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<art>
   <ui>1029-242X-2010-215416</ui>
   <ji>1029-242X</ji>
   <fm>
      <dochead>Research Article</dochead>
      <bibl>
         <title>
            <p>Applications of Wirtinger Inequalities on the Distribution of Zeros of the Riemann Zeta-Function</p>
         </title>
         <aug>
            <au ca="yes" id="A1"><snm>Saker</snm><fnm>SamirH</fnm><insr iid="I1"/><insr iid="I2"/><email>shsaker@mans.edu.eg</email></au>
         </aug>
         <insg>
            <ins id="I1"><p>Department of Mathematics, King Saud University, Riyadh 11451, Saudi Arabia</p></ins>
            <ins id="I2"><p>Department of Mathematics, Mansoura University, Mansoura 35516, Egypt</p></ins>
         </insg>
         <source>Journal of Inequalities and Applications</source>
         <issn>1029-242X</issn>
         <pubdate>2010</pubdate>
         <volume>2010</volume>
         <issue>1</issue>
         <fpage>215416</fpage>
         <url>http://www.journalofinequalitiesandapplications.com/content/2010/1/215416</url>
         <xrefbib><pubid idtype="doi">10.1155/2010/215416</pubid></xrefbib>
      </bibl>
      <history><rec><date><day>10</day><month>10</month><year>2010</year></date></rec><acc><date><day>17</day><month>12</month><year>2010</year></date></acc><pub><date><day>4</day><month>1</month><year>2011</year></date></pub></history>
      <cpyrt><year>2010</year><collab>Samir H. Saker.</collab><note>This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</note></cpyrt>
      <abs>
         <sec>
            <st>
               <p/>
            </st>
            <p>On the hypothesis that the <inline-formula><graphic file="1029-242X-2010-215416-i1.gif"/></inline-formula>th moments of the Hardy <inline-formula><graphic file="1029-242X-2010-215416-i2.gif"/></inline-formula>-function are correctly predicted by random matrix theory and the moments of the derivative of <inline-formula><graphic file="1029-242X-2010-215416-i3.gif"/></inline-formula> are correctly predicted by the derivative of the characteristic polynomials of unitary matrices, we establish new large spaces between the zeros of the Riemann zeta-function by employing some Wirtinger-type inequalities. In particular, it is obtained that <inline-formula><graphic file="1029-242X-2010-215416-i4.gif"/></inline-formula> which means that consecutive nontrivial zeros often differ by at least 6.1392 times the average spacing.</p>
         </sec>
      </abs>
   </fm>
   <bdy>
      <sec>
         <st>
            <p>1. Introduction</p>
         </st>
         <p>The Riemann zeta-function is defined by </p>
         <p>
            <display-formula id="M11">
               <graphic file="1029-242X-2010-215416-i5.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>and by analytic continuation elsewhere except for a simple pole at <inline-formula><graphic file="1029-242X-2010-215416-i6.gif"/></inline-formula>. The identity between the Dirichlet series and the Euler product (taken over all prime numbers <inline-formula><graphic file="1029-242X-2010-215416-i7.gif"/></inline-formula> ) is an analytic version of the unique prime factorization in the ring of integers and reflects the importance of the zeta-function for number theory. The functional equation</p>
         <p>
            <display-formula id="M12">
               <graphic file="1029-242X-2010-215416-i8.gif"/>
            </display-formula>
         </p>
         <p>implies the existence of so-called trivial zeros of <inline-formula><graphic file="1029-242X-2010-215416-i9.gif"/></inline-formula> at <inline-formula><graphic file="1029-242X-2010-215416-i10.gif"/></inline-formula> for any positive integer <inline-formula><graphic file="1029-242X-2010-215416-i11.gif"/></inline-formula>; all other zeros are said to be nontrivial and lie inside the so-called critical strip <inline-formula><graphic file="1029-242X-2010-215416-i12.gif"/></inline-formula>. The number <inline-formula><graphic file="1029-242X-2010-215416-i13.gif"/></inline-formula> of nontrivial zeros of <inline-formula><graphic file="1029-242X-2010-215416-i14.gif"/></inline-formula> with ordinates in the interval <inline-formula><graphic file="1029-242X-2010-215416-i15.gif"/></inline-formula>,<inline-formula><graphic file="1029-242X-2010-215416-i16.gif"/></inline-formula> is asymptotically given by the Riemann-von Mangoldt formula (see [<abbr bid="B1">1</abbr>]) </p>
         <p>
            <display-formula id="M13">
               <graphic file="1029-242X-2010-215416-i17.gif"/>
            </display-formula>
         </p>
         <p>Consequently, the frequency of their appearance is increasing and the distances between their ordinates is tending to zero as <inline-formula><graphic file="1029-242X-2010-215416-i18.gif"/></inline-formula>.</p>
         <p>The Riemann zeta-function is one of the most studied transcendental functions, having in view its many applications in number theory, algebra, complex analysis, and statistics as well as in physics. Another reason why this function has drawn so much attention is the celebrated Riemann conjecture regarding nontrivial zeros which states that all nontrivial zeros of the Riemann zeta-function <inline-formula><graphic file="1029-242X-2010-215416-i19.gif"/></inline-formula> lie on the critical line <inline-formula><graphic file="1029-242X-2010-215416-i20.gif"/></inline-formula>. The distribution of zeros of <inline-formula><graphic file="1029-242X-2010-215416-i21.gif"/></inline-formula> is of great importance in number theory. In fact any progress in the study of the distribution of zeros of this function helps to investigate the magnitude of the largest gap between consecutive primes below a given bound. Clearly, there are no zeros in the half plane of convergence <inline-formula><graphic file="1029-242X-2010-215416-i22.gif"/></inline-formula>, and it is also known that <inline-formula><graphic file="1029-242X-2010-215416-i23.gif"/></inline-formula> does not vanish on the line <inline-formula><graphic file="1029-242X-2010-215416-i24.gif"/></inline-formula>. In the negative half plane, <inline-formula><graphic file="1029-242X-2010-215416-i25.gif"/></inline-formula> and its derivative are oscillatory and from the functional equation there exist so-called trivial (real) zeros at <inline-formula><graphic file="1029-242X-2010-215416-i26.gif"/></inline-formula> for any positive integer <inline-formula><graphic file="1029-242X-2010-215416-i27.gif"/></inline-formula> (corresponding to the poles of the appearing Gamma-factors), and all nontrivial (nonreal) zeros are distributed symmetrically with respect to the critical line <inline-formula><graphic file="1029-242X-2010-215416-i28.gif"/></inline-formula> and the real axis.</p>
