Research article

Almost primes in Piatetski-Shapiro sequences

  • Received: 01 June 2021 Accepted: 22 June 2021 Published: 24 June 2021
  • MSC : 11B83, 11L07

  • The Piatetski-Shapiro sequences are sequences of the form (nc)n=1 for c>1 and cN. It is conjectured that there are infinitely many primes in Piatetski-Shapiro sequences for c(1,2). For every R1, 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

    Related Papers:

    [1] Jinyun Qi, Zhefeng Xu . Almost primes in generalized Piatetski-Shapiro sequences. AIMS Mathematics, 2022, 7(8): 14154-14162. doi: 10.3934/math.2022780
    [2] Yukai Shen . $ k $th powers in a generalization of Piatetski-Shapiro sequences. AIMS Mathematics, 2023, 8(9): 22411-22418. doi: 10.3934/math.20231143
    [3] Zhao Xiaoqing, Yi Yuan . Square-free numbers in the intersection of Lehmer set and Piatetski-Shapiro sequence. AIMS Mathematics, 2024, 9(12): 33591-33609. doi: 10.3934/math.20241603
    [4] Min Zhang, Fei Xue, Jinjiang Li . On the Waring–Goldbach problem for two squares and four cubes. AIMS Mathematics, 2022, 7(7): 12415-12436. doi: 10.3934/math.2022689
    [5] Li Zhu . On pairs of equations with unequal powers of primes and powers of 2. AIMS Mathematics, 2025, 10(2): 4153-4172. doi: 10.3934/math.2025193
    [6] Jing Huang, Ao Han, Huafeng Liu . On a Diophantine equation with prime variables. AIMS Mathematics, 2021, 6(9): 9602-9618. doi: 10.3934/math.2021559
    [7] Gen Li, Liqun Hu, Xianjiu Huang . On pairs of equations in eight prime cubes and powers of 2. AIMS Mathematics, 2023, 8(2): 3940-3948. doi: 10.3934/math.2023197
    [8] Bingzhou Chen, Jiagui Luo . On the Diophantine equations $x^2-Dy^2=-1$ and $x^2-Dy^2=4$. AIMS Mathematics, 2019, 4(4): 1170-1180. doi: 10.3934/math.2019.4.1170
    [9] Vladimir Edemskiy, Chenhuang Wu . On the $ k $-error linear complexity of binary sequences of periods $ p^n $ from new cyclotomy. AIMS Mathematics, 2022, 7(5): 7997-8011. doi: 10.3934/math.2022446
    [10] Jing Huang, Qian Wang, Rui Zhang . On a binary Diophantine inequality involving prime numbers. AIMS Mathematics, 2024, 9(4): 8371-8385. doi: 10.3934/math.2024407
  • The Piatetski-Shapiro sequences are sequences of the form (nc)n=1 for c>1 and cN. It is conjectured that there are infinitely many primes in Piatetski-Shapiro sequences for c(1,2). For every R1, 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,cN).

    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 px:pN(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 R1, 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

    |{nx:ncisanRalmostprime}|xlogx

    holds for all sufficiently large x. In particular, we have

    c3:=889741=1.1997,c4:=2588216071=1.6104,

    and

    cR:=31283(8R1)(R5).

    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):=tt12={t}12(tR).

    The letter p always denotes a prime. For the Piatetski-Shapiro sequence (nc)n=1, we denote γ:=c1. We use notation of the form mM as an abbreviation for M<m2M.

    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 FG, GF and F=O(G) are all equivalent to the statement that the inequality |F|C|G| holds with some constant C>0. FG means that FGF.

    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

    dDmaxgcd(s,d)=1||{aA,asmodd}|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,R5.

    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(aA)

    holds with some real number ρ<RδR. Then

    |{aA:ais anR-almost prime}|ρNlogN.

    Lemma 2.2. Let M1 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)|λfor1xM,

    then for the sum

    S=1H2Hh=H+1|Mhm=1e(hHf(m))|,

    where the integer Mh satisfies 1MhM for each h[H+1,2H], we have

    SMε(Mλ1/6H1/9+Mλ1/5+M3/4)+λ1/3.

    Proof. See [17,Theorem 1].

    Lemma 2.3. For any H1 there are numbers ah,bh such that

    |ψ(t)0<|h|Hahe(th)||h|Hbhe(th),ah1|h|,bh1H.

    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):=(l12,k+12)

    the A-process and B-process of the exponent pair, respectively.

    The set we sieve is

    A:={mxc:m=nc for integer n}.

    For any dD, where D is a fixed power of x, we estimate

    Ad:={mA:d|m}.

