Modified cosmology models from thermodynamical approach

Thermodynamical Formalism for a Modified Shift Map

We introduce a transfer operator and use it to prove some theorems of a classical flavor from thermodynamical formalism (including existence and uniqueness of appropriately defined Gibbs states and equilibrium states for potential functions satisfying Dini’s condition and stochastic laws for Hölder continuous potential and observable functions) in a novel setting: the “alphabet” E is a compact ...

Modified gravity and cosmology

Tensor-vector-scalar-modified gravity: from small scale to cosmology.

The impressive success of the standard cosmological model has suggested to many that its ingredients are all that one needs to explain galaxies and their systems. I summarize a number of known problems with this programme. They might signal the failure of standard gravity theory on galaxy scales. The requisite hints as to the alternative gravity theory may lie with the modified Newtonian dynami...

Observational constraints on cosmology from modified Friedmann equation

Recent measurements of type Ia supernovae as well as other concordant observations suggest that the expansion of our universe is accelerating. A dark energy component has usually been invoked as the most feasible mechanism for the acceleration. However, the effects arising from possible extra dimensions can mimic well the role of a dark energy through a modified Friedmann equation. In this work...

Thermodynamical approach to quantifying quantum correlations.

We consider the amount of work which can be extracted from a heat bath using a bipartite state rho shared by two parties. In general it is less then the amount of work extractable when one party is in possession of the entire state. We derive bounds for this "work deficit" and calculate it explicitly for a number of different cases. In particuar, for pure states the work deficit is exactly equa...