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Diploma thesis - Fachbereich Physik

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3.2. GROUND-STATE ENERGY WITHOUT EXTERNAL CURRENT 41<br />

For the general case k ≥ 3, it is helpful to rewrite (3.10) in the form<br />

∞∑<br />

φ k (x) = c (k)<br />

m xm , with c (k)<br />

m ≡ 0 for m > k + 2 , (3.14)<br />

m=1<br />

as this allows the application of the Cauchy product rule to the product of the derivatives<br />

φ ′ k−l (x) and φ′ l (x) in (3.9). The recursively determinable solution for the φ k(x) and the<br />

energy corrections ǫ k is then obtained as<br />

c (k)<br />

m<br />

ǫ k<br />

=<br />

(m + 2)(m + 1)¯h<br />

2mMω<br />

= −¯h2<br />

M c(k) 2 − ¯h2<br />

2M<br />

c (k) ¯h<br />

m+2 +<br />

2mMω<br />

∑k−1<br />

l=1<br />

∑ ∑<br />

k−1 m+1<br />

l=1<br />

n=1<br />

with c (k)<br />

m<br />

n(m + 2 − n) c (l)<br />

n c (k−l)<br />

m+2−n ,<br />

≡ 0 for m > k + 2 , (3.15)<br />

c (l)<br />

1 c(k−l) 1 . (3.16)<br />

Applying this result leads to the expansion coefficients and the energy correction in the third<br />

order of the coupling constant:<br />

c (3)<br />

1 = − 5A3¯h<br />

M 4 ω 7 + 6AB¯h<br />

M 3 ω 5 ,<br />

And for the fourth order one obtains<br />

c(3) 2 = 0 , c (3)<br />

3 = − 13A3<br />

12M 3 ω 6 + 3AB<br />

2M 2 ω 4 ,<br />

c (3)<br />

4 = 0 , c (3)<br />

5 = − A3<br />

10M 2¯hω 5 +<br />

c (4)<br />

1 = 0 , c (4)<br />

2 = 305A4¯h<br />

32M 5 ω − 123A2 B¯h<br />

+ 21B2¯h<br />

9 8M 4 ω 7 8M 3 ω , 5<br />

c (4)<br />

4 = 99A4<br />

64M 4 ω 8 − 47A2 B<br />

16Mω 6 + 11B2<br />

16M 2 ω 4 ,<br />

c (4)<br />

6 =<br />

5A 4<br />

48M 3¯hω 7 −<br />

AB<br />

5M¯hω 3 , (3.17)<br />

and ǫ 3 = 0 . (3.18)<br />

c(4) 3 = 0 ,<br />

c(4) 5 = 0 ,<br />

A2 B<br />

4M 2¯hω 5 + B 2<br />

12M¯hω 3 , (3.19)<br />

and ǫ 4 = − 465A4¯h 3<br />

32M 6 ω 9 + 171A2 B¯h 3<br />

8M 5 ω 7 − 21B2¯h 3<br />

8M 4 ω 5 . (3.20)<br />

Comparing (3.13), (3.18), and (3.20) with (2.188), one sees that the result obtained by<br />

Bender-Wu recursion is indeed identical to the one obtained by explicitly evaluating Feynman<br />

diagrams. Since one wants to drive the expansion to higher orders, it is important to optimize<br />

the recursion formula with regard to its evaluation by a computer. To this end, it is helpful to<br />

introduce natural units, in which one has ¯h = 1, M = 1. Furthermore, since calculations on a<br />

computer can be performed more effectively when dealing with mere rational numbers, which<br />

are not afflicted with parameters like A, B, or ω, it is desirable to expand the coefficients<br />

and the energy corrections ǫ k in products of powers of these parameters. Dimensional<br />

considerations lead to the following approaches for the coefficients c (k)<br />

c (k)<br />

m<br />

m :<br />

⌊k/2⌋<br />

c (k)<br />

m = ∑ A k−2λ B λ<br />

c(k)<br />

ω5k/2−m/2−2λ m,λ ,<br />

λ=0<br />

with c(k)<br />

m,λ<br />

≡ 0 for m > k + 2 , (3.21)

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