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Brane inflation and the production of topological defects at the end of the inflationary phase are discussed. After a description of the inflationary setup we discuss the properties of the cosmic strings produced at the end of inflation. Specific examples of brane inflation are described: $D-\bar D$ inflation, $D3/D7$ inflation and modular inflationdoi:10.1098/rsta.2008.0065 pmid:18534933 fatcat:olhm7qbajbdujoxdb4hldbmvwu