ 1ðxÞ þH22ðxÞ 2ðxÞ ¼ E 2ðxÞ,
K3�ðx� x3Þ 1ðxÞ þH33ðxÞ 3ðxÞ ¼ E 3ðxÞ:
ð14Þ
Now for simplicity, we consider the case where
K2¼K3¼K0 and x2¼x3¼xc. Then integrating the
above three equations from xc� � to xcþ � (where
�! 0) we get the following three boundary conditions
��h2
2m
d 1ðxÞ
dx
� �xcþ�xc��
þK0 2ðxcÞ þ K0 3ðxcÞ ¼ 0,
��h2
2m
d 2ðxÞ
dx
� �xcþ�xc��
þK0 1ðxcÞ ¼ 0,
��h2
2m
d 3ðxÞ
dx
� �xcþ�xc��
þK0 1ðxcÞ ¼ 0: ð15Þ
Also we have three more boundary conditions
1ðxc � �Þ ¼ 1ðxc þ �Þ,
2ðxc � �Þ ¼ 2ðxc þ �Þ,
3ðxc � �Þ ¼ 3ðxc þ �Þ: ð16Þ
Using the above six boundary conditions one can
derive analytical expressions for the transition prob-
ability from one diabatic potential to the other.
3.3. N channel scattering problems
Here we start with a particle moving on any of the N
diabatic curves and the problem is to calculate the
probability that the particle will still be in the diabatic
curve after a time t. We write the probability amplitude
for the particle as
CðxÞ ¼
1ðxÞ
2ðxÞ
3ðxÞ
:
:
:
NðxÞ
0BBBBBBBBBBB@
1CCCCCCCCCCCA, ð17Þ
where n(x) is the probability amplitude
for the nth state and n can take any value from 1
to N. The Hamiltonian matrix of this system is
given by
H ¼
H11ðxÞ V12ðxÞ V13ðxÞ : : V1NðxÞ
V21ðxÞ H22ðxÞ 0 0 0 0
V31ðxÞ 0 H33ðxÞ 0 0 0
: : : : : :
: : : : : :
VN1ðxÞ 0 0 0 0 HNNðxÞ
0BBBBBBBB@
1CCCCCCCCA,
ð18Þ
where Hnn(x), V1n(x) and Vn1(x) are defined by
HnnðxÞ ¼ ��h2
2m
@2
@x2þ VnðxÞ,
V1nðxÞ ¼ Vn1ðxÞ ¼ Kn�ðx� xnÞ: ð19Þ
The time-independent Schrodinger equation for this
problem is given by
H11ðxÞ K2�ðx�x2Þ K3�ðx�x3Þ : : KN�ðx�xNÞ
K2�ðx�x2Þ H22ðxÞ 0 0 0 0
K3�ðx�x3Þ 0 H33ðxÞ 0 0 0
: : : : : :
: : : : : :
KN�ðx�xNÞ 0 0 0 0 HNNðxÞ
0BBBBBBBB@
1CCCCCCCCA
�
1ðxÞ
2ðxÞ
3ðxÞ
:
:
:
NðxÞ
0BBBBBBBBBBB@
1CCCCCCCCCCCA¼E
1ðxÞ
2ðxÞ
3ðxÞ
:
:
:
NðxÞ
0BBBBBBBBBBB@
1CCCCCCCCCCCA: ð20Þ
This matrix representation is equivalent to the follow-
ing equations
H11ðxÞ 1ðxÞ þXn¼Nn¼2
Kn�ðx� xnÞ nðxÞ ¼ E 1ðxÞ,
Kn�ðx� xnÞ 1ðxÞ þHnnðxÞ nðxÞ ¼ E nðxÞ: ð21Þ
Now for simplicity, we consider the case where
K2¼K3¼ � � � ¼KN¼K0 and x2¼x3 � � � ¼ xN¼ xc.
