Primordial Non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure : Figure 1

]>Primordial Non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure : Figure 1

(a)

(b)

(c)

Figure 1: Triangle types contributing to the bispectrum corresponding to “squeezed” or local configurations with

k_{3} ≪ k_{1}, k_{2}

(a), equilateral configurations with

k_{3} \approx k_{1} \approx k_{2}

(b), and flattened configurations with

k_{3} \approx k_{1} + k_{2}

(c).