Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, 7 figures

Scientific paper

10.1088/0264-9381/23/9/025

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We impose a suitable dynamics of the expansion allowing to derive exact Friedmann-Robertson-Walker solutions once the coupling function is given as input. Self-interaction potentials of single and double exponential types emerge as result of our choice of the coupling function. The stability and existence of the solutions is discussed in some detail. Although, in general, models with appropriated interaction between the components of the cosmic mixture are useful to handle the coincidence problem, in the present study the coincidence can not be evaded due to the choice of the solution generating ansatz.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-432127

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.