Integrating the above equations from xc� � to xcþ �(where �! 0) we get the following N boundary
conditions
��h2
2m
d 1ðxÞ
dx
� �xcþ�xc��
þK0
Xn¼Nn¼2
nðxcÞ ¼ 0,
��h2
2m
d nðxÞ
dx
� �xcþ�xc��
þK0 1ðxcÞ ¼ 0: ð22Þ
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Also we have N more boundary conditions
nðxc � �Þ ¼ nðxc þ �Þ ð23Þ
Using all 2N boundary conditions one can derive
analytical expressions for the transition probability
from one diabatic potential to the other.
4. Multi-channel scattering problems: Green’s
function method
4.1. Two channel scattering problems
We start with the time-independent Schrodinger
equation for a two state system
H11ðxÞ V12ðxÞ
V21ðxÞ H22ðxÞ
� � 1ðxÞ
2ðxÞ
� �¼ E
1ðxÞ
2ðxÞ
� �: ð24Þ
The above two equations can be written in the
following form
2ðxÞ ¼ V12ðxÞ�1 E�H11ðxÞ½ � 1ðxÞ,
2ðxÞ ¼ E�H22ðxÞ½ ��1V21ðxÞ 1ðxÞ: ð25Þ
Eliminating 2(x) from the above two equations we get
E�H11ðxÞ½ � 1ðxÞ � V12ðxÞ E�H22ðxÞ½ ��1
V21ðxÞ 1ðxÞ ¼ 0: ð26Þ
The above equations simplify considerably if V12(x)
and V21(x) are Dirac Delta functions at xc, which in
operator notation may be written as V¼K0S¼K0jxci
hxcj. The above equation now becomes
E�H11ðxÞ½ � � K20jxcihxcj E�H22ðxÞ½ �
�1jxcihxcj
� � 1ðxÞ ¼ 0: ð27Þ
This may be written as
H11ðxÞ þ K20�ðx� xcÞG
02ðxc, xc;EÞ
� 1ðxÞ ¼ E 1ðxÞ:
ð28Þ
The above equation can be written in the following
form
E�H11½ � 1ðxÞ ¼ K20�ðx� xcÞG
02ðxc, xc;EÞ 1ðxÞ, ð29Þ
where the right-hand side is considered as an inhomo-
geneous term. The general solution of this equation
can be written as
1ðxÞ ¼ 0ðxÞ þ K20G
01ðx,xc;EÞG
02ðxc, xc;EÞ 1ðxcÞ,
ð30Þ
where 0(x) is a solution of the homogeneousequations
E�H11½ � 0ðxÞ ¼ 0, E�H11½ �G01ðx, x
0;EÞ ¼ �ðx� x0Þ:
ð31Þ
In the above equations
1ðxÞ ¼
Z 1�1
dx0Gðx,x0;EÞ 0ðx0Þ,
0ðxÞ ¼
Z 1�1
dx0G01ðx, x
0;EÞ 0ðx0Þ: ð32Þ
So Equation (30) can be written asZ 1�1
dx0Gðx,x0;EÞ 0ðx0Þ ¼
Z1�1
dx0G01ðx,x
0;EÞ 0ðx0Þ
þK20G
01ðx,xc;EÞG
02ðxc,xc;EÞ
�
Z 1�1
dx0Gðxc,x0;EÞ 0ðx
0Þ:
ð33Þ
The solution in terms of Green’s function is as follows
Gðx, x0;EÞ ¼ G01ðx, x
0;EÞ þ K20G
01ðx, xc;EÞG
02ðxc, xc;EÞ
� Gðxc, x0;EÞ: ð34Þ
In the above equation we put x¼ xc
Gðxc,x0;EÞ ¼ G0
1ðxc, x0;EÞ þ K2
0G01ðxc, xc;EÞ
� G02ðxc, xc;EÞGðxc, x
0;EÞ: ð35Þ
After simplification, we get
Gðxc,x0;EÞ ¼
G01ðxc, x
0;EÞ
1� K20G
01ðxc, xc;EÞG
02ðxc, xc;EÞ
, ð36Þ
so that
Gðx, x0;EÞ ¼ G01ðx, x
0;EÞ
þK2
0G01ðx, xc;EÞG
02ðxc, xc;EÞG
01ðxc, x
0;EÞ
1� K20G
01ðxc,xc;EÞG
02ðxc, xc;EÞ
:
ð37Þ
Using this expression of G(x, x0;E) one can calculatethe wave function and from the wave function one caneasily calculate the transition probability from onediabatic potential to the other.
