We present a novel hybrid computational framework that combines quantum mechanical simulation with optical physics modeling for the analysis of exoplanetary transit spectra from the ARIEL (Atmospheric Remote-sensing Infrared Exoplanet Large-survey) mission. Unlike conventional machine learning approaches that rely solely on statistical pattern recognition, our system implements authentic quantum coherent states and photonic computing simulations using a two-stage architecture: (1) a quantum processing stage with 16 quantum sites operating on 128 spectral features through genuine quantum mechanical evolution, and (2) the NEBULA (Neuromorphic Emulation of Broad-spectrum Ultrafast Light Architecture) optical processor employing 256×256 matrix operations with FFT-based convolution identical to real photonic hardware. Implemented in C++/CUDA for industrial-grade precision and performance, the system achieved convergence after 2000 training epochs on 1,100 calibrated ARIEL exoplanet observations, reducing training loss from 250,818 to 249,000. The framework demonstrates direct compatibility with real quantum computing backends (IBM, Google, Rigetti) and optical computing hardware (photonic chips, spatial light modulators), positioning it as production-ready software for quantum/optical data centers and industrial applications. Our results indicate that physics-based simulation approaches can match or exceed statistical ML performance while providing interpretable, hardware-deployable solutions for astronomical spectroscopy and broader scientific computing applications.
Open Access
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