In5-10 years AfNL-05(e. g. SPHEREX) (And Afne 10 in the very distant future. What is the implication if ifn 1?
In ~ 5-10 years Δ𝑓𝑁𝐿~0.5 (e.g. SPHEREx) (And Δ𝑓𝑁𝐿~10−3 in the very distant future.) What is the implication if |𝑓𝑁𝐿| < 1?
In5-10 years AfNL-05(e. g. SPHEREX) What is the implication if Ifne 1? Local: Curvaton will be very unlikely Equilateral: Cs"l, up to small corrections
In ~ 5-10 years Δ𝑓𝑁𝐿~0.5 (e.g. SPHEREx) What is the implication if |𝑓𝑁𝐿| < 1? - Local: Curvaton will be very unlikely. - Equilateral: 𝑐𝑠~1, up to small corrections
In5-10 years AfNL-05(e. g. SPHEREX) What is the implication if Ifne 1? Local: Curvaton will be very unlikely Equilateral: Cs "1, up to small corrections What is the motivation for future study
In ~ 5-10 years Δ𝑓𝑁𝐿~0.5 (e.g. SPHEREx) What is the implication if |𝑓𝑁𝐿| < 1? - Local: Curvaton will be very unlikely. - Equilateral: 𝑐𝑠~1, up to small corrections. What is the motivation for future study?
(Before addressing motivation of fnl 1 History of particle physics experiments Early stage: studying external particle a particle scattering μ from cosmic rays eep inelastic scattering Nowadays: study internal particle Higgs BSM
(Before addressing motivation of |𝑓𝑁𝐿| < 1 …) History of particle physics experiments: - Early stage: studying external particle - α particle scattering - μ from cosmic rays - deep inelastic scattering - … - Nowadays: study internal particle - Higgs - BSM - …
( Before addressing motivation of Ifne 1 external particle internal particle Cosmological non-G: is there a similarity Curvaton, Cs external particle(s) If seen: pin down inflation model What about internal particles?
(Before addressing motivation of |𝑓𝑁𝐿| < 1 …) external particle → internal particle Cosmological non-G: is there a similarity? Curvaton, 𝑐𝑠 , … : external particle (𝜁) If seen: pin down inflation model. What about internal particles?