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Astrophysical observations provide strong evidence that more than 80% of allmatter in the Universe is in the form of dark matter (DM). Two leadingcandidates of particles beyond the Standard Model that could constitute all ora fraction of the DM content are the so-called Weakly Interacting MassiveParticles (WIMPs) and Axion-Like Particles (ALPs). The upcoming CherenkovTelescope Array, which will observe gamma rays between 20 GeV and 300 TeV withunprecedented sensitivity, will have unique capabilities to search for these DMcandidates. A particularly promising target for WIMP searches is the GalacticCenter. WIMPs with annihilation cross sections correctly producing the DM relicdensity will be detectable with CTA, assuming an Einasto-like density profileand WIMP masses between 200 GeV and 10 TeV. Regarding new physics beyond DM,CTA observations will also enable tests of fundamental symmetries of naturesuch as Lorentz invariance.

Probing Dark Matter and Fundamental Physics with the Cherenkov Telescope Array