From Sanford Lab, July 6, 2021: Celebrate Neutrino Day with SURF’s Star Chronicles on Friday, July 9, and Saturday, July 10. See the line-up of virtual events streaming through Gather.town, a free and simple platform, where attendees can explore the events and interact with others as they would in real life.
From Forbes, May 14, 2021: Fermilab senior scientist Don Lincoln discusses measuring the size of neutron stars and the result of a measurement showing that the centers of neutron stars are stiff and not squishy.
From Forbes, Feb. 17, 2021: Fermilab scientist Don Lincoln contextualizes the accomplishment of researchers working at the Japan Proton Accelerator Research Complex, or J-PARC. They have made an atomic nucleus that contains an unstable particle called the hyperon, or cascade particle. This could help in understanding neutron stars.
From Forbes, Feb. 10, 2021: Fermilab scientist Don Lincoln explains why there should be equal amounts of matter and antimatter in the universe. There aren’t. He discusses several current theories that try to explain the discrepancy. Better understanding this imbalance is an aim of ongoing experiments, such as DUNE, which is being built at Fermilab.
From CNN, Feb. 4, 2021: Fermilab scientist Don Lincoln contextualizes a recent signal that some think may be a sign of extraterrestrial intelligence, explaining the hubbub around the recent a transmission originating from Proxima Centauri. With hope for hearing such a signal one day and pride for humanity’s legacy of looking skyward, Lincoln cautions against reading too much into this transmission, which hasn’t yet been vetted with scientific review.
From Universe Today, Feb. 3, 2021: Recent published results from the Dark Energy Survey point to intracluster light — feeble light from rogue stars that don’t belong to a galaxy — as a potential pathway to measure dark matter. Fermilab scientist Yuanyuan Zhang contextualizes the findings.
From Super Interessante, Jan. 31, 2021: A team of researchers from Fermilab and the National Observatory in Brazil used the light of solitary stars to calculate the mass of some of the largest structures in the cosmos — galaxy clusters. In addition to taking the most detailed measurement ever published of intracluster light, the team’s new method of measurement can help further investigate dark matter.