ar X iv : a st ro - p h / 03 02 26 4 v 2 6 J un 2 00 3 Quintessence and the Curvature of the Universe after WMAP

نویسنده

  • F. Steiner
چکیده

Received (received date) Revised (revised date) We study quintessence models with a constant (effective) equation of state. It is investigated whether such quintessence models are consistent with a negative spatial curvature of the Universe with respect to the anisotropy of the cosmic microwave background radiation measured by the WMAP mission. If the reionization is negligibly small, it is found that such models with negative curvature are admissible due to a geometrical degeneracy. However, a very high optical depth τ to the surface of last scattering, as indicated by the polarization measurements of WMAP, would rule out such models.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : a st ro - p h / 04 03 69 9 v 1 3 0 M ar 2 00 4 Reionization , SLOAN , and WMAP : is the Picture Consistent ?

I show that advanced simulations of cosmological reionization are able to fit the observed data on the mean transmitted flux in the hydrogen Lyman-alpha line at z ∼ 6. At the same time, posteriori models can be constructed that also produce a large value (20%) for the Thompson scattering optical depth, consistent with the WMAP measurements. Thus, it appears that a consistent picture emerges in ...

متن کامل

ar X iv : a st ro - p h / 06 03 53 9 v 2 27 M ar 2 00 6 Inflation models after WMAP year three

In a recent paper [1] we discussed a range of models for the origin of the curvature perturbation and the tensor perturbation, including constraints on the spectral index n coming from WMAP year one data. In this note we update the discussion to include WMAP year three data [2]. The models assume that the curvature perturbation is generated from the vacuum fluctuation of the inflaton field, so ...

متن کامل

ar X iv : a st ro - p h / 06 06 12 4 v 1 6 J un 2 00 6 Inhomogeneous Cosmology , Inflation and Late - Time Accelerating Universe

An inhomogeneous cosmology describing a spacetime without symmetry is shown to be able to inflate the early universe and explain the late-time acceleration of the universe without a cosmological constant and negative pressure dark energy and avoid the coincidence problem. e-mail: [email protected]

متن کامل

ar X iv : a st ro - p h / 06 06 12 4 v 2 3 0 M ay 2 00 7 Inhomogeneous Cosmology , Inflation and Late - Time Accelerating Universe

An exact inhomogeneous solution of Einstein’s field equations is shown to be able to inflate in a non-uniform way in the early universe and explain anomalies in the WMAP power spectrum data. It is also possible for the model to explain the accelerated expansion of the universe by late-time inhomogeneous structure. e-mail: [email protected]

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003