Primordial non-Gaussianities record interactions of elds in the early universe, which can be viewed as collision events in a "Cosmological Collider" with huge energy. In this talk, I shall introduce the workings of the Cosmological Collider as an explorer of new physics at very high scales, and describe the Standard Model spectrum during in ation and its "background signals" in Cosmological Collider. The nontrivial quantum correction during in ation plays a crucial role in this process, which I shall describe in detail.
