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Supernova remnants are often presented as the most probable sources ofGalactic cosmic rays. This idea is supported by the accumulation of evidencethat particle acceleration is happening at supernova remnant shocks.Observations in the TeV range have especially contributed to increase theunderstanding of the mechanisms, but many aspects of the particle accelerationat supernova remnant shocks are still debated. The Cherenkov telescope array isexpected to lead to the detection of many new supernova remnants in the TeV andmulti-TeV range. In addition to the individual study of each, the study ofthese objects as a population can help constrain the parameters describing theacceleration of particles and increase our understanding of the mechanismsinvolved.

Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array