This not a proof of the Riemann Hypothesis (RH). Its purpose is to explore a simple idea: that horizons supply a natural quantum clock.
This idea does not turn the zeros into energy levels. It gives them a different physical meaning: they are horizon times.
A Horizon That Stretches Light
Let $V>0$ be an affine coordinate along a horizon light ray, and let $\kappa>0$ be the surface gravity. Horizon time acts as
$$V(t)=e^{\kappa t}V.$$
A wavefunction $\psi(V)\in L^2(\mathbb R_+ dV)$ has norm $\int_0^\infty |\psi(V)|^2 dV$. Probability conservation requires
$$(U_t\psi)(V) = e^{-\kappa t/2}\psi(e^{-\kappa t}V).$$
Writing $U_t=e^{-i\widehat Ht/\hbar}$ gives
$$\widehat H = -i\hbar\kappa \left( V\frac{d}{dV}+\frac12 \right).$$
The factor $1/2$ is the Jacobian term required by unitarity.
Introduce logarithmic horizon position,
$$q=\ln(V/V_0), \qquad \chi(q)=\sqrt V \psi(V).$$
Since $dV=V dq$,
$$\int_0^\infty |\psi(V)|^2 dV = \int_{-\infty}^{\infty}|\chi(q)|^2 dq $$
In this coordinate,
$$\widehat H = -i\hbar\kappa\frac{d}{dq}$$
and $\chi(q,t)=\chi(q-\kappa t,0)$. Exponential stretching in $V$ has become ordinary translation in $q$.
The generalized eigenmodes are
$$\langle V|\lambda\rangle = \frac{1}{\sqrt{2\pi}} V^{-1/2} \exp\left( i\lambda\ln\frac{V}{V_0} \right),$$
with energies $E_\lambda=\hbar\kappa\lambda$. The horizon spectrum is continuous.
Preparing the Riemann State
Define
$$\xi(s) = \frac12s(s-1)\pi^{-s/2} \Gamma\left(\frac{s}{2}\right)\zeta(s),$$
and $\Xi(u) = \xi\left(\frac12+iu\right)$. For real $u$,
$$\Xi(u) = \int_{-\infty}^{\infty} \Phi(\lambda)e^{-iu\lambda} d\lambda,$$
where $\Phi$ is real, even, positive and rapidly decreasing. Therefore
$$p_\Xi(\lambda) = \frac{\Phi(\lambda)}{\Xi(0)}$$
is a normalised probability density: $\int_{-\infty}^{\infty}p_\Xi(\lambda) d\lambda=1$.
Prepare the state
$$|\Omega_\Xi\rangle = \int_{-\infty}^{\infty} \sqrt{p_\Xi(\lambda)} |\lambda\rangle d\lambda.$$
The square root is essential: $p_\Xi(\lambda)$ is the probability density, while $\sqrt{p_\Xi(\lambda)}$ is the quantum amplitude.
The Zeros Become Times
Each mode evolves as $|\lambda\rangle \longmapsto e^{-i\kappa t\lambda}|\lambda\rangle$. Therefore
$$\mathcal A(t) = \langle\Omega_\Xi| e^{-i\widehat Ht/\hbar} |\Omega_\Xi\rangle = \int_{-\infty}^{\infty} p_\Xi(\lambda)e^{-i\kappa t\lambda} d\lambda = \frac{\Xi(\kappa t)}{\Xi(0)}.$$
If $\gamma_n$ is a real zero of $\Xi$, then $\mathcal A\left(\gamma_n/\kappa\right)=0$. Thus the state becomes orthogonal to its initial state at
$$\boxed{\kappa t_n=\gamma_n.}$$
In logarithmic position space, define
$$\chi_\Xi(q) = \frac{1}{\sqrt{2\pi}} \int_{-\infty}^{\infty} \sqrt{p_\Xi(\lambda)} e^{i\lambda q} d\lambda.$$
Then
$$\mathcal A(t) = \int_{-\infty}^{\infty} \chi_\Xi^*(q) \chi_\Xi(q-\kappa t) dq$$
The zeros are displacements at which the logarithmic horizon wavepacket becomes orthogonal to its translated copy.
