Distributional cosmological quantities solve the paradox of soft singularity crossing
L\'aszl\'o \'A. Gergely, Zolt\'an Keresztes, Alexander Yu. Kamenshchik

TL;DR
This paper explores how distributional methods can resolve the paradoxes associated with crossing soft singularities, like the Sudden Future Singularity, in cosmological models involving exotic matter fields.
Contribution
It introduces a distributional approach to redefine cosmological quantities, enabling smooth crossing of soft singularities in models with anti-Chaplygin gas and tachyon fields.
Findings
Regular energy density and Hubble parameter across the singularity
Hubble parameter and expansion rate exhibit mirror symmetry
Pressure and deceleration parameter contain Dirac delta contributions
Abstract
Both dark energy models and modified gravity theories could lead to cosmological evolutions different from either the recollapse into a Big Crunch or exponential de Sitter expansion. The newly arising singularities may represent true endpoints of the evolution or allow for the extension of geodesics through them. In the latter case the components of the Riemann tensor representing tidal forces diverge. Sudden Future Singularities (SFS) occur at finite time, finite scale factor and finite Hubble parameter, only the deceleration parameter diverges. The energy density of a perfect fluid is regular and its pressure diverges at the SFS. A particular SFS, the Big Brake occurs when the energy density vanishes and the expansion arrives at a full stop at the singularity. Such scenarios are generated by either a particular scalar field (the tachyon field) or the anti-Chaplygin gas. By adding…
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