Now Ethan Nadler, a computational astrophysicist at UC San Diego, has calculated the mass below which halos fail to form stars. This work was done using analytic predictions from galaxy formation theory and cosmological simulations.
"Historically, our understanding of dark matter has been linked to its behavior in galaxies. A detection of completely dark halos would open up a new window to study the universe," stated Nadler.
Previously, this threshold for star formation was thought to be between 100 million to 1 billion solar masses due to cooling of atomic hydrogen gas. Nadler's research shows that star formation can occur in halos down to 10 million solar masses through molecular hydrogen cooling.
With the Rubin Observatory coming online later this year and JWST already making unprecedented observations of our universe, there will soon be new data to test these predictions and reveal whether completely dark halos exist. This may have far-reaching consequences for cosmology and the nature of dark matter.
Research Report:The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold
Related Links
UCSD
Stellar Chemistry, The Universe And All Within It
| Subscribe Free To Our Daily Newsletters |
| Subscribe Free To Our Daily Newsletters |
