Cooling of Neutron Stars Revisited: Application of Low Energy Theorems

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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6 pages, 2 figures. To appear in the Proceedings of "Bologna 2000: Structure of the Nucleus at the Dawn of the Century",May 29

Scientific paper

Cooling of neutrons stars proceeds mainly via neutrino emission; As an example we study the modified neutrino bremsstrahlung process $nn \to nn\nu\bar{\nu}.$ The radiated energy is small compared to other scales in the system. Hence one can use low-energy theorems to compute the neutrino emissivity in terms of the non-radiative process, ie the on-shell $T$ matrix. We find that the use of the $T-$matrix as compared to previous estimates based upon one pion exchange leads a substantial reduction of the predicted emissivity.

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