Tidal energy effects of dark matter halos on early-type galaxies

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Article in Book "Energy Research Developments: Tidal Energy, Energy Efficiency and Solar Energy" published by NOVA PUBLISHERS,

Scientific paper

Tidal interactions between neighboring objects span across the whole admissible range of lengths in nature: from, say, atoms to clusters of galaxies i.e. from micro to macrocosms. According to current cosmological theories, galaxies are embedded within massive non-baryonic dark matter (DM) halos, which affects their formation and evolution. It is therefore highly rewarding to understand the role of tidal interaction between the dark and luminous matter in galaxies. The current investigation is devoted to Early-Type Galaxies (ETGs), looking in particular at the possibility of establishing whether the tidal interaction of the DM halo with the luminous baryonic component may be at the origin of the so-called "tilt" of the Fundamental Plane (FP). The extension of the tensor virial theorem to two-component matter distributions implies the calculation of the self potential energy due to a selected subsystem, and the tidal potential energy induced by the other one. The additional assumption of homeoidally striated density profiles allows analytical expressions of the results for some cases of astrophysical interest. The current investigation raises from the fact that the profile of the (self + tidal) potential energy of the inner component shows maxima and minima, suggesting the possible existence of preferential scales for the virialized structure, i.e. a viable explanation of the so called "tilt" of the FP. It is found that configurations related to the maxima do not suffice, by themselves, to interpret the FP tilt, and some other relation has to be looked for.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Tidal energy effects of dark matter halos on early-type galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Tidal energy effects of dark matter halos on early-type galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tidal energy effects of dark matter halos on early-type galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-57356

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.