The Piatetski-Shapiro sequences are sequences of the form (⌊nc⌋)∞n=1 for c>1 and c∉N. It is conjectured that there are infinitely many primes in Piatetski-Shapiro sequences for c∈(1,2). For every R≥1, we say that a natural number is an R-almost prime if it has at most R prime factors, counted with multiplicity. In this paper, we prove that there are infinitely many R-almost primes in Piatetski-Shapiro sequences if c∈(1,cR) and cR is an explicit constant depending on R.
Citation: Victor Zhenyu Guo. Almost primes in Piatetski-Shapiro sequences[J]. AIMS Mathematics, 2021, 6(9): 9536-9546. doi: 10.3934/math.2021554
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The Piatetski-Shapiro sequences are sequences of the form (⌊nc⌋)∞n=1 for c>1 and c∉N. It is conjectured that there are infinitely many primes in Piatetski-Shapiro sequences for c∈(1,2). For every R≥1, we say that a natural number is an R-almost prime if it has at most R prime factors, counted with multiplicity. In this paper, we prove that there are infinitely many R-almost primes in Piatetski-Shapiro sequences if c∈(1,cR) and cR is an explicit constant depending on R.
The Piatetski-Shapiro sequences are sequences of the form
N(c):=(⌊nc⌋)∞n=1(c>1,c∉N). |
Such sequences have been named in honor of Piatetski-Shapiro [13], who published the first paper in this problem. He showed that the counting function
π(c)(x):=|{ prime p≤x:p∈N(c)}| |
satisfies the asymptotic relation
π(c)(x)∼x1/clogxas x→∞, |
if
1<c<1211=1.0909…. |
The range for c of the asymptotic formula of π(c)(x) has been improved by several mathematicians over the years. Kolesnik [7] improved this result to
1<c<109=1.1111…. |
Graham and Leitmann [10] using the method of exponent pairs independently improved the range to
1<c<6962=1.1129…. |
Graham did not publish his paper. Heath-Brown [4] applied the Weyl's shift and the exponent pair method, together with his decomposition of the Von Mangoldt function, extended the range to
1<c<755662=1.1404…. |
Kolesnik [8] using the method of multiple exponential sums improved the range to
1<c<3934=1.1470…. |
Liu and Rivat [12] applied the double large sieve to Type I sums and extended the range to
1<c<1513=1.1538…. |
Rivat [14] improved the range in his PhD thesis to
1<c<61215302=1.1544…. |
Rivat and Sargos [15] held the best record to be
1<c<28172426=1.1611…. |
We mention that Leitmann and Wolke [11] proved that the asymptotic formula holds for almost all c∈(1,2) in the sense of Lebesgue measure.
Rivat also considered to prove that there are infinitely many Piatetski-Shapiro primes by giving a lower bound of π(c)(x). He used a sieve method and showed that
π(c)(x)≫x1/clogx |
if
1<c<76=1.1666⋯. |
Later, Baker, Harman and Rivat [1] and Jia [6] improved this range to
1<c<2017=1.1764…. |
Jia [5] extended the range again to
1<c<1311=1.1818…. |
Kumchev [9] improved the range to
1<c<4538=1.1842…. |
Eventually, Rivat and Wu [16] gave the best range up to now, which is
1<c<243205=1.1853…. |
We remark that if c∈(0,1) then N(c) contains all natural numbers, hence contains all primes. The estimation of Piatetski-Shapiro primes is an approximation of the well-known conjecture that there exists infinitely many primes of the form n2+1.
It is conjectured that there are infinitely many Piatetski-Shapiro primes for c∈(1,2). However, the best known bound for c is still far from 2 and the range for c has not been improved for almost 20 years. We approach this problem in a different direction. For every R≥1, we say that a natural number is an R-almost prime if it has at most R prime factors, counted with multiplicity. The study of almost primes is an intermediate step to the investigation of primes. In this paper, we prove there are infinitely many almost primes in Piatetski-Shapiro sequences.
Theorem 1.1. For any fixed c∈(1,cR) we have
|{n≤x:⌊nc⌋isanR−almostprime}|≫xlogx |
holds for all sufficiently large x. In particular, we have
c3:=889741=1.1997…,c4:=2588216071=1.6104…, |
and
cR:=3−1283(8R−1)(R≥5). |
Recall that the best known range that there are infinitely many Piatetski-Shapiro primes is (1,1.1853) and c3=1.1997>1.1853. Hence our theorem for 3-almost primes provides a bigger range of c than that of prime numbers. Moreover, when R=6 we have that
c6=295141=2.0921, |
which is greater than 2.
We denote by ⌊t⌋ and {t} the integer part and the fractional part of t, respectively. As is customary, we put e(t):=e2πit. We make considerable use of the sawtooth function defined by
ψ(t):=t−⌊t⌋−12={t}−12(t∈R). |
The letter p always denotes a prime. For the Piatetski-Shapiro sequence (⌊nc⌋)∞n=1, we denote γ:=c−1. We use notation of the form m∼M as an abbreviation for M<m≤2M.