         <p>There are three directions regarding the studies of the zeros of the Riemann zeta-function. The first direction is concerned with the existence of simple zeros. It is conjectured that all or at least almost all zeros of the zeta-function are simple. For this direction, we refer to the papers by Conrey [<abbr bid="B2">2</abbr>] and Cheer and Goldston [<abbr bid="B3">3</abbr>].</p>
         <p>The second direction is the most important goal of number theorists which is the determination of the moments of the Riemann zeta-function on the critical line. It is important because it can be used to estimate the maximal order of the zeta-function on the critical line, and because of its applicability in studying the distribution of prime numbers and divisor problems. For more details of the second direction, we refer the reader to the papers in [<abbr bid="B4">4</abbr>&#8211;<abbr bid="B6">6</abbr>] and the references cited therein. For further classical results from zeta-function theory, we refer to the monograph [<abbr bid="B7">7</abbr>] of Ivi&#263; and the papers by Kim [<abbr bid="B8">8</abbr>&#8211;<abbr bid="B11">11</abbr>].</p>
         <p>For completeness in the following we give a brief summary of some of these results in this direction that we will use in the proof of the main results. It is known that the behavior of <inline-formula><graphic file="1029-242X-2010-215416-i29.gif"/></inline-formula> on the critical line is reflected by the Hardy <inline-formula><graphic file="1029-242X-2010-215416-i30.gif"/></inline-formula>-function <inline-formula><graphic file="1029-242X-2010-215416-i31.gif"/></inline-formula> as a function of a real variable, defined by</p>
         <p>
            <display-formula id="M14">
               <graphic file="1029-242X-2010-215416-i32.gif"/>
            </display-formula>
         </p>
         <p>It follows from the functional equation (1.2) that <inline-formula><graphic file="1029-242X-2010-215416-i33.gif"/></inline-formula> is an infinitely often differentiable function which is real for real <inline-formula><graphic file="1029-242X-2010-215416-i34.gif"/></inline-formula> and moreover <inline-formula><graphic file="1029-242X-2010-215416-i35.gif"/></inline-formula>. Consequently, the zeros of <inline-formula><graphic file="1029-242X-2010-215416-i36.gif"/></inline-formula> correspond to the zeros of the Riemann zeta-function on the critical line. An important problem in analytic number theory is to gain an understanding of the moments of the Hardy <inline-formula><graphic file="1029-242X-2010-215416-i37.gif"/></inline-formula>-function <inline-formula><graphic file="1029-242X-2010-215416-i38.gif"/></inline-formula> function <inline-formula><graphic file="1029-242X-2010-215416-i39.gif"/></inline-formula> and the moments of its derivative <inline-formula><graphic file="1029-242X-2010-215416-i40.gif"/></inline-formula> which are defined by </p>
         <p>
            <display-formula id="M15">
               <graphic file="1029-242X-2010-215416-i41.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>For positive real numbers <inline-formula><graphic file="1029-242X-2010-215416-i42.gif"/></inline-formula>, it is believed that </p>
         <p>
            <display-formula id="M16">
               <graphic file="1029-242X-2010-215416-i43.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>for positive constants <inline-formula><graphic file="1029-242X-2010-215416-i44.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i45.gif"/></inline-formula> will be defined later.</p>
         <p>Keating and Snaith [<abbr bid="B12">12</abbr>] based on considerations from random matrix theory conjectured that </p>
         <p>
            <display-formula id="M17">
               <graphic file="1029-242X-2010-215416-i46.gif"/>
            </display-formula>
         </p>
         <p>where</p>
         <p>
            <display-formula id="M18">
               <graphic file="1029-242X-2010-215416-i47.gif"/>
            </display-formula>
         </p>
         <p>where <inline-formula><graphic file="1029-242X-2010-215416-i48.gif"/></inline-formula> is the Barnes <inline-formula><graphic file="1029-242X-2010-215416-i49.gif"/></inline-formula>-function (for the definition of the Barnes <inline-formula><graphic file="1029-242X-2010-215416-i50.gif"/></inline-formula>-function and its properties, we refer to [<abbr bid="B5">5</abbr>]).</p>
         <p>Hughes [<abbr bid="B5">5</abbr>] used the Random Matrix Theory (RMT) and stated an interesting conjecture on the moments of the Hardy <inline-formula><graphic file="1029-242X-2010-215416-i51.gif"/></inline-formula>-function and its derivatives at its zeros subject to the truth of Riemann's hypothesis when the zeros are simple. This conjecture includes for fixed <inline-formula><graphic file="1029-242X-2010-215416-i52.gif"/></inline-formula> the asymptotic formula of the moments of the form</p>
         <p>
            <display-formula id="M19">
               <graphic file="1029-242X-2010-215416-i53.gif"/>
            </display-formula>
         </p>
         <p>where <inline-formula><graphic file="1029-242X-2010-215416-i54.gif"/></inline-formula> is defined as in (1.8) and the product is over the primes. Hughes [<abbr bid="B5">5</abbr>] was able to establish the explicit formula</p>
         <p>
            <display-formula id="M110">
               <graphic file="1029-242X-2010-215416-i55.gif"/>
            </display-formula>
         </p>
         <p>in the range <inline-formula><graphic file="1029-242X-2010-215416-i56.gif"/></inline-formula>, where <inline-formula><graphic file="1029-242X-2010-215416-i57.gif"/></inline-formula> is an explicit rational function of <inline-formula><graphic file="1029-242X-2010-215416-i58.gif"/></inline-formula> for each fixed <inline-formula><graphic file="1029-242X-2010-215416-i59.gif"/></inline-formula>. The functions <inline-formula><graphic file="1029-242X-2010-215416-i60.gif"/></inline-formula> as introduced by Hughes [<abbr bid="B5">5</abbr>] are given in the following: </p>
