Authors: Iyer R*
This work presents a comprehensive theoretical and computational analysis quantifying energy densities and particle genesis mechanisms with early universe through advanced physics simulations and analytical derivations. A novel mathematical physics framework introducing Superluminal Magnetic General Condensate (SMGC) is developed, extending what is well known within PHYSICS literature having classical electromagnetic energy density to the Lorentz-violating regimes near the Planck scale. By incorporating magnetic fields that are monopole-sourced and a superluminal coherence velocity term, the energy density quantitative expression, \({\rho _{SMGC}}\)~\({{B_m^2} \over {2{\mu _0}}}\left( {1 + \alpha {{{\nu ^2}} \over {{c^2}}}} \right)\), with v > c, emerges naturally, predicting densities of order 10⁴² J/m³. These values align with plausible conditions typically during early universe primordial symmetry breaking and inflationary epochs. The model integrates well beyond-standard-model physics concepts such as tachyonic fields, monopole condensates, and the Lorentz-violating extensions, providing a quantifiable pathway for the early-universe superluminal coherence without causal paradoxes. Further, the Hod–PDP Particle Genesis Mechanism is theoretically formulated, linking scalar-field tunneling and quantum decay processes to the baryon asymmetry generation consistent with Sakharov conditions. Quantitative estimates using semiclassical tunneling actions at QCD-scale temperatures yield efficient baryogenesis with SE ≈ 1, supporting observed matter–antimatter imbalance. Collectively, these results provide an integrative theoretical foundation that helps to explore superluminal condensates and baryogenesis processes within the extreme cosmological conditions.
Keywords: Superluminal Magnetic Condensate; Magnetic Monopoles; Lorentz Violation; Quantum Fields Theory; Baryogenesis; Early Universe Physics; Tachyonic Fields; Grand Unified Theories; Planck-Scale Gauge Cosmology
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