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(1)

Lattice points in some special three-dimensional

convex bodies with points of Gaussian

curvature zero at the boundary

Ekkehard Kr¨ atzel

Abstract. We investigate the number of lattice points in special three-dimensional convex bodies. They are called convex bodies of pseudo revolution, because we have in one special case a body of revolution and in another case even a super sphere. These bodies have lines at the boundary, where all points have Gaussian curvature zero. We consider the influence of these points to the lattice rest in the asymptotic representation of the number of lattice points.

Keywords: convex bodies, lattice points, points with Gaussian curvature zero Classification: 11P21, 11H06

1. Introduction and statement ofresult

Let

F

denotethedistance functionoftheconvexbodyPR

3

. That is

F

(

t 1 , t 2 , t 3

)=

n

(

|t 1 | κ

+

|t 2 | κ

)

k κ

+

|t 3 | k o 1

k ,

PR

3

=

{

(

t 1 , t 2 , t 3

)

R 3

:

F

(

t 1 , t 2 , t 3

)

1

}.

It is assumedthat

κ, k N

, 2

κ k

,

k >

3,

κ

adivisorof

k

. Then we have

abodyof revolutionfor

κ

=2andasuperspherefor

κ

=

k

. Therefore,wecall

PR

3

abody ofpseudorevolutioningeneral.

Weconsiderthepoints(

t 1 , t 2 , t 3

)attheboundaryand weareconnedto the

points

t 1 , t 2 , t 3

0withoutlossofgenerality. Weput

F

(

t 1 , t 2 , t 3

)=1

, t 3

=

f

(

t 1 , t 2

)

,

where

f

isgivenby

f

(

t 1 , t 2

)=

1

(

t κ 1

+

t κ 2

)

k κ

1

k .

The

Gaussian

curvaturein suchapointisdenedby

K

=

H

(

f

(

t 1 , t 2

))

(1+

f t 2 1

(

t 1 , t 2

)+

f t 2 2

(

t 1 , t 2

))

2

(2)

where

H

(

f

(

t 1 , t 2

))denotesthe

Hessian

H

(

f

(

t 1 , t 2

))=

f t 1 t 1

(

t 1 , t 2

)

f t 2 t 2

(

t 1 , t 2

)

f t 2 1 t 2

(

t 1 , t 2

)

.

Inthepresentcasewendbymeansof longbutsimplecalculations

K

= (

k

1)(

κ

1)(

t 1 t 2

)

κ− 2

(

t κ 1

+

t κ 2

)

2 k κ 2

t k− 3 2

(

t 2 3 k− 2

+(

t 2 1 κ− 2

+

t 2 2 κ− 2

)

2 k κ 2

)

2 .

From thisit isseenthat wehavethefollowingpointswith

Gaussian

curvature

K

=0attheboundary:

(1)Bodyofrevolution(

κ

=2): Thecurve

t 2 1

+

t 2 2

=1

, t 3

=0

andtheisolatedpoints(

t 1 , t 2 , t 3

)=(0

,

0

, ±

1).

(2)Supersphere(

κ

=

k

): Thecurves

t k 2

+

t k 3

=1

, t 1

=0;

t k 1

+

t k 3

=1

, t 2

=0;

t k 1

+

t k 2

=1

, t 3

=0

.

(3)Bodyofpseudorevolution(2

< κ < k

): Thecurves

t k 2

+

t k 3

=1

, t 1

=0;

t k 1

+

t k 3

=1

, t 2

=0;

t κ 1

+

t κ 2

=1

, t 3

=0

.

Theatpoints(

t 1 , t 2 , t 3

)=(0

,

0

, ±

1)areofexceptionalimportanceinallthree casesandthepoints(

t 1 , t 2 , t 3

)=(

±

1

,

0

,

0),(

t 1 , t 2 , t 3

)=(0

, ±

1

,

0)aremeaningful

aswellinthecases(2)and (3).

Theaimofthepaperistoinvestigatethenumberoflatticepointsinthedilated

bodyofpseudorevolution

x

PR

3

,thatis:

(1)

A k,κ

(

x

;PR

3

)=#

n

(

n 1 , n 2 , n 3

)

Z 3

:(

|n 1 | κ

+

|n 2 | κ

)

k κ

+

|n 3 | k x o

.