    We know that rdA if and only if

    rdnc<rd+1andrdx.

    Within O(1) the cardinality of Ad is equal to the number of integers nx for which the interval ((nc1)d1,ncd1] contains a natural number. Hence

    |Ad|=nx(ncd1(nc1)d1)+O(1)=Xd1+nx(ψ((nc1)d1)ψ(ncd1))+O(1),

    where

    X:=nx1=x.

    By Lemma 2.1 we need to show that for any sufficiently small ε>0

    dD||Ad|Xd1|Xxε/3=x1ε/3

    for sufficiently large x. Splitting the range of d into dyadic subintervals, it is sufficient to prove that

    dD1|N<nN1(ψ((nc1)d1)ψ(ncd1))|x1ε/2 (3.1)

    holds uniformly for D1D,Nx,N1N. Our aim is to establish (3.1) with D as large as possible. We define

    S:=N<nN1(ψ((nc1)d1)ψ(ncd1)). (3.2)

    By Lemma 2.3 and taking that

    H=Dxε,

    we have

    S=S1+O(S2),

    where

    S1:=N<nN10<|h|Hah(e(h(nc1)d1)e(hncd1))

    and

    S2:=N<nN1|h|Hbh(e(h(nc1)d1)+e(hncd1)).

    We consider S1. Writing that

    ϕh:=e(hd1)11,

    we obtain that

    S1=N<nN10<|h|Hahϕhe(hncd1)0<hHh1N<nN1e(hncd1). (3.3)

    Using the exponent pair (k,l), we have

    N<nN1e(hncd1)(hd1Nc1)kNl+(hd1)1N1c. (3.4)

    Substituting (3.4) to S1 and (3.1), it becomes that

    dD1|S1|dD1|0<hHh1(hkdkNkck+l+h1dN1c)|dD1|HkdkNkck+l+H1dN1c|HkD1kNkck+l+H1D2N1cDxkck+l+kε+D2x1c.

    Now we consider S2. The contribution of S2 from h=0 is

    N<nN1bhNH1. (3.5)

    Substituting (3.5) to (3.1), we have

    dD1NH1DNH1x1ε/2,

    The contribution of S2 from h0 is

    =N<nN10<|h|Hbh(e(h(mc1)d1)+e(hmcd1))N<nN10<|h|Hbhϕhe(hncd1)0<hHH1N<nN1e(hncd1), (3.6)

    which can be estimated by the same method of S1. By (3.4), we write (3.6) to be

    dD1|0<hHH1(hkdkNkck+l+h1dN1c)|HkD1kNkck+l+H1D2N1clogHDxkck+l+kε+D2x1c.

    Therefore, to make (3.1) to be true, we need that

    Dxkck+l+kεx1ε/2, (3.7)

    and

    D2x1cx1ε/2. (3.8)

    Combining (3.7) and (3.8), we obtain that

    Dmin(xc/2ε/4,x1kc+klε). (3.9)

    We apply the weighted sieve with the choice

    R=3,δ3=0.074267

    and choose

    ΛR=3340=11740<RδR.

    By (3.9) we require that

    1kc+kl>40117andc2>40117, (3.10)

    then by Lemma 2.1, A contains x/logxR-almost primes. To achieve (3.10), we need that

    c<70117l117k+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=413125=487125<RδR.

    Similarly to (3.10), we need that

    1kc+kl>125487andc2>125487, (3.11)

    which requires that

    c<362487l487k+1=2588216071=1.6104,

    by taking the exponent pair

    BABABAABAAB(0,1)=(33128,75128).

    For R5, we estimate (3.2) by Lemma 2.2. By (3.3) we have that

    S1logHmax1THS(T,N),

    where

    S(T,N):=1ThTnNe(hd1nc).

    By Lemma 2.2 with f(n)=Td1(n+N)c and

    λ=c(c1)(c2)Td1Nc3,

    it follows that

    S(T,N)N1+ε(Td1Nc3)1/6T1/9+N1+ε(Td1Nc3)1/5+N3/4+ε+(Td1Nc3)1/3T1/18d1/6Nc/6+1/2+ε+T1/5d1/5Nc/5+2/5+ε+N3/4+ε+T1/3d1/3N1c/3.

    Hence

    S1H1/18d1/6Nc/6+1/2+ε+H1/5d1/5Nc/5+2/5+ε+N3/4+ε+d1/3N1c/3.

    The contribution of S2 from h0 can be estimated by the same method and achieve the same upper bound, which means that (3.6) is

    H1/18d1/6Nc/6+1/2+ε+H1/5d1/5Nc/5+2/5+ε+N3/4+ε+d1/3N1c/3.