4.2. Three channel scattering problems
We start with the time-independent Schrodingerequation for a three state system, given by
H11ðxÞ V12ðxÞ V13ðxÞ
V21ðxÞ H22ðxÞ 0
V31ðxÞ 0 H33ðxÞ
0B@
1CA
1ðxÞ
2ðxÞ
3ðxÞ
0B@
1CA ¼ E
1ðxÞ
2ðxÞ
3ðxÞ
0B@
1CA:ð38Þ
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This matrix equation can be written in the following
form
H11ðxÞ � E½ � 1ðxÞ þ V12ðxÞ 2ðxÞ þ V13ðxÞ 3ðxÞ ¼ 0,
H22ðxÞ � E½ � 2ðxÞ þ V21ðxÞ 1ðxÞ ¼ 0,
H33ðxÞ � E½ � 3ðxÞ þ V31ðxÞ 1ðxÞ ¼ 0:
ð39Þ
The above equation after rearranging is given below
E�H11ðxÞ½ � 1ðxÞ � V12ðxÞ 2ðxÞ � V13ðxÞ 3ðxÞ ¼ 0,
ð40Þ
2ðxÞ ¼ E�H22ðxÞ½ ��1V21ðxÞ 1ðxÞ, ð41Þ
3ðxÞ ¼ E�H33ðxÞ½ ��1V31ðxÞ 1ðxÞ: ð42Þ
After eliminating both 2(x) and 3(x) from
Equation (40) we get�E�H11ðxÞ½ � � V12ðxÞ E�H22ðxÞ½ �
�1V21ðxÞ � V13ðxÞ
E�H33ðxÞ½ ��1V31ðxÞÞ 1ðxÞ ¼ 0: ð43Þ
The above equations are true for any general V12, V21,
V13 and V31. The above equations simplify consider-
ably if V12, V13, V31 and V21 are Dirac Delta functions,
which we write in operator notation as V12¼V21¼
K2S¼K2jx2ihx2j and V13¼V31¼K3S¼K3jx3ihx3j.
The above equation now becomes�E�H11ðxÞ½ � � K2
2�ðx� x2ÞG02ðx2, x2;EÞ � K2
3�ðx� x3Þ
� G02ðx3, x3;EÞ
� 1ðxÞ ¼ 0: ð44Þ
This may be written as
E�H12ðxÞ½ � � K23�ðx� x3ÞG
03ðx3,x3;EÞ
� � 1ðxÞ ¼ 0,
ð45Þ
where
H12ðxÞ ¼ H11ðxÞ þ K22�ðx� x2ÞG
02ðx2, x2;EÞ: ð46Þ
For H12(x), one can find the corresponding Green’s
function G12(x, x0;E) using the method as we have used
in the two-state case.
