Inflationary nonsingular quantum cosmological model

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

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

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Nonsingular Regenerating Inflationary Universe

A new version of the inflationary universe scenario is suggested which provides a possible solution of the cosmological singularity

متن کامل

Inflationary Cosmological Perturbations of Quantum-Mechanical Origin

This review article aims at presenting the theory of inflation. We first describe the background spacetime behavior during the slow-roll phase and analyze how inflation ends and the Universe reheats. Then, we present the theory of cosmological perturbations with special emphasis on their behavior during inflation. In particular, we discuss the quantum-mechanical nature of the fluctuations and s...

متن کامل

On stability of simplest nonsingular inflationary cosmological models within general relativity and gauge theories of gravity

In this paper we provide approximate analytical analysis of stability of nonsingular inflationary chaotic-type cosmological models. Initial conditions for nonsingular solutions at the bounce correspond to dominance of potential part of the energy density of the scalar field over its kinetic part both within general relativity and gauge theories of gravity. Moreover, scalar field at the bounce e...

متن کامل

Nonsingular Cosmological Models with a Variable Cosmological Term Λ

Exact solutions of the Einstein’s field equations describing a spherically symmetric cosmological model without a big bang or any other kind of singularity recently obtained by Dadhich and Patel (2000) are revisited. The matter content of the model is a shear-free perfect fluid with isotropic pressure and a radial heat flux. Three different exact solutions are obtained for both perfect fluid an...

متن کامل

Cosmological Perturbations in an Inflationary Universe

After introducing the perturbed metric tensor in a Friedmann-Robertson–Walker (FRW) background we review how the metric perturbations can be split into scalar, vector and tensor perturbations according to their transformation properties on spatial hypersurfaces and how these perturbations transform under small coordinate transformations. This allows us to introduce the notion of gauge-invariant...

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

ژورنال

عنوان ژورنال: Physical Review D

سال: 2007

ISSN: 1550-7998,1550-2368

DOI: 10.1103/physrevd.76.083521