Harmonic Entanglement Theory Paper (PDF)

Emergent Gravity

The entangleon, the holographic metric, the composite graviton with its ultraviolet cutoff, and Newton's constant from the Sakharov mechanism.

The emergent chain

HET derives gravitational physics in a chain:

bond oscillators \(\;\to\;\) continuum entangleon \(\phi\;\to\;\) composite graviton \(h_{\mu\nu}\;\to\;\) Newton's constant \(\;\to\;\) Newtonian force law.

Each step is taken explicitly. The bond is the harmonic oscillator of the previous section; the continuum field is its long-wavelength limit; the metric perturbation is its second-derivative composite; Newton's constant follows from the Sakharov mechanism on \(Q_3\times I\); the Newtonian force law is the long-wavelength projection of the linearised Einstein equation coupled to conserved stress-energy.

The continuum limit

In the long-wavelength limit the bond coordinate \(D_{\mathrm{KL}}\) is replaced by a continuum scalar field \(\phi(x)\) — the entangleon. Its action is the Klein–Gordon form

\[ \mathcal{S}[\phi] \;=\; \int\! d^{4}x\;\bigl( \tfrac12\partial_\mu\phi\,\partial^{\mu}\phi - \tfrac12 m_\phi^{2}\phi^{2}\bigr), \qquad m_\phi^{2} \;=\; \kappa_P\,m_P^{2} \;=\; 32\,m_P^{2}, \]

so \(m_\phi = 4\sqrt{2}\,m_P\). The factor \(\kappa_P = 32\) is the per-bond pinning constant set by the curvature of the Kubo–Mori potential at the vacuum on \(Q_3\).

Holographic derivation of the metric

The discrete Ryu–Takayanagi first law on a bond reads \(\delta D_{\mathrm{KL}} = \delta A_{\min}/4\ell_P^{2}\), tying bond entropy variations to extremal-surface areas in Planck units. In the continuum this becomes

\[ h_{\mu\nu}(x) \;=\; -\frac{\ell_P^{2}}{\log\chi}\, \partial_\mu\partial_\nu\langle\phi\rangle(x). \]

The metric perturbation is the second-derivative composite of the entangleon's expectation value. The factor \(1/\log\chi\) carries the Bekenstein–Hawking normalisation \(\log\chi = 1/4\) into the metric.

The graviton

The graviton is the spin-2 mode of \(h_{\mu\nu}\). Two-point function structure follows immediately from the composite definition: the graviton propagator is built from two entangleon propagators with two derivatives at each end,

\[ \langle h_{\mu\nu}(x)\,h_{\rho\sigma}(y)\rangle \;\sim\; \Bigl(\frac{\ell_P^{2}}{\log\chi}\Bigr)^{2} \partial_\mu\partial_\nu\partial_\rho\partial_\sigma\,G_\phi(x-y), \]

with \(G_\phi(k) = i/(k^{2} - m_\phi^{2})\). The four derivatives \(\to k_\mu k_\nu k_\rho k_\sigma\) and the entangleon propagator together give the spin-2 two-point function in the long-wavelength regime \(k^{2}\ll m_\phi^{2}\), and a natural ultraviolet cutoff at

\[ k_{\mathrm{UV}} \;=\; m_\phi \;=\; 4\sqrt{2}\,m_P. \]

Above \(k_{\mathrm{UV}}\) the entangleon resolves into the discrete bond degrees of freedom of \(Q_3\) and no continuum graviton exists. The composite-graviton structure, together with the bond discreteness as a physical ultraviolet regulator, is proposed to address the non-renormalisability of perturbative quantum gravity.

The hyperoctahedral \(B_3\) symmetry of \(Q_3\) selects the two-dimensional irreducible representation \(W_2\) on the 24-dimensional hinge space of the prism \(Q_3\times I\). The multiplicity of \(W_2\) is 3, so the spin-2 graviton mode lives on \(\dim W_2 \times m_{W_2} = 2\times 3 = 6\) — the six faces of \(Q_3\).

Newton's constant: the Sakharov derivation

Integrating out the entangleon on the prism \(Q_3\times I\) yields the Einstein–Hilbert action with a finite induced Newton's constant. With the bond oscillator's curvature \(\kappa_P\) and the bond ceiling \(\log\chi = 1/4\), the Sakharov mechanism gives

\[ G_N \;=\; \frac{1}{2\pi\log\chi} \;=\; \tfrac{2}{\pi}\,\ell_P^{2} \quad\text{at } \log\chi=\tfrac14, \]

equivalently \(G_N = \ell_P^{2}\) in Bekenstein–Hawking normalisation. The derivation is closed-form: no continuum loop integral needs to be regulated, since the cube provides its own short-distance structure.

Linearised Einstein equation and Newtonian limit

Coupled to a conserved stress-energy tensor \(T_{\mu\nu}\), the metric \(h_{\mu\nu}\) satisfies the linearised Einstein equation

\[ \Box h_{\mu\nu} \;-\;\partial_\mu\partial^{\alpha}h_{\alpha\nu} \;-\;\partial_\nu\partial^{\alpha}h_{\alpha\mu} \;+\;\partial_\mu\partial_\nu h \;-\;\eta_{\mu\nu}\bigl(\Box h - \partial^{\alpha}\partial^{\beta}h_{\alpha\beta}\bigr) \;=\; -16\pi G_N\,T_{\mu\nu}. \]

In the static, long-wavelength limit with \(T_{00} = \rho(x)\), the 00-component reduces to Poisson's equation \(\nabla^{2}\Phi = 4\pi G_N\rho\), recovering the Newtonian force law

\[ \mathbf{F} \;=\; -\frac{G_N M m}{r^{2}}\,\hat{\mathbf r}. \]

The chain from bond oscillator to Newtonian force is closed without free parameters beyond \(\log\chi = 1/4\), \(d = 3\), and \(\kappa_P = 32\).