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The National Science Foundation has awarded up to $21.4 million for the design of telescopes for CMB-S4, an international experiment that will study the cosmic microwave background and help us understand the beginning, history, and makeup of the universe. Berkeley Lab leads the project for DOE and also plays a lead role in technology development.
Researchers can use the radio-quiet far side of the moon to listen for a never-before-heard signal from the “Dark Ages” of the universe. The LuSEE-Night experiment will act as a pathfinder for future experiments, testing equipment and techniques in the harsh lunar environment.
Researchers have channeled the universe’s earliest light – a relic of the universe’s formation known as the cosmic microwave background – to solve a missing-matter mystery and learn new things about galaxy formation. Their work could also help us to better understand dark energy and test Einstein’s theory of general relativity by providing new details about the rate at which galaxies are moving toward us or away from us.
The largest collaborative undertaking yet to explore the relic light emitted by the infant universe has taken a step forward with the U.S. DOE’s selection of Berkeley Lab to lead the partnership of national labs, universities, and other institutions that are joined in the effort to carry out the DOE roles and responsibilities.
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