NSF delays major cosmic microwave background experiment
DOI: 10.1063/pt.oevl.gwou
A cosmic microwave background telescope at the South Pole near where the proposed CMB-S4 telescopes would be placed.
Alexander Pollak/University of Chicago
This article is adapted from a 15 May
A planned $800 million project to study ancient cosmic radiation using ultrasensitive telescopes at the South Pole and in Chile will not progress to the design stage “in its current form,” NSF announced on 7 May. The agency said the strong scientific support for the Cosmic Microwave Background Stage 4 (CMB-S4) experiment is outweighed by the urgent need to upgrade aging infrastructure at the South Pole and elsewhere in Antarctica.
NSF “must prioritize the recapitalization of critical infrastructure at the South Pole so that the groundbreaking research it enables can continue to thrive,” said Chris Smith, the interim director of the agency’s astronomical sciences division, at a National Academies of Sciences, Engineering, and Medicine meeting
The decision to not move the project from the development to the design phase is specific to its current form, leaving the door open to pursuing an alternative approach, Smith emphasized. And he said that NSF remains committed to CMB science and will continue to support current studies of the early universe at the South Pole and in Chile.
In development for more than a decade, the CMB-S4 project would install more than 500 000 cryogenically cooled superconducting detectors in telescopes at the South Pole and in the Chilean Atacama Desert to measure the CMB with unprecedented precision. Research goals include searching for evidence of primordial gravitational waves, an expected signature of cosmological inflation, in CMB polarization measurements. Jointly funded by NSF and the Department of Energy, the experiment was slated to begin observations in the early 2030s
Recent major planning exercises by US astronomy and particle-physics communities have identified CMB-S4 as a top priority (see Physics Today, February 2024, page 18
The NSF decision was a surprise and a disappointment for the hundreds of scientists involved in the project, particularly junior researchers considering their future careers, says Kevin Huffenberger. A spokesperson for the CMB-S4 Science Collaboration and a physics professor at Florida State University, Huffenberger was informed of the decision the day before the public announcement. “We absolutely want the project to continue,” he says.
Huffenberger and Jim Strait, the CMB-S4 project director and a physicist at Lawrence Berkeley National Laboratory, say that the team has considered a Chile-only option and is now working on developing a new plan that does not involve the South Pole. But Huffenberger adds that project leaders “hope that the South Pole becomes available again, because our analysis does show that it is the best place to do the early-universe, primordial gravitational-wave portion of our science.”
The High Energy Physics Advisory Panel received a briefing
Cottam also said there is an urgent need to lift buildings at the South Pole because of the accumulation of snow, which has begun to deform steel support beams. How to prioritize solving those infrastructure challenges will be covered in the forthcoming South Pole Station Master Plan.
Asked when NSF will resume approving new projects at the South Pole, Cottam said a clearer timeline for the infrastructure upgrades would be available by the end of the year, once the master plan is completed. A draft of the plan
NSF’s latest budget request to Congress anticipates that South Pole station upgrades will continue through the end of the decade