THE HOT DARK MATTER MODEL: FURTHER INVESTIGATION
e outer region with the dominant hot dark matter (the parabolic orbit of the test particle). It was assumed that the hot dark matter consists of hypothetical Planck neutrinos arising in the decay of the protons at the Planck scale. Galaxies formed from the baryonic matter, and the hot dark matter ap...
Main Author: | D. L. Khokhlov |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2020-11-01
|
Series: | Odessa Astronomical Publications |
Subjects: | |
Online Access: | http://oap.onu.edu.ua/article/view/216299 |
Similar Items
-
Model of the Galaxy with Hot Dark Matter
by: Khokhlov Dmitri L.
Published: (2018-12-01) -
Cuspy dark matter density profiles in massive dwarf galaxies
by: Bolatto, A.D, et al.
Published: (2022) -
Constraining Dark Matter Properties with Dwarf Galaxies and Galaxy Clusters
by: Kim, Stacy Yeonchi
Published: (2019) -
A comparison of two mass distributions applicable to globular clusters and dwarf galaxies
by: Ninković Slobodan D.
Published: (2004-01-01) -
Measuring dark matter profiles non-parametrically in dwarf spheroidal galaxies
by: Jardel, John Raymond
Published: (2014)