Authors: Iyer R*
The microphysical structure of strongly interacting matter in the early Universe remains a central question for quantum chromodynamics (QCD) and gravitational-wave (GW) cosmology. In this work, sequel paper to the author’s seminal article on early universe superluminal condensate seed particles, we investigate hadronic crystal phases - Skyrmion-type topological lattices as well having the scalar-field–driven quantum hadron lattices (QHLs) - that may have formed near the QCD epoch and acted as coherent high-frequency gravitational-wave emitters. The author has already thoroughly quantitatively algorithmically modeled early universe mechanisms leading to baryogenesis. Building on the rich astro quantum physics literature, nonlinear SU (2) Skyrme Lagrangian for the baryonic solitons, and recent developments in optical Skyrme lattices, we model the early- Universe hadron ordering and its dynamical response using a combination of typical analytical derivations. Also, quadrupole radiation theory in linearized general relativity having 1D/2D curved-extent “spacetime” scalar-field simulations make it highly rigorous model. We compute quadrupole moments for oscillating Skyrmion crystals as well as perturbative hadron lattices, obtaining GHz– THz oscillation modes with intrinsic moments Q ~ 10−35 kg cdotppm2 . Individually, baryons generate negligible strains ( 36 33 ) single h ~ 10− −10− , but collective phase locking, curvature-induced compression, and Kerr-like rotational enhancements lead to macroscopic coherent emission. Numerical simulations incorporating quantum (Coleman–Weinberg), thermal, and curvature corrections reveal stable kink–antikink lattices, mode-locked vibrational spectra, and high coherence factors. For lattice domains with N ~ 1012 −1015 baryons, the total strain reaches 22 21 total h ~ 10− −10− , placing such micro–GW signals within the projected sensitivity of emerging high-frequency GW detectors that are available from physics literature and the practical infrastructure. These results indicate that early-Universe hadronic crystals may have produced detectable levels of the high-frequency stochastic backgrounds, offering a novel observational channel into the microstructure of QCD matter and the nonlinear dynamics of baryon topology in the first microseconds after the Big Bang, currently norm of astrophysical universal genesis process.
Keywords: Early Universe; Hadronic Crystals; Skyrmion Lattices; Quantum Hadron Lattices (QHLs); Micro Gravitational Waves; High-Frequency Gravitational Waves; Quadrupole Radiation; Cosmological QCD Phase; Coherent GW Emission; Numerical Simulations
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