         <p>
            <display-formula id="M111">
               <graphic file="1029-242X-2010-215416-i61.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>where <inline-formula><graphic file="1029-242X-2010-215416-i62.gif"/></inline-formula>, This sequence is continuous, and it is believed that both the nominator and denominator are monic polynomials in <inline-formula><graphic file="1029-242X-2010-215416-i63.gif"/></inline-formula>. Using (1.10) and the definitions of the functions <inline-formula><graphic file="1029-242X-2010-215416-i64.gif"/></inline-formula>, we can obtain the values of <inline-formula><graphic file="1029-242X-2010-215416-i65.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i66.gif"/></inline-formula>. As indicated in [<abbr bid="B13">13</abbr>] Hughes [<abbr bid="B5">5</abbr>] evaluated the first four functions and then writes a numerical experiment suggesting the next three. The values of <inline-formula><graphic file="1029-242X-2010-215416-i67.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i68.gif"/></inline-formula> have been collected in [<abbr bid="B6">6</abbr>]. To the best of my knowledge there is no explicit formula to find the values of the function <inline-formula><graphic file="1029-242X-2010-215416-i69.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i70.gif"/></inline-formula>. This limitation of the values of <inline-formula><graphic file="1029-242X-2010-215416-i71.gif"/></inline-formula> leads to the limitation of the values of the lower bound between the zeros of the Riemann zeta-function by applying the moments (1.9). To overcame this restriction, we will use a different explicit formula of the moments to establish new values of the distance between zeros.</p>
         <p>Conrey et al. [<abbr bid="B4">4</abbr>] established the moments of the derivative, on the unit circle, of characteristic polynomials of random unitary matrices and used this to formulate a conjecture for the moments of the derivative of the Riemann zeta-function on the critical line. Their method depends on the fact that the distribution of the eigenvalues of unitary matrices gives insight into the distribution of zeros of the Riemann zeta-function and the values of the characteristic polynomials of the unitary matrices give a model for the value distribution of the Riemann zeta-function. Their formulae are expressed in terms of a determinant of a matrix whose entries involve the <inline-formula><graphic file="1029-242X-2010-215416-i72.gif"/></inline-formula>-Bessel function and, alternately, by a combinatorial sum. They conjectured that</p>
         <p>
            <display-formula id="M112">
               <graphic file="1029-242X-2010-215416-i73.gif"/>
            </display-formula>
         </p>
         <p>where <inline-formula><graphic file="1029-242X-2010-215416-i74.gif"/></inline-formula> is the arithmetic factor and defined as in (1.8) and </p>
         <p>
            <display-formula id="M113">
               <graphic file="1029-242X-2010-215416-i75.gif"/>
            </display-formula>
         </p>
         <p>where </p>
         <p>
            <display-formula id="M114">
               <graphic file="1029-242X-2010-215416-i76.gif"/>
            </display-formula>
         </p>
         <p>and <inline-formula><graphic file="1029-242X-2010-215416-i77.gif"/></inline-formula> denotes the set of partitions <inline-formula><graphic file="1029-242X-2010-215416-i78.gif"/></inline-formula> of <inline-formula><graphic file="1029-242X-2010-215416-i79.gif"/></inline-formula> into nonnegative parts. They also gave some explicit values of <inline-formula><graphic file="1029-242X-2010-215416-i80.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i81.gif"/></inline-formula>. These values will be presented in Section 2 and will be used to establish the main results in this paper.</p>
         <p>The third direction in the studies of the zeros of the Riemann zeta-function is the gaps between the zeros (finding small gaps and large gaps between the zeros) on the critical line when the Riemann hypothesis is satisfied. In the present paper we are concerned with the largest gaps between the zeros on the critical line assuming that the Riemann hypothesis is true.</p>
         <p>Assuming the truth of the Riemann hypothesis Montgomery [<abbr bid="B14">14</abbr>] studied the distribution of pairs of nontrivial zeros <inline-formula><graphic file="1029-242X-2010-215416-i82.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i83.gif"/></inline-formula> and conjectured, for fixed <it>&#945;</it>,<inline-formula><graphic file="1029-242X-2010-215416-i84.gif"/></inline-formula> satisfying <inline-formula><graphic file="1029-242X-2010-215416-i85.gif"/></inline-formula>, that </p>
         <p>
            <display-formula id="M115">
               <graphic file="1029-242X-2010-215416-i86.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>This so-called pair correlation conjecture plays a complementary role to the Riemann hypothesis. This conjecture implies the essential simplicity hypothesis that almost all zeros of the zeta-function are simple. On the other hand, the integral on the right hand side is the same as the one observed in the two-point correlation of the eigenvalues which are the energy levels of the corresponding Hamiltonian which are usually not known with uncertainty. This observation is due to Dyson and it restored some hope in an old idea of Hilbert and Polya that the Riemann hypothesis follows from the existence of a self-adjoint Hermitian operator whose spectrum of eigenvalues correspond to the set of nontrivial zeros of the zeta-function.</p>
         <p>Now, we assume that <inline-formula><graphic file="1029-242X-2010-215416-i87.gif"/></inline-formula> are the zeros of <inline-formula><graphic file="1029-242X-2010-215416-i88.gif"/></inline-formula> in the upper half-plane (arranged in nondecreasing order and counted according multiplicity) and <inline-formula><graphic file="1029-242X-2010-215416-i89.gif"/></inline-formula> are consecutive ordinates of all zeros and define</p>
         <p>
            <display-formula id="M116">
