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In its first six years of operations, the Fermi Gamma-ray Space Telescope has revolutionized our view of the gamma-ray Universe. Thanks to its unprecedented performance, the Large Area Telescope onboard Fermi has detected more than two thousand sources and unveiled new classes of gamma-ray emitters. In particular, pulsars are the main contributors to the gamma-ray source population in our Galaxy and are relevant not only to astrophysics. In fact, they are excellent natural laboratories to probe the laws of physics under extreme conditions, e.g. of gravity and electromagnetic fields. Among the population of the new gamma-ray pulsars detected by Fermi, the young, energetic ones are also very promising candidate sources of continuous gravitational waves. I will review the recent Fermi results on pulsars and discuss the possible perspectives for multimessenger observations of these sources

High-energy pulsars from gamma rays to gravitational waves