    Together with the contribution of S2 from h=0, by (3.5) we obtain that the left-hand side of (3.1) is

    dD1|S|dD1|H1/18d1/6Nc/6+1/2+ε+H1/5d1/5Nc/5+2/5+ε+N3/4logH+d1/3N1c/3|H1/18D5/6Nc/6+1/2+ε+H1/5D4/5Nc/5+2/5+ε+DN3/4logH+D4/3N1c/3D8/9xc/6+1/2+19ε/18+Dxc/5+2/5+6ε/5+Dx3/4+ε+D4/3x1c/3.

    To ensure the left-hand side of (3.1) is x1ε/2, we require that

    Dmin(x9/163c/16ε,x3/5c/5ε,x1/4ε,xc/4ε). (3.12)

    We apply the weighted sieve with the choice

    δR=0.124820(R5)

    and choose

    ΛR=R18<RδR.

    To apply Lemma 2.1, by (3.12) we need that

    min(916316c,35c5,14,c4)>1R18,

    which gives that

    c<31283(8R1).

    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.



    [1] R. C. Baker, G. Harman, J. Rivat, Primes of the form nc, J. Number Theory, 50 (1995), 261–277. doi: 10.1006/jnth.1995.1020
    [2] S. W. Graham, G. Kolesnik, Van der Corput's method of exponential sums, London Mathematical Society Lecture Note Series, 126. Cambridge University Press, Cambridge, 1991.
    [3] G. Greaves, Sieves in Number Theory, Results in Mathematics and Related Areas, Vol. 43, Springer-Verlag, Berlin, 2001.
    [4] D. R. Heath-Brown, The Pjateckiǐ-Šapiro prime number theorem, J. Number Theory, 16 (1983), 242–266. doi: 10.1016/0022-314X(83)90044-6
    [5] C. H. Jia, On Pjateckiǐ-Šapiro prime number theorem II, Sci. China Ser. A, 36 (1993), 913–926.
    [6] C. H. Jia, On Pjateckiǐ-Šapiro prime number theorem, Chin. Ann. Math. Ser. B, 15 (1994), 9–22.
    [7] G. A. Kolesnik, The distribution of primes in sequences of the form nc, Mat. Zametki, 2 (1967), 117–128.
    [8] G. A. Kolesnik, Primes of the form nc, Pacific J. Math., 118 (1985), 437–447. doi: 10.2140/pjm.1985.118.437
    [9] A. Kumchev, On the distribution of prime numbers of the form nc, Glasg. Math. J., 41 (1999), 85–102. doi: 10.1017/S0017089599970477
    [10] D. Leitmann, Abschätzung trigonometrischer Summen (German), J. Reine Angew. Math., 317 (1980), 209–219.
    [11] D. Leitmann, D. Wolke, Primzahlen der Gestalt [f(n)] (German), Math. Z., 145 (1975), 81–92. doi: 10.1007/BF01214500
    [12] H. Q. Liu, J. Rivat, On the Pjateckiǐ-Šapiro prime number theorem, Bull. Lond. Math. Soc., 24 (1992), 143–147. doi: 10.1112/blms/24.2.143
    [13] I. I. Piatetski-Shapiro, On the distribution of prime numbers in the sequence of the form f(n), Mat. Sb., 33 (1953), 559–566.
    [14] J. Rivat, Autour d'un theorem de Piatetski-Shapiro, Thesis, Université de Paris Sud, 1992.
    [15] J. Rivat, S. Sargos, Nombres premiers de la forme nc, Canad. J. Math., 53 (2001), 414–433. doi: 10.4153/CJM-2001-017-0
    [16] J. Rivat, J. Wu, Prime numbers of the form nc, Glasg. Math. J., 43 (2001), 237–254.
    [17] O. Robert, P. Sargos, A third derivative test for mean values of exponential sums with application to lattice point problems, Acta Arith., 106 (2003), 27–39. doi: 10.4064/aa106-1-2
    [18] J. D. Vaaler, Some extremal problems in Fourier analysis, Bull. Amer. Math. Soc., 12 (1985), 183–216. doi: 10.1090/S0273-0979-1985-15349-2
  • This article has been cited by:

    1. Jinyun Qi, Zhefeng Xu, Almost primes in generalized Piatetski-Shapiro sequences, 2022, 7, 2473-6988, 14154, 10.3934/math.2022780
  • Reader Comments
  • © 2021 the Author(s), licensee AIMS Press. This is an open access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0)
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Metrics

Article views(2644) PDF downloads(130) Cited by(1)

Other Articles By Authors

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return

Catalog