Difference between revisions of "Asymptotics of H t"

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(Riemann-Siegel formula)
(Riemann-Siegel formula)
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:<math>H_t(x+iy) = \frac{1}{8} ( F_{t,N}(\frac{1+ix+y}{2}) + \overline{F_{t,M}(\frac{1+ix-y}{2})} + R_{t,N,M}( \frac{1+ix+y}{2} ) ).</math>
 
:<math>H_t(x+iy) = \frac{1}{8} ( F_{t,N}(\frac{1+ix+y}{2}) + \overline{F_{t,M}(\frac{1+ix-y}{2})} + R_{t,N,M}( \frac{1+ix+y}{2} ) ).</math>
  
A good choice for <math>N,M</math> appears to be <math>N=M=\sqrt{x/4\pi}</math>.
+
A good choice for <math>N,M</math> appears to be <math>N=M=\lfloor \sqrt{x/4\pi}\rfloor</math>.
  
 
Now for asymptotics.  For <math>\lambda</math> in the first quadrant, one has
 
Now for asymptotics.  For <math>\lambda</math> in the first quadrant, one has
Line 207: Line 207:
 
To compute the integral, we make the change of variables <math>w = 2\pi i M + z</math> and note that
 
To compute the integral, we make the change of variables <math>w = 2\pi i M + z</math> and note that
 
:<math> w^{s-1} e^{-Nw} = (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( (s-1) \log(1 + \frac{z}{2\pi i M}) - N z)</math>
 
:<math> w^{s-1} e^{-Nw} = (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( (s-1) \log(1 + \frac{z}{2\pi i M}) - N z)</math>
:<math> \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( - \frac{i}{4\pi} z^2 )</math>
+
:<math> \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( - \frac{i}{4\pi} z^2 + \frac{s-2\pi i MN}{2\pi i M} z)</math>
 
so we expect
 
so we expect
:<math> \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \ dw \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN )  \int_C \frac{\exp( -\frac{i}{4\pi} z^2)}{e^z - 1}\ dz</math>
+
:<math> \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \ dw \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN )  \int_C \frac{\exp( -\frac{i}{4\pi} z^2 + \frac{s-2\pi i MN}{2\pi i M} z)}{e^z - 1}\ dz</math>
 
where <math>C</math> is a contour that goes counter-clockwise around the origin (as well as all the lower imaginary zeroes of <math>e^{z-1}</math>).
 
where <math>C</math> is a contour that goes counter-clockwise around the origin (as well as all the lower imaginary zeroes of <math>e^{z-1}</math>).

Revision as of 01:41, 5 February 2018

Asymptotics for [math]t=0[/math]

The approximate functional equation (see e.g. [T1986, (4.12.4)]) asserts that

[math]\displaystyle \zeta(s) = \sum_{n \leq N} \frac{1}{n^s} + \pi^{s-1/2} \frac{\Gamma((1-s)/2)}{\Gamma(s/2)} \sum_{n \leq N} \frac{1}{n^{1-s}} + O( t^{-\sigma/2} )[/math]

for [math]s = \sigma +it[/math] with [math]t[/math] large, [math]0 \lt \sigma \lt 1[/math], and [math]N := \sqrt{t/2\pi}[/math]. This implies that

[math]\displaystyle \xi(s) = F(s) + F(1-s) + O( \Gamma(\frac{s+4}{2}) t^{-\sigma/2} )[/math]

where

[math]\displaystyle F(s) := \frac{s(s-1)}{2} \pi^{-s/2} \Gamma(s/2) \sum_{n=1}^N \frac{1}{n^s}.[/math]

Writing

[math]\displaystyle \frac{s(s-1)}{2} \Gamma(s/2) = 2 \Gamma(\frac{s+4}{2}) - 3 \Gamma(\frac{s+2}{2})[/math]

we have [math]F(s) = 2 F_0(s) - 3 F_{-1}(s)[/math], where

[math]\displaystyle F_j(s) := \pi^{-s/2} \Gamma(\frac{s+4}{2} + j) \sum_{n=1}^N \frac{1}{n^s}.[/math]

