
3
III. SIMULATION & RESULTS
We performed a high-fidelity simulation (N = 50, 000) introducing this “Genesis Curl” to the
initial conditions. To distinguish the primordial signal from thermal noise, we analyzed the spin
parity of resolved massive halos (N
p
> 20).
A. Results: Mass-Dependent Bias
The simulation reveals a distinct symmetry breaking in the high-mass population (Figure 1):
• Spin Alignment: We measure a bias ratio of ≈ 64.3% (18/28 massive halos) in favor of
the lattice curl direction.
• Mass Dependence: When the detection threshold is lowered to include dwarf halos, the
signal dilutes to ≈ 55%, confirming that thermal noise dominates at low masses.
This ≈ 64% baseline matches the specific alignment signal found in observational studies of HI-
rich galaxies (≈ 2/3) [2]. This suggests that the strong alignment observed in the simulation
corresponds to the Pristine regime detected by JWST.
IV. CONCLUSION
We resolve the tension between Early Galaxy observations and TTT by introducing a Topologi-
cal Initial Condition. The universe did not start with zero rotation; it started with a Genesis Curl.
Late-time gravity does not create spin; it merely redistributes the angular momentum inherited
from the vacuum crystallization, subject to the kinematic limits of lattice ghost drag (1/208).
[1] I. Labb´e et al., Nature 616, 266 (2023).
[2] E. Tempel et al., A&A 557, A21 (2013).
[3] B. Blue et al., MNRAS 528, 123 (2024).
[4] R. Kulkarni, The Selection-Stitch Model (SSM), Zenodo (2026).
[5] R. Kulkarni, SSM Theory Simulation Scripts, GitHub (2026).
[6] R. Kulkarni, Fermion Chirality from Non-Bipartite Topology, Zenodo (2026).