Especiallywestudytheinuence ofthepointswith

Gaussian

curvaturezeroto theasymptoticrepresentationof

A k,κ

(

x

;PR

3

).

In[3]adetaileddescriptionisgivenforthecaseofsuperspheres. Seealsothe

paper[5]. Therefore,weareherein therstplaceinterestedforthecase

κ < k

,

butwedonotexcludethecase

κ

=

k

.

It is not too hard to obtain the following asymptotic representation for

A k

(

x

;PR

3

)fromtheresultsofthepaper[7]:

A k,κ

(

x

;PR

3

)=vol(PR

3

)

x 3

+

H k,κ, 1

(

x

)+

H k,κ, 2

(

x

)+

O

x 5 3 3k 2

+

O

x 3 2

log

3 x

.

(3)

Thesecond main term

H k,κ, 1

(

x

)is acertainfunction of

x

comingfrom the at

points(

t 1 , t 2 , t 3

)=(0

,

0

, ±

1)andcan beestimatedby

H k,κ, 1

(

x

)

x 2 2 k .

Analogously,thethirdmainterm

H k,κ, 2

(

x

)isacertainfunctionof

x

comingfrom

theatpoints(

t 1 , t 2 , t 3

)=(

±

1

,

0

,

0)

,

(0

, ±

1

,

0)andcanbeestimatedby

H k,κ, 2

(

x

)

x 2 1 κ 1 k .

Thersterrortermresultsfromtheotherpointswith

Gaussian

curvaturezero andtheseconderrortermresultsfromthepointswith

Gaussian

curvaturenon- zero.

Inthispaperwewillgiveexplicitrepresentationsofthesecondandthirdmain

terms which automatically show that the above upper bounds are at the same

time lower bounds. Further we give an improved estimation of the rst error

term.

Letthegeneralized

Bessel

functions

J ν ( k )

(

x

)bedened by

(2)

J ν ( k )

(

x

)=

2

π

(

ν

+1

1 k

)

x

2

2 Z 1

0

1

t k ν− 1

k

cos

xt dt,

where isthegammafunction,

k, ν

arerealnumberswith

k

1,

ν > 1 k

. Further

let

(3)

ψ ( ν k )

(

x

)=2

π

ν

+1

1

k

X

n =1

x πn

2 J ν ( k )

(2

πnx

)

,

whichisabsolutelyconvergentfor

ν > 1 k

. Foraproofsee [3].

Theorem1. Let

κ, k N

,2

κ k

,

k >

3,

κ

adivisorof

k

. Then

(4)

A k,κ

(

x

;PR

3

)=vol(PR

3

)

x 3

+

H k,κ, 1

(

x

)+

H k,κ, 2

(

x

)+

k,κ

(

x

)

with

H k,κ, 1

(

x

)=

2

2

(

1 κ

)

κ

(

κ 2

)

ψ ( 3 k /k )

(

x

)=

O,

x 2 k 2

,

(5)

H k,κ, 2

(

x

)=8

x Z 1

0 t k

1

t k 1

k 1

ψ 2 ( κ )

(

xt

)

dt

=

O,

x 2 κ 1 1 k

,

(6)

k,κ

(

x

)

x 119 73 146k 165

(log

x

)

315 146

+

x 3 2

log

3 x.

(7)

(4)

2. Preparation of the problem

Wend,bysymmetry,

A k,κ

(

x

;PR

3

)=16(

S 1 , 2 , 3

+

S 1 , 3 , 2

+

S 3 , 1 , 2

)+

O

(

x

)

,

where

S i,j,k

aretriplesums

S i,j,k

=

X

n 1

X

n 2

X

n 3

1

withthesummationconditions

SC

(

S i,j,k

):0

n i n j n k ,

(

n κ 1

+

n κ 2

)

κ k

+

n k 3 x k , n i

=0

, n i

=

n j , n j

=

n k

getafactor 1

2

.

Webeginthesummationprocessin eachsumwith

n i

.