The [math]F_{-1}[/math] term sums to [math]O( \Gamma(\frac{s+4}{2}) t^{-\sigma/2} )[/math], hence

[math]\displaystyle \xi(s) = 2F_0(s) + 2F_0(1-s) + O( \Gamma(\frac{s+4}{2}) t^{-\sigma/2} )[/math]

and thus

[math]\displaystyle H(x+iy) = \frac{1}{4} F_0( \frac{1+ix-y}{2} ) + \frac{1}{4} \overline{F_0( \frac{1+ix+y}{2} )} + O( \Gamma(\frac{9+ix+y}{2}) x^{-(1+y)/2} ).[/math]

One would expect the [math]\sum_{n=1}^N \frac{1}{n^s}[/math] term to remain more or less bounded (this is basically the Lindelof hypothesis), leading to the heuristics

[math]\displaystyle |F_0(\frac{1+ix \pm y}{2})| \asymp \Gamma(\frac{9+ix \pm y}{2}).[/math]

Since [math]\Gamma(\frac{9+ix - y}{2}) \approx \Gamma(\frac{9+ix+y}{2}) (ix)^{-y}[/math], we expect the [math]F_0( \frac{1+ix+y}{2} )[/math] term to dominate once [math]y \gg \frac{1}{\log x}[/math].

Asymptotics for [math]t \gt 0[/math]

Let [math]z=x+iy[/math] for large [math]x[/math] and positive bounded [math]y[/math]. We have

[math]\displaystyle H_t(z) = \frac{1}{2} \int_{-\infty}^\infty e^{tu^2} \Phi(u) \exp(izu)\ du[/math]

where

[math]\displaystyle \Phi(u) = \sum_{n=1}^\infty (2\pi^2 n^4 e^{9u} - 3\pi n^2 e^{5u}) \exp(-\pi n^2 e^{4u}).[/math]

We can shift contours to

[math]\displaystyle H_t(z) = \frac{1}{2} \int_{i\theta-\infty}^{i\theta+\infty} e^{tu^2} \Phi(u) \exp(izu)\ du[/math]

to any [math]-\pi/8 \lt \theta \lt \pi/8[/math] that we please; it seems that a good choice will be [math]\theta = \mathrm{arg} (ix+y+9) \approx \frac{\pi}{8} - \frac{y+9}{x}[/math]. By symmetry, we thus have

[math]\displaystyle H_t(z) = G_t(x+iy) + \overline{G_t(x-iy)}[/math]

where

[math]\displaystyle G_t(z) := \int_{i\theta}^{i\theta+\infty} e^{tu^2} \Phi(u) \exp(izu)\ du.[/math]

By Fubini's theorem we have

[math]\displaystyle G_{t}(x \pm i y) = \sum_{n=1}^\infty \pi^2 n^4 \int_{i\theta}^{i\theta+\infty} \exp( tu^2 - \pi n^2 e^{4u} + (ix \mp y + 9) u)\ du[/math]
[math] \displaystyle - \sum_{n=1}^\infty \frac{3}{2} \pi n^2 \int_{i\theta}^{i\theta+\infty} \exp( tu^2 - \pi n^2 e^{4u} + (ix \mp y + 5) u)\ du.[/math]

The second terms end up being about [math]O(1/x)[/math] the size of the first terms and we will ignore them for now. Making the change of variables [math]u = \frac{1}{4} \log \frac{ix \pm y + 9}{4\pi n^2} + v[/math], we basically have

[math] \displaystyle G_t(x \pm iy) \approx \sum_{n=1}^\infty \pi^2 n^4 (\frac{ix \pm y+9}{4\pi n^2})^{\frac{ix \mp y+9}{4}} \int_{-\frac{1}{4} \log \frac{|ix\pm y+9|}{4\pi n^2}}^\infty \exp( \frac{t}{16} (\log \frac{ix \pm y+9}{4\pi n^2} + v)^2 + (ix \mp y + 9) (v - \frac{1}{4} e^{4v}) )\ dv.[/math]

