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Quantum-Corrected Cosmological Perturbation Solver
License: Dual
🔬 Overview
A complete computational framework for cosmological perturbation theory with first-principles quantum corrections. This package implements:
Quantum-corrected Mukhanov-Sasaki equations with backreaction from quantum fields
Full Boltzmann integration with quantum scattering terms
Tensor perturbations (gravitational waves) with quantum sources
Integration with CLASS/CAMB for validation
Planck 2018 data validation with Bayesian evidence computation
Production-ready pipeline for cosmological parameter constraints
🚀 Features
Core Physics
Quantum stress-energy perturbations using Schwinger-Keldysh formalism
Bunch-Davies & α-vacuum initial conditions with quantum corrections
Renormalization schemes: adiabatic (4th order), point-splitting, dimensional
Self-consistent backreaction between metric and quantum fields
Features
- 📜 License Dual License Structure This software is available under two distinct licenses: Academic/Non-Commercial License (FREE) For: Academic researchers, students, non-profit organizations Permissions: Free use, modification, and distribution Use in academic research and publications Classroom and educational use Requirements: Cite the original work in publications No commercial use allowed Personal Commercial License (REQUIRED) For: Companies, commercial organizations, for-profit use Requirements: License required for any commercial use Contact: Tony E. Ford - 📧 tlcagford@gmail.com Commercial licensing terms negotiated individually Usage Rights Summary Use Case License Required Cost Academic Research No FREE University Teaching No FREE Personal Projects No FREE Commercial Product YES Negotiable Corporate R&D YES Negotiable SaaS Integration YES Negotiable