E�H11½ � 1ðxÞ ¼ K22�ðx� x2ÞG
02ðx2, x2;EÞ 1ðxÞ, ð47Þ
where the right-hand side is considered as an inhomo-
geneous term. The general solution of this equation
can be written as
1ðxÞ ¼ 0ðxÞ þ
Z 1�1
dxG01ðx, x
0;EÞK22�ðx
0 � x2Þ
� G02ðx2, x2;EÞ 1ðx
0Þ, ð48Þ
where 0(x) is a solution of the homogeneous equation
ðE�H11Þ 0ðxÞ ¼ 0, ð49Þ
where
ðE�H11ÞG01ðx,x
0;EÞ ¼ �ðx� x0Þ: ð50Þ
So
1ðxÞ ¼ 0ðxÞ þ K22G
01ðx,x2;EÞG
02ðx2,x2;EÞ 1ðx2Þ:
ð51Þ
In the above expression
1ðxÞ ¼
Z 1�1
dx0G12ðx, x0;EÞ 0ðx
0Þ,
0ðxÞ ¼
Z 1�1
dx0G01ðx, x
0;EÞ 0ðx0Þ: ð52Þ
So Equation (51) can be written asZ 1�1
dx0G12ðx, x0;EÞ 0ðx
0Þ
¼
Z 1�1
dx0G01ðx, x
0;EÞ 0ðx0Þ
þ K22G
01ðx, x2;EÞG
02ðx2, x2;EÞ
�
Z 1�1
dx0G12ðx2, x0;EÞ 0ðx
0Þ: ð53Þ
The solution in terms of Green’s function, extracted
from the last equation
G12ðx, x0;EÞ ¼ G0
1ðx, x0;EÞ þ K2
2G01ðx, x2;EÞ
� G02ðx2, x2;EÞG12ðx2, x
0;EÞ: ð54Þ
In the above equation we put x¼ x2 to get
G12ðx2, x0;EÞ ¼ G0
1ðx2, x0;EÞ þ K2
2G02ðx2, x2;EÞ
� G01ðx2, x2;EÞG12ðx2, x
0;EÞ: ð55Þ
So after simplification we get
G12ðx2, x0;EÞ ¼
G01ðx2, x
0;EÞ
1� K22G
01ðx2, x2;EÞG
02ðx2, x2;EÞ
,
ð56Þ
so that
G12ðx,x0;EÞ ¼G0
1ðx,x0;EÞ
þK2
2G01ðx,x2;EÞG
02ðx2,x2;EÞG
01ðx2,x
0;EÞ
1�K22G
01ðx2,x2;EÞG
02ðx2,x2;EÞ
:
ð57Þ
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Now we will incorporate the effect of a third state
which is coupled to the first state only, i.e. we will solve
Equation (46) in terms of Green’s function.
G13ðx,x0;EÞ¼G12ðx,x
0;EÞ
þK2
2G12ðx,x3;EÞG02ðx3,x3;EÞG12ðx3,x
0;EÞ
1�K22G12ðx3,x3;EÞG
02ðx3,x3;EÞ
:
ð58Þ
In the above expression, we have Green’s function for
the three-state scattering problem using a delta
function coupling model. Using the above expression
one can calculate the wave function and from the wave
function one can easily calculate the transition prob-
ability from one diabatic potential to the other.
4.3. N channel scattering problems
We start with the time-independent Schrodinger
equation for a N state system, given by
H11ðxÞ V12ðxÞ V13ðxÞ : : V1NðxÞ
V21ðxÞ H22ðxÞ 0 0 0 0
V31ðxÞ 0 H33ðxÞ 0 0 0
: : : : : :
: : : : : :
VN1ðxÞ 0 0 : : HNNðxÞ
0BBBBBBBB@
1CCCCCCCCA
1ðxÞ
2ðxÞ
3ðxÞ:
:
NðxÞ
0BBBBBB@
1CCCCCCA
¼E
1ðxÞ
2ðxÞ
3ðxÞ
:
:
NðxÞ
0BBBBBBBB@
1CCCCCCCCA: ð59Þ
This matrix equation can be written in the following
form
H11ðxÞ � E½ � 1ðxÞ þXn¼Nn¼2
V1nðxÞ nðxÞ ¼ 0,