The function [math]\exp( (ix \mp y + 9) (v - \frac{1}{4} e^{4v}) )[/math] decays rapidly away from [math]v=0[/math]. This suggests firstly that this integral is going to be very small when [math]n \gg N := \sqrt{x/4\pi}[/math] (since the left limit of integration will then be to the right of the origin), so we will assume heuristically that [math]n[/math] is now restricted to the range [math]n \leq N[/math]. Next, we approximate [math]\exp( \frac{t}{16} (\log \frac{ix \pm y+9}{4\pi n^2} + v)^2)[/math] by [math]\exp( \frac{t}{16} \log^2 \frac{ix \pm y+9}{4\pi n^2} )[/math], and then send the left limit off to infinity to obtain (heuristically)

[math] \displaystyle G_t(x \pm iy) \approx \sum_{n \leq N} \pi^2 n^4 (\frac{ix \pm y+9}{4\pi n^2})^{\frac{ix \mp y+9}{4}} \exp( \frac{t}{16} \log^2 \frac{ix \pm y+9}{4\pi n^2} ) \int_{-\infty}^\infty \exp( (ix \mp y + 9) (v - \frac{1}{4} e^{4v}) )\ dv.[/math]

Making the change of variables [math]w := \frac{ix \mp y + 9}{4} e^{4v}[/math] we see that

[math]\int_{-\infty}^\infty \exp( (ix \mp y + 9) (v - \frac{1}{4} e^{4v}) )\ dv = \frac{1}{4} \Gamma(\frac{ix \mp y + 9}{4}) (\frac{4}{ix \mp y + 9})^{\frac{ix \mp y+9}{4}}[/math]

and thus

[math] \displaystyle G_t(x \pm iy) \approx \Gamma(\frac{ix \mp y + 9}{4}) \sum_{n \leq N} \frac{\pi^2}{4} n^4 (\frac{1}{\pi n^2})^{\frac{ix \mp y+9}{4}} \exp( \frac{t}{16} \log^2 \frac{ix \pm y+9}{4\pi n^2} ) [/math]

which simplifies a bit to

[math] \displaystyle G_t(x \pm iy) \approx \frac{1}{4} \pi^{-\frac{ix \mp y + 1}{4}} \Gamma(\frac{ix \mp y + 9}{4}) \sum_{n \leq N} \frac{\exp( \frac{t}{16} \log^2 \frac{ix \pm y+9}{4\pi n^2} )}{n^{\frac{1 \mp y + ix}{2}}} [/math]

and thus we heuristically have

[math] H_t(x+iy) \approx \frac{1}{4} F_t( \frac{1+ix-y}{2} ) + \frac{1}{4} \overline{F_t( \frac{1+ix+y}{2} )} [/math]

where

[math]F_t( s ) := \pi^{-s/2} \Gamma(\frac{s+4}{2}) \sum_{n \leq N} \frac{\exp( \frac{t}{16} \log^2 \frac{s+4}{2\pi n^2} )}{n^{s}}.[/math]

Here we can view [math]N[/math] as a function of [math]s[/math] by the formula [math]N = \mathrm{Im}(s)/2\pi[/math].

To understand these asymptotics better, let us inspect [math]H_t(x+iy)[/math] for [math]t\gt0[/math] in the region

[math]x+iy = T + \frac{a+ib}{\log T}; \quad t = \frac{\tau}{\log T}[/math]

with [math]T[/math] large, [math]a,b = O(1)[/math], and [math]\tau \gt \frac{1}{2}[/math]. If [math]s = \frac{1+ix-y}{2}[/math], then we can approximate

