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Big Bang Nucleosynthesis and Neutrino Cosmology

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arxiv 1903.09187 v3 pith:NDOWT6EL submitted 2019-03-21 astro-ph.CO

Evan B. Grohs , J. Richard Bond , Ryan J. Cooke , George M. Fuller , Joel Meyers , Mark W. Paris This is my paper · ORCID
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keywords bangcapabilitiesneutrinonucleosynthesisadvancingadventastrophysicsbackground
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There exist a range of exciting scientific opportunities for Big Bang Nucleosynthesis (BBN) in the coming decade. BBN, a key particle astrophysics "tool" for decades, is poised to take on new capabilities to probe beyond standard model (BSM) physics. This development is being driven by experimental determination of neutrino properties, new nuclear reaction experiments, advancing supercomputing/simulation capabilities, the prospect of high-precision next-generation cosmic microwave background (CMB) observations, and the advent of 30m class telescopes.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    CMB-S4 forecasts: the two-site design reaches sigma(Neff)=0.029 in seven years, the Chile-only revised design reaches 0.030 in nine, and a cosmic-variance-limited survey would reach 0.0073.

  2. Prospects and Limitations for Constraining Light Relics with Primordial Abundance Measurements

    astro-ph.CO 2019-08 conditional novelty 5.0 of 10

    A Fisher forecast shows that order-of-magnitude improvements in helium-4 abundance measurements could yield light-relic constraints near CMB-S4 sensitivity, but deuterium measurements alone will not be competitive.

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