Non-Gaussianity and Statistical Anisotropy from Vector Field Populated Inflationary Models

Table 1

Order of magnitude of 𝑓_𝑁𝐿 in different scenarios.

	𝑓^𝑠𝑁𝐿	𝑓^𝐴𝑁𝐿	𝑓^𝑁𝐴𝑁𝐿
general case	1(1+𝛽)^2𝑁𝜙𝜙𝑁^2𝜙	𝛽(1+𝛽)^2𝑁𝐴𝐴𝑁^2𝜙	𝛽^2(1+𝛽)^2𝑔^2𝑐(𝑚𝐻)^2
v.inflation	𝜖𝜙(1+((𝐴/𝑚𝑃)𝜖𝜙)^2)^2	𝜖^2𝜙(1+((𝐴/𝑚𝑃)𝜖𝜙)^2)^2(𝐴𝑚𝑃)^2	𝜖^2𝜙𝑔^2𝑐(1+((𝐴/𝑚𝑃)𝜖𝜙)^2)^2(𝐴^2𝑚𝑃𝐻)^2
v.curvaton	𝜖𝜙(1+(𝐴𝑚𝑃/𝐴^2𝑡𝑜𝑡)^2𝜖𝜙𝑟^2)^2	𝜖^2𝜙𝑟^3(1+(𝐴𝑚𝑃/𝐴^2𝑡𝑜𝑡)^2𝜖𝜙𝑟^2)^2(𝐴𝑚^2𝑃𝐴^3𝑡𝑜𝑡)^2	𝜖^2𝜙𝑟^3𝑔^2𝑐(1+(𝐴𝑚𝑃/𝐴^2𝑡𝑜𝑡)^2𝜖𝜙𝑟^2)^2(𝐴^2𝑚^2𝑃𝐴^3𝑡𝑜𝑡𝐻)^2