[math] \pi^{-s/2} \approx \pi^{-\frac{1+iT}{4}}[/math]
[math] \Gamma(\frac{s+4}{2}) \approx \Gamma(\frac{9+iT}{2}) T^{\frac{ia-b}{4 \log T}} = \exp( \frac{ia-b}{4} ) \Gamma(\frac{9+iT}{2}) [/math]
[math] \frac{1}{n^s} \approx \frac{1}{n^{\frac{1+iT}{2}}}[/math]
[math] \exp( \frac{t}{16} \log^2 \frac{s+4}{2\pi n^2} ) \approx \exp( \frac{t}{16} \log^2 \frac{s+4}{2\pi} - \frac{t}{4} \log T \log n )[/math]
[math] \approx \exp( \frac{\tau}{16} \log T + \frac{i \pi \tau}{16} ) \frac{1}{n^{\frac{\tau}{4}}} [/math]

leading to

[math] F_t(\frac{1+ix-y}{2}) \approx \pi^{-\frac{1+iT}{4}} \Gamma(\frac{9+iT}{2}) \exp( \frac{ia-b}{4} ) \exp( \frac{\tau}{16} \log T + \frac{i \pi \tau}{16} ) \sum_n \frac{1}{n^{\frac{1+iT}{2} + \frac{\tau}{4}}}[/math]
[math] \approx \pi^{-\frac{1+iT}{4}} \Gamma(\frac{9+iT}{2}) \zeta(\frac{1+iT}{2} + \frac{\tau}{4}) \exp( \frac{ia-b}{4} ).[/math]

Similarly for [math]F_t(\frac{1+ix+y}{2}) [/math] (replacing [math]b[/math] by [math]-b[/math]). If we make a polar coordinate representation

[math] \frac{1}{2} \pi^{-\frac{1+iT}{4}} \Gamma(\frac{9+iT}{2}) \zeta(\frac{1+iT}{2} + \frac{\tau}{4}) = r_{T,\tau} e^{i \theta_{T,\tau}}[/math]

one thus has

[math] H_t(x+iy) \approx \frac{1}{2} ( r_{T,\tau} e^{i \theta_{T,\tau}} \exp( \frac{ia-b}{4} ) + r_{T,\tau} e^{-i \theta_{T,\tau}} \exp(\frac{-ia+b}{4}) ) [/math]
[math] = r_{T,\tau} \cos( \frac{a+ib}{4} + \theta_{T,\tau} ).[/math]

Thus locally [math]H_t(x+iy)[/math] behaves like a trigonometric function, with zeroes real and equally spaced with spacing [math]4\pi[/math] (in [math]a[/math]-coordinates) or [math]\frac{4\pi}{\log T}[/math] (in [math]x[/math] coordinates). Once [math]\tau[/math] becomes large, further increase of [math]\tau[/math] basically only increases [math]r_{T,\tau}[/math] and also shifts [math]\theta_{T,\tau}[/math] at rate [math]\pi/16[/math], causing the number of zeroes to the left of [math]T[/math] to increase at rate [math]1/4[/math] as claimed in [KKL2009].

Riemann-Siegel formula

Proposition 1 (Riemann-Siegel formula) For any natural numbers [math]N,M[/math] and complex number [math]s[/math] that is not an integer, we have

[math]\zeta(s) = \sum_{n=1}^N \frac{1}{n^s} + \pi^{s-\frac{1}{2}} \frac{\Gamma((1-s)/2)}{\Gamma(s/2)} \sum_{m=1}^M \frac{1}{m^{1-s}} + \frac{e^{-i\pi s} \Gamma(1-s)}{2\pi i} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1}\ dw[/math]

where [math]w^{s-1} := \exp((s-1) \log w)[/math] and we use the branch of the logarithm with imaginary part in [math][0,2\pi)[/math], and [math]C_M[/math] is any contour from [math]+\infty[/math] to [math]+\infty[/math] going once anticlockwise around the zeroes [math]2\pi i m[/math] of [math]e^w-1[/math] with [math]|m| \leq M[/math], but does not go around any other zeroes.

Proof This equation is in [T1986, p. 82], but we give a proof here. The right-hand side is meromorphic in [math]s[/math], so it will suffice to establish that

  1. The right-hand side is independent of [math]N[/math];
  2. The right-hand side is independent of [math]M[/math];
  3. Whenever [math]\mathrm{Re}(s)\gt1[/math] and [math]s[/math] is not an integer, the right-hand side converges to [math]\zeta(s)[/math] if [math]M=0[/math] and [math]N \to \infty[/math].

