Loop Quantum Cosmology Matter Bounce Reconstruction from \(F(R)\) Gravity Using an Auxiliary Field

Abstract

Using the reconstruction technique with an auxiliary field, we investigate which \(F(R)\) gravities can produce the matter bounce cosmological solutions. Owing to the specific functional form of the matter bounce Hubble parameter, the reconstruction technique leads, after some simplifications, to the same Hubble parameter as in the matter bounce scenario. Focusing the study to the large and small cosmic time \(t\) limits, we were able to find which \(F(R)\) gravities can generate the matter bounce Hubble parameter. In the case of small cosmic time limit, which corresponds to large curvature values, the \(F(R)\) gravity is \(F(R)\sim R+\alpha R^2\), which is an inflation generating gravity, and at small curvature, or equivalently, large cosmic time, the \(F(R)\) gravity generating the corresponding limit of the matter bounce Hubble parameter, is \(F(R)\sim \frac{1}{R}\), a gravity known to produce late-time acceleration. Thus we have the physically appealing picture in which a Jordan frame \(F(R)\) gravity that imitates the matter bounce solution at large and small curvatures, can generate Starobinsky inflation and late-time acceleration. Moreover, the scale factor corresponding to the reconstruction technique coincides almost completely to the matter bounce scenario scale factor, when considered in the aforementioned limiting curvature cases. This is scrutinized in detail, in order to examine the validity of the reconstruction method in these limiting cases, and according to our analysis, exact agreement is achieved.