Forexample,summingin

S 1 , 2 , 3

over

n 1

,weobtain

"

x k n k 3

κ

k n κ 2

1

κ #

+ 1

2 for

x k n k 3

κ

k n κ 2

1

κ < n 2

and

n 2

otherwise. Ifweuse[

y

]+

1 2

=

y −ψ

(

y

),wegetatermwhichcanbewritten

asanintegral,andatermwiththe

ψ

-functionasaremainder. Hence

16

S 1 , 2 , 3

=

S 1 (1) , 2 , 3

+

2 , 3

(

x

)+

O

(

x

)

.

Here

S (1) 1 , 2 , 3

=16

X

n 2

X

n 3

Z

t 1

dt 1

withthesummation-integrationconditions

SIC X

n 2

X

n 3

Z

t 1

!

:0

t 1 n 2 n 3 ,

(

t κ 1

+

n κ 2

)

κ k

+

n k 3 x k ,

n 2

=

n 3

getsafactor

1

2

and

(8)

2 , 3

(

x

)=

16

X

( n 1 ,n 2 ) ∈D 2,3

ψ x k n k 3

κ

k n κ 2

1

κ !

,

(5)

where

D 2 , 3

denotesthedomain

D 2 , 3

=

(

t 2 , t 3

)

R 2

:0

x k t k 3

κ

k t κ 2 < t κ 2 t κ 3

.

Inthenextstepwesumover

n 2

in

S 1 (1) , 2 , 3

andobtainsimilarly

16

S 1 , 2 , 3

=

S 1 (2) , 2 , 3

+

P 2 , 3

(

x

)+

2 , 3

(

x

)+

O

(

x

)

with

S 1 (2) , 2 , 3

=16

X

n 3

Z

t 1

Z

t 2

dt 1 dt 2 ,

SIC X

n 3

Z

t 1

Z

t 2

!

:0

t 1 t 2 n 3 ,

(

t κ 1

+

t κ 2

)

k κ

+

n k 3 x k

and

P 2 , 3

(

x

)=

16

X

n 3

Z

t 1

ψ x k n k 3

κ

k t κ 1

1

κ ! dt 1

(9)

SIC X

n 3

Z

t 1

!

: 0

t 1 n 3 ,

x k n k 3

κ

k n κ 3 < t κ 1

1

2

x k n k 3

κ

k .

Inthelast stepwesumover

n 3

in

S 1 (2) , 2 , 3

and nallyweobtain

(10) 16

S 1 , 2 , 3

=

S 1 (3) , 2 , 3

+

H 2 , 3

(

x

)+

P 2 , 3

(

x

)+

2 , 3

(

x

)+

O

(

x

)

,

where

S 1 (3) , 2 , 3

=16

Z

t 1

Z

t 2

Z

t 3

dt 1 dt 2 dt 3 ,

(11)

IC Z

t 1

Z

t 2

Z

t 3

:0

t 1 t 2 t 3 ,

(

t κ 1

+

t κ 2

)

k κ

+

t k 3 x k ,

H 2 , 3

(

x

)=

16

Z

t 1

Z

t 2

ψ

x k

(

t κ 1

+

t κ 2

)

k κ

1

k

dt 1 dt 2 ,

(12)

IC Z

t 1

Z

t 2

=0

t k 1 t k 2 x k

(

t κ 1

+

t κ 2

)

k κ .

(6)

Inthesamewayweobtainfortheothertriplesums:

(13) 16

S 1 , 3 , 2

=

S 1 (3) , 3 , 2

+

H 3 , 2

(

x

)+

P 3 , 2

(

x

)+

3 , 2

(

x

)+

O

(

x

)

,

where

S (3) 1 , 3 , 2

=16

Z

t 1

Z

t 2

Z

t 3

dt 1 dt 2 dt 3 ,

(14)

IC Z

t 1

Z

t 2

Z

t 3

: 0

t 1 t 3 t 2 ,

(

t κ 1

+

t κ 2

)

k κ

+

t k 3 x k ,

H 3 , 2

(

x

)=

16

Z

t 1

Z

t 3

ψ x k t k 3

κ

k t κ 1

1

κ !

dt 1 dt 3 ,

(15)

IC Z

t 1

Z

t 3

: 0

t κ 1 t κ 3 x k t k 3

κ

k t κ 1 ,

P 3 , 2

(

x

)=

16

X

n 2

Z

t 1

ψ

x k

(

t κ 1

+

n κ 2

)

κ k

1

k dt 1 ,

(16)

SIC X

n 2

Z

t 1

!

