Analytic bounds on late-time axion-scalar cosmologies
Gary Shiu (Department of Physics, University of Wisconsin-Madison, 1150 University Avenue, Madison, WI, 53706, USA); Flavio Tonioni (Instituut voor Theoretische Fysica, KU Leuven, Celestijnenlaan 200D, Leuven, B-3001, Belgium); Hung Tran (Department of Mathematics, University of Wisconsin-Madison, 480 Lincoln Drive, Madison, WI, 53706, USA)
The cosmological dynamics of multiple scalar/pseudoscalar fields are difficult to solve, especially when the field-space metric is curved. This presents a challenge in determining whether a given model can support cosmic acceleration, without solving for the on-shell solution. In this work, we present bounds on late-time FLRW-cosmologies in classes of theories that involve arbitrary numbers of scalar and pseudoscalar fields coupled both kinetically (leading to a curved field space metric) and through scalar potentials. Such bounds are proven analytically, independently of initial conditions, with no approximation in the field equations and without referring to explicit solutions. Besides their broad applications to cosmological model building, our bounds can be applied to studying asymptotic cosmologies of certain classes of string compactifications.
