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Question on neutron freeze-out

  1. Jun 16, 2012 #1
    Hello,

    I was reading about big bang nucleosynthesis recently (If it helps, I'm using Mukhanov) and it was calculating the abundance of neutrons. It seems to say that [itex]X_n→X_n^{eq} [/itex] (It says that [itex]X_n^{eq} [/itex] is the equilibrium abundance of neutrons) as [itex]t→0.[/itex] So...does that mean that the neutrons have an abundance when they are first created and that is changed by the interactions with the protons?
     
  2. jcsd
  3. Jun 17, 2012 #2

    mathman

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    I am not familiar with the context. However, free neutrons are radioactive with a half life of a little under 15 minutes, decaying into proton + electron + anti-neutrino.
     
  4. Jun 17, 2012 #3

    BillSaltLake

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    Due to pair production, at around t = 1μ sec, neutrons would have existed (along with antineutrons) in roughly the same number as photons. Then after ~ 10 μ sec, the antineutrons were gone and the neutrons were down to around 1 per billion photons. (There were also proton- antiproton pairs but they should have completely annihilated.) Then the neutrons began to decay with half life ~900 sec. Most decayed into protons (+ electron & neutrino), but some were captured as the (stable) nuclei of 2H, 3He, 4He, and 7Li.
    I'm not sure which "t→0" is referred to (wrt 900 sec or 1μ sec).
     
    Last edited: Jun 17, 2012
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