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Thesis First Advance PDF

1) The document derives the Paraxial Helmholtz Equation and proposes an ansatz to solve it. 2) Several substitutions are made to obtain a differential equation for the normalization factor N(z) and a separate differential equation for the function S(z). 3) A change of variables is used to reduce the equation for S(z) to the Ermakov equation for a new function w(z). 4) Expressions are obtained relating the original unknown functions N(z) and S(z) to the new function w(z), solving the Paraxial Helmholtz Equation.

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Gerardo Jimenez
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0% found this document useful (0 votes)
110 views4 pages

Thesis First Advance PDF

1) The document derives the Paraxial Helmholtz Equation and proposes an ansatz to solve it. 2) Several substitutions are made to obtain a differential equation for the normalization factor N(z) and a separate differential equation for the function S(z). 3) A change of variables is used to reduce the equation for S(z) to the Ermakov equation for a new function w(z). 4) Expressions are obtained relating the original unknown functions N(z) and S(z) to the new function w(z), solving the Paraxial Helmholtz Equation.

Uploaded by

Gerardo Jimenez
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
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Download as PDF, TXT or read online on Scribd
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First Advances of Thesis

Gerardo Jimenez Trejo

April 17, 2020

First we are going to solve the Paraxial Helmholtz Equation as follows:


i ∂U −1 n0
= 2 ∇⊥ U + Ω2 r 2 U (1)
k0 ∂z 2k0 n0 2
Now with this we will purpose the following ansatz. Let U (r, z) = N (z)eiS(z)r where N (z) is just
2

a normalization factor and S(z) is a function top be determined.


With this let us calculate the solutions
 
dU iS(z)r2 dN (z) iS(z)r2 2 dS(z) dN (z) dS(z)
=e + N (z)e ir =e iS(z)r2 2
+ ir N (z) (2)
dz dz dz dz dz
     
1 d d 1 d d iS(z)r2 N (z) d d iS(z)r2
∇⊥ U = r U = r N (z)e = r e
r dr dr r dr dr r dr dr

N (z) d  2
 N (z)S(z) [2i] d  2
 N (z)S(z) [2i]
irS(z)(2r)eiS(z)r = r2 eiS(z)r = 2r + 2ir3 S(z)

=
r dr r dr r

(3)
2
∇⊥ U = N (z)S(z)[4i]eiS(z)r (1 + ir2 S(z))
Then we replace this results in the Paraxial Helmholtz Equation and then we obtain the follow-
ing.
  
i iS(z)r2 dN (z) 2 dS(z) −1 h 2
i
e + ir N (z) = 2 N (z)S(z)[4i]eiS(z)r (1 + ir2 S(z)) +
k0 dz dz 2k0 n0

n0 2 2  2

+ Ω r N (z)eiS(z)r
2

 
i dN (z) dS(z) −1   n0
+ ir2 N (z) = 2 N (z)S(z)[4i](1 + ir2 S(z)) + Ω2 r2 (N (z))
k0 dz dz 2k0 n0 2

Then if we divide by N (z) the whole expression we will obtain the following terms
i dN (z) dS(z) 2 2iS(z) k0 n0 2 2
− r2 = S(z)2 r2 − + Ω r
N (z) dz dz k0 n0 k0 n0 2
Then we will separate the imaginary and real terms of each other and we will obtain the following
1 dN (z) −2
= S(z)
N (z) dz k0 n0
d −2

ln(N (z)) = S(z) (4)
dz k0 n0
The next equation do not have any relation with r because this expressions are in the ask Dra.
Sara

1
dS(z) 2 k 0 n0 2 2
−r2 = S(z)2 r2 + Ω r
dz k0 n0 2
dS(z) 2 k 0 n0 2
= S(z)2 + Ω
dz k0 n0 2
   2
d 2 2
S(z) + S(z) + Ω2 = 0 (5)
dz k0 n0 k0 n0
The last equation 5 can be reduced to other one, that we know the solutions now. Let us purpose
the following change of variable: let α = k02n0 and β = S(z). With this we will make the following
assumptions. β ∈ C ⇒ αβ = αβR + iαβI where αβ 0 = αβR0 + iαβI0 is the derivative of β function.
Then if we replace this solution to the equation.
d
(αβ 0 ) + (α2 β 2 ) + Ω2 = 0
dz
0
⇒ α(βR + iβI0 ) + α(βR
2
+ 2iβR βI − βI2 ) + Ω2 = 0 (6)
Taking the imaginary part of the last equation.
βI0
βI0 + α(2βR βI ) = 0 ⇒ = −2αβR ⇒
βI
d
−2αβR = (ln βI ) (7)
dz
The last expression tell us that the function βR ∝ d
dz ln w ⇒

d
βR = κ ln w (8)
dz
Then replacing the expression of βR in 7 we will obtain the following

−2ακ(ln βR )0 = ln(βI )0 ⇒ −2ακ(ln βR ) + ln(λ) = ln(βI )


ln w−2ακ λ = ln(βI )