               <graphic file="1029-242X-2010-215416-i90.gif"/>
            </display-formula>
         </p>
         <p>and set </p>
         <p>
            <display-formula id="M117">
               <graphic file="1029-242X-2010-215416-i91.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>These numbers have received a great deal of attention. In fact, important results concerning the values of them have been obtained by some authors. It is generally believed that <inline-formula><graphic file="1029-242X-2010-215416-i92.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i93.gif"/></inline-formula>. Selberg [<abbr bid="B15">15</abbr>] proved that</p>
         <p>
            <display-formula id="M118">
               <graphic file="1029-242X-2010-215416-i94.gif"/>
            </display-formula>
         </p>
         <p>and the average of <inline-formula><graphic file="1029-242X-2010-215416-i95.gif"/></inline-formula> is 1. Note that <inline-formula><graphic file="1029-242X-2010-215416-i96.gif"/></inline-formula> is the average spacing between zeros. Fujii [<abbr bid="B16">16</abbr>] also showed that there exist constants <inline-formula><graphic file="1029-242X-2010-215416-i97.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i98.gif"/></inline-formula> such that </p>
         <p>
            <display-formula id="M119">
               <graphic file="1029-242X-2010-215416-i99.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>for a positive proportion of <inline-formula><graphic file="1029-242X-2010-215416-i100.gif"/></inline-formula>. Mueller [<abbr bid="B17">17</abbr>] obtained</p>
         <p>
            <display-formula id="M120">
               <graphic file="1029-242X-2010-215416-i101.gif"/>
            </display-formula>
         </p>
         <p>assuming the Riemann hypothesis. Montgomery and Odlyzko [<abbr bid="B18">18</abbr>] showed, assuming the Riemann hypothesis, that</p>
         <p>
            <display-formula id="M121">
               <graphic file="1029-242X-2010-215416-i102.gif"/>
            </display-formula>
         </p>
         <p>Conrey et al. [<abbr bid="B19">19</abbr>] improved the bounds in (1.21) and showed that, if the Riemann hypothesis is true, then </p>
         <p>
            <display-formula id="M122">
               <graphic file="1029-242X-2010-215416-i103.gif"/>
            </display-formula>
         </p>
         <p>Conrey et al. [<abbr bid="B20">20</abbr>] obtained a new lower bound and proved that</p>
         <p>
            <display-formula id="M123">
               <graphic file="1029-242X-2010-215416-i104.gif"/>
            </display-formula>
         </p>
         <p>assuming the generalized Riemann hypothesis for the zeros of the Dirichlet <inline-formula><graphic file="1029-242X-2010-215416-i105.gif"/></inline-formula>-functions. Bui et al. [<abbr bid="B21">21</abbr>] improved (1.23) and obtained</p>
         <p>
            <display-formula id="M124">
               <graphic file="1029-242X-2010-215416-i106.gif"/>
            </display-formula>
         </p>
         <p>assuming the Riemann hypothesis. Ng in [<abbr bid="B22">22</abbr>] improved (1.24) and proved that</p>
         <p>
            <display-formula id="M125">
               <graphic file="1029-242X-2010-215416-i107.gif"/>
            </display-formula>
         </p>
         <p>assuming the generalized Riemann hypothesis for the zeros of the Dirichlet <inline-formula><graphic file="1029-242X-2010-215416-i108.gif"/></inline-formula>-functions.</p>
         <p>Hall in [<abbr bid="B23">23</abbr>] (see also Hall [<abbr bid="B24">24</abbr>]) assumed that <inline-formula><graphic file="1029-242X-2010-215416-i109.gif"/></inline-formula> is the sequence of distinct positive zeros of the Riemann zeta-function <inline-formula><graphic file="1029-242X-2010-215416-i110.gif"/></inline-formula> arranged in nondecreasing order and counted according multiplicity and defined the quantity </p>
         <p>
            <display-formula id="M126">
               <graphic file="1029-242X-2010-215416-i111.gif"/>
            </display-formula>
         </p>
         <p>and showed that <inline-formula><graphic file="1029-242X-2010-215416-i112.gif"/></inline-formula>, and the lower bound for <inline-formula><graphic file="1029-242X-2010-215416-i113.gif"/></inline-formula> bear direct comparison with such bounds for <inline-formula><graphic file="1029-242X-2010-215416-i114.gif"/></inline-formula> dependent on the Riemann hypothesis, since if this were true the distinction between <inline-formula><graphic file="1029-242X-2010-215416-i115.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i116.gif"/></inline-formula> would be nugatory. Of course <inline-formula><graphic file="1029-242X-2010-215416-i117.gif"/></inline-formula> and the equality holds if the Riemann hypothesis is true. Hall [<abbr bid="B23">23</abbr>] used a Wirtinger-type inequality of Beesack and proved that</p>
         <p>
            <display-formula id="M127">
               <graphic file="1029-242X-2010-215416-i118.gif"/>
            </display-formula>
         </p>
         <p>In [<abbr bid="B25">25</abbr>] Hall proved a Wirtinger inequality and used the moment </p>
         <p>
            <display-formula id="M128">
               <graphic file="1029-242X-2010-215416-i119.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>due to Ingham [<abbr bid="B26">26</abbr>], and the moments</p>
         <p>
            <display-formula id="M129">
               <graphic file="1029-242X-2010-215416-i120.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>due to Conrey [<abbr bid="B27">27</abbr>], and obtained</p>
         <p>
            <display-formula id="M130">
               <graphic file="1029-242X-2010-215416-i121.gif"/>
            </display-formula>
         </p>
         <p>Hall [<abbr bid="B24">24</abbr>] proved a new generalized Wirtinger-type inequality by using the calculus of variation and obtained a new value of <inline-formula><graphic file="1029-242X-2010-215416-i122.gif"/></inline-formula> which is given by</p>
         <p>
            <display-formula id="M131">
               <graphic file="1029-242X-2010-215416-i123.gif"/>
            </display-formula>
         </p>