We begin with the first claim. It suffices to show that the right-hand sides for [math]N[/math] and [math]N-1[/math] agree for every [math]N \gt 1[/math]. Subtracting, it suffices to show that

[math]0 = \frac{1}{N^s} + \frac{e^{-i\pi s} \Gamma(1-s)}{2\pi i} \int_{C_M} \frac{w^{s-1} (e^{-Nw} - e^{-(N-1)w}}{e^w-1}\ dw.[/math]

The integrand here simplifies to [math]- w^{s-1} e^{-Nw}[/math], which on shrinking [math]C_M[/math] to wrap around the positive real axis becomes [math]N^{-s} \Gamma(s) (1 - e^{2\pi i(s-1)})[/math]. The claim then follows from the Euler reflection formula [math]\Gamma(s) \Gamma(1-s) = \frac{\pi}{\sin(\pi s)}[/math].

Now we verify the second claim. It suffices to show that the right-hand sides for [math]M[/math] and [math]M-1[/math] agree for every [math]M \gt 1[/math]. Subtracting, it suffices to show that

[math]0 = \pi^{s-\frac{1}{2}} \frac{\Gamma((1-s)/2)}{\Gamma(s/2)} \frac{1}{M^{1-s}} + \frac{e^{-i\pi s} \Gamma(1-s)}{2\pi i} \int_{C_M - C_{M-1}} \frac{w^{s-1} e^{-Nw}}{e^w-1}\ dw.[/math]

The contour [math]C_M - C_{M-1}[/math] encloses the simple poles at [math]+2\pi i M[/math] and [math]-2\pi i M[/math], which have residues of [math](2\pi i M)^{s-1} = - i (2\pi M)^{s-1} e^{\pi i s/2}[/math] and [math](-2\pi i M)^{s-1} = i (2\pi M)^{s-1} e^{3\pi i s/2}[/math] respectively. So, on canceling the factor of [math]M^{s-1}[/math] it suffices to show that

[math]0 = \pi^{s-\frac{1}{2}} \frac{\Gamma((1-s)/2)}{\Gamma(s/2)} + e^{-i\pi s} \Gamma(1-s) (2\pi)^{s-1} i (e^{3\pi i s/2} - e^{\pi i s/2}).[/math]

But this follows from the duplication formula [math]\Gamma(1-s) = \frac{\Gamma(\frac{1-s}{2}) \Gamma(1-\frac{s}{2})}{\pi^{1/2} 2^s}[/math] and the Euler reflection formula [math]\Gamma(\frac{s}{2}) \Gamma(1-\frac{s}{2}) = \frac{\pi}{\sin(\pi s/2)}[/math].

Finally we verify the third claim. Since [math]\zeta(s) = \lim_{N \to \infty} \sum_{n=1}^\infty \frac{1}{n^s}[/math], it suffices to show that

[math]\lim_{N \to \infty} \int_{C_0} \frac{w^{s-1} e^{-Nw}}{e^w-1}\ dw = 0.[/math]

We take [math]C_0[/math] to be a contour that traverses a [math]1/N[/math]-neighbourhood of the real axis. Writing [math]C_0 = \frac{1}{N} C'_0[/math], with [math]C'_0[/math] independent of [math]N[/math], we can thus write the left-hand side as

[math]\lim_{N \to \infty} N^{-s} \int_{C'_0} \frac{w^{s-1} e^{-w}}{e^{w/N}-1}\ dw,[/math]

and the claim follows from the dominated convergence theorem. [math]\Box[/math]

Applying the Riemann-Siegel formula to the Riemann xi function [math]\xi(s) = \frac{s(s-1)}{2} \pi^{-s/2} \Gamma(s/2) \zeta(s)[/math], we have