Throughout the paper, implied constants in symbols O, ≪ and ≫ may depend (where obvious) on the parameters c,ε but are absolute otherwise. For given functions F and G, the notations F≪G, G≫F and F=O(G) are all equivalent to the statement that the inequality |F|≤C|G| holds with some constant C>0. F≍G means that F≪G≪F.
As we have mentioned the following notion plays a crucial role in our arguments. We specify it to the form that is suited to our applications; it is based on a result of Greaves [3] that relates level of distribution to R-almost primality. More precisely, we say that an N-element set of integers A has a level of distribution D if for a given multiplicative function f(d) we have
∑d≤Dmaxgcd(s,d)=1||{a∈A,a≡smodd}|−f(d)dN|≤Nlog2N. |
As in [3,pp. 174–175] we define the constants
δ2:=0.044560,δ3:=0.074267,δ4:=0.103974 |
and
δR:=0.124820,R≥5. |
We have the following result, which is [3,Chapter 5,Proposition 1].
Lemma 2.1. Suppose A is an N-element set of positive integers with a level of distribution D and degree ρ in the sense that
a<Dρ(a∈A) |
holds with some real number ρ<R−δR. Then
|{a∈A:ais anR-almost prime}|≫ρNlogN. |
Lemma 2.2. Let M≥1 and λ be positive real numbers and let H be a positive integer. If f:[1,M]→R is a real valued function with three continuous derivatives, which satisfies
λ≤|f(3)(x)|≪λfor1≤x≤M, |
then for the sum
S=1H2H∑h=H+1|Mh∑m=1e(hHf(m))|, |
where the integer Mh satisfies 1≤Mh≤M for each h∈[H+1,2H], we have
S≪Mε(Mλ1/6H−1/9+Mλ1/5+M3/4)+λ−1/3. |
Proof. See [17,Theorem 1].
Lemma 2.3. For any H≥1 there are numbers ah,bh such that
|ψ(t)−∑0<|h|≤Hahe(th)|≤∑|h|≤Hbhe(th),ah≪1|h|,bh≪1H. |
Proof. See [18].
We also need the method of exponent pair. A detailed definition of exponent pair can be found in [2,Page 31]. For an exponent pair (k,l), we denote
A(k,l):=(k2k+2,k+l+12k+2) |
and
B(k,l):=(l−12,k+12) |
the A-process and B-process of the exponent pair, respectively.
The set we sieve is
A:={m≤xc:m=⌊nc⌋ for integer n}. |
For any d≤D, where D is a fixed power of x, we estimate
Ad:={m∈A:d|m}. |
We know that rd∈A if and only if
rd≤nc<rd+1andrd≤x. |
Within O(1) the cardinality of Ad is equal to the number of integers n≤x for which the interval ((nc−1)d−1,ncd−1] contains a natural number. Hence
|Ad|=∑n≤x(⌊ncd−1⌋−⌊(nc−1)d−1⌋)+O(1)=Xd−1+∑n≤x(ψ((nc−1)d−1)−ψ(ncd−1))+O(1), |
where
X:=∑n≤x1=x. |
By Lemma 2.1 we need to show that for any sufficiently small ε>0
∑d≤D||Ad|−Xd−1|≤Xx−ε/3=x1−ε/3 |
for sufficiently large x. Splitting the range of d into dyadic subintervals, it is sufficient to prove that
∑d∼D1|∑N<n≤N1(ψ((nc−1)d−1)−ψ(ncd−1))|≪x1−ε/2 | (3.1) |
holds uniformly for D1≤D,N≤x,N1∼N. Our aim is to establish (3.1) with D as large as possible. We define
S:=∑N<n≤N1(ψ((nc−1)d−1)−ψ(ncd−1)). | (3.2) |
By Lemma 2.3 and taking that
H=Dxε, |
we have
S=S1+O(S2), |
where
S1:=∑N<n≤N1∑0<|h|≤Hah(e(h(nc−1)d−1)−e(hncd−1)) |
and
S2:=∑N<n≤N1∑|h|≤Hbh(e(h(nc−1)d−1)+e(hncd−1)). |
We consider S1. Writing that
ϕh:=e(hd−1)−1≪1, |
we obtain that
S1=∑N<n≤N1∑0<|h|≤Hahϕhe(hncd−1)≪∑0<h≤Hh−1∑N<n≤N1e(hncd−1). | (3.3) |
Using the exponent pair (k,l), we have
∑N<n≤N1e(hncd−1)≪(hd−1Nc−1)kNl+(hd−1)−1N1−c. | (3.4) |