: 0

t k 1 x k

(

t κ 1

+

n κ 2

)

k κ < n k 2 ,

3 , 2

(

x

)=

16

X

( n 3 ,n 2 ) ∈D 3,2

ψ x k n k 3

κ

k n κ 2

1

κ ! ,

(17)

D 3 , 2

=

(

t 3 , t 2

)

R 2

:0

x k t k 3

κ

k t κ 2 < t κ 3 t κ 2

.

Finally,weobtainfor

S 3 , 1 , 2

(18) 16

S 3 , 1 , 2

=

S 3 (3) , 1 , 2

+

H 1 , 2

(

x

)+

P 1 , 2

(

x

)+

1 , 2

(

x

)+

O

(

x

)

,

where

S (3) 3 , 1 , 2

=16

Z

t 1

Z

t 2

Z

t 3

dt 1 dt 2 dt 3 ,

(19)

IC Z

t 1

Z

t 2

Z

t 3

: 0

t 3 t 1 t 2 ,

(

t κ 1

+

t κ 2

)

k κ

+

t k 3 x k ,

(7)

H 1 , 2

(

x

)=

16

Z

t 3

Z

t 1

ψ x k t k 3

κ

k t κ 1

1

κ !

dt 1 dt 3 ,

(20)

IC Z

t 3

Z

t 1

: 0

t κ 3 t κ 1

1

2

x k t k 3

κ

k ,

P 1 , 2

(

x

)=

16

X

n 2

Z

t 3

ψ x k t k 3

κ

k n κ 2

1

κ ! dt 3 ,

(21)

SIC X

n 2

Z

t 3

!

: 1

2

x k t k 3

κ

k < n κ 2 x k t k 3

κ

k t κ 3 ,

1 , 2

(

x

)=

16

X

( n 1 ,n 2 ) ∈D 1,2

ψ

x k

(

n κ 1

+

n κ 2

)

k κ

1

k ,

(22)

D 1 , 2

=

n

(

t 1 , t 2

)

R 2

:0

x k

(

t κ 1

+

t κ 2

)

k κ < t k 1 t k 2

o .

3. Representationof the tripleintegrals

Itisclearthatitfollowsfrom (11),(14)and(19)

S 1 (3) , 2 , 3

+

S 1 (3) , 3 , 2

+

S 3 (3) , 1 , 2

=vol(PR

3

)

x 3 ,

whichisthemaintermin(4).

4. Representationand estimationofthe double integrals

Webeginwith

H 2 , 3

(

x

). Wewritetheintegrationconditionin(12)in theform 0

t 1 t 2 , t κ 1

+

t κ 2

x k t k 2

κ

k .

Wehave

x k t k 2

κ

k x κ

2

κ k .

Weintegrateonlyupto

x κ 1 2

. Theremainderisoforder

x

. Hence,bysubstituting

t 1 t 1 x

,

t 2 t 2 x

,weobtain

H 2 , 3

(

x

)=

16

x 2

Z

t 1

Z

t 2

ψ

x

1

(

t κ 1

+

t κ 2

)

κ k

1

k

dt 1 dt 2

+

O

(

x

)

, IC

Z

t 1

Z

t 2

: 0

t 1 t 2 , t κ 1

+

t κ 2

1

2

.

