Supermassive Black Holes Active Galactic Nuclei Accretion Disks Formation Galaxy Characteristics Formation of Galaxies Accretion Processes Galaxy Formation Overmassive Black Holes Galaxy Mergers Feedback Mechanisms Galaxy Interaction Big Bang Theory Effects on Galaxies Galaxy Dynamics Black Hole Formation Black Hole Feedback Neutron Stars Gravitational Waves Eddington Limit Stellar-mass Black Holes Galactic Nuclei Formation and Behavior Intermediate Mass Black Holes Energy Sources Matter Interaction Exoplanets Primordial Black Holes Star Formation Hawking Radiation Supernovae Cosmic Phenomena
Radboud University researchers reveal white dwarfs will evaporate in 10^78 years, revising the universe's projected end from 10^1100 years.