Spectral Line Broadening in High-Gravity Environments as a Test for Viscous Fermionic Condensate
Spectral Line Broadening in High-Gravity Environments as a Test for Viscous Fermionic Condensate
This paper defines a quantitative criterion for identifying the presence of a viscous fermionic medium (psi-field) using high-resolution X-ray spectroscopy data from the XRISM mission. The Fermionic Universe Hypothesis (FUH) postulates that space-time is a physical medium with a non-zero viscosity (eta) and a characteristic fermion mass (m_psi). Near supermassive objects, this medium reaches peak density, leading to anomalous energy dissipation of traversing photons.
m_psi = 4.8 keV, 6.4 keV, Mathematical Criterion for XRISM, Falsification Conditions, XRISM, Fermionic Universe Hypothesis, X-ray, FUH, Quantitative Prediction, Spectral Line Broadening, Project OCEAN, The Physical Mechanism, Viscous Fermionic Condensate
m_psi = 4.8 keV, 6.4 keV, Mathematical Criterion for XRISM, Falsification Conditions, XRISM, Fermionic Universe Hypothesis, X-ray, FUH, Quantitative Prediction, Spectral Line Broadening, Project OCEAN, The Physical Mechanism, Viscous Fermionic Condensate
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