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On some sums involving the integral part function
Kui Liu, Jie Wu, Zhishan Yang
To cite this version:
Kui Liu, Jie Wu, Zhishan Yang. On some sums involving the integral part function. 2021. �hal- 03331946�
KUI LIU, JIE WU & ZHISHAN YANG
Abstract. Denote by τk(n), ω(n) and µ2(n) the number of representations of n as product ofk natural numbers, the number of distinct prime factors ofn and the char- acteristic function of the square-free integers, respectively. Let [t] be the integral part of real numbert. Forf =ω,2ω, µ2, τk, we prove that
X
n6x
fhx n
i
=xX
d>1
f(d)
d(d+ 1) +Oε(xθf+ε)
forx→ ∞, whereθω= 11053,θ2ω = 199, θµ2 = 25,θτk = 10k−15k−1 andε >0 is an arbitrarily small positive number. These improve the corresponding results of Bordell`es.
1. Introduction
Denote by [t] the integral part of the real number t. Recently Bordell`es, Dai, Heyman, Pan and Shparlinski [3] established an asymptotic formula of
Sf(x) := X
n6x
fhx n
i
under some simple assumptions of f. Subsequently, Wu [9] and Zhai [10] improved their results independently. In particular, if f(n)ε nε for any ε > 0 and all n > 1, then [9, Theorem 1.2(i)] or [10, Theorem 1] yields the following asymptotic formula
(1.1) Sf(x) = xX
d>1
f(d)
d(d+ 1) +Oε(x1/2+ε)
as x → ∞. Ma and Wu [7] observed that if f is factorizable in certain sense, then it is possible to break the 12-barrier for the error term of (1.1). In particular, for the von Mangoldt function Λ(n), they proved, with the help of the Vaughan identity and the technique of one-dimensional exponential sum, that
(1.2) SΛ(x) =xX
d>1
Λ(d)
d(d+ 1) +Oε(x35/71+ε) (x→ ∞).
Using similar idea to the classical divisor function τ(n), Ma and Sun [6] showed that
(1.3) Sτ(x) = xX
d>1
τ(d)
d(d+ 1) +Oε(x11/23+ε) (x→ ∞).
Subsequently, with the help of a result of Baker on 2-dimensional exponential sums [1, Theorem 6], Bordell`es [2] sharpened the exponents in (1.2)-(1.3) and also studied some new examples. Denote byτk(n),ω(n) andµ2(n) the number of representations ofn as product
Date: September 2, 2021.
2010Mathematics Subject Classification. 05A17, 11N37, 11P82.
Key words and phrases. partition function, asymptotic formula, polynomial, saddle-point method.
1
of k natural numbers, the number of distinct prime factors of n and the characteristic function of the square-free integers, respectively. His results can be stated as follows:
(1.4) X
n6x
fhx n
i
=xX
d>1
f(d)
d(d+ 1) +Oε(xϑf+ε), with
f Λ ω 2ω µ2 τ τ3 τk (k>4)
ϑf 97 203
455 914
97 202
1919 4268
19 40
283 574
4k3−k−2 8k3−2k−2
Very recently, Liu, Wu and Yang [5] succeeded to improve Bordell`es’ exponent 20397 to 199 for Λ. Their principal tool is a new estimate on 3-dimensional exponential sums.
The aim of this paper is to propose better exponents than all others cases of the above table.
Theorem 1. Under the previous notation, the asymptotic formula (1.4) holds with f ω 2ω µ2 τk (k>2)
ϑf 11053 199 25 10k−15k−1
The key point of proving Theorem 1 is to establish good bounds for Sfδ(x, D) := X
D<d62D
f(d)ψ x d+δ
.
where ψ(t) := {t} − 12 and {t} means the fractional part of real number t. Let P be the set of all primes and define
(1.5) 1P(n) :=
(1 if n ∈P,
0 otherwise, 1(n)≡1, µ(n) :=˜
(µ(d) if n =d2, 0 otherwise.
