Dark Energy in the Early Universe

Dark Energy in the Early Universe

Dark energy is causing the expansion of the universe to accelerate. The most common model for dark energy has a negligible dark energy density in the early universe. The authors use measurements of the CMB power spectrum to constrain the density of dark energy in the early universe.

It’s Not Easy Being Blue

It’s Not Easy Being Blue

Blue stragglers are stars that, given their mass, should have already evolved beyond the main sequence, and their existence has been a mystery to astronomers for decades. These stars must somehow have gained mass during their main sequence lifetimes; stellar collisions and mass transfer were proposed as the most likely mechanisms that could cause this to happen. A unique combination of observations, simulations, and statistical analysis was recently used to constrain their formation process.