[math]\xi(s) = F_{0,N}(s) + \overline{F_{0,M}(\overline{1-s})} + R_{0,N,M}(s)[/math]

where

[math]F_{0,N}(s) := \frac{s(s-1)}{2} \pi^{-s/2} \Gamma(s/2) \sum_{n=1}^N \frac{1}{n^s}[/math]

and

[math]R_{0,N,M}(s) := \frac{s(s-1)}{2} \pi^{-s/2} \Gamma(s/2) \frac{e^{-i\pi s} \Gamma(1-s)}{2\pi i} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1}\ dw.[/math]

In preparation for applying the heat equation, we now write [math]F_{0,N}(s)[/math] and [math]R_{0,N,M}(s)[/math] as Fourier-Laplace transforms for [math]s[/math] in the first quadrant. Firstly we have

[math]\frac{s(s-1)}{2} \Gamma(s/2) = 2 \Gamma(\frac{s+4}{2}) - 3 \Gamma(\frac{s+2}{2})[/math]

so that

[math]F_{0,N}(s) = \sum_{n=1}^N 2 \Gamma(\frac{s+4}{2}) (\pi n^2)^{-s/2} - 3 \Gamma(\frac{s+2}{2}) (\pi n^2)^{-s/2}.[/math]

Since (by a change of variables [math]x=e^u[/math]) we have

[math]\Gamma(z) = \int_0^\infty x^{s} e^{-x}\ \frac{dx}{x} = \int_{-\infty}^\infty \exp( su - e^u )\ du \quad (1)[/math]

we thus have

[math]F_{0,N}(s) = \sum_{n=1}^N 2 \int_{-\infty}^\infty \exp( \frac{s+4}{2} u - e^u - \frac{s}{2} \log \pi n^2 )\ du - 3 \int_{-\infty}^\infty \exp( \frac{s+2}{2} u - e^u - \frac{s}{2} \log \pi n^2 )\ du.[/math]

We can shift the [math]u[/math] contour to a contour [math]\Gamma[/math] that starts at [math]i\infty[/math] and ends at [math]+\infty[/math], staying within a bounded distance of the lower imaginary and right real axes. One should think of the first summand as the main term and the second one as a lower order term (about [math]O(1/|s|)[/math] smaller in practice). In [math]s[/math] coordinates, the backwards heat equation becomes

[math]\partial_t F_{0,N}(s) = \frac{1}{4} \partial_{ss} F_{0,N}(s)[/math]

and so the evolution becomes

[math]F_{t,N}(s) = \sum_{n=1}^N 2 \int_{\Gamma} \exp( \frac{s+4}{2} u - e^u - \frac{s}{2} \log \pi n^2 + \frac{t}{16} (u - \log \pi n^2)^2 )\ du - 3 \int_{\Gamma} \exp( \frac{s+2}{2} u - e^u - \frac{s}{2} \log \pi n^2 \frac{t}{16} (u - \log \pi n^2)^2 )\ du.[/math]

Note that because we shifted contours to [math]\Gamma[/math], the integrand here remains absolutely integrable. If we shift the first variable of integration by [math]\log \frac{s+4}{2}[/math] and the second by [math]\log \frac{s+2}{2}[/math], we obtain

[math]F_{t,N}(s) = 2 \sum_{n=1}^N \frac{\exp( \frac{s+4}{2} \log \frac{s+4}{2} - \frac{s+4}{2})}{(\pi n^2)^{s/2}} \int_\Gamma \exp( \frac{s+4}{2} (1 + u - e^u) + \frac{t}{16} (u + \log \frac{s+4}{2\pi n^2})^2 )\ du[/math]
[math] - 3 \sum_{n=1}^N \frac{\exp( \frac{s+2}{2} \log \frac{s+2}{2} - \frac{s+2}{2})}{(\pi n^2)^{s/2}} \int_\Gamma \exp( \frac{s+2}{2} (1 + u - e^u) + \frac{t}{16} (u + \log \frac{s+2}{2\pi n^2})^2 )\ du.[/math]

