From Forbes, May 18, 2021: Fermilab’s Don Lincoln explains the Karlsruhe Tritium Neutrino Experiment, in Germany that has improved our understanding of the mass of this insubstantial denizen of the microcosm.
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From Wired, May 18, 2021: So imagine the excitement on April 7, when more than 200 physicists from seven countries convened on a Zoom call for a kind of nonexplosive gender-reveal party. What was to be disclosed was not a baby’s sex but the fate of particle physics.
From the Black Hills Pioneer, May 17, 2021 Activities at the Sanford Lab to have significant benefits for over the next decade as the construction of DUNE continues.
From Smithsonian Magazine, May 13, 2021: A group of scientists say the phenomenon could indicate dark matter speeding through our world at more than 300 miles a second. Fermilab’s Dan Hooper is quoted in this story about the study of flashes seen in ordinary lightning storms showing evidence of super-dense chunks of dark matter as they zip through our atmosphere.
From KOTA-TV (Rapid City, SD), May 16, 2021: Sanford has a $1.6 billion economic impact and generates over 1,000 jobs in South Dakota.
DESI will capture and study the light from tens of millions of galaxies and other distant objects to better understand our universe and the properties of dark energy. The formal start of DESI’s five-year survey follows a four-month trial run of its custom instrumentation that captured 4-million spectra of galaxies — more than the combined output of all previous spectroscopic surveys. Fermilab has contributed multiple components to the international collaboration led by Berkeley Lab.
From EIN Presswire, May 14, 2021; LBNL’s LArPix experiment result is a leap forward in how to detect and record signals in liquid argon time projection chambers (LArTPCs), a technology of choice for future neutrino and dark matter experiments such as Fermilab’s DUNE.
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.