Complex Horizon Time and the Riemann Hypothesis
Because $\Phi$ decreases rapidly, the amplitude has an entire continuation:
$$\mathcal A_{\mathbb C}(t) = \frac{ \xi\left(\frac12+i\kappa t\right) }{ \xi\left(\frac12\right) }, \qquad t\in\mathbb C.$$
Let $\rho=\beta+i\gamma$ be a nontrivial zero of $\zeta$. The corresponding amplitude zero satisfies $\frac12+i\kappa t_\rho=\rho$. Hence
$$\boxed{ \kappa t_\rho = \gamma-i\left(\beta-\frac12\right). }$$
Therefore $\operatorname{Re}(\kappa t_\rho)=\gamma$ and $\operatorname{Im}(\kappa t_\rho)=\frac12-\beta$. It follows that
$$\operatorname{Im}t_\rho=0 \quad\Longleftrightarrow\quad \beta=\frac12.$$
Thus
$$\boxed{ \mathrm{RH} \quad\Longleftrightarrow\quad \text{every zero of }\mathcal A_{\mathbb C}(t) \text{ occurs at real Lorentzian time}. }$$
A critical-line zero is a physical orthogonality event. An off-line zero would occur only at complex time, where the amplitude is an analytic continuation rather than a unitary overlap.
Since nontrivial zeros satisfy $0<\beta<1$, the critical strip becomes
$$\left|\operatorname{Im}t\right| < \frac{1}{2\kappa}.$$
The Riemann Hypothesis says that every amplitude zero in this strip lies on its real-time centre.
The de Sitter Horizon
Nothing above requires a black-hole singularity. It uses only stationary horizon dilation.
For de Sitter space,
$$ds^2 = -\left(1-H_{\mathrm{dS}}^2r^2\right)dt^2 + \frac{dr^2}{1-H_{\mathrm{dS}}^2r^2} + r^2d\Omega^2,$$
the cosmological horizon lies at $r_c=H_{\mathrm{dS}}^{-1}$, with surface gravity $\kappa=H_{\mathrm{dS}}$. Therefore
$$\mathcal A_{\mathrm{dS}}(t) = \frac{\Xi(H_{\mathrm{dS}}t)}{\Xi(0)},$$
and $t_n^{\mathrm{dS}} = \gamma_n/H_{\mathrm{dS}}$. The universal variable is dimensionless horizon time, $\tau=\kappa t$. For a thermal horizon, $k_BT_H=\hbar\kappa/(2\pi)$, so
$$\frac{k_BT_Ht_\rho}{\hbar} = \frac{\gamma}{2\pi} - \frac{i}{2\pi} \left(\beta-\frac12\right).$$
What is new with this idea?
Spectral proposals impose boundary conditions that discretise a dilation Hamiltonian and interpret the Riemann zeros as energy levels. Here the dilation spectrum remains continuous. The arithmetic information is encoded instead in one state's spectral density. This differs from the boundary-condition construction in Black Holes, Quantum Chaos, and the Riemann Hypothesis.
Other quantum constructions produce zeta-related Loschmidt amplitudes through engineered states, spectra and interactions. Here the horizon supplies the translation generator directly.
Thus
$$\boxed{ \text{critical-line Riemann zero} \quad\longleftrightarrow\quad \text{horizon orthogonality time}. }$$
More fully,
$$\boxed{ \mathrm{RH} \quad\Longleftrightarrow\quad \text{all zeros of the continued horizon coherence lie on the unitary-time axis}. }$$
What This Does Not Explain
The horizon supplies the dilation dynamics, but the special state supplies the arithmetic content. Our framework does not explain why gravity would prepare
$$p_\Xi(\lambda) = \frac{\Phi(\lambda)}{\Xi(0)}.$$
It simply proves what follows if that state is prepared. It does not prove the Riemann Hypothesis, and complex time is not directly observable.
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