Relativistic Contraction-Shrinking Theory Data for Cosmological Analysis

Encompassing theoretical data related to the Relativistic Contraction-Shrinking Theory (RKST), authored by Johannes Schenk. The theory proposes an emergent gravitational constant and a reinterpretation of cosmic acceleration as vacuum contraction, validated against solar-system tests and galactic dynamics from the SPARC sample.

Use Cases

• Analyze the coupling between the microscopic proton radius (rp) and the cosmological Dirac number (N) to model the emergent gravitational constant G.
• Validate the theory's predicted phantom equation-of-state parameter (w ≈ -1.05) against observational data for accelerated expansion.
• Test the chameleon screening mechanism and scale invariance properties within the Horndeski class scalar-tensor framework.
• Apply the energy partitioning model to the cosmological constant problem using the theory's matter sector binding of vacuum energy.

Strengths

• Theory is validated against classical solar-system tests of General Relativity.
• Theory reproduces galactic dynamics from the SPARC sample without requiring dark matter.
• Dataset is associated with a peer-reviewed theoretical framework (RKST) within the Horndeski class.

Limitations

• Dataset size, row count, column structure, and specific file formats are unknown.
• Data appears to be purely theoretical, lacking empirical observational records.
• Theoretical validation scope is limited to mentioned tests (solar-system, SPARC); broader cosmological applicability is unconfirmed.

Provenance

Source

Johannes Schenk Dataverse

Collection Method

Theoretical derivation and modeling within the Relativistic Contraction-Shrinking Theory (RKST) framework.

Freshness

Last updated on 2026-02-22.