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2021
DOI: 10.48550/arxiv.2111.09541
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Big Bang Nucleosynthesis Limits and Relic Gravitational Waves Detection Prospects

Tina Kahniashvili,
Emma Clarke,
Jonathan Stepp
et al.

Abstract: We revisit the big bang nucleosynthesis (BBN) limits on primordial magnetic fields and/or turbulent motions accounting for the decaying nature of turbulent sources between the time of generation and BBN. This leads to larger estimates for the gravitational wave (GW) signal than previously expected. We address the detection prospects through space-based interferometers (for GWs generated around the electroweak energy scale) as well as pulsar timing arrays and astrometric missions (for GWs generated around the q… Show more

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Cited by 3 publications
(3 citation statements)
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References 60 publications
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“…BBN was one of the first probes used to constrain PMFs [104][105][106][107][108][109]. Although current constraints are around a fraction of a µG, two orders of magnitude weaker than the ones from other probes, BBN offers an interesting prospect for the future using GWs [110].…”
Section: Jcap07(2024)086mentioning
confidence: 99%
“…BBN was one of the first probes used to constrain PMFs [104][105][106][107][108][109]. Although current constraints are around a fraction of a µG, two orders of magnitude weaker than the ones from other probes, BBN offers an interesting prospect for the future using GWs [110].…”
Section: Jcap07(2024)086mentioning
confidence: 99%
“…Cosmology Due to the limited lifetime of the neutron, Big Bang Nucleosynthesis (BBN) is greatly sensitive to the Hubble expansion rate and, therefore, to the number of relativistic degrees of freedom N e f f [225][226][227]. This severely constrains the possibility of having new light particles in thermal equilibrium with neutrinos at temperatures of a few MeV.…”
Section: New Neutrino Interactions With Light Mediatorsmentioning
confidence: 99%
“…Cosmology -Due to the limited lifetime of the neutron, Big Bang Nucleosynthesis (BBN) is greatly sensitive to the Hubble expansion rate and, therefore, to the number of relativistic degrees of freedom N ef f [223][224][225]. This severely constrains the possibility of having new light particles in thermal equilibrium with neutrinos at temperatures of a few MeV.…”
Section: New Neutrino Interactions With Light Mediatorsmentioning
confidence: 99%