SOME REMARKS FOR THE SPECTRUM OF THE p-LAPLACIAN ON SASAKIAN MANIFOLDS
TAE Ho KANG AND JIN SUK PAK
1. Introduction
Let (M, g) be a compact manifold of dimension n with metric tensor g. Let t:i. P = d6 + 6d be the Laplace-Beltrami operator acting on the space of smooth p-forms. Then we have the spectrum of t:i. P for each
O~p~n
SpecP(M,g) = {O ::;
Al,p ::; A2,p'"i +oo},
where each eigenvalue is repeated according to its multiplicity. Many authors have studied the relationship between the spectrum of M and the geometry of M. And also, Z.Olszak[ 1 ], J.S.Pak, J.C.Jeong and W.T.Kim[2], S.Yamaguchi and G.Chiiman[ 7] and others studied the spectrum of Sasakian manifolds. In this paper we shall prove
jTHEOREM A. Let M = (M,fj>,e,TJ,g) and M ' = (M',q/,e',TJI,g') be compact c-Einstem Sasakian manifolds with SpeeP M = SpeeP M ' for an arbitrazy fixed p ~ 1 (which implies dimM=dimM'=n). If (n,p) rt {(15, 1),(15,2),(15, 13),(15, 14)}, then M is of constant fj>- sectional curvature c if and only if M ' is of constant fj>'-sectional cur- vature c' =c.
Received March 25, 1994.
1991 AMS Subject Classifications: 53C12j 53A50.
Key words: Sasakian manifold, spectrum, contact Bochner curvature tensor
This research was partially supported by TGRC-KOSEF and the Basic Science
Research Institute Program, Ministry of Education, 1994, Project No. BSRI-94-
1404.
342 Tae Ho Kang and Jin Suk Pak
THEOREM B. Let M = (M,4>,e,Tf,g) and M' = (M',4>',e,Tf,g) be compact Sasakian manifolds witb SpeeP(M)
'7CSpeeP(M')(whicb impliesdimM=c#mM' =n). If n is. given, tbere exists an integer p(O ~ p ~ n) such" tbat M is of conStant </J- sectional curvature c if and only
if M' is of constant 4>'- sectional curvature c = c'.
2. Preliminaries
By R = (Ri~A:)' P = (RjA:) = (R,lA:) and
( j= (gjA: RjA:) we de- note the Riemannian curvature tensor, the Ricci tensor and the scalar curvature, respectively, and 9 = (gij) is a Riemannian metric ten- sor on M, (gij ) = (gij)
- I .For the tensor field T on M we denote
ITI the norm of T with respect to g. Then for each p ~ 2m +
l( =dimM) the Minakshisundaram-Pleijel-Gaifney asymptotic expan-
sion iorSpeeP-(M~-gYisgi~enby - - - . --.
00
~ 2m+l
N
L.J exp( -Aa,pt) = (47rt)-
2[ao,p + tal,p + ... + t aN,p]
a=O
+ o(t N - m + i ) as t 1 0,
where ao,p, al,p, a2,p, ... are numbers' which can be expressed by ( see [ 3])
a2,p
= 2.. r [{s(2rn+ 1) _60(2m - 1) +180(2m - 3)}
0-2360JM P p-l p-2
(2.3) + {-2emp+~) +.180e:_-/) -720e:_-23) } IpI
2-t. { ~e:p~.':);:~~C:-e--/) t~~~.e;~~2~)} 1!l12J ~¥,
where dM denotes the volume element of M, and (:) = 0 fork ~ 0 or _
r < o.
Let M = (M,4>,e,7],9) be a compact Sasakian manifold (cf. [ 8 D. This means that M is a (2m + I)-dimensional compact differ- entiable manifold with a normal contact metric structure (4),e,7],9), where 4> = (4)f),e = (e i ),7] = (7]i) are tensor fields of type (1,1), (1,0), (0,1) respectively.
Now we introduce the tensor fields H = (Hkjih) and Q = (Qij) on
M defined by
c+3 c - l
H kjih = Rkjih - -4-(9kh9ji - 9ki9jh) - -4-(4)kh4>ji - 4>ki4>jh - 24>kj4>ih - 9kh7]j7]i + 9ki7]j7]h - gji7]k7]h + gjh7]k7]i),
Qij = Rij - agij - b7]i7]j, where c =
q -m(3m + 1),a = ..!!- - 1 and
m(m + 1) 2m
Then we have
b = 2m+ 1 - - . q
2m (2.4)
IHI2 = IRI 2 _ 2 q2 + 4(3m + 1) q _ 4m(2m + 1)(3m + 1),
m( m + 1) m + 1 m + 1
(2.5) IQI 2 = Ipl2 - 2~ q2 + 2q - 2m(2m + 1).
