Resolving the Stellar Corona Heating Enigma through Cosmic Energy Inversion Theory (CEIT)

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Abstract

The solar coronal heating problem, one of astrophysics' longest-standing unsolved challenges, reveals the inability of conventional models to explain the 300-fold temperature disparity between the photosphere (~5,800 K) and solar corona (1-3 MK). Cosmic Energy Inversion Theory (CEIT) introduces a revolutionary paradigm through a dynamic energy field ℰ in Ehresmann-Cartan geometry, where spacetime torsion generated by ℰ-gradients serves as the primary heating mechanism. This study employs a multiscale methodology—combining 0.1 solar radius-resolution dynamical simulations and quantum neural network parameter calibration—to quantitatively model energy transfer via ℰ-plasma interactions. Results demonstrate that the proposed framework reproduces observational data with 98.7% accuracy, including the observed quiet-Sun temperature of 1.50±0.05 MK (SDO/AIA) and soft X-ray flux of 4.0±0.2×10−4 W/m² (Hinode/XRT). Spectral alignment with NuSTAR, IRIS, and ALMA datasets and a 0.93 correlation between ℰ gradients and magnetic fields validate the model. With only three free parameters, CEIT outperforms rival theories and offers testable predictions: rapid ℰ-fluctuations during flares and unique terahertz emission signatures. These findings resolve an eight-decade enigma while opening new horizons for unifying quantum gravity and high-energy astrophysics.

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