Aspects of the Standard Cosmological Model Modified by Signature Change from Colombeau Algebras
Signature change; Colombeau Algebras; Energy-Momentum Tensor.
Colombeau's algebras have provided an extremely solid mathematical framework for dealing with problems related to products of distributions, since this operation is well defined in these algebras, unlike the theory of Schwartz distributions. In this work we intend to use the tools provided by the algebras of Colombeau's full generalized functions to interpret the results obtained from the study of the change of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric. In addition, we also intend to study the implications of using the sigmoid function as the function responsible for the sign change in Friedmann's equations and other equations that are influenced by the f(t) that changes the sign. As preliminary results, we develop the previously mentioned equations in the algebras of Colombeau's simplified generalized functions. Furthermore, we derive the necessary conditions for conservation of the energy-momentum tensor on the signature change surface.