A Sasakian manifold M = (M, 4>,~, 7],g) is called a space of constant 4>-sectional C'UM1ature c(resp.c-Einstein) if H(resp.Q) vanishes identi- cally. It is well known that a space of constant 4>-sectional curvature is c-Einstein. For any c-Einstein manifold of dimension ~ 5, the scalar curvature is necessarily constant. A 3-dimensional c-Einstein manifold means that the scalar curvature is constant. On any 3-dimensional Sasakian manifold the tensor field H vanishes, but in this case the scalar curvature may be non-constant. Therefore, in dimension 3, it is of constant 4>-sectionaJ. curvature if and only if q is constant.
We also consider the so-called contact Bochner curvature tensor field B = (Bkjih) defined on M by (cf. [1 ,7])
B kjih = Rkjih - 2m 1 + 4 (gkhRji - gkiRjh - gjhRki + 9jiRkh - 4>khRjl4>~ + 4>ki R jl4>i - rPjiRkl4>i + rPjhRkl4>~
+ 24>kjRilrPi + 24>ihRklrP~ - Rkh7]j7]i + Rki'T}j'T}h
344 Tae Ho Kang and Jin Suk Pak
(2.8) (2.7)
. . ) r-4 ( )
- Rji''lk''lh + Rjh"lk"li + 2m + 4 9kh9ji - 9ki9jh
+ 2m r+2m + 4( <Pkh<Pji - <Pki<Pjh - 2<Pkj<Pih)
- 2m r + 4(9kh T/j"li - 9ki"ljT/h + 9ji"lk"lh - 9jhT/kT/i),
0'+ 2m .
where r = 2m + 2· Then we also obtaIn (2.6)
I BI 2 _ IRI 2 _ _ 8_
1 1 2 2 2
- m+2 P + (m+ l)(m + 2)0-
4(3m2 + 3m - 2) 2 8(13m + 14)
+ (m+1)(m+2) 0'-24m +36m-56+ (m+1)(m+2)"
Moreover, it may be easily seen that H = 0 if and only if B = 0 and Q = o. From (2.4)"'(2.6), we have
IRI 2 = IBI 2 + _8_ IQI2 + 2 0'2 _ 4(3m + 1) 0- m + 2 m( m + 1) (m + 1) 24 2 36 56 8(4m 2 - 2m - 7)
+ m - m+ + .
m+1
For p <I. {I, 2, 3, 2m, 2m + I}, substituting (2.7) into (2.3) yields a2,p = a lM f [4PI IBI 2 + ~2P21Q12 m+ . + m m+ (4 1)P30- 2
16 . 16m
+ - - 1 P 4 0' + - - 1Ps] dM,
m+ m+' .
where
PI := PI(m,p) = 8m4 - (60p + 8)m3 + (210p2 -120p - 2)m2 + ( -180p3 + 225p2 - 75p + 2)m
+ 45p4 - 90p3 + 60p2 - 15p,
.,', P 2 : - :P 2 (m;p),:,: '-4m
S+(180p-'f'28)fu
4 -(450p2 -300}J~23)m3 + (360p3 - 465p2 + 15p - 7)m2
- (90p4 - 180p3 + 45p2 -15p - 6)m - 30p2 + 30p,
P3 := P
3(m,p) = 20m
6-(120p + 4)ms + (240p2 - 9)m
4- (180p3 + 30p2 - 120p + 1l)m 3
+ (45p 4 + 90p3 - 180p2 - 15p + 1)m 2 - (45p 4 - 90p3 + 15p 2 - 3)m - 15p 2 + 15p,
._ (2;n_-2
3 )
Q . - ,
360p(p - 1)(2m - p + 1)(2m - p)
P 4 and Ps are also constant depending only on m and p.
For pE {I,2,3,2m,2m + I}, the formula (2.3) is of the form
j(2.9)
f[ 2 8 2 4 2
a2,p = f3 lM 4Q11BI + m + 2 Q21QI + m(m + 1) Q3(7
16 16m
+ - - 1 Q4(7 + - - 1 Qs] dM,
m+ m+
where for i = 1,2,3,4,5 (i) if p = I,m ~ 2, then
1
f3 = 360'
P i (m,l)
Qi = Qi(m) = 2m(2m -1)(2m - 2)' while for (m,p) = (1,1), Q1 = -6, Q2 = 1:5, Q3 = 9,
(ii) if p = 2,m ~ 2, then
while for (m,p) = (1,2), (iii) if p = 3, m ~ 2, then
1
f3=2x360' Q Q
Pi(m,2)
i = i(m) = (2m -1)(2m _ 2)' Q1 = -12,Q2 = 2,Q3 165 = 18,
1
f3 = 6 x 360' while for (m,p) = (1,3),
Q . = Q.(m) = Pi(m,3)
I I