Now we manipulate [math]R_{0,N,M}(s)[/math]. Firstly, from the duplication formula [math]\Gamma(1-s) = \frac{\Gamma(\frac{1-s}{2}) \Gamma(1-\frac{s}{2})}{\pi^{1/2} 2^s}[/math] and the Euler reflection formula [math]\Gamma(\frac{s}{2}) \Gamma(1-\frac{s}{2}) = \frac{\pi}{\sin(\pi s/2)}[/math] we have

[math] \Gamma(s/2) \Gamma(1-s) = \frac{\pi^{1/2}}{2^s \sin(\pi s/2)} \Gamma(\frac{1-s}{2})[/math]

and thus

[math]R_{0,N,M}(s) = \frac{s(s-1)}{2} \frac{\pi^{(1-s)/2}}{2^s \sin(\pi s/2)} \Gamma(\frac{1-s}{2}) \frac{e^{-i\pi s}}{2\pi i} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1}\ dw.[/math]

Next, we have

[math]\frac{s(s-1)}{2} \Gamma(\frac{1-s}{2}) = 2 \Gamma(\frac{5-s}{2}) - 3 \Gamma(\frac{3-s}{2})[/math]

and hence by (1)

[math]R_{0,N,M}(s) = 2 \frac{\pi^{(1-s)/2}}{2^s \sin(\pi s/2)} \frac{e^{-i\pi s}}{2\pi i} \int_{-\infty}^\infty \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{5-s}{2} u - e^u ) \ dw du[/math]
[math] - 3 \frac{\pi^{(1-s)/2}}{2^s \sin(\pi s/2)} \frac{e^{-i\pi s}}{2\pi i} \int_{-\infty}^\infty \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{3-s}{2} u - e^u ) \ dw du.[/math]

We can shift the [math]u[/math] contour to a contour [math]\overline{\Gamma}[/math] that starts at [math]-i\infty[/math] and ends at [math]+\infty[/math], staying within a bounded distance of the lower imaginary and right real axes. Next, from the geometric series formula one has

[math] \frac{1}{\sin(\pi s/2)} = -2i e^{i\pi s/2} \sum_{n=0}^\infty e^{\pi i n s}[/math]

and hence

[math]R_{0,N,M}(s) = - 2 \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \int_{\overline{\Gamma}} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{5-s}{2} u - e^u ) \ dw du[/math]
[math] + 3 \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \int_{\overline{\Gamma}} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{3-s}{2} u - e^u ) \ dw du.[/math]

We can then evolve by the heat flow to obtain

[math]R_{t,N,M}(s) = - 2 \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \int_\Gamma \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{5-s}{2} u - e^u + \frac{t}{16} (-u + \pi i (2n-1) + \log \frac{w}{4\pi})^2 ) \ dw du[/math]
[math] + 3 \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \int_{\overline{\Gamma}} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{3-s}{2} u - e^u + \frac{t}{16} (-u + \pi i (2n-1) + \log \frac{w}{4\pi})^2 ) ) \ dw du,[/math]

noting that the integrals here are absolutely convergent for [math]t \gt 0[/math]. We now have the exact formula

[math]H_t(x+iy) = \frac{1}{8} ( F_{t,N}(\frac{1+ix+y}{2}) + \overline{F_{t,M}(\frac{1+ix-y}{2})} + R_{t,N,M}( \frac{1+ix+y}{2} ) ).[/math]

A good choice for [math]N,M[/math] appears to be [math]N=M=\lfloor \sqrt{x/4\pi}\rfloor[/math].