Then we have the following relations:
ω=1P∗1, τk=τk−1∗1, 2ω =µ2∗τ, µ2 = ˜µ∗1.
Thus when f = ω, τk,2ω, µ2, we can use these relations to decompose Sfδ(x, D) into bilinear forms
Sωδ(x, D) := X
D<d`62D
1P(d)ψ x d`+δ
, (1.6)
Sτδk(x, D) := X
D<d`62D
τk−1(d)ψ x d`+δ
, (1.7)
S2δω(x, D) := X
D<d2`62D
µ(d)τ(`)ψ x d2`+δ
, (1.8)
Sµδ2(x, D) := X
D<d2`62D
µ(d)ψ x d2`+δ
. (1.9)
In the third section, we shall use the Fourier analyse and the technique of multiple expo- nential sums to establish our bounds for these bilinear forms.
2. Preliminary lemmas
In this section, we shall cite three lemmas, which will be needed in the next section.
The first one is [5, Proposition 3.1].
Lemma 2.1. Let α >0, β >0, γ >0 and δ ∈R be some constants. For X >0, H >1, M >1 and N >1, define
(2.1) Sδ=Sδ(H, M, N) := X
h∼H
X
m∼M
X
n∼N
ah,mbne
XMβNγ Hα
hα mβnγ+δ
,
wheree(t) := e2πit, the ah,m andbnare complex numbers such that|ah,m|61and|bn|61, and m∼M means that M < m62M. For any ε >0 we have
Sδ (XκH2+κM2+κN1+κ+λ)1/(2+2κ)+HM N1/2 + (HM)1/2N +X−1/2HM N Xε uniformly forM >1,N >1, H 6Mβ−1Nγ and06δ61/ε, where(κ, λ)is an exponent pair and the implied constant depends on (α, β, γ, ε) only.
The second one is the Vaughan identity [8, formula (3)].
Lemma 2.2. There are six real arithmetic functionsαk(n)verifyingαk(n)τ(n) log(2n) for (n>1, 16k 66) such that for D>1 and any arithmetical function g, we have
(2.2) X
D<d62D
Λ(d)g(d) = S1+S2+S3+S4, where τ(n) is the classic divisor function and
S1 := X
m6D1/3
α1(m) X
D<`mn62D
g(mn),
S2 := X
m6D1/3
α2(m) X
D<`mn62D
g(mn) logn,
S3 := X X
D1/3<m,n6D2/3 D<`mn62D
α3(m)α4(n)g(mn),
S4 := X X
D1/3<m,n6D2/3 D<`mn62D
α5(m)α6(n)g(mn).
The same result also holds for the M¨obius function µ.
The third one is due to Vaaler (see [4, Theorem A.6]).
Lemma 2.3. Let ψ(t) := {t} − 12, where {t} means the fractional part of real number t.
For x>1 and H >1, we have
ψ(x) =− X
16|h|6H
Φ h H+ 1
e(hx)
2πih +RH(x),
where Φ(t) := πt(1− |t|) cot(πt) +|t| and the second term RH(x) satisfies
(2.3) |RH(x)|6 1
2H+ 2 X
06|h|6H
1− |h|
H+ 1
e(hx).
3. bilinear forms
The aim of this section is to establish some non-trivial bounds for the bilinear forms given by (1.6), (1.9), (1.7) and (1.8). For the convenience, we consider
(3.1) SΛ∗1δ (x, D) := X
D<d`62D
Λ(d)ψ x
d`+δ
,
instead ofSωδ(x, D). The following proposition gives the required estimate forSΛ∗1δ (x, D).
Proposition 3.1. For any ε >0, we have
(3.2) SΛ∗1δ (x, D)ε (x19D87)1/133+ (x171D624)1/1026 xε
uniformly for x > 3, D 6 x57/103 and 0 6 δ 6 ε−1, where the implied constant depends on ε only.
