Measuring Reionization, Neutrino Mass, and Cosmic Inflation with BFORE

Abstract

BFORE is a NASA high-altitude ultra-long-duration balloon mission proposed to measure the cosmic microwave background (CMB) across half the sky during a 28-day mid-latitude flight launched from Wanaka, New Zealand. With the unique access to large angular scales and high frequencies provided by the balloon platform, BFORE will significantly improve measurements of the optical depth to reionization tau, breaking parameter degeneracies needed for a measurement of neutrino mass with the CMB. The large angular scale data will enable BFORE to hunt for the large-scale gravitational wave B-mode signal, as well as the degree-scale signal, each at the r~0.01 level. The balloon platform allows BFORE to map Galactic dust foregrounds at frequencies where they dominate, in order to robustly separate them from CMB signals measured by BFORE, in addition to complementing data from ground-based telescopes. The combination of frequencies will also lead to velocity measurements for thousands of galaxy clusters, as well as probing how star-forming galaxies populate dark matter halos. The mission will be the first near-space use of TES multichroic detectors (150/217 GHz and 280/353 GHz bands) using highly-multiplexed mSQUID microwave readout, raising the technical readiness level of both technologies.

arXiv comment8 pages, 4 figures, to appear in Proceedings of Low Temperature Detectors 17

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Cited by in corpus (5)

• The Simons Observatory: Science goals and forecasts
• Neutrino Mass from Cosmology: Probing Physics Beyond the Standard Model
• Full-sky beam convolution for cosmic microwave background applications
• A forecast of the sensitivity on the measurement of the optical depth to reionization with the GroundBIRD experiment
• Cosmological Implications of a Neutrino Mass Detection