(8)

Putting

t κ 1

+

t κ 2

=

z κ

weget,bysymmetry,

H 2 , 3

(

x

)=

8

x 2

Z

z κ 1 2 z κ− 1 ψ

x

1

z k 1

k dz

Z z

0

(

z κ t κ 1

)

κ 1 1

dt 1

+

O

(

x

)

=

8

2

(

1 κ

)

x 2 κ

(

κ 2

)

Z

z κ 1 2

x

1

z k 1

k

dz

+

O

(

x

)

=

8

2

(

1 κ

)

x 2 κ

(

κ 2

)

Z 1

0 z k− 1

1

z k 2

k 1

ψ

(

xz

)

dz

+

O

(

x

)

,

whereagaintheintegralfrom 0upto(1

z −k/κ

)

1 /k

isoforder

1 x

. Bymeansof

the

Fourier

representationofthe

ψ

-function,

(23)

ψ

(

t

)=

1

π X n =1

1

n

sin(2

πnt

)

dt,

weobtain

H 2 , 3

(

x

)=

8

2

(

1 κ

)

x 2 πκ

(

κ 2

)

X n =1

1

n Z 1

0 z k− 1

1

z k 2

k 1

sin(2

πnxz

)

dz

+

O

(

x

)

= 8

2

(

1 κ

)

x 3 κ

(

2 κ

)

X n =1

Z 1

0

1

z k 2

k

cos(2

πnxz

)

dz

+

O

(

x

)

and,by(2)and(3),

H 2 , 3

(

x

)=4

π 2

(

κ 1

) (

κ 2

+1)

x 3 κ

(

κ 2

)

X n =1

(

πnx

)

3 2 J 3 ( k /k )

(2

πnx

)+

O

(

x

)

= 2

2

(

1 κ

)

κ

(

2 κ

)

ψ 3 ( k /k )

(

x

)+

O

(

x

)

.

Hence

H 2 , 3

(

x

)=

H k,κ, 1

(

x

)+

O

(

x

)

and the representation (5) is obtained. The asymptotic representation of the

generalized

Bessel

functionsisgivenin Lemma3.11of[3]. Weobtain

J 3 ( k /k )

(2

πnx

)=

nx

( k

2

πnx 2

k

cos

2

πnx π

2

2

k

+1

+

O

1

nx )

.

(9)

Hence,itfollowswithapositiveconstant

c H k,κ, 1

(

x

)=

cx 2 2 k

X n =1

n 1 k 2

sin

2

πnx π k

+

O

(

x

)

.

Thus,theestimationsin(5)areclear.

Inorderto obtaintheterm

H k,κ, 2

(

x

)weadd

H 3 , 2

(

X

)and

H 1 , 2

(

x

). Thenwe

getfrom(15)and(20)

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=

16

x 2 Z

t 1

Z

t 3

ψ x

1

t k 3

κ

k t κ 1

1

κ !

dt 1 dt 3 ,

IC Z

t 1

Z

t 3

: 0

t κ 1

1

2

1

t k 3

κ

k ,

0

t κ 3

1

t k 3

κ

k t κ 1 .

Bymeansofthesubstitution

t κ 1

=(1

t k 3

)

κ/k z κ

weobtain

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=16

x 2

Z

z

Z

t 3

z κ− 1

1

t k 3

κ

k z κ 1

κ 1

ψ

(

xz

)

dt 3 dz, IC

Z

z

Z

t 3

: 1

2

1

t k 3

κ

k z k , t k 3

+

z k

1

,

0

t 3 z.

Wemayextendthedomainofintegrationsuchthatthenewintegrationconditions

aregivenby

IC Z

z

Z

t 3

:

t k 3

+

z k

1

,

0

t k 3

1

2

.

The integral overthe new domain is of order

1

x

which can be seen by partial

integratingwithrespectto

z

. Nowwesubstitute1

t k 3

=

t k

. Then

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=

=

16

x 2 Z 1

2 −1/k dt Z t

0 t k− 1

1

t k 1

k 1

z κ− 1

(

t κ z κ

)

κ 1 1 ψ

(

xz

)

dz

+

O

(

x

)

.

Thesubstitution

z zt

gives

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=

=

16

x 2 Z 1

2 −1/k t k

1

t k 1

k 1

dt Z 1

0 z κ− 1

( 1

z κ

)

1 κ 1 ψ

(

xtz

)

dz

+

O

(

x

)

.