Proof. Applying the Vaughan identity (2.2) withg(d) = ψ d`+δx
, it follows that (3.3) SΛ∗1δ (x, D) = SΛ∗1δ,1 +SΛ∗1δ,2 +SΛ∗1δ,3 +SΛ∗1δ,4 ,
where
SΛ∗1δ,1 :=X
`6D
X
m6(D/`)1/3
α1(m) X
D<`mn62D
ψ x
`mn+δ
,
SΛ∗1δ,2 :=X
`6D
X
m6(D/`)1/3
α2(m) X
D<`mn62D
ψ x
`mn+δ
logn, SΛ∗1δ,3 :=X
`6D
X X
(D/`)1/3<m,n6(D/`)2/3 D<`mn62D
α3(m)α4(n)ψ x
`mn+δ
,
SΛ∗1δ,4 :=X
`6D
X X
(D/`)1/3<m,n6(D/`)2/3 D<`mn62D
α5(m)α6(n)ψ x
`mn+δ
.
Using Lemma 2.3 and splitting the intervals of summation into the dyadic intervals, we can write
(3.4)
SΛ∗1δ,j =− 1 2πi
X
H0
X
L
X
M
X
N
SΛ∗1δ,j,[(H0, L, M, N) +SΛ∗1δ,j,[(H0, L, M, N)
+X
L
X
M
X
N
SΛ∗1δ,j,†(L, M, N), where 16H0 6H 6D, ah := Hh0Φ Hh+1
1 and SΛ∗1δ,1,[ =SΛ∗1δ,1,[(H0, L, M, N) := 1
H0 X
h∼H0
X
`∼L
X
m∼M
X
n∼N D<`mn62D
ahα1(m)e hx
`mn+δ
,
SΛ∗1δ,1,† =SΛ∗1δ,1,†(L, M, N) :=X
`∼L
X
m∼M
X
n∼N D<`mn62D
α1(m)RH x
`mn+δ
,
and SΛ∗1δ,j,[(H0, L, M, N), SΛ∗1δ,j,†(L, M, N) can be defined similarly for j = 2,3,4. We have
(3.5) LM N D, M 6(D/L)1/3 for j = 1,2
and
(3.6) LM N D, (D/L)1/3 6M 6(D/L)1/2 6N 6(D/L)2/3 for j = 3,4.
In the last case, we have considered the symmetry of m and n.
A. Bounds of SΛ∗1δ,j for j = 1,2.
Since we can remove the factor lognby a simple partial integration, we only treatSΛ∗1δ,1 . IfL6D1/5, applying the exponent pair (16,46) to the sum over n, we have
SΛ∗1δ,1,[ xε 1 H0
X
h∼H0
X
`∼L
X
m∼M
xH0 LM N2
1/6
N4/6+ xH0 LM N2
−1
xε (xHL5M5N2)1/6+x−1(LM N)2 . In view ofL6D1/5 and (3.5), we derive that
(3.7) SΛ∗1δ,1,[ (x5D17H5)1/30+x−1D2 xε for H0 6H 6D and (L, M, N) verifying (3.5).
Next we suppose that D1/5 6 L 6 D9/19. Firstly we remove the extra multiplicative condition D < `mn62D at the cost of a factor (logx)2 and then apply Lemma 2.1 with α=β =γ = 1, (X, H, M, N) = (xH0/LM N, H0, LM, N) and (κ, λ) = (12,12) to get
(3.8)
SΛ∗1δ,1,[ (xL4M4N3)1/6+LM N1/2 + (LM)1/2N +x−1/2(LM N)3/2 xε (x3D10L2)1/18+ (D2L)1/3 +DL−1/2+ (x−1D3)1/2
xε (x171D624)1/1026+D9/10+ (x−1D3)1/2
xε
for H0 6 H 6 D20/57 (6 (D/L)2/3 6 N) and (L, M, N) verifying (3.5) and D1/5 6 L 6 D9/19.
