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The peeling behaviour of the Weyl tensor near null infinity is determined foran asymptotically flat higher dimensional spacetime. The result isqualitatively different from the peeling property in 4d. To leading order, theWeyl tensor is type N. The first subleading term is type II. The next term isalgebraically general in 6 or more dimensions but in 5 dimensions another typeN term appears before the algebraically general term. The Bondi energy flux iswritten in terms of "Newman-Penrose" Weyl components.

Peeling of the Weyl tensor and gravitational radiation in higher dimensions