λ
⇒ βI = (9)
w−2ακ
 
The equation 9 and 8 will be replaced in the real part of 6 with the term βR0 = κ w00
w − w02
w2
and we will obtain the following.
0
α(βR + α2 βR
2
− αβI2 ) + Ω2 = 0
 00  0 2
w02
  
w w λ
ακ − 2 + α2 κ −α + Ω2 = 0
w w w w2ακ

w00 w02 2 2 λ
+ 2 κ α − ακ − α2 2ακ + Ω2 = 0

ακ
w w w
In order to obtain a new dierential equation, we have to purpose that κ2 α2 − ακ = 0 this


mean that κ = α1 , then if we replace the value of it, and make the term λ in a convenient way, such
that λ = 1 we will obtain the following equation.
d2 w 4
2
+ Ω2 w = 2 2 3 (10)
dx k0 n0 w
The equation 10 is the well known Ermakov equation. Then going back to 5 we can write the
complete solution in terms of our new function w. With αβ = k02n0 S(z) = αβR +iαβI . The equation
9 has the form of βI = w12 and 8 will be βR = ww .
0

2
2 1 2i 1 d
S(z) = + where = ln(w(z)) (11)
k0 n0 R(z) k0 n0 w2 R(z) dz
As we can see the new function w is involved in all our unknown functions. In this way we will
replace the equation 11 in 5 and we will obtain the following.
−d d 2i
ln (N (z)) = ln(w(z)) +
dz dz k0 n0 w2
Z z
d d d 2dz̃
− ln (N (z)) = ln(w(z)) + i χ(z) where χ(z) =
dz dz dz k0 n0 w2 (z̃)
N (z) 1
= e−iχ(z)
N0 w
N0 −iχ(z)
N (z) = e (12)
w
Now, let us take the Ermakov equation (10). We know from the literature, that while we know
a particular solution of this equation we are able to nd the general solution in terms of this. Let
µ(z) solution and wp (z) a particular solution of the Ermakov equation, the general solution can be
written as follows.
1
w(z) = ± aµ2 (z) + bµ(z)wp (z) + cwp2 (z) 2 (13)


Where the coecients had to fullll this relation. 4ac − b2 = W2α


0
and W0 is the wronskian
of the equation. In order to nd a linearly independent function, the wronskian of the function
has to be zero. When we nd the solution to the homogeneous equation we are able to nd the
d2 w
complete solution in the form of equation 13. Then solving the following relation 2 + Ω2 w = 0
dz
the particular solution is wp = cos Ωz and its orthogonal complement is µ = sin Ωz .
Then let us calculate the wornskian of the solutions in order to guarantee the orthogonality of
the system.

wp µ cos Ωz sin Ωz
W0 = 0 = =Ω
wp µ0 −Ω sin Ωz Ω cos Ωz

The replacing the particular solution of the homogeneous in the equation 13 as follows.
1  1
w(z) = ± a sin2 Ωz + b sin Ωz cos Ωz + c cos2 Ωz 2 = k12 cos Ω(z − z0 ) + k22 sin Ω(z − z0 ) 2 (14)


We can represent, the term in the coecient b as a shift in z. With this we can nd two
possibilities b = 0 ⇒ z0 6= 0 or b 6= 0 ⇒ z0 = 0, we choose the second option and then we expand
the solution w(z) by the trigonometrical options.

w(z) = [k12 (cos2 Ωz cos2 Ωz0 + 2 cos Ωz cos Ωz0 sin Ωz sin Ωz0 + sin2 Ωz sin2 Ωz0 )+
1
+k22 (sin2 Ωz cos2 Ωz0 − 2 sin Ωz cos Ωz0 cos Ωz sin Ωz0 + cos2 Ωz sin2 Ωz0 )] 2

= [sin2 Ωz k12 sin2 Ωz0 + k22 cos2 Ωz0 + cos Ωz sin Ωz 2 cos Ωz0 sin Ωz0 (k12 − k22 )
 
| {z } | {z }
a b
1
2
k12 cos2 Ωz0 k22 sin2 Ωz0

+ cos Ωz + ] 2
| {z }
c

Then the coecients will be the following

3
a = k12 sin2 Ωz0 + k22 cos2 Ωz0
b = 2 cos Ωz0 sin Ωz0 (k12 − k22 )
c = k12 cos2 Ωz0 + k22 sin2 Ωz0

And these fulllls the relation 4ac − b2 = 2α and we obtain form the literature k1 = w0


this mean an initial condition and from the relation between the coecients k12 k22 = Ωα 2 . Then


replacing in the equation 14 we obtain the following.

 21
α2

w(z) = ± w0 cos Ω(z − z0 ) + sin Ω(z − z0 )
w0 Ω 2
 1
1 2
= ±w0 cos Ω(z − z0 ) + sin Ω(z − z0 ) (15)
zR Ω

Where zR = wα0 and z0 can be understood as the place where the beam starts. Now to recover the
homogeneous case, we just can

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