What question did this study set out to answer?

This research aims to evaluate different models of baryonic interaction in the Fornax dwarf spheroidal galaxy.

June 27, 2026Open Access

CDN-338: The Fornax Nu Test

Puntos clave

This research aims to evaluate different models of baryonic interaction in the Fornax dwarf spheroidal galaxy.
Applied a public-data Jeans dispersion test on Fornax dSph.
Compared Newtonian baryons, MOND, GCFT BE, and NFW models under similar conditions.
Utilized fixed parameters for light-profile, stellar mass, and anisotropy.
Identified distinct behaviors of baryonic models, with GCFT BE showing significant differences in dispersion.
MOND model displayed different gravitational effects compared to traditional Newtonian calculations.
Fixed-concentration NFW model confirmed existing theories on dark matter distribution.

Resumen

A public-data Fornax dSph Jeans dispersion test of the locked GCFT Bose-Einstein interpolation law, comparing Newtonian baryons, MOND simple, GCFT BE, and fixed-concentration NFW under matched light-profile, stellar-mass, and anisotropy assumptions.

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