HnnðxÞ � E½ � nðxÞ þ Vn1ðxÞ 1ðxÞ ¼ 0: ð60Þ
The above equations after rearrangement are given
below as
E�H11ðxÞ½ � 1ðxÞ �XNn¼2
V1nðxÞ nðxÞ ¼ 0, ð61Þ
nðxÞ ¼ E�HnnðxÞ½ ��1Vn1ðxÞ 1ðxÞ: ð62Þ
After eliminating n(x) from Equation (61) we get
E�H11ðxÞ½ � 1ðxÞ �XNn¼2
V1nðxÞ E�HnnðxÞ½ ��1
Vn1ðxÞ 1ðxÞ ¼ 0: ð63Þ
The above equations are true for any general V1n and
Vn1. The above equation simplifies considerably if V1n
and Vn1 are Dirac Delta functions, which we write in
operator notation as V1n¼Vn1¼KnS¼Knjxnihxnj. The
above equation now becomes
E�H11ðxÞ½ ��XNn¼2
K2n�ðx�xnÞG
0nðxn,xn;EÞ
! 1ðxÞ ¼ 0:
ð64Þ
This may be written as
E�H12ðxÞ½ ��XNn¼3
K2n�ðx�xnÞG
0nðxn,xn;EÞ
! 1ðxÞ ¼ 0,
ð65Þ
where
H12ðxÞ ¼ H11ðxÞ þ K22�ðx� x2ÞG
02ðx2, x2;EÞ: ð66Þ
For H12(x), one can find the corresponding Green’s
function G12(x, x0;E) using the method as we have used
in the two-state case. Similarly we can define H13(x),
so that
E�H13ðxÞ½ ��XNn¼4
K2n�ðx�xnÞG
0nðxn,xn;EÞ
! 1ðxÞ ¼ 0,
ð67Þ
where
H13ðxÞ ¼ H12ðxÞ þ K23�ðx� x3ÞG
03ðx3, x3;EÞ: ð68Þ
For H13(x), one can find the corresponding Green’s
function G13(x, x0;E) using the method as we have used
in the two-state case. This is possible because we have
already derived analytical expression for G12(x, x0;E).
So if the analytical expression of G12(x, x0;E) is known,
it is possible to derive an analytical expression of G13(x,
x0;E) using the method we have discussed for the two
channel case. Using the same analogy, an analytical
expression of G1n(x, x0;E) (for any ‘n’) can be derived, if
we know the analytical expression for G1[n� 1](x, x0;E).
So we can define H1(N� 1)(x), in the following equation
E�H1½N�1�ðxÞ�
�K2N�ðx�xNÞG
0NðxN,xN;EÞ
� � 1ðxÞ ¼ 0,
ð69Þ
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where
H1½N�1�ðxÞ ¼ H11ðxÞ þXN�1n¼2
K2n�ðx� xnÞG
0nðxn, xn;EÞ:
ð70Þ
In this case, one can find the Green’s function
G1N(x,x0;E) using the method as we have already
used for two-channel case.
G1Nðx,x0;EÞ
¼G1½N�1�ðx,x0;EÞ
þK2
2G1½N�1�ðx,xN;EÞG0NðxN,xN;EÞG1½N�1�ðxN,x
0;EÞ
1�K22G1½N�1�ðxN,xN;EÞG0
NðxN,xN;EÞ:
ð71Þ
So it is possible to derive an analytical expression for
G1N(x, x0;E) and using G1N(x, x0;E), one can calculate
a wave function explicitly and from the wave function
one can easily calculate the transition probability from
one diabatic potential to all other diabatic potentials.