Now for asymptotics. For [math]\lambda[/math] in the first quadrant, one has

[math] \int_\Gamma \exp( \lambda( 1+u-e^u) )\ du = \exp( \lambda - \lambda \log \lambda ) \Gamma(\lambda) [/math]

and then on integrating by parts

[math] \int_\Gamma \exp( \lambda( 1+u-e^u) ) (1 - e^u)\ du = 0[/math]

and

[math] \int_\Gamma \exp( \lambda( 1+u-e^u) ) u (1 - e^u)\ du = -\frac{1}{\lambda} \exp( \lambda - \lambda \log \lambda ) \Gamma(\lambda).[/math]

This suggests the stationary phase asymptotic

[math] \int_\Gamma \exp( \lambda( 1+u-e^u) ) f(u) = \exp( \lambda - \lambda \log \lambda ) \Gamma(\lambda) (f(0) + \frac{f''(0) - f'(0)}{2 \lambda} + O( \|f\|/\lambda^2) )[/math]

for reasonable functions [math]f[/math], with a reasonable norm [math]\|f\|[/math]. This suggests

[math]F_{t,N}(s) \approx 2 \sum_{n=1}^N \frac{\Gamma( \frac{s+4}{2} )}{(\pi n^2)^{s/2}} \exp( \frac{t}{16} \log^2 \frac{s+4}{2\pi n^2} ) (1 + (\frac{t}{16} + \frac{t^2}{128} \log^2 \frac{s+4}{2\pi n^2} - \frac{t}{16} \log \frac{s+4}{2\pi n^2} ) \frac{2}{s+4} )[/math]
[math]- 3 \sum_{n=1}^N \frac{\Gamma( \frac{s+2}{2} )}{(\pi n^2)^{s/2}} \exp( \frac{t}{16} \log^2 \frac{s+2}{2\pi n^2} ).[/math]

Now we heuristically estimate [math]R_{t,N,M}(s) [/math] term to top order. We discard the second term as being lower order. The critical point for [math]u[/math] is [math]u = \log \frac{5-s}{2}[/math], so we approximate [math]\frac{t}{16} (-u + \pi i (2n-1) + \log \frac{w}{4\pi})^2 )[/math] by [math]\frac{t}{16} (\pi i (2n-1) + \log \frac{w}{2\pi(5-s)})^2 )[/math] and arrive at

[math]R_{t,N,M}(s) \approx - 2 \Gamma(\frac{5-s}{2}) \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \exp( \frac{t}{16} (\pi i (2n-1) + \log \frac{w}{2\pi(5-s)})^2 ) \ dw.[/math]

The critical point of [math]w^s e^{-Nw}[/math] occurs at [math]w = \frac{s}{N}[/math]. Approximating [math]\log \frac{w}{2\pi(5-s)}[/math] by [math]\log \frac{s}{2\pi N (5-s)}[/math], we thus have

[math]R_{t,N,M}(s) \approx - 2 \Gamma(\frac{5-s}{2}) \frac{\pi^{(-s-1)/2}}{2^s} \sum_{n=0}^\infty e^{\pi i (n-\frac{1}{2})s} \exp( \frac{t}{16} (\pi i (2n-1) + \log \frac{s}{2\pi N(5-s)})^2 ) \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \ dw.[/math]

The [math]n=0[/math] term should dominate quite strongly, thus

[math]R_{t,N,M}(s) \approx - 2 \Gamma(\frac{5-s}{2}) \frac{\pi^{(-s-1)/2}}{2^s} e^{-\pi i s/2} \exp( \frac{t}{16} (-\pi i + \log \frac{s}{2\pi N(5-s)})^2 ) \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \ dw.[/math]

To compute the integral, we make the change of variables [math]w = 2\pi i M + z[/math] and note that

[math] w^{s-1} e^{-Nw} = (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( (s-1) \log(1 + \frac{z}{2\pi i M}) - N z)[/math]
[math] \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \exp( - \frac{i}{4\pi} z^2 + \frac{s-2\pi i MN}{2\pi i M} z)[/math]

so we expect

[math] \int_{C_M} \frac{w^{s-1} e^{-Nw}}{e^w-1} \ dw \approx (2\pi i M)^{s-1} \exp( - 2\pi i MN ) \int_C \frac{\exp( -\frac{i}{4\pi} z^2 + \frac{s-2\pi i MN}{2\pi i M} z)}{e^z - 1}\ dz[/math]

where [math]C[/math] is a contour that goes counter-clockwise around the origin (as well as all the lower imaginary zeroes of [math]e^{z-1}[/math]).