28–29 May 2026
HUN-REN Centre
Europe/Budapest timezone

Microscopic structure of spacetime from neutron star oscillations

29 May 2026, 15:00
20m
HUN-REN Centre

HUN-REN Centre

1054 Budapest Alkotmány utca 29.

Speaker

Anna Horváth

Description

In addition to the well-known one time and three infinite spatial dimensions of spacetime, many theories also consider the existence of extra dimensions. The Kaluza-Klein model expands spacetime with one spatial dimension, which is curled up in a microscopic circle, thus affecting particles on quantum mechanical scales. In neutron stars, where matter is subject to extremely strong gravitational effects, gravity could become comparable in strength to the other fundamental interactions and provide corrections to the equation of state. Thus low energy effects of quantum gravity could be present.

The effect of a strong gravitational field on massive particles is studied, indeed, corrections to the uncertainty and the dispersion relations are considered. Understanding microscopical effects induced by the structure of spacetime is crucial to build consistent models of macroscopic phenomena, which can be compared to astronomical data e.g. through neutron star oscillations.

A. Horváth, A. Wojnar, G.G. Barnaföldi: “The effects of strong gravity on the dispersion relation of massive particles in the Kaluza–Klein theory”, https://arxiv.org/abs/2510.16631

Authors

Dr Aneta Wojnar (University of Wrocław) Anna Horváth Emese Forgacs-Dajka (Eövös University, Department of Astronomy, Budapest, Hungary) Dr Gergely Barnafoldi (HUN-REN Wigner Reseach Centre for Physics)

Presentation materials