5. Exact analytical solutions: three simple cases
5.1. Constant potential case
In region 1 ( x5 xc), the time-independent Schrodinger
equation for the first potential is given by
��h2
2m
@2 1ðxÞ
@x2þ V1 1ðxÞ ¼ E 1ðxÞ: ð72Þ
The above equation has the following solution
1ðxÞ ¼ A expðik1xÞ þ B expð�ik1xÞ, ð73Þ
where k1¼ [(2m/�h2)(E�V1)]1/2. In region 2 (x4 xc),
the time-independent Schrodinger equation for the first
potential is given by
��h2
2m
@2 1ðxÞ
@x2þ V1 1ðxÞ ¼ E 1ðxÞ: ð74Þ
The physically acceptable solution of the above
equation is given by
1ðxÞ ¼ C expðik1xÞ: ð75Þ
In region 1 ( x5 xc), the time-independent Schrodinger
equation for the second potential is given by
��h2
2m
@2 2ðxÞ
@x2þ V2 2ðxÞ ¼ E 2ðxÞ: ð76Þ
The physically acceptable solution is given by
2ðxÞ ¼ D expð�ik2xÞ, ð77Þ
where k2¼ [(2m/�h2)(E�V2)]1/2. In region 2 (x4 xc),
the time-independent Schrodinger equation for the
second potential is given by
��h2
2m
@2 2ðxÞ
@x2þ V2 2ðxÞ ¼ E 2ðxÞ: ð78Þ
The physically acceptable solution is given by
2ðxÞ ¼ F expðik2xÞ: ð79Þ
Here we put xc¼ 0. Now using four boundary
conditions we calculate
F
A
2¼ imK0k1�h
2
ðk1k2�h4 þm2K20Þ
2
ð80Þ
and
D
A
2¼ imK0k1�h
2
ðk1k2�h4 þm2K20Þ
2
: ð81Þ
So, the transition probability is given by
T ¼ 2k2k1
imK0k1�h2
ðk1k2�h4 þm2K20Þ
2
: ð82Þ
In our numerical calculation we use atomic units so
that �h¼ 1. In atomic units, we set V1(x)¼ 0, V2(x)¼ 5,
K0¼ 1.0 and m¼ 1.0. The result of our calculation is
shown in Figure 1.
5.2. Linear potential case
The time-independent Schrodinger equation for the
case where a linear potential coupled to another linear
p
Figure 1. The plot of transition probability from oneconstant potential to another constant potential as a functionof energy of incident particle (K0¼ 1.0).
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potential through a Dirac delta interaction is given
below (see Figure 2).
� �h2
2m@2
@x2þp1x K0�ðx�xcÞ
K0�ðx�xcÞ ��h2
2m@2
@x2�p2x
! 1ðxÞ
2ðxÞ
� �¼E
1ðxÞ
2ðxÞ
� �:
ð83Þ
Equation (83) can be split into two equations
��h2
2m
@2
@x2þ p1x
� � 1ðxÞ þ K0�ðxÞ 2ðxÞ ¼ E 1ðxÞ,
��h2
2m
@2
@x2� p2x
� � 2ðxÞ þ K0�ðxÞ 1ðxÞ ¼ E 2ðxÞ:
ð84Þ
In our calculation, we use p1¼ p2¼ 1. The time-
independent Schrodinger equation for the first diabatic
potential is given below,
��h2
2m
@2
@x2þ x
� � 1ðxÞ ¼ E 1ðxÞ: ð85Þ
In region 1 (x5 xc) the physically acceptable solution
is given below
1ðxÞ ¼ ðAþ BÞAi 21=3ð�Eþ xÞ
� þ iðA� BÞBi 2
1=3ð�Eþ xÞ�
: ð86Þ
Here, Ai[z] and Bi[z] represent the Airy functions. In
the above expression A denotes the probability
amplitude for motion along the positive direction and
B denotes the probability amplitude for motion along
the negative direction [15]. The physically acceptable
solution in region 2 (x4 xc) is given by
1ðxÞ ¼ CAi 21=3ð�Eþ xÞ
� : ð87Þ
In this region the net flux is zero [24].
