Determinants and Their Applications in Mathematical Physics

(Chris Devlin) #1

164 4. Particular Determinants


=



r=0

(p)re

(r+p)t

r!

,

where


(p)r=p(p+ 1)(p+2)···(p+r−1) (4.12.52)

and denote the corresponding determinant byE


(p)
n :

E

(p)
n =



ψ

(p)
m



n

, 0 ≤m≤ 2 n− 2 ,

where


ψ

(p)
m

=D

m
f

=



r=0

(p)r(r+p)
m
e
(r+p)t

r!

. (4.12.53)

Theorem 4.59.


E

(p)
n =

e
n(2p+n−1)t/ 2

(1−e
t
)
n(p+n−1)

n− 1

r=1

r!(p)r.

Proof. Put


gr=

αre

t

(1−e
t
)
2

,αrconstant,

and note that, from (4.12.48),


g 1 =D

2
(logf)

=

pe

t

(1−et)^2

,

so thatα 1 =pand


loggr= logαr+t−2 log(1−e

t
),

D

2
(loggr)=

2 e

t

(1−e
t
)
2

. (4.12.54)

Substituting these functions into the differential–difference equation, it is


found that


αn=nα 1 +2

n− 1

r=1

(n−r)

=n(p+n−1). (4.12.55)

Hence,


gn=

n(p+n−1)e
t

(1−e
t
)
2

,

gn−r=

(n−r)(p+n−r−1)e

t

(1−e
t
)
2

. (4.12.56)
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