activity
20242026
collaborators

6 papers

astro-ph.GA2026

Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with hyperconical modified gravity

Robert Monjo

Gas-rich ultra-diffuse galaxies (UDGs) are an unusually sharp test for gravity models tied to the baryonic Tully--Fisher relation because several systems appear to rotate too slowl…

hep-ph2025

Weak mixing angle under colored gravity

Robert Monjo

Colored gravity, based on symmetry, emerges naturally in the complexification of Lorentzian manifolds and integrates U(1) electromagnetism as a subcase. This work e…

gr-qc2024

From colored gravity to electromagnetism

Robert Monjo, Álvaro Rodríguez-Abella, Rutwig Campoamor-Stursberg

The gauge formalism in \textit{telepalallel gravity} provides an interesting viewpoint to describe interactions according to an anholonomic observer's tetrad basis. Without going i…

gr-qc2024

Galaxy rotation curve in hyperconical universes: a natural relativistic MOND

Robert Monjo

Modified Newtonian dynamics (MOND) and similar proposals can (at least partially) explain the excess rotation of galaxies or the equivalent mass-discrepancy acceleration, without (…

astro-ph.CO2024

Hydrostatic equilibrium of X-ray gas in X-COP clusters with HMG

Robert Monjo

Modified Newtonian Dynamics (MOND) was originally proposed to model galaxy rotation curves without dark matter. However, MOND presents difficulties in explaining the Radial Acceler…

astro-ph.CO2024

Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing

Robert Monjo

Despite the success of dark-matter models, unresolved issues require exploring alternatives such as modified gravity theories. In this context, we examine the compatibility of the…