Defines a criterion for detecting a viscous fermionic medium using high-resolution X-ray data, indicating significant energy effects near supermassive objects.
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.
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Alexander Shlyapik (2026) studied this question.
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