introducing a wave function $W$ in the series, to replace the cosine function (itself a particular case). But we still keep $\lambda(n)=n$$\lambda(n)=\log n$. The goal is to show that RH can be generalized in a new way, different (I think) from the Generalized Riemann Hypothesis (GRH). The classic GRH involves L-functions while my version does not. This offers more hopes to solve Riemann's conjecture, by first trying to prove it for the easiest $W$, and understand what those $W$'s having a RH attached to them (as opposed to those that do not) have in common. In the three examples below, $\alpha=0, \beta=1$, while $\gamma=0$ for the $\phi_1$ series attached to the real part, and $\gamma=-\frac {\pi}{2}$ for the shifted $\phi_2$ series attached to the imaginary part. The classic RH corresponds to the cosine wave: $W(x)=\cos x$.
I added this note: Interestingly, when $\sigma=\frac{1}{2}$ the orbit does not have a hole anymore as predicted, yet the error points are still distributed on a similar ring.
Vincent Granville
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I added the section "more interesting results" featuring a generalization of RH very different from the current versions (not involving L-function), and spectacular plots for the orbit as well as the error when using only the first 200 terms in the series representing $\phi$
Vincent Granville
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I fixed an error in formula $(\star)$ in the appendix. The error did not have any impact on the final results, so the conclusions remain unchanged.
Vincent Granville
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Vincent Granville
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Added at the bottom: Appendix: simplified formula for $|\zeta(s)|^2$, when $\frac{1}{2}<\Re(s)<1$
Vincent Granville
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