When D9/196L6D, we apply the exponent pair (16,46) to the sum over ` to get SΛ∗1δ,1,[ xε 1
H0 X
h∼H0
X
m∼M
X
n∼N
xH0 L2M N
1/6
L4/6+ xH0 L2M N
−1
xε (xHL2M5N5)1/6 +x−1H0−1(LM N)2 . From this we deduce that
(3.9) SΛ∗1δ,1,[ (x19D68H19)1/114+x−1D2 xε for H0 6H 6D and (L, M, N) verifying (3.5) and D9/196L6D.
Combining (3.7), (3.8) and (3.9), we obtain
(3.10) SΛ∗1δ,1,[ (x171D624)1/1026+D9/10+ (x−1D3)1/2 + (x19D68H19)1/114+ (x5D17H5)1/30
xε
for H0 6 H 6 D20/57 and (L, M, N) verifying (3.5), where we have used the fact that x−1D2 6(x−1D3)1/2. The same bound holds for SΛ,†δ,2. Therefore for j = 1,2, we have (3.11) SΛ∗1δ,j (x171D624)1/1026+D9/10+ (x−1D3)1/2
+ (x19D68H19)1/114+ (x5D17H5)1/30 xε for H 6D20/57 and (L, M, N) verifying (3.5).
B. Bounds of SΛ∗1δ,j for j = 3,4.
In this case, we should estimate SΛ∗1δ,3,[ =SΛ∗1δ,3,[(H0, L, M, N) := 1
H0 X
h∼H0
X
`∼L
X
m∼M
X
n∼N D<`mn62D
ahα3(m)α4(n)e hx
`mn+δ
,
SΛ∗1δ,3,†=SΛ∗1δ,3,†(L, M, N) := X
`∼L
X
m∼M
X
n∼N D<`mn62D
α3(m)α4(n)RH x
`mn+δ
,
for (L, M, N) verifying (3.6).
Firstly we bound SΛ∗1δ,3,[(H0, L, M, N). We remove the extra multiplicative condition D/` < mn 6 2D/` at the cost of a factor logx. By Lemma 2.1 with α = β = γ = 1, (X, H, M, N) = (xH0/LM N, H0, M, LN) and (κ, λ) = (12,12), we can derive
(3.12) SΛ∗1δ,3,[ ε (xL3M4N3)1/6+M(LN)1/2+M1/2LN + (x−1DH0)1/2 xε ε (x2D7L−1)1/12+ (D5L)1/6+ (x−1DH0)1/2
xε,
for H0 6H 6D1/2 (6 (LD)1/2 6LN) and (L, M, N) verifying (3.6), where we have re- moved the term (D3L−1)1/4 (6(D5L)1/6). On the other hand, we can apply the exponent pair (16,46) to the sum over ` (similar to (3.7)) to get
(3.13) SΛ∗1δ,3,[ (xD5HL−3)1/6+x−1D2 xε for H0 6H 6D and (L, M, N) verifying (3.6).
From (3.12) and (3.13), we deduce that
(3.14) SΛ∗1δ,3,[ ε (x2D7L−1)1/12+ (xD20H)1/24+ (x−1DH)1/2+x−1D2 xε,
for H 6D1/2 and (L, M, N) verifying (3.6), where we have used the following estimate min{(D5L)1/6,(xD5HL−3)1/6}6((D5L)1/6)1824((xD5HL−3)1/6)246 = (xD20H)1/24. Secondly we boundSΛ∗1δ,3,†. Using (2.3) of Lemma 2.3, we have
SΛ∗1δ,3,†xεX
`∼L
X
m∼M
X
n∼N
RH x
`mn+δ
xε H
X
`∼L
X
m∼M
X
n∼N
X
06|h|6H
1− |h|
H+ 1
e hx
`mn+δ
xε DH−1+ max
16H06H
eSΛ∗1δ,3,†(H0, L, M, N)
,
where
SeΛ∗1δ,3,†(H0, L, M, N) := 1 H
X
`∼L
X
m∼M
X
n∼N
X
h∼H0
1− |h|
H+ 1
e hx
`mn+δ
.
