Weak-scale implications of thermal leptogenesis in SUSY

Sacha Davidson

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arXiv · hep-ph/0304120

Weak-scale implications of thermal leptogenesis in SUSY

Sacha Davidson

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Abstract

Thermal leptogenesis is an attractive mechanism for generating the baryon asymmetry of the Universe. However, in supersymmetric models, the parameter space is severely restricted by the gravitino bound on the reheat temperature $T_{RH}$. Using a parametrisation of the seesaw in terms of weak-scale inputs, the low-energy footprints of thermal leptogenesis are discussed.

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Sacha Davidson. 2004-02-14. Weak-scale implications of thermal leptogenesis in SUSY. https://arxiv.org/abs/hep-ph/0304120

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