A cosmological theory that predicts a late-time accelerated attractor with a constant dark matter to dark energy ratio can be said to solve the Coincidence Problem. Such cosmologies are naturally generated in the context of non-standard gravity theories under conformal transformation because of the resulting couplings between scalar fields and matter. The present work examines four classes of these transformed theories and finds that only a small subset--those with a single scalar field--are capable of solving the Coincidence Problem. Comment: 27 pages LaTe
We analyse theories that do not have a de Sitter vacuum and cannot lead to slow-roll quintessence, b...
We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to e...
Although the cosmic concordance cosmology is quite successful in fitting data, fine tuning and coinc...
A cosmological theory that predicts a late-time accelerated attractor with a constant dark matter to...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
Our theoretical understanding of the dynamical evolution of the Universe has certainly improved duri...
Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a genera...
In an undulant universe, cosmic expansion is characterized by alternating periods of acceleration an...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We consider dark energy models obtained from the general conformal transformation of the Kropina met...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We consider a generic cosmological model which allows for non-gravitational direct couplings between...
The increasing observational pressure on the standard cosmological model motivates analyses going be...
Mounting observational data confirm that about 73 % of the energy density con-sists of dark energy w...
A nonminimally coupled quintessence model is investigated and the conditions for a stationary soluti...
We analyse theories that do not have a de Sitter vacuum and cannot lead to slow-roll quintessence, b...
We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to e...
Although the cosmic concordance cosmology is quite successful in fitting data, fine tuning and coinc...
A cosmological theory that predicts a late-time accelerated attractor with a constant dark matter to...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
Our theoretical understanding of the dynamical evolution of the Universe has certainly improved duri...
Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a genera...
In an undulant universe, cosmic expansion is characterized by alternating periods of acceleration an...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We consider dark energy models obtained from the general conformal transformation of the Kropina met...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We consider a generic cosmological model which allows for non-gravitational direct couplings between...
The increasing observational pressure on the standard cosmological model motivates analyses going be...
Mounting observational data confirm that about 73 % of the energy density con-sists of dark energy w...
A nonminimally coupled quintessence model is investigated and the conditions for a stationary soluti...
We analyse theories that do not have a de Sitter vacuum and cannot lead to slow-roll quintessence, b...
We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to e...
Although the cosmic concordance cosmology is quite successful in fitting data, fine tuning and coinc...