Quantum cosmological backreactions. I. Cosmological space adiabatic perturbation theory

نویسندگان

چکیده

Quantum cosmology, including quantum cosmological inhomogeneities, is a promising framework for describing the very early universe in which all degrees of freedom are being considered as dynamical and quantum. However, many previous discussions on this subject consider perturbations test fields curved spacetime with effective modifications thus neglect certain interactions subsystems, namely backreaction inhomogeneous background. In series four papers, first, we aim at improving treatment effects that arise due to backreactions between matter geometry well homogeneous freedom. We employ technique space adiabatic perturbation theory form developed by Panati, Spohn, Teufel relies familiar Born-Oppenheimer approximation. extend scheme field perturbative setting show leads presently neglected correction terms Friedmann equations. first article, provide detailed introduction iterative examine generic challenges encountered its application cosmology. Our results will allow direct comparison observations.

برای دانلود رایگان 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

Cosmological background solutions and cosmological backreactions

The cosmological backreaction proposal, which attempts to account for observations without a primary dark energy source in the stress-energy tensor, has been developed and discussed by means of different approaches. Here, we focus on the concept of cosmological background solutions in order to develop a framework to study the backreaction proposal.

متن کامل

Cosmological Perturbation Theory

This is a review on cosmological perturbation theory. After an introduction, it presents the problem of gauge transformation. Gauge invariant variables are introduced and the Einstein and conservation equations are written in terms of these variables. Some examples, especially perfect fluids and scalar fields are presented in detail. The generation of perturbations during inflation is studied. ...

متن کامل

Space-Adiabatic Perturbation Theory

We study approximate solutions to the Schrödinger equation iε∂ψt(x)/∂t = H(x,−iε∇x)ψt(x) with the Hamiltonian H the Weyl quantization of the symbol H(q, p) taking values in the space of bounded operators on the Hilbert space Hf of fast “internal” degrees of freedom. By assumption H(q, p) has an isolated energy