         <p>Hall [<abbr bid="B28">28</abbr>] employed the generalized Wirtinger inequality obtained in [<abbr bid="B24">24</abbr>], simplified the calculus used in [<abbr bid="B24">24</abbr>] and converted the problem into one of the classical theory of equations involving Jacobi-Schur functions. Assuming that the moments in (1.9) are correctly predicted by RMT, Hall [<abbr bid="B28">28</abbr>] proved that </p>
         <p>
            <display-formula id="M132">
               <graphic file="1029-242X-2010-215416-i124.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>In [<abbr bid="B29">29</abbr>] the authors applied a technique involving the comparison of the continuous global average with local average obtained from the discrete average to a problem of gaps between the zeros of zeta-function assuming the Riemann hypothesis. Using this approach, which takes only zeros on the critical line into account, the authors computed similar bounds under assumption of the Riemann hypothesis when (1.9) holds. They then showed that for fixed positive integer <inline-formula><graphic file="1029-242X-2010-215416-i125.gif"/></inline-formula></p>
         <p>
            <display-formula id="M133">
               <graphic file="1029-242X-2010-215416-i126.gif"/>
            </display-formula>
         </p>
         <p>holds for any <inline-formula><graphic file="1029-242X-2010-215416-i127.gif"/></inline-formula> for more than <inline-formula><graphic file="1029-242X-2010-215416-i128.gif"/></inline-formula> proportion of the zeros <inline-formula><graphic file="1029-242X-2010-215416-i129.gif"/></inline-formula> with a computable constant <inline-formula><graphic file="1029-242X-2010-215416-i130.gif"/></inline-formula>.</p>
         <p>Hall [<abbr bid="B13">13</abbr>] developed the technique used in [<abbr bid="B28">28</abbr>] and proved that</p>
         <p>
            <display-formula id="M134">
               <graphic file="1029-242X-2010-215416-i131.gif"/>
            </display-formula>
         </p>
         <p>The improvement of this value as obtained in [<abbr bid="B13">13</abbr>] is given by</p>
         <p>
            <display-formula id="M135">
               <graphic file="1029-242X-2010-215416-i132.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>In this paper, first we apply some well-known Wirtinger-type inequalities and the moments of the Hardy <inline-formula><graphic file="1029-242X-2010-215416-i133.gif"/></inline-formula>-function and the moments of its derivative to establish some explicit formulas for <inline-formula><graphic file="1029-242X-2010-215416-i134.gif"/></inline-formula>. Using the values of <inline-formula><graphic file="1029-242X-2010-215416-i135.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i136.gif"/></inline-formula>, we establish some lower bounds for <inline-formula><graphic file="1029-242X-2010-215416-i137.gif"/></inline-formula> which improves the last value of <inline-formula><graphic file="1029-242X-2010-215416-i138.gif"/></inline-formula>. In particular it is obtained that <inline-formula><graphic file="1029-242X-2010-215416-i139.gif"/></inline-formula> which means that consecutive nontrivial zeros often differ by at least 6.1392 times the average spacing. To the best of the author knowledge the last value obtained for <inline-formula><graphic file="1029-242X-2010-215416-i140.gif"/></inline-formula> in the literature is the value obtained by Hall in (1.35) and nothing is known regarding <inline-formula><graphic file="1029-242X-2010-215416-i141.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i142.gif"/></inline-formula>.</p>
      </sec>
      <sec>
         <st>
            <p>2. Main Results</p>
         </st>
         <p>In this section, we establish some explicit formulas for <inline-formula><graphic file="1029-242X-2010-215416-i143.gif"/></inline-formula> and by using the same explicit values of <inline-formula><graphic file="1029-242X-2010-215416-i144.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i145.gif"/></inline-formula> we establish new lower bounds for <inline-formula><graphic file="1029-242X-2010-215416-i146.gif"/></inline-formula>. The explicit values of <inline-formula><graphic file="1029-242X-2010-215416-i147.gif"/></inline-formula> using the formula </p>
         <p>
            <display-formula id="M21">
               <graphic file="1029-242X-2010-215416-i148.gif"/>
            </display-formula>
         </p>
         <p>are calculated in the following for <inline-formula><graphic file="1029-242X-2010-215416-i149.gif"/></inline-formula>:</p>
         <p>
            <display-formula id="M22">
               <graphic file="1029-242X-2010-215416-i150.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>The explicit values of the parameter <inline-formula><graphic file="1029-242X-2010-215416-i151.gif"/></inline-formula> that has been determined by Conrey et al. [<abbr bid="B4">4</abbr>] for <inline-formula><graphic file="1029-242X-2010-215416-i152.gif"/></inline-formula> are given in the following: </p>
         <p>
            <display-formula id="M23">
               <graphic file="1029-242X-2010-215416-i153.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>Now, we are in a position to prove our first results in this section which gives an explicit formula of the gaps between the zeros of the Riemann zeta-function. This will be proved by applying an inequality due to Agarwal and Pang [<abbr bid="B30">30</abbr>].</p>
         <p>Theorem 2.1. </p>
         <p>Assuming the Riemann hypothesis, one has </p>
         <p>
            <display-formula id="M24">
               <graphic file="1029-242X-2010-215416-i154.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>Proof. </p>
         <p>To prove this theorem, we employ the inequality </p>
         <p>
            <display-formula id="M25">
               <graphic file="1029-242X-2010-215416-i155.gif"/>
            </display-formula>
         </p>
         <p>with <inline-formula><graphic file="1029-242X-2010-215416-i156.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i157.gif"/></inline-formula>, that has been proved by Agarwal and Pang [<abbr bid="B30">30</abbr>]. As in [<abbr bid="B25">25</abbr>] by a suitable linear transformation, we can deduce from (2.5) that if <inline-formula><graphic file="1029-242X-2010-215416-i158.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i159.gif"/></inline-formula>, then </p>
