Energy-Momentum Squared Gravity
arXiv:1607.06049 · doi:10.1103/PhysRevD.94.044002
Abstract
A new covariant generalization of Einstein's general relativity is developed which allows the existence of a term proportional to in the action functional of the theory ( is the energy-momentum tensor). Consequently the relevant field equations are different from general relativity only in the presence of matter sources. In the case of a charged black hole, we find exact solutions for the field equations. Applying this theory to a homogeneous and isotropic space-time, we find that there is a maximum energy density , and correspondingly a minimum length , at early universe. This means that there is a bounce at early times and this theory avoids the existence of an early time singularity. Moreover we show that this theory possesses a true sequence of cosmological eras. Also, we argue that although in the context of the standard cosmological model the cosmological constant does not play any important role in the early times and becomes important only after the matter dominated era, in this theory the "repulsive" nature of the cosmological constant plays a crucial role at early times for resolving the singularity.
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