Determinants and Their Applications in Mathematical Physics

(Chris Devlin) #1

258 6. Applications of Determinants in Mathematical Physics


Hence, referring to the first equation in (4.5.10),


[
B

(n+1)
1 ,n+1

] 2

y


2 n
=(2n+1)BnBn+1,

BnBn+1(y 2 n− 1 −y 2 n+1)=BnB

(n+1)
11
−Bn+1B

(n)
11

=B

(n+1)
n+1,n+1

B

(n+1)
11
−Bn+1B

(n+1)
1 ,n+1;1,n+1

=

[

B

(n+1)
1 ,n+1

] 2

Hence,


y


2 n(y^2 n−^1 −y^2 n+1)=2n+1,

which proves the theorem whennis even. 


6.6 The Matsukidaira–Satsuma Equations


6.6.1 A System With One Continuous and One Discrete


Variable


LetA
(n)
(r) denote the Turanian–Wronskian of orderndefined as follows:


A

(n)
(r)=


∣f
r+i+j− 2



n

, (6.6.1)

wherefs=fs(x) andf



s=fs+1. Then,

A

(n)
11 (r)=A

(n−1)
(r+2),

A

(n)
1 n
(r)=A

(n−1)
(r+1).

Let


τr=A

(n)
(r). (6.6.2)

Theorem 6.7.




τr+1 τr

τr τr− 1









τ

′′
r τ


r

τ


r τr





=





τ


r+1 τr+1

τ


r τr









τ


r τr

τ


r− 1 τr−^1





for all values ofnand all differentiable functionsfs(x).


Proof. Each of the functions


τr± 1 ,τr+2,τ


r,τ

′′
r,τ


r± 1

can be expressed as a cofactor ofA


(n+1)
with various parameters:

τr=A

(n+1)
n+1,n+1
(r),

τr+1=(−1)

n
A

(n+1)
1 ,n+1
(r)

=(−1)

n
A

(n+1)
n+1, 1 (r)

τr+2=A

(n+1)
11
(r).
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