         <p>
            <display-formula id="M26">
               <graphic file="1029-242X-2010-215416-i160.gif"/>
            </display-formula>
         </p>
         <p>Now, we follow the proof of [<abbr bid="B24">24</abbr>] and supposing that <inline-formula><graphic file="1029-242X-2010-215416-i161.gif"/></inline-formula> is the first zero of <inline-formula><graphic file="1029-242X-2010-215416-i162.gif"/></inline-formula> not less than <inline-formula><graphic file="1029-242X-2010-215416-i163.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i164.gif"/></inline-formula> the last zero not greater than <inline-formula><graphic file="1029-242X-2010-215416-i165.gif"/></inline-formula>. Suppose further that for <inline-formula><graphic file="1029-242X-2010-215416-i166.gif"/></inline-formula>, we have </p>
         <p>
            <display-formula id="M27">
               <graphic file="1029-242X-2010-215416-i167.gif"/>
            </display-formula>
         </p>
         <p>and apply the inequality (2.6), to obtain </p>
         <p>
            <display-formula id="M28">
               <graphic file="1029-242X-2010-215416-i168.gif"/>
            </display-formula>
         </p>
         <p>Since the inequality remains true if we replace <inline-formula><graphic file="1029-242X-2010-215416-i169.gif"/></inline-formula> by <inline-formula><graphic file="1029-242X-2010-215416-i170.gif"/></inline-formula>, we have </p>
         <p>
            <display-formula id="M29">
               <graphic file="1029-242X-2010-215416-i171.gif"/>
            </display-formula>
         </p>
         <p>Summing (2.9) over <inline-formula><graphic file="1029-242X-2010-215416-i172.gif"/></inline-formula>, applying (1.7), (1.12) and as in [<abbr bid="B24">24</abbr>], we obtain </p>
         <p>
            <display-formula id="M210">
               <graphic file="1029-242X-2010-215416-i173.gif"/>
            </display-formula>
         </p>
         <p>whence </p>
         <p>
            <display-formula id="M211">
               <graphic file="1029-242X-2010-215416-i174.gif"/>
            </display-formula>
         </p>
         <p>This implies that </p>
         <p>
            <display-formula id="M212">
               <graphic file="1029-242X-2010-215416-i175.gif"/>
            </display-formula>
         </p>
         <p>and then we obtain the desired inequality (2.1). The proof is complete.</p>
         <p>Using the values of <inline-formula><graphic file="1029-242X-2010-215416-i176.gif"/></inline-formula> and <inline-formula><graphic file="1029-242X-2010-215416-i177.gif"/></inline-formula> and (2.1) we have the new lower values for <inline-formula><graphic file="1029-242X-2010-215416-i178.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i179.gif"/></inline-formula> in Table <tblr tid="T1">1</tblr>.</p>
         <tbl id="T1"><title><p>Table 1</p></title><tblbdy cols="5">
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i180.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i181.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i182.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i183.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i184.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>1.2442</p>
         </c>
         <c ca="center">
            <p>1.7675</p>
         </c>
         <c ca="center">
            <p>2.2265</p>
         </c>
         <c ca="center">
            <p>2.6544</p>
         </c>
         <c ca="center">
            <p>3.0545</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i185.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i186.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i187.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i188.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i189.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>3.4259</p>
         </c>
         <c ca="center">
            <p>3.7676</p>
         </c>
         <c ca="center">
            <p>4.0806</p>
         </c>
         <c ca="center">
            <p>4.3681</p>
         </c>
         <c ca="center">
            <p>4.6342</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i190.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i191.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i192.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i193.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i194.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>4.8827</p>
         </c>
         <c ca="center">
            <p>5.1169</p>
         </c>
         <c ca="center">
            <p>5.3393</p>
         </c>
         <c ca="center">
            <p>5.5515</p>
         </c>
         <c ca="center">
            <p>5.7550</p>
         </c>
      </r>
   </tblbdy></tbl>
         <p>One can easily see that the value of <inline-formula><graphic file="1029-242X-2010-215416-i195.gif"/></inline-formula> in Table <tblr tid="T1">1</tblr> does not improve the lower bound in (1.35) due to Hall, but the the approach that we used is simple and depends only on a well-known Wirtinger-type inequality and the asymptotic formulas of the moments. In the following, we employ a different inequality due to Brneti&#263; and Pe&#269;ari&#263; [<abbr bid="B31">31</abbr>] and establish a new explicit formula for <inline-formula><graphic file="1029-242X-2010-215416-i196.gif"/></inline-formula> and then use it to find new lower bounds.</p>
         <p>Theorem 2.2. </p>
         <p>Assuming the Riemann hypothesis, one has </p>
         <p>
            <display-formula id="M213">
               <graphic file="1029-242X-2010-215416-i197.gif"/>
            </display-formula>
         </p>
         <p>where <inline-formula><graphic file="1029-242X-2010-215416-i198.gif"/></inline-formula> is defined by </p>
         <p>
            <display-formula id="M214">
               <graphic file="1029-242X-2010-215416-i199.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>Proof. </p>
         <p>To prove this theorem, we apply the inequality </p>
         <p>
            <display-formula id="M215">
               <graphic file="1029-242X-2010-215416-i200.gif"/>
            </display-formula>
         </p>
