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After a period of inflationary expansion, the Universe reheated and reachedfull thermal equilibrium at the reheating temperature. In this talk, based onthe paper, arXiv:0710.3349, we point out that, in the context of effectivelow-energy supersymmetric models, LHC measurements may allow one to determinereheating temperature as a function of the mass of the dark matter particleassumed to be either an axino or a gravitino. An upper bound on their mass andon the reheating temperature may also be derived.

Determining Reheating Temperature at LHC with Axino or Gravitino Dark Matter