2 1 0 Ju l 2 00 1 Hamilton - Jacobi approach to pre - big bang cosmology and the problem of initial conditions

نویسنده

  • Margus Saal
چکیده

The Hamilton-Jacobi equation for the string cosmology is solved using the gradient expansion method. The zeroth order solution is taken to be the standard pre-big bang model and the second order solution is found for the dilaton and the three-metric. It indicates that corrections generated by inhomogeneities of the seed metric are suppressed near the singularity and are growing towards the asymptotic past, but corrections generated by the dilaton inhomogeneities are growing near the singularity and are suppressed in the past. Possible influences of initial metric inhomogeneities on the pre-big bang superinflation are discussed.

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

2 6 O ct 1 99 9 Hamilton - Jacobi approach to pre - big bang cosmology and the problem of initial conditions

The Hamilton-Jacobi equation for the low energy string effective action is solved using the gradient expansion method. The field equations are also expanded by the number of spatial gradients and the second order solution is found for the three-metric. The second order solution allows us to study the influence of initial inhomogeneities to the duration of pre-big bang superinflation. We conclud...

متن کامل

Anisotropic ’hairs’ in string cosmology

In most models, inflation is driven by the potential energy of a scalar field. This has similar effects as adding vacuum energy or, equivalently, a positive cosmological constant. For these models Wald [1] proved a cosmic no hair theorem, which implies that an initial shear is inflated away [2]. A couple of years ago, a new mechanism of inflation has been proposed, where inflation is due to the...

متن کامل

Initial Conditions and the Structure of the Singularity in Pre-Big-Bang Cosmology

We propose a picture, within the pre-big-bang approach, in which the universe emerges from a bath of plane gravitational and dilatonic waves. The waves interact gravitationally breaking the exact plane symmetry and lead generically to gravitational collapse resulting in a singularity with the Kasner-like structure. The analytic relations between the Kasner exponents and the initial data are exp...

متن کامل

ar X iv : a st ro - p h / 01 07 22 2 v 1 1 2 Ju l 2 00 1 Tracking The Baryon Density From The Big Bang To The Present

The primordial abundances of deuterium, helium, and lithium probe the baryon density of the universe only a few minutes after the Big Bang. Of these relics from the early universe, deuterium is the baryometer of choice. After reviewing the current observational status (a moving target!), the BBN baryon density is derived and compared to independent estimates of the baryon density several hundre...

متن کامل

ar X iv : g r - qc / 0 10 40 65 v 1 1 9 A pr 2 00 1 Properties of the quasistationary universe in context of the Big - bang cosmology problems

The model of quantum universe as a cosmological system in quasistationary state is considered. It is shown that in proposed approach the difficulties of the standard Big-bang cosmology do not arise. The theory predicts the observed dimensions of the nonhomogeneities of matter density and the amplitude of the fluctuations of the cosmic background radiation temperature in the Universe and points ...

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 2001