Universality of galactic surface densities within one dark halo scale-length
Gianfranco Gentile, Benoit Famaey, HongSheng Zhao, Paolo Salucci

TL;DR
This paper reveals that both dark matter and luminous matter surface densities are constant within one dark halo scale length across diverse galaxies, indicating a fundamental correlation in galaxy structure.
Contribution
It demonstrates that luminous matter surface density is also constant within the dark halo scale length, extending the universality of galactic surface densities.
Findings
Dark matter surface density is constant within one halo scale length.
Luminous matter surface density is also constant within this radius.
The gravitational acceleration due to luminous matter is uniform at this scale.
Abstract
It was recently discovered that the mean dark matter surface density within one dark halo scale length - the radius within which the volume density profile of dark matter remains approximately flat - is constant across a wide range of galaxies. This scaling relation holds for galaxies spanning a luminosity range of 14 magnitudes and the whole Hubble sequence. Here we report that the luminous matter surface density is also constant within one scale length of the dark halo. This means that the gravitational acceleration generated by the luminous component in galaxies is always the same at this radius. Although the total luminous-to-dark matter ratio is not constant, within one halo scale length it is constant. Our finding can be interpreted as a close correlation between the enclosed surface densities of luminous and dark matter in galaxies.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