The time-independent Schrodinger equation for the
second diabatic potential is given below
��h2
2m
@2
@x2� x
� � 2ðxÞ ¼ E 2ðxÞ: ð88Þ
In region1 (x5 xc) the physically acceptable solution is
2ðxÞ ¼ DAi 21=3ð�E� xÞ
� : ð89Þ
In this region the net flux is zero [15]. In region 2
(x4 xc) the physically acceptable solution is
2ðxÞ ¼ F Ai 21=3ð�E� xÞ
� � iBi 2
1=3ð�E� xÞ� � �
:
ð90Þ
Using the four boundary conditions mentioned in
Section 3.1 (here we put xc¼ 0), we have derived an
analytical expression for the transition probability
from one diabatic potential to the other diabatic
potential and the final expression is given below:
T ¼NL
DL
2, ð91Þ
where
NL ¼ 4� 21=3Ai �21=3E
� 2�Ai �2
1=3E�
B0i �21=3E
� � A0i �2
1=3E�
Bi �21=3E
� �ð92Þ
and
DL¼4Ai �21=3E
� 4�8iAi �2
1=3E� 3
Bi �21=3E
� þ22=3A0i �2
1=3E� 2
Bi �21=3E
� 2þAi �2
1=3E� 2
� 22=3B0i �21=3E
� 2�4Bi �2
1=3E� 2h i
�25=3Ai �21=3E
� A0i �2
1=3E�
Bi �21=3E
� B0i �2
1=3E�
:
ð93Þ
In our numerical calculation we set p1¼ 1, p2¼ 1,
K0¼ 1 and m¼ 1 in atomic units. The result of our
calculation is shown in Figure 3.
5.3. Exponential potential case
The time-independent Schrodinger equation for the
case where an exponential potential coupled to another
exponential potential through a Dirac delta interaction
is given below (see Figure 4).
� �h2
2m@2
@x2þ V0 expðaxÞ K0�ðx� xcÞ
K0�ðx� xcÞ � �h2
2m@2
@x2þ V0e
�ax
! 1ðxÞ
2ðxÞ
� �
¼ E 1ðxÞ
2ðxÞ
� �: ð94Þ
Figure 2. Schematic diagram of the two-state problem,where one linear potential is coupled to another linearpotential in the diabatic representation.
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Equation (94) can be split into the following two
equations
��h2
2m
@2
@x2þV0 expðaxÞ
� � 1ðxÞþK0�ðx�xcÞ 2ðxÞ ¼E 1ðxÞ,
��h2
2m
@2
@x2þV0 expð�axÞ
� � 2ðxÞþK0�ðx�xcÞ 1ðxÞ ¼E 2ðxÞ:
ð95Þ
In our calculation we took V0¼ 1.0 and a¼ 1. The
time-independent Schrodinger equation for the first
diabatic potential is given below
��h2
2m
@2
@x2þ V0 expðaxÞ
� � 1ðxÞ ¼ E 1ðxÞ: ð96Þ
In the region x5 xc, the solution of the above equationis given below
1ðxÞ ¼ AIð2ið2EÞ1=2Þ 2½2 expðxÞ�
1=2� �
þ BIð�2ið2EÞ1=2Þ 2½2 expðxÞ�
1=2� �
: ð97Þ
Here In(z) represents the modified Bessel function ofthe first kind. In the above expression A denotes theprobability amplitude for motion along the positivedirection and B denotes the probability amplitude formotion along the negative direction [15]. In the region,where x4 xc, the physically acceptable solution is
1ðxÞ ¼ CKð�2ið2EÞ1=2Þ 2½2 expðxÞ�
1=2� �
: ð98Þ
Here Kn(z) represents the modified Bessel function ofthe second kind. In this region the net flux is zero [15].
