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The backbone of the large-scale structure of the Universe is determined byprocesses on a cosmological scale and by the gravitational interaction of thedominant dark matter. However, the mobile baryon population shapes theappearance of these structures. Theory predicts that most of the baryons residein vast unvirialized filamentary structures that connect galaxy groups andclusters, but the observational evidence is currently lacking. Because themajority of the baryons are supposed to exist in a large-scale, hot and dilutegaseous phase, X-rays provide the ideal tool to progress our understanding.Observations with the Athena+ X-ray Integral Field Unit will reveal thelocation, chemical composition, physical state and dynamics of the activepopulation of baryons.

The Hot and Energetic Universe: The missing baryons and the warm-hot intergalactic medium