Substituting (3.4) to S1 and (3.1), it becomes that
∑d∼D1|S1|≪∑d∼D1|∑0<h≤Hh−1(hkd−kNkc−k+l+h−1dN1−c)|≪∑d∼D1|Hkd−kNkc−k+l+H−1dN1−c|≪HkD1−kNkc−k+l+H−1D2N1−c≪Dxkc−k+l+kε+D2x1−c. |
Now we consider S2. The contribution of S2 from h=0 is
∑N<n≤N1bh≪NH−1. | (3.5) |
Substituting (3.5) to (3.1), we have
∑d∼D1NH−1≪DNH−1≪x1−ε/2, |
The contribution of S2 from h≠0 is
=∑N<n≤N1∑0<|h|≤Hbh(e(h(mc−1)d−1)+e(hmcd−1))≪∑N<n≤N1∑0<|h|≤Hbhϕhe(hncd−1)≪∑0<h≤HH−1∑N<n≤N1e(hncd−1), | (3.6) |
which can be estimated by the same method of S1. By (3.4), we write (3.6) to be
≪∑d∼D1|∑0<h≤HH−1(hkd−kNkc−k+l+h−1dN1−c)|≪HkD1−kNkc−k+l+H−1D2N1−clogH≪Dxkc−k+l+kε+D2x1−c. |
Therefore, to make (3.1) to be true, we need that
Dxkc−k+l+kε≪x1−ε/2, | (3.7) |
and
D2x1−c≪x1−ε/2. | (3.8) |
Combining (3.7) and (3.8), we obtain that
D≪min(xc/2−ε/4,x1−kc+k−l−ε). | (3.9) |
We apply the weighted sieve with the choice
R=3,δ3=0.074267 |
and choose
ΛR=3−340=11740<R−δR. |
By (3.9) we require that
1−kc+k−l>40117andc2>40117, | (3.10) |
then by Lemma 2.1, A contains ≫x/logxR-almost primes. To achieve (3.10), we need that
c<70−117l117k+1. |
Taking the exponent pair
BAAAAAB(0,1)=(1942,3263), |
we have that
c<889741=1.1997…. |
We apply the weighted sieve with the choice
R=4,δ4=0.103974 |
and choose
ΛR=4−13125=487125<R−δR. |
Similarly to (3.10), we need that
1−kc+k−l>125487andc2>125487, | (3.11) |
which requires that
c<362−487l487k+1=2588216071=1.6104…, |
by taking the exponent pair
BABABAABAAB(0,1)=(33128,75128). |
For R≥5, we estimate (3.2) by Lemma 2.2. By (3.3) we have that
S1≪logHmax1≪T≪HS(T,N), |
where
S(T,N):=1T∑h∼T∑n∼Ne(hd−1nc). |
By Lemma 2.2 with f(n)=Td−1(n+N)c and
λ=c(c−1)(c−2)Td−1Nc−3, |
it follows that
S(T,N)≪N1+ε(Td−1Nc−3)1/6T−1/9+N1+ε(Td−1Nc−3)1/5+N3/4+ε+(Td−1Nc−3)−1/3≪T1/18d−1/6Nc/6+1/2+ε+T1/5d−1/5Nc/5+2/5+ε+N3/4+ε+T−1/3d1/3N1−c/3. |
Hence
S1≪H1/18d−1/6Nc/6+1/2+ε+H1/5d−1/5Nc/5+2/5+ε+N3/4+ε+d1/3N1−c/3. |
The contribution of S2 from h≠0 can be estimated by the same method and achieve the same upper bound, which means that (3.6) is
≪H1/18d−1/6Nc/6+1/2+ε+H1/5d−1/5Nc/5+2/5+ε+N3/4+ε+d1/3N1−c/3. |
Together with the contribution of S2 from h=0, by (3.5) we obtain that the left-hand side of (3.1) is
∑d∼D1|S|≪∑d∼D1|H1/18d−1/6Nc/6+1/2+ε+H1/5d−1/5Nc/5+2/5+ε+N3/4logH+d1/3N1−c/3|≪H1/18D5/6Nc/6+1/2+ε+H1/5D4/5Nc/5+2/5+ε+DN3/4logH+D4/3N1−c/3≪D8/9xc/6+1/2+19ε/18+Dxc/5+2/5+6ε/5+Dx3/4+ε+D4/3x1−c/3. |
To ensure the left-hand side of (3.1) is ≪x1−ε/2, we require that
D≪min(x9/16−3c/16−ε,x3/5−c/5−ε,x1/4−ε,xc/4−ε). | (3.12) |
We apply the weighted sieve with the choice
δR=0.124820(R≥5) |
and choose
ΛR=R−18<R−δR. |
To apply Lemma 2.1, by (3.12) we need that
min(916−316c,35−c5,14,c4)>1R−18, |
which gives that
c<3−1283(8R−1). |
The author is supported in part by the National Natural Science Foundation of China (No. 11901447), the China Postdoctoral Science Foundation (No. 2019M653576) and the Natural Science Foundation of Shaanxi Province (No. 2020JQ-009).
The author declares no conflicts of interest in this paper.
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1. | Jinyun Qi, Zhefeng Xu, Almost primes in generalized Piatetski-Shapiro sequences, 2022, 7, 2473-6988, 14154, 10.3934/math.2022780 |