23–26 Sept 2014
DESY Hamburg
Europe/Berlin timezone

Relic density computations at NLO: infrared finiteness and thermal correction

24 Sept 2014, 14:40
20m
Seminar room 4A (DESY)

Seminar room 4A

DESY

Speaker

Mr Francesco Dighera (Technische Universitaet Muenchen)

Description

There is an increasing interest in accurate dark matter relic density predictions, which requires next-to-leading order (NLO) calculations. The method applied up to now uses zero-temperature NLO calculations of annihilation cross sections in the standard Boltzmann equation for freeze-out, and is conceptually problematic, since it ignores the finite-temperature infrared (IR) divergences from soft and collinear radiation and virtual effects. I address this problem systematically by starting from non-equilibrium quantum field theory, and demonstrate on a realistic model that soft and collinear temperature-dependent divergences cancel in the collision term. This analysis provides justification for the use of the freeze-out equation in its conventional form and determines the leading finite-temperature correction to the annihilation cross section. This turns out to have a remarkably simple structure.

Authors

Dr Andrzej Hryczuk (Technische Universitaet Muenchen) Mr Francesco Dighera (Technische Universitaet Muenchen) Prof. Martin Beneke (Technische Universitaet Muenchen)

Presentation materials