The Big Bang nucleosynthesis and finite temperature field theory

Physics

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Scientific paper

We consider electromagnetic corrections at finite temperature and their effect on the nucleosynthesis in the standard Big Bang scenario. This requires discussing the finite, temperature dependent correction to the neutron-proton mass difference as well as making use of a previous result on the temperature correction to the mass of the electron. We find that these corrections do not affect the conventional results of e.g. the helium abundance to any appreciable extent.
Research supported by the Swedish Natural Science Research Council, contract no. 7310-108.

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