Cosmological Collider Phenomenology: the Standard Model and Beyond

APA

Xianyu, Z. (2019). Cosmological Collider Phenomenology: the Standard Model and Beyond. Perimeter Institute for Theoretical Physics. https://pirsa.org/19050028

MLA

Xianyu, Zhong-Zhi. Cosmological Collider Phenomenology: the Standard Model and Beyond. Perimeter Institute for Theoretical Physics, May. 21, 2019, https://pirsa.org/19050028

BibTex

          @misc{ scivideos_PIRSA:19050028,
            doi = {10.48660/19050028},
            url = {https://pirsa.org/19050028},
            author = {Xianyu, Zhong-Zhi},
            keywords = {Particle Physics},
            language = {en},
            title = {Cosmological Collider Phenomenology: the Standard Model and Beyond},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2019},
            month = {may},
            note = {PIRSA:19050028 see, \url{https://scivideos.org/pirsa/19050028}}
          }
          

Zhong-Zhi Xianyu Harvard University

Source Repository PIRSA
Collection

Abstract

The n-point correlation functions (n>2) of primordial fluctuations, known as primordial non-Gaussianities, encode rich information about the physical degrees of freedom and their interactions at inflation scale, and can be viewed as signals from a cosmological collider with huge energy. In this talk we introduce recent theoretical attempts to extract new physics at the inflation scale from primordial non-Gaussianities, including possible discovery channels, the background signals from the standard model, and signals from new physics such as heavy neutrinos, and a possible way to turn inflation into a Higgs collider.