22–26 Jul 2024
Europe/Lisbon timezone

Can relativistic effects explain galactic dynamics without the need for dark matter?

24 Jul 2024, 15:45
15m
Auditorium E10B

Auditorium E10B

Department of Physics (University of Coimbra)

Speaker

Filipe Costa (CAMGSD - IST Universidade de Lisboa)

Description

In a growing number of recent works, it has been claimed that "gravitomagnetism" and/or non-linear general relativistic effects can play a leading role in galactic dynamics, partially or totally replacing dark matter. Using the 1+3 "quasi-Maxwell" formalism (and generalizing it for null geodesics), we show, on general grounds, such hypothesis to be impossible. We demonstrate that (i) the observed gravitational lensing effects rule out any galactic model (linear or non-linear) based on gravitomagnetism, and (ii) the non-linear contributions to the gravitational field actually weaken gravitational attraction, thereby only aggravating the need for dark matter. I shall also briefly dissect the misunderstandings at the origin of the recently proposed relativistic "galactic" models, most notably the Balasin-Grumiller solution, which serves as an archetypal example for the two key observations above.

Authors

Filipe Costa (CAMGSD - IST Universidade de Lisboa) Prof. José Natário (CAMGSD - IST Universidade de Lisboa)

Presentation materials