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Fractal-Layered Holographic Cosmology: A Testable Framework for Hubble Tension, CMB Anomalies, and Early Structure Formation

31 Juli 2025   12:02 Diperbarui: 31 Juli 2025   12:02 337
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Inovasi. Sumber ilustrasi: PEXELS/Jcomp

The universe is partitioned into quasi-independent topological layers or "bubbles," each governed by slightly different local curvature, expansion rate, and phase,

These layers emerge from quantum tunneling genesis, generating non-smooth transitions between adjacent domains,

Each layer has its own metric g(i)g^{(i)}_{\mu\nu}, and transitions are encoded through matching conditions at the boundaries using Israel junction formalism or effective scattering matrices,

The photon path follows a piecewise geodesic across multiple domains, accumulating phase shifts, lensing-like distortions, and amplitude modulations.

3. Ray-Tracing Setup

We model CMB photon trajectories originating from the surface of last scattering by:

  1. Embedding N concentric layered domains with varying curvature kik_i, scale factor evolution ai(t)a_i(t), and local gravitational potential fluctuations i\Phi_i,

  2. Solving null geodesics numerically for each region using:
     d2xd2+dxddxd=0\frac{d^2 x^\mu}{d\lambda^2} + \Gamma^{\mu}_{\alpha\beta} \frac{dx^\alpha}{d\lambda} \frac{dx^\beta}{d\lambda} = 0
     where \lambda is the affine parameter,

  3. At each boundary, applying continuity and refractive-like rules to compute transmission/reflection of wavefront distortions (phase slips, deflections),

  4. Recording total angular deflection, phase rotation, and redshift history along the full path to compute the effective CMB temperature anisotropy:
     TT(n^)+[ddt+int]d\frac{\Delta T}{T} (\hat{n}) \sim \Phi + \int_{\gamma} \left[ \frac{d\Phi}{dt} + \Theta_{\text{int}} \right] d\lambda
     where int\Theta_{\text{int}} encodes interference across layers.

4. Simulation Results

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