(10)

Wetaketheintegralwithrespectto

t

from 0upto 1,sincethenewpartof the

integralisof order

1

x

. Asin caseof

H 2 , 3

(

x

) weusethe

Fourier

representation (23)ofthe

ψ

-functionandweobtainanalogously

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=

=

16

π

1

k

+1

x 2 Z 1

0 t k +1

1

t k 1

k 1 X n =1

1

n J 2 ( κ )

(2

πnxt

)

dt

+

O

(

x

)

=8

x Z 1

0 t k

1

t k 1

k 1

ψ 2 ( κ )

(

xt

)

dt

+

O

(

x

)

.

Hence

H 3 , 2

(

x

)+

H 1 , 2

(

x

)=

H k,κ, 2

(

x

)+

O

(

x

)

and the representation (6) is obtained. For the asymptotic representation we

use(24). Clearly,theintegralfrom0upto

1

2

isoforder

1

x

. Therefore,weusethe

asymptoticrepresentationof thegeneralized

Bessel

function from Lemma 3.11 in[3]for

t 1 2

. Then

J 2 ( κ )

(2

πnxt

)=

1

π

κ

2

πnxt 1

κ

cos

2

πnxt π

2

1

κ

+1

+

O

1

nx

.

Hence,itfollowswithapositiveconstant

a H k,κ, 2

(

x

)=

=

ax 2 κ 1 X n =1

n 1 1 κ Z 1

1 2

t k +1 κ 1

1

t k 1

k 1

sin

2

πnxt π

2

κ

dt

+

O

(

x

)

.

The remaining integral has a singularity at

t

= 1. We obtain the asymptotic

representationoftheintegralveryeasybymeansofChapter3,Section11from[1].

We use a special case of formula (11.6) on page 24: Let

φ

(

t

) be continuously dierentiablein

α t β

. Let

φ

(

α

)=0. Then,if 0

< µ <

1,

Z β

α e ixt

(

β t

)

µ− 1 φ

(

t

)

dt

= (

µ

)

x µ e ixβ− 1 2 µπi φ

(

β

)+

O

1

x

.

Thecondition

φ

(

α

)=0isnotnecessary. Incase of

φ

(

α

)

6

=0thepoint

α

yields

anerrortermoforder1

/x

. Thus, withaconstant

b 6

=0,weget

H k,κ, 2

(

x

)=

bx 2 κ 1 k 1

X n =1

n 1 1 κ 1 k

sin

2

πnx π

2

1

κ

1

k

+

O

(

x

)

.

Hence,theestimations(6)followimmediately.

(11)

5. Estimationsof sumsand integrals

Theaimofthischapteristoestimatethesumsandintegrals(9),(16)and(21).

Lemma1. Assumethatforall

z

with

1 2 z

1andforall

τ

with

x 2 k τ k x k X

xk 2 <n k ≤τ k

ψ

x k n k 1

k z

k, 2 , 3

(

x

)

.

Then

(25)

P 2 , 3

(

x

)

x 1 1

k, 2 , 3

(

x

)

1 1

κ .

Proof:

Itiseasilyseenthatin(9)thecondition

t 1 n 3

issuperuousandthat

x k n k 3

κ

k n κ 3 >

0

⇐⇒ n k 3 > x k

2

.

Further,consider

16

X Z

ψ x k n k 3

κ

k t κ 1

1

κ ! dt 1 ,

SIC XZ

: 0

t κ 1

x k n k 3

κ

k n κ 3 , x k

2

k/κ

+1

< n k 3 x k

2

.

It is seenat once that this termis of order

x

. Nowwebring (9) and thisterm

togetherandobtain

P 2 , 3

(

x

)=

16

X Z

ψ x k n k 3 κ

k t κ 1 1

κ ! dt 1 ,

SIC XZ

: 0

t κ 1

1

2

x k n k 3

κ

k , x k

2

k/κ

+1

< n k 3 x k

2

.

Nowweput

t 1

=(

x k n k 3

)

1 /k t

. Then

P 2 ,k

(

x

)=

=

16

Z 2 −1/κ

0

X

xk

2 k/κ +1 <n k 3 xk 2

x k n k 3

1

k ψ

x k n k 3

1

k

( 1

t κ

)

1 κ

dt

+

O

(

x

)

=

16(

I 1

+

I 2

)+

O

(

x

)

.

