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38 Chapter 1 PRIMES!<br />

conjectured. The famous conjecture of H. Cramér asserts that<br />

lim sup(pn+1<br />

− pn)/ ln<br />

n→∞<br />

2 n =1.<br />

A. Granville has raised some doubt on the value of this limsup, suggesting<br />

thatitmaybeasleastaslargeas2e −γ ≈ 1.123. For primes above 100, the<br />

largest known value of (pn+1 − pn)/ ln 2 n is ≈ 1.210 when pn = 113. The<br />

next highest known values of this quotient are ≈ 1.175 when pn = 1327, and<br />

≈ 1.138 when pn = 1693182318746371, this last being a recent discovery of<br />

B. Nyman.<br />

The prime gaps pn+1 − pn, which dramatically showcase the apparent<br />

local randomness of the primes, are on average ∼ ln n; this follows from the<br />

PNT (Theorem 1.1.4). The Cramér–Granville conjecture, mentioned in the<br />

last paragraph, implies that these gaps are infinitely often of magnitude ln 2 n,<br />

and no larger. However, the best that we can currently prove is that pn+1 −pn<br />

is infinitely often at least of magnitude<br />

ln n ln ln n ln ln ln ln n/(lnlnlnn) 2 ,<br />

an old result of P. Erdős and R. Rankin. We can also ask about the minimal<br />

order of pn+1−pn. The twin-prime conjecture implies that (pn+1−pn)/ ln n has<br />

liminf 0, but until very recently the best we knew was the result of H. Maier<br />

that the liminf is at most a constant that is slightly less than 1/4. As we go to<br />

press for this 2nd book edition, a spectacular new result has been announced<br />

by D. Goldston, J. Pintz, and C. Yildirim: Yes, the liminf of (pn+1 − pn)/ ln n<br />

is indeed 0.<br />

1.4.2 Computational successes<br />

The Riemann hypothesis (RH) remains open to this day. However, it became<br />

known after decades of technical development and a great deal of computer<br />

time that the first 1.5 billion zeros in the critical strip (ordered by increasing<br />

positive imaginary part) all lie precisely on the critical line Re(s) =1/2 [van<br />

de Lune et al. 1986]. It is highly intriguing—and such is possible due to a<br />

certain symmetry inherent in the zeta function—that one can numerically<br />

derive rigorous placement of the zeros with arithmetic of finite (yet perhaps<br />

high) precision. This is accomplished via rigorous counts of the number of<br />

zeros to various heights T (that is, the number of zeros σ + it with imaginary<br />

part t ∈ (0,T]), and then an investigation of sign changes of a certain real<br />

function that is zero if and only if zeta is zero on the critical line. If the sign<br />

changes match the count, all of the zeros to that height T are accounted for<br />

in rigorous fashion [Brent 1979].<br />

The current height to which Riemann-critical-zero computations have<br />

been pressed is that in [Gourdon and Sebah 2004], namely the RH is intact up<br />

to the 10 13 -th zero. Gourdon has also calculated 2 billion zeros near t =10 24 .<br />

This advanced work uses a variant of the parallel-zeta method of [Odlyzko<br />

and Schönhage 1988] discussed in Section 3.7.2. Another important pioneer

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