         <p>that has been proved by Brneti&#263; and Pe&#269;ari&#263; [<abbr bid="B31">31</abbr>], where <inline-formula><graphic file="1029-242X-2010-215416-i201.gif"/></inline-formula> is continuous function on <inline-formula><graphic file="1029-242X-2010-215416-i202.gif"/></inline-formula> with <inline-formula><graphic file="1029-242X-2010-215416-i203.gif"/></inline-formula>. Proceeding as in the proof of Theorem 2.1 and employing (2.15), we may have </p>
         <p>
            <display-formula id="M216">
               <graphic file="1029-242X-2010-215416-i204.gif"/>
            </display-formula>
         </p>
         <p>This implies that </p>
         <p>
            <display-formula id="M217">
               <graphic file="1029-242X-2010-215416-i205.gif"/>
            </display-formula>
         </p>
         <p>which is the desired inequality (2.13). The proof is complete.</p>
         <p>To find the new lower bounds for <inline-formula><graphic file="1029-242X-2010-215416-i206.gif"/></inline-formula> we need the values of <inline-formula><graphic file="1029-242X-2010-215416-i207.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i208.gif"/></inline-formula>. These values are calculated numerically in Table <tblr tid="T2">2</tblr>.</p>
         <tbl id="T2"><title><p>Table 2</p></title><tblbdy cols="5">
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i209.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i210.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i211.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i212.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i213.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i214.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i215.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i216.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i217.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i218.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i219.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i220.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i221.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i222.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i223.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i224.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i225.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i226.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i227.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i228.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i229.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i230.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i231.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i232.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i233.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i234.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i235.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i236.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i237.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i238.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
   </tblbdy></tbl>
         <p>Using these values and the values of <inline-formula><graphic file="1029-242X-2010-215416-i239.gif"/></inline-formula>,<inline-formula><graphic file="1029-242X-2010-215416-i240.gif"/></inline-formula>, and the explicit formula (2.13) we have the new lower bounds for <inline-formula><graphic file="1029-242X-2010-215416-i241.gif"/></inline-formula> in Table <tblr tid="T3">3</tblr>.</p>
         <tbl id="T3"><title><p>Table 3</p></title><tblbdy cols="5">
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i242.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i243.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i244.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i245.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i246.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>1.3505</p>
         </c>
         <c ca="center">
            <p>1.9902</p>
         </c>
         <c ca="center">
            <p>2.4905</p>
         </c>
         <c ca="center">
            <p>2.9389</p>
         </c>
         <c ca="center">
            <p>3.3508</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i247.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i248.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i249.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i250.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i251.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>3.7287</p>
         </c>
         <c ca="center">
            <p>4.0736</p>
         </c>
         <c ca="center">
            <p>4.3875</p>
         </c>
         <c ca="center">
            <p>4.6742</p>
         </c>
         <c ca="center">
            <p>4.9384</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i252.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i253.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i254.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i255.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i256.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>5.1845</p>
         </c>
         <c ca="center">
            <p>5.4159</p>
         </c>
         <c ca="center">
            <p>5.6353</p>
         </c>
         <c ca="center">
            <p>5.8444</p>
         </c>
         <c ca="center">
            <p>6.0449</p>
         </c>
      </r>
   </tblbdy></tbl>
         <p>We note from Table <tblr tid="T3">3</tblr> that the value of <inline-formula><graphic file="1029-242X-2010-215416-i257.gif"/></inline-formula> improves the value <inline-formula><graphic file="1029-242X-2010-215416-i258.gif"/></inline-formula> that has been obtained by Hall.</p>
         <p>Finally, in the following we will employ an inequality to Beesack [<abbr bid="B32">32</abbr>, page 59] and establish a new explicit formula for <inline-formula><graphic file="1029-242X-2010-215416-i259.gif"/></inline-formula> and use it to find new values of its lower bounds.</p>
         <p>Theorem 2.3. </p>
         <p>Assuming the Riemann hypothesis, one has </p>
         <p>
            <display-formula id="M218">
               <graphic file="1029-242X-2010-215416-i260.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>Proof. </p>
         <p>To prove this theorem, we apply the inequality </p>
         <p>
            <display-formula id="M219">