(12)

Applyingpartialsummationweobtainbymeansoftheconditionofthelemma

I 1

=

Z y

0

X

xk

2 k/κ +1 <n k 3 xk 2

x k n k 3

1

k ψ x k n k 3

1

k

( 1

t κ

)

1 κ

dt

xy

k, 2 , 3

(

x

)

.

In

I 2

, where the integral is taken from

y

up to 2

1

, we use the

Fourier

expansionofthe

ψ

-function(23)and obtain

I 2

=

1

π

X

xk

2 k/κ +1 <n k 3 xk 2

x k n k 3

1

k X m =1

1

m

Z 2 −1/κ

y t 1 −κ

(1

t κ

)

1 1 κ

× t κ− 1

(1

t κ

)

1 κ 1

sin

2

πm

x k n k 3

1

k

(1

t κ

)

1 κ

dt

= 1

2

π 2 X m =1

1

m 2

X

xk

2 k/κ +1 <n k 3 xk 2

 

t 1 −κ

(1

t κ

)

1 κ 1

cos

2

πm

x k n k 3

1 1

k

(1

t κ

)

κ 1

2 −1/k y

Z 2 −1/κ

y

d dt

t 1 −κ

(1

t κ

)

1 1 κ

cos

2

πm

x k n k 3

1 1

k

(1

t κ

)

κ 1

dt )

.

We estimate the sum over

n 3

with

van der Corput’s

simplest theorem (see Theorem2.1in [3]). Thenwegetexactlyin thesamewayasonpage183of[3]

I 2 x 1 2 y 1 −κ .

Nowweput

y

=

x 1 2

k, 2 , 3

(

x

)

1

κ .

Thentheestimationsof

I 1

and

I 2

areequalandweobtain(25).

Lemma2. Assumethatforall

z

with1

z

2andforall

u

with

1+ x k z k < u k

x k X

1+zk xk <n k ≤u k

ψ

x k n k z k 1

k

k, 3 , 2

(

x

)

.

(13)

Then

(26)

P 3 , 2

(

x

)

x 1 1

k, 3 , 2

(

x

)

1 1

κ .

Proof:

Theproofisquitethesameas theprooftoLemma1suchthat weomit

it.

Lemma3. Assumethat

X

2 <n κ ≤t κ

ψ

(

t κ n κ

)

1 κ

κ, 1 , 2

(

x

)

.

Then

(27)

P 1 , 2

(

x

)

x 1 2k 1

κ, 1 , 2

(

x

)

1 1

k . Proof:

Consider

16

Z x

0

X

( x k −t k 3 ) κ/k −t κ 3 <n κ 2 ( x k −t k 3 ) κ/k

ψ x k t k 3

κ

k n κ 2

1

κ ! dt 3 .

It is easily seen that this term is of order

x

. Now we bring (21)and this term

togetherandobtain

P 1 , 2

(

x

)=

=

16

Z x

0

X

1 2 ( x k −t k 3 ) κ/k <n κ 2 ( x k −t k 3 ) κ/k

ψ x k t k 3

κ

k n κ 2

1

κ !

dt 3

+

O

(

x

)

.

Putting

x k t k 3

=

t k

then

P 1 , 2

(

x

)=

16

Z x

0 t k− 1

x k t k 1

k 1 X

2 <n κ 2 ≤t κ

ψ

(

t κ n κ 2

)

κ 1

dt

+

O

(

x

)

.

Here wehavethe samesituation asin Lemma 4.8 of[3]. Using this result (27)

followsimmediately.

Estimations of the error terms

k, 2 , 3

(

x

),

k, 3 , 2

(

x

),

κ, 1 , 2

(

x

):

G. Kuba

[8]

haspointedoutthat

M.N. Huxley’s

[2]methodisapplicabletotheabovesums.

Assumethat

a, b, c, d

arexedpositiverealnumbers. Thenheproved

X

( X 2b ) 1/k −d<n≤ ( X−ack b ) 1/k −d

ψ

X b

(

n

+

d

)

k a

! 1

k

X

ab 46

73k

log

X 2

ab k 1

315 146

.

参照

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