Thursday, October 2, 2008

Big Bang Nucleosynthesis

        Went for my evening walk listening again to “Nucleosynthesis”. It starts with the “Big Bang Nucleosynthesis” at ten billion degrees where high-speed collisions occur in a soup of Protons, Neutrons, and Electrons. A free Proton catches an Electron and becomes a Hydrogen atom. The Hydrogen atom fuses with another Hydrogen atom to form Deuterium with one Proton and one Neutron, and releases a Positron (antielectron-antimatter that is annihilated when it encounters and Electron, producing two high-energy Photons- Gamma Rays), and a Neutrino (an elementary particle that has little mass and doesn’t carry an electric charge). Then the Deuterium fuses into Helium-3, and two Helium-3 fuses into Helium-4 that is very stable. An increase in energy was released as heavier isotopes and elements were fused. In the first three minutes after the Big Bang most of the Deuterium was converted into Helium and small amounts of Lithium, and nothing heavier because things cooled down and the process stopped. I’ll listen to it again hopefully tomorrow and write about Stellar Nucleosynthesis.

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