For the second diabatic potential, the time-inde-pendent Schrodinger equation is given below
��h2
2m
@2
@x2þ V0 expð�axÞ
� � 2ðxÞ ¼ E 2ðxÞ: ð99Þ
In the region, where x4 xc, the physically acceptablesolution is
2ðxÞ ¼ FIð�2ið2EÞ1=2Þ 2½2 expð�xÞ�
1=2� �
: ð100Þ
In the region, where x5 xc, the physically acceptablesolution is
2ðxÞ ¼ DKð�2ið2EÞ1=2Þ 2½2 expðxÞ�
1=2� �
: ð101Þ
In this region the net flux is zero [15]. Using fourboundary conditions as discussed in Section 3.1 (withxc¼ 0), we have derived an analytical expression forthe transition probability from one exponential poten-tial to the other exponential potential, and is given by
T ¼ 1�NE
DE
2, ð102Þ
where
NE ¼ �Ið2:83iE1=2Þð2:83Þ
Ið�2:83iE1=2Þð2:83Þ� Kð�2:83iE1=2Þð2:83Þ
� ð½Ið�2:83iE1=2�1Þð2:83Þ þ I1�ð2:83iE1=2Þð2:83Þ�
� Ið2:83iE1=2Þð2:83ÞðIð�2:83iE1=2Þð2:83Þ½Kð�2:83iE1=2�1Þ
� ð2:83Þ þ K1�ð2:83iE1=2Þð2:83Þ�
þ ½Ið�2:83iE1=2�1Þð2:83Þ þ I1�ð2:83iE1=2Þð2:83Þ�
� Kð�2:83iE1=2Þð2:83ÞÞ � Ið�2:83iE1=2Þð2:83Þ
� ½Ið2:83iE1=2�1Þð2:83Þ þ Ið2:83iE1=2þ1Þð2:83Þ�
� ðIð�2:83iE1=2Þð2:83Þ½Kð�2:83iE1=2�1Þð2:83Þ
þ K1�ð2:83iE1=2Þð2:83Þ� þ ½Ið�2:83iE1=2�1Þð2:83Þ
þ I1�ð2:83iE1=2Þð2:83Þ�Kð�2:83iE1=2Þð2:83ÞÞÞ
c
Figure 4. Schematic diagram of the two-state problem,where one exponential potential is coupled to anotherexponential potential in the diabatic representation.
p
Figure 3. The plot of transition probability from one linearpotential to another linear potential, as a function of energyof incident particle (K0¼ 1.0).
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and
DE¼ Ið�2:83E1=2Þð2:83ÞðIð�2:83E1=2Þð2:83Þ2ð�Kð�2:83iE1=2�1Þð2:83Þ
2
�2Kð1�2:83iE1=2Þð2:83ÞKð�2:83iE1=2�1Þð2:83Þ
�Kð1�2:83iE1=2Þð2:83Þ2þ0:08Kð�2:83iE1=2Þð2:83Þ
2Þ
þðIð�2:83E1=2�1Þð2:83Þþ Ið1�2:83iE1=2Þð2:83ÞÞ
� Ið�2:83E1=2Þð2:83Þð�2Kð�2:83E1=2�1Þð2:83Þ
�2Kð1�2:83iE1=2Þð2:83ÞÞKð�2:83iE1=2Þð2:83Þ
þð�Ið�2:83E1=2�1Þð2:83Þ2�2Ið1�2:83iE1=2Þð2:83Þ
� Ið�2:83E1=2�1Þð2:83Þ� Ið1�2:83iE1=2Þð2:83Þ2Þ
�Kð�2:83E1=2Þð2:83Þ2Þ
In our numerical calculation we set K0¼ 1 and m¼ 1 in
atomic units. The result of our calculation is shown in
Figure 5.
6. Conclusions
We have proposed a general method for finding an
exact analytical solution for the multi-channel quan-
tum scattering problem in the presence of a delta
function coupling. Our solution is quite general and is
valid for any potential. We have also extended our
model to deal with general one-dimensional multi-
channel scattering problems. The same procedure is
also applicable to the case where S is a non-local
operator and may be represented by S� j f i K0 hgj,
where f and g are arbitrary acceptable functions.
Choosing both of them to be Gaussian should be an
improvement over the delta function coupling model. S
may even be a linear combination of such operators.
Acknowledgements
One of the authors (A.C.) thanks Prof. K.L. Sebastian forsuggesting this very interesting problem. A.C. would like tothank Prof. M.S. Child for his kind interest, suggestions andencouragements.
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Figure 5. The plot of transition probability from oneexponential potential to the other as a function of energyof incident particle (K0¼ 1.0).
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