Approaching Lambda without fine-tuning

Details Approaching Lambda without fine-tuning Approaching Lambda without fine-tuning

2004-03-19

arxiv.org/abs/astro-ph/0403480v2

Phys.Rev. D70 (2004) 061301

Astronomy and Astrophysics

Astrophysics

References added; figures labels enlarged. To appear on PrD

Scientific paper

10.1103/PhysRevD.70.061301

We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy density needs to initially lie in a narrow range in order for its present value to be consistent with observations. As recently noticed, this problem becomes particularly severe in canonical Quintessence scenarios, when trying to reproduce the behavior of a cosmological constant, i.e. when the dark energy equation of state w_Q approaches -1: these models may be reconciled with a large basin of attraction only by requiring a rapid evolution of w_Q at low reshifts, which is in conflict with the most recent estimates from type Ia Supernovae discovered by Hubble Space Telescope. Next, we focus on scalar-tensor theories of gravity, discussing the implications of a coupling between the Quintessence scalar field and the Ricci scalar (``Extended Quintessence''). We show that, even if the equation of state today is very close to -1, by virtue of the scalar-tensor coupling the quintessence trajectories still possess the attractive feature which allows to reach the present level of cosmic acceleration starting by a set of initial conditions which covers tens of orders of magnitude; this effect, entirely of gravitational origin, represents a new important consequence of the possible coupling between dark energy and gravity.

Affiliated with

Also associated with

No associations

Rating

Approaching Lambda without fine-tuning 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 Approaching Lambda without fine-tuning, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Approaching Lambda without fine-tuning will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-335874