Clearly we can bound SeΛ∗1δ,3,†(H0, L, M, N) in the same way as SΛ∗1δ,3,[(H0, L, M, N) and get (3.15) SΛ∗1δ,3,† ε DH−1+ (x2D7L−1)1/12+ (xD20H)1/24+ (x−1DH)1/2+x−1D2
xε for H 6D1/2 and (L, M, N) verifying (3.6). Thus (3.14) and (3.15) imply that (3.16) SΛ∗1δ,j ε (x2D7)1/12+x−1D2+DH−1+ (xD20H)1/24+ (x−1DH)1/2
xε, for j = 3,4, H 6D1/2 and (L, M, N) verifying (3.6).
C.End of proof of (3.2).
Inserting (3.11) and (3.16) into (3.3) , we find that
SΛ∗1δ (x, D) (x171D624)1/1026+ (x2D7)1/12+D9/10+ (x−1D3)1/2
+DH−1 + (x19D68H19)1/114+ (x5D17H5)1/30+ (xD20H)1/24 xε for H 6D20/57, where we have removed the term (x−1DH)1/2 6(x−1D3)1/2. Optimising H over [1, D20/57], it follows that
SΛ∗1δ (x, D) (x171D624)1/1026+ (x2D7)1/12+D9/10+ (x−1D3)1/2 + (x19D87)1/133+ (x5D22)1/35+ (xD21)1/25+D9/19 + (x19D68)1/114+ (x5D17)1/30+ (xD20)1/24
xε
which implies the required inequality, since the 5th term dominates the 7th one provided D6x171/308 and the first term dominates the others ones provided D6x57/103.
The second proposition gives the required estimate for Sτδk(x, D) defined as in (1.7).
Proposition 3.2. Let k >2 be an integer. For any ε >0, we have (3.17) Sτδk(x, D)k,ε (xkD4k−1)1/6kxε
uniformly for x> 3, 1 6D 6 xmin{4k/(5k+1),k/(2k−2)} and 06 δ 6 ε−1, where the implied constant depends on k and ε only.
Proof. Noticing thatτk =τk−1∗1, using Lemma 2.3 and splitting the interval of summation into the dyadic intervals, we can write
(3.18)
Sτδk(x, D) = − 1 2πi
X
H0
X
M
X
N
Sτδ,[k(H0, M, N) +Sτδ,[k(H0, M, N)
+X
M
X
N
Sτδ,†k(M, N),
where H 6D,M N D (i.e. DM N D),N >D1/k,ah := Hh0Φ H+1h
1 and Sτδ,[k(H0, M, N) := 1
H0 X
h∼H0
ah X
m∼M
X
n∼N D<mn62D
τk−1(m)e hx mn+δ
,
Sτδ,†k(M, N) := X
m∼M
X
n∼N D<mn62D
τk−1(m)RH x mn+δ
.
Firstly we boundSτδ,[k(H0, M, N). Applying the exponent pair (12,12) to the sum overn, it follows that
(3.19)
Sτδ,[k(H0, M, N) xε H0
X
h∼H0
X
m∼M
n xh mN2
1/2
N1/2+ xh mN2
−1o
(xH0M N−1)1/2 +x−1D2 xε.
On the other hand, we remove the extra multiplicative condition D < mn 6 2D at the cost of a factor logx, and then apply Lemma 2.1 with α = β = γ = 1, (X, H, M, N) = (xH0/M N, H0, M, N) and (κ, λ) = (12,12) to get
Sτδ,[k(H0, M, N) (xM4N3)1/6+M N1/2+H0−1/2M1/2N + (x−1H0−1M3N3)1/2 Xε
provided H0 6H 6D1/k (6N). Using M N D and N >D1/k, we can derive that (3.20) Sτδ,[k(H0, M, N) (xkD4k−1)1/6k+D1−1/(2k)+H0−1/2M1/2N+ (x−1D3)1/2
xε (xkD4k−1)1/6k+H0−1/2M1/2N
xε
for H0 6 H 6 D1/k. In the last inequality, we can remove D1−1/(2k) and (x−1D3)1/2 because they can be absorbed by (xkD4k−1)1/6k for D 6 xmin{4k/(5k+1),k/(2k−2)}. From (3.19) and (3.20), we deduce that
(3.21) Sτδ,[k(H0, M, N)(xkD4k−1)1/6kxε
for H0 6 H 6 D1/k and M N = D 6 xmin{4k/(5k+1),k/(2k−2)}, where we have used the following estimates
min{(xH0M N−1)12, H0−12M12N}6((xH0M N−1)12)13(H0−12M12N)23
= (xH0−1M3N3)16 6(xD3)1/6
and max{(xD3)1/6, x−1D2}6(xkD4k−1)1/6k for D6x7k/(8k+1). On the other hand, (2.3) of Lemma 2.3 allows us to derive that
Sτδ,†k(M, N)
6 X
m∼M
X
n∼N
RH x mn+δ
6 1
2H+ 2 X
06|h|6H
1− |h|
H+ 1 X
m∼M
X
n∼N
e xh
d2mn+δ
.
