Gravito-Rotational Acceleration Theory for Compact Stellar Objects

A 1.2 MB PDF by Mohamed Elmansour Hassani introduces the concept of Gravito-Rotational Acceleration, a combination of gravitational and rotational forces not addressed in existing gravity theories. The paper extends the Combined Gravitational Action framework to self-rotating bodies and calculates specific maximum internal magnetic field strengths for the Sun and magnetars. It was last updated on May 11, 2026, and is shared under a CC-BY-4.0 license.

Use Cases

• Testing theoretical models of stellar structure based on the proposed gravito-rotational acceleration concept.
• Analyzing the implications of combined gravitational and rotational forces for compact object dynamics.
• Benchmarking calculated magnetic field strengths (e.g., 1.68716e5 G for the Sun) against other astrophysical models.

Strengths

• Provides specific calculated values, such as a maximum internal magnetic field strength of 5.6e18 G for magnetars.
• The 1.2 MB PDF file offers a complete, self-contained theoretical treatment.

Limitations

• Column-level documentation is absent; the paper's data and model specifics must be extracted manually from the text.
• Row count is unknown, which may limit suitability assessment for quantitative analysis.

Provenance

Source

figshare

Collection Method

Theoretical derivation and calculation.

Freshness

Last updated 2026-05-11 18:05:16; freshness should be verified.