neutrino decoupling
event in the early universe, around 1 second after the Big Bang, when the universe cooled down sufficiently so that neutrinos ceased significantly interacting with baryonic matter
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neutrino decoupling
Summary
neutrino decoupling is a cosmological epoch[1]. It draws 51 Wikipedia views per month (cosmological_epoch category, ranking #4 of 8).[2]
Key Facts
- neutrino decoupling's instance of is recorded as cosmological epoch[3].
- neutrino decoupling's part of is recorded as early universe[4].
- neutrino decoupling's point in time is recorded as -13787000000-00-00T00:00:00Z[5].
- neutrino decoupling's Freebase ID is recorded as /m/06w4s7p[6].
- neutrino decoupling's has effect is recorded as cosmic microwave background[7].
- neutrino decoupling's temperature is recorded as {'unit': 'Q11579', 'amount': '+10000000000'}[8].
- neutrino decoupling's defining formula is recorded as T\sim\left(\frac{\sqrt G}{G_{\mathrm F}^2}\right)^{1/3}\sim1\;\mathrm{MeV}[9].
- neutrino decoupling's Unified Astronomy Thesaurus ID is recorded as 1101[10].
- neutrino decoupling's Microsoft Academic ID is recorded as 11006701[11].
- neutrino decoupling's in defining formula is recorded as G[12].
Why It Matters
neutrino decoupling draws 51 Wikipedia views per month (cosmological_epoch category, ranking #4 of 8).[2] It has Wikipedia articles in 5 language editions, a strong signal of global cultural recognition.[13] It is known by 3 alternative names across languages and contexts.[14]