August 31, 2026 to September 4, 2026
Auditorio José Adem, Mexico
America/Mexico_City timezone

Galactic dynamics from pure torsion

Not scheduled
20m
Auditorio José Adem, Mexico

Auditorio José Adem, Mexico

Av Instituto Politécnico Nacional 2508, San Pedro Zacatenco, Gustavo A. Madero, 07360, Mexico-City, Mexico
Talk

Speaker

Sergio Mendoza

Description

I present a relativistic modified gravity theory based on a scalar function of the torsion tensor. In the weak-field limit, the field equations naturally reduce to the deep-MOND regime without introducing dark matter. This framework simultaneously reproduces the observed deflection of light across individual galaxies and clusters, and yields an exact derivation of the baryonic Tully-Fisher relation. These results suggest that torsional degrees of freedom offer a viable, covariant completion of MOND that passes critical gravitational lensing tests.

Authors

Sergio Mendoza Sarahí Silva García (Universidad Nacional Autónoma de México)

Presentation materials

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