When h6= 0, we can bound the triple sums as before. Thus (3.22) Sτδ,†k(M, N) DH−1+ (xkD4k−1)1/6k
xε for H 6D1/k and M N D6xmin{4k/(5k+1),k/(2k−2)}.
Inserting (3.21) and (3.22) into (3.18) and takingH =D1/k, we can obtain the required
inequality.
The third proposition gives the required estimate forS2δω(x, D) defined as in (1.8).
Proposition 3.3. For any ε >0, we have
S2δω(x, D)ε (x2D7)1/12xε
uniformly for x > 3 and 1 6 D 6 x8/11 and 0 6 δ 6 ε−1, where the implied constant depends on ε only.
Proof. Firstly we write
S2δω(x, D) = X
d6√ 2D
µ(d) X
D/d2<`62D/d2
τ(`)ψ x/d2
`+δ/d2
= X
d6√ 2D
µ(d)Sτδ/d2(x/d2, D/d2).
Secondly it is easy to see that D6 x8/11 implies D/d2 6 (x/d2)8/11. Thus we can apply
Proposition 3.2 with k= 2 to get the required result.
The last proposition gives the required estimate for Sµδ2(x, D) defined as in (1.9).
Proposition 3.4. For any ε >0, we have
Sµδ2(x, D)ε (xD3)1/7+ (xD2)1/6 xε
uniformly for x>3, 16D6x8/11 and 06δ6ε−1, where the implied constant depends on ε only.
Proof. Using Lemma 2.3 and splitting the interval of summation [1,2D] into the dyadic intervals (L,2L], we can write
(3.23) Sµδ2 =− 1 2πi
X
L
Sµδ,[2(L) +Sµδ,[2(L)
+X
L
Sµδ,†2(L), where H 6D and
Sµδ,[2(L) := X
h6H
1
hΦ h H+ 1
X
`∼L
X
(D/`)1/2<d6(2D/`)1/2
µ(d)e hx d2`+δ
,
Sµδ,†2(L) :=X
`∼L
X
(D/`)1/2<d6(2D/`)1/2
µ(d)RH x d2`+δ
.
Inverting the order of summations and applying the exponent pair (16,46) to the sum over
`, it follows that
(3.24)
Sµδ,[2(L) X
h∼H
1 h
X
(D/2L)1/2<d6(2D/L)1/2
xh d2L2
1/6
L4/6+ xh d2L2
−1
(xD2H)1/6+x−1D2 xε.
On the other hand, (2.3) of Lemma 2.3 allows us to derive that Sµδ,†2(L)
6 X
(D/2L)1/2<d6(2D/L)1/2
X
`∼L
RH x d2`+δ
6 1
2H+ 2 X
06|h|6H
1− |h|
H+ 1
X
(D/2L)1/2<d6(2D/L)1/2
X
`∼L
e xh d2`+δ
.
