Abstract
Abstract
The heat invariants or the Minakshisundaram-Pleijel heat coefficients
a
k
n
=
a
k
n
(M) (k ≥ 0) describe the asymptotic expansion of the heat kernel HM on any N = 4 n-dimensional (n ≥ 1) compact Riemannian manifold M; associated with the coefficients
a
k
n
is the Minakshisundaram-Pleijel zeta function ζM = ζM(s) (s
∈ C). In this paper, we introduce and study a new class of heat coefficients, namely, the Maclaurin heat coefficients
b
2
m
n
=
b
2
m
n
(
t
)
(t > 0 , m 0) (i.e., the coefficients appearing in the Maclaurin expansion of the heat kernel HM(t, θ)) in terms of the classical and generalised Minakshisundaram-Pleijel coefficients
a
k
n
and
a
k
,
j
n
,
m
=
a
k
,
j
n
,
m
(M) (0 ⩽ j ⩽ m) respectively, when M = P
n
(H) (n ≥ 1), a quaternionic projective space. Remarkable asymptotic expansions for the Maclaurin spectral functions
b
2
m
n
(
t
)
are established. We also introduce and construct new zeta functions
Z
p
n
(
H
)
m
(m ≥ 0) associated with these Maclaurin heat coefficients (generalised Minakshisundaram-Pleijel zeta functions), and it is interesting to see that these generalised zeta functions can be explicitly understood in terms of the classical (Minakshisundaram-Pleijel) zeta functions.
Subject
General Physics and Astronomy
Cited by
2 articles.
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