               <graphic file="1029-242X-2010-215416-i261.gif"/>
            </display-formula>
         </p>
         <p>that has been proved by Beesack [<abbr bid="B32">32</abbr>, page 59], where <inline-formula><graphic file="1029-242X-2010-215416-i262.gif"/></inline-formula> is continuous function on <inline-formula><graphic file="1029-242X-2010-215416-i263.gif"/></inline-formula> with <inline-formula><graphic file="1029-242X-2010-215416-i264.gif"/></inline-formula>. Proceeding as in Theorem 2.1 by using (2.19), we may have </p>
         <p>
            <display-formula id="M220">
               <graphic file="1029-242X-2010-215416-i265.gif"/>
            </display-formula>
         </p>
         <p>This implies that </p>
         <p>
            <display-formula id="M221">
               <graphic file="1029-242X-2010-215416-i266.gif"/>
            </display-formula>
         </p>
         <p>which is the desired inequity (2.18). The proof is complete.</p>
         <p>Using these values and the values of <inline-formula><graphic file="1029-242X-2010-215416-i267.gif"/></inline-formula>,<inline-formula><graphic file="1029-242X-2010-215416-i268.gif"/></inline-formula>, and the explicit formula in (2.18) we have the new lower bounds for <inline-formula><graphic file="1029-242X-2010-215416-i269.gif"/></inline-formula> in Table <tblr tid="T4">4</tblr>.</p>
         <tbl id="T4"><title><p>Table 4</p></title><tblbdy cols="5">
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i270.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i271.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i272.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i273.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i274.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>1.7321</p>
         </c>
         <c ca="center">
            <p>2.2635</p>
         </c>
         <c ca="center">
            <p>2.7080</p>
         </c>
         <c ca="center">
            <p>3.1257</p>
         </c>
         <c ca="center">
            <p>3.5177</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i275.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i276.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i277.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i278.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i279.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>3.8814</p>
         </c>
         <c ca="center">
            <p>4.215</p>
         </c>
         <c ca="center">
            <p>4.5196</p>
         </c>
         <c ca="center">
            <p>4.7985</p>
         </c>
         <c ca="center">
            <p>5.0560</p>
         </c>
      </r>
      <r>
         <c ca="center" cspan="5">
            <p/>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i280.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i281.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i282.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i283.gif"/>
               </inline-formula>
            </p>
         </c>
         <c ca="center">
            <p>
               <inline-formula>
                  <graphic file="1029-242X-2010-215416-i284.gif"/>
               </inline-formula>
            </p>
         </c>
      </r>
      <r>
         <c ca="left">
            <p>5.2962</p>
         </c>
         <c ca="center">
            <p>5.5225</p>
         </c>
         <c ca="center">
            <p>5.7373</p>
         </c>
         <c ca="center">
            <p>5.9424</p>
         </c>
         <c ca="center">
            <p>6.1392</p>
         </c>
      </r>
   </tblbdy></tbl>
         <p>We note from Table <tblr tid="T4">4</tblr>, that the values of <inline-formula><graphic file="1029-242X-2010-215416-i285.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i286.gif"/></inline-formula> are compatible with the values of <inline-formula><graphic file="1029-242X-2010-215416-i287.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i288.gif"/></inline-formula> that has been obtained by Hall [<abbr bid="B13">13</abbr>, Table <inline-formula><graphic file="1029-242X-2010-215416-i289.gif"/></inline-formula>] and since there is no explicit value of <inline-formula><graphic file="1029-242X-2010-215416-i290.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i291.gif"/></inline-formula>, to obtain the values of <inline-formula><graphic file="1029-242X-2010-215416-i292.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i293.gif"/></inline-formula> the author in [<abbr bid="B13">13</abbr>] stopped the estimation for <inline-formula><graphic file="1029-242X-2010-215416-i294.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i295.gif"/></inline-formula>. </p>
         <p>We notice that the calculations can be continued as above just if one knows the explicit values of <inline-formula><graphic file="1029-242X-2010-215416-i296.gif"/></inline-formula> for <inline-formula><graphic file="1029-242X-2010-215416-i297.gif"/></inline-formula> where the values </p>
         <p>
            <display-formula id="M222">
               <graphic file="1029-242X-2010-215416-i298.gif"/>
            </display-formula>
         </p>
         <p/>
         <p>are easy to calculate. Note that the values of <inline-formula><graphic file="1029-242X-2010-215416-i299.gif"/></inline-formula> that we have used in this paper are adapted from the paper by Conrey et al. [<abbr bid="B4">4</abbr>]. It is clear that the values of <inline-formula><graphic file="1029-242X-2010-215416-i300.gif"/></inline-formula> are increasing with the increase of <inline-formula><graphic file="1029-242X-2010-215416-i301.gif"/></inline-formula> and this may help in proving the conjecture of the distance between of the zeros of the Riemann zeta-function.</p>
      </sec>
   </bdy>
   <bm>
      <ack>
         <sec>
            <st>
               <p>Acknowledgments</p>
            </st>
            <p>The author is very grateful to the anonymous referees for valuable remarks and comments which significantly contributed to the quality of the paper. The author thanks Deanship of Scientific Research and the Research Centre in College of Science in King Saud University for encouragements and supporting this project.</p>
         </sec>
      </ack>
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