The international collaboration presented their first results with new data in four years, featuring a new low-energy sample of electron neutrinos and a dataset doubled in size.
The new state-of-the-art QUIET laboratory will study the performance of qubits isolated from cosmic radiation. Its above ground counterpart is LOUD and together they will enable controlled experiments of quantum sensors.
Fermi National Accelerator Laboratory announced Jim Kerby as project director for Long-Baseline Neutrino Facility for the Deep Underground Neutrino Experiment (LBNF/DUNE-US) He will be responsible for managing all aspects of the project in the U.S. as Fermilab leads the execution of the largest international DOE project ever hosted on U.S. soil.
Leadership appointment enhances team at Fermilab with extensive operations experience.
Spring brings new life to Fermi National Accelerator Laboratory as calving season begins for the lab’s herd of American bison. Today, two bison calves were born at Fermilab. The lab has a long tradition of providing habitat for bison, connecting particle physics research to the Midwestern prairie. This season, 20 baby bison are expected.
Fermilab’s Chief Research Officer Bonnie Fleming has been elected to the prestigious American Academy of Arts & Sciences, honoring excellence and leadership throughout her science career.
A partnership between Fermilab and xLight Inc. will focus on producing advanced semiconductors in the United States using extreme ultraviolet light and accelerator technology.
Researchers have used the Dark Energy Spectroscopic Instrument to make the largest 3D map of our universe and world-leading measurements of dark energy, the mysterious cause of its accelerating expansion.
New Mexico-based artist Agnes Chavez will work with scientists at Fermilab to explore new ways to use data visualization, light, sound and space to communicate the importance and relevance of science, in particular research on particles called neutrinos.
The Dark Energy Survey has measured the BAO scale when the universe was half its present age with an accuracy of 2%, the most accurate determination yet at such an early epoch. It is the first time an imaging-only measurement is competitive with large spectroscopy campaigns specifically designed to detect this signal.