When h6= 0, as before we apply the exponent pair (16,46) to the sum over ` and obtain (3.25) Sµδ,†2(L) DH−1+ (xD2H)1/6+x−1D2
xε. Inserting (3.24) and (3.25) into (3.23), it follows that
Sµδ2 DH−1+ (xD2H)1/6+x−1D2 xε for H 6D. OptimisingH on [1, D], we find that
Sµδ2 (xD3)1/7+ (xD2)1/6+x−1D2 xε
This implies the required result, sincex−1D2 6(xD3)1/7 for D6x8/11.
4. Proof of Theorem 1
Letf =ω orτk or 2ω orµ2 and letNf ∈[1, x1/2) be a parameter which can be chosen later. First we write
(4.1) Sf(x) =X
n6x
fhx n
i
=Sf†(x) +Sf](x) with
Sf†(x) := X
n6Nf
fhx n
i
, Sf](x) := X
Nf<n6x
fhx n
i .
In our case, we havef(n)ε nε for any ε >0 and all n>1. Thus
(4.2) Sf†(x)ε Nfxε.
In order to boundSf](x), we put d= [x/n]. Noticing that
x/n−1< d6x/n ⇔ x/(d+ 1)< n 6x/d, we can derive that
(4.3)
Sf](x) = X
d6x/Nf
f(d) X
x/(d+1)<n6x/d
1
= X
d6x/Nf
f(d)x
d −ψx d
− x
d+ 1 +ψ x d+ 1
=xX
d>1
f(d)
d(d+ 1) +Rf1(x, Nf)−Rf0(x, Nf) +O(Nf), where we have used the following bounds
x X
d>x/Nf
f(d)
d(d+ 1) ε Nfxε, X
d6Nf
f(d) ψ x
d+ 1
−ψx d
εNfxε
and
Rfδ(x, Nf) = X
Nf<d6x/Nf
f(d)ψ x d+δ
.
Combining (4.1), (4.2) and (4.3), it follows that Sf(x) = xX
d>1
f(d)
d(d+ 1) +Oε |Rf1(x, Nf)|+|Rf0(x, Nf)|+Nfxε .
Thus in order to prove Theorem 1, it suffices to show that (4.4) Rfδ(x, Nf)Nfxε (x>1) for
f ω τk 2ω µ2
Nf x53/110 x(5k−1)/(10k−1) x9/19 x2/5
4.1. Proof of (4.4) with f =ω.
We haveNω =x53/110. In order to apply (3.2) of Proposition 3.1, we must switch from Rωδ(x, Nω) = X
Nω<p`6x/Nω
ψ x p`+δ
= X
Nω<p`6x/Nω
Λ(p)
logpψ x p`+δ
to
Reωδ(x, Nω, t) :=X
d6t
Λ(d) X
Nω/d<`6(x/Nω)/d
ψ x
d`+δ
.
For this, we need to estimate the contribution of prime powers:
R1 := X
Nω<pν`6x/Nω
`6(x/Nω)53/114, ν>2
Λ(pν)
logpνψ x pν`+δ
= X
Nω<pν`6x/Nω
`6(x/Nω)53/114, ν>2
1
νψ x pν`+δ
,
R2 := X
Nω<pν`6x/Nω
`>(x/Nω)53/114, ν>2
Λ(pν)
logpνψ x pν`+δ
= X
Nω<pν`6x/Nω
`>(x/Nω)53/114, ν>2
1
νψ x pν`+δ
.
Firstly we have trivially R1 X
`6(x/Nω)53/114
(x/Nω`)1/2 (x/Nω)167/228x167/440.
On the other hand, applying [10, Lemma 2.4] with (κ, λ) = (12,12), we can derive that R2 = X
pν6(x/Nω)61/114 ν>2
1 ν
X
(x/Nω)53/114<`6x/Nωpν
ψ x pν`+δ
X
pν6(x/Nω)61/114 ν>2
max
(x/Nω)53/114<N16x/Nωpν N1<N262N1
N1
X
N1<`6N2
1
`ψ x pν`+δ
X
pν6(x/Nω)61/114 ν>2
max
(x/Nω)53/114<N16x/Nωpν N1<N262N1
N12
(x/pν) + (x/pν)1/3
X
pν6(x/Nω)61/114 ν>2
x
Nω2pν + (x/pν)1/3
x/Nω2+x1/3(x/Nω)(61/114)/6 x167/440
Thus we can write
(4.5)
Rωδ(x, Nω) = X
Nω<d`6x/Nω
Λ(d) logdψ
x d`+δ
+O x167/440
=
Z x/Nω
2−
1
logtdReωδ(x, Nω, t) +O x167/440 max
26t6x/Nω
eRωδ(x, Nω, t)
+x167/440.
WritingDj :=x/(2jNω), we have Nω 6Dj 6x/Nω 6 x57/110 for 06j 6 log(x/Nlog 2ω2). Thus we can apply (3.2) of Proposition 3.1 to get
|eRωδ(x, Nω, t)|6 X
06j6log(x/Nω2)/log 2
|SΛ∗1δ (x, Dj)|
X
06j6log(x/Nω2)/log 2
(x19D87j )1/133+ (x171D624j )1/1026 xε (x106Nω−87)1/133+ (x795Nω−624)1/1026
xε
for all 26t6x/Nω. Inserting this into (4.5), we get the required result.
4.2. Proof of (4.4) with f =τk.
We have Nτk = x(5k−1)/(10k−1). Let Dj := x/(2jNτk), then we easily see that Nτk 6 Dj 6x/Nτk 6xmin{4k/(5k+1),k/(2k−2)} for 06j 6 log(x/N
τk2 )
log 2 . Thus Proposition 3.2 gives us
|Rτδk(x, Nτk)|6 X
06j6log(x/Nτk2 )/log 2
|Sτδk(x, Dj)|
X
06j6log(x/Nτk2 )/log 2
(xkD4k−1j )1/6kxε (x5k−1Nτ−(4k−1)
k )1/6kxε, which implies the required result.
4.3. Proof of (4.4) with f = 2ω.
We have N2ω = x9/19. Let Dj := x/(2jN2ω), then N2ω 6 Dj 6 x/N2ω 6 x10/19 for 06j 6 log(x/Nlog 222ω). Noticing that 2ω = ˜µ∗τ, we can apply Proposition 3.3 to get
|R2δω(x, N2ω)|6 X
06j6log(x/N22ω)/log 2
|S2δω(x, Dj)|
X
06j6log(x/N22ω)/log 2
(x2D7j)1/12xε (x9N2−7ω )1/12xε,
which implies the required result.
4.4. Proof of (4.4) with f =µ2.
We have Nµ2 = x2/5. Let Dj := x/(2jNµ2), then Nµ2 6 Dj 6 x/Nµ2 6 x3/5 for 06j 6 log(x/N
µ22)
log 2 . Noticing that µ2 = ˜µ∗1, we can apply Proposition 3.4 to get
|Rµδ2(x, Nµ2)|6 X
06j6log(x/Nµ22)/log 2
|Sµδ2(x, Dj)|
X
06j6log(x/Nµ22)/log 2
(xDj3)1/7+ (xD2j)1/6 xε (x4Nµ−32 )1/7 + (x3Nµ−22 )1/6
xε, which implies the required result.
Acknowledgement. This work is supported in part by the National Natural Science Foundation of China (Grant Nos. 12071238, 11771252, 11971370 and 12071375) and by the NSF of Chongqing (Grant No. cstc2019jcyj-msxm1651).
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Kui Liu, School of Mathematics and Statistics, Qingdao University, 308 Ningxia Road, Qingdao, Shandong 266071, China
E-mail address: liukui@qdu.edu.cn
Jie Wu, CNRS UMR 8050, Laboratoire d’Analyse et de Math´ematiques Appliqu´ees, Universit´e Paris-Est Cr´eteil, 94010 Cr´eteil cedex, France
E-mail address: jie.wu@u-pec.fr
Zhishan Yang, School of Mathematics and Statistics, Qingdao University, 308 Ningxia Road, Qingdao, Shandong 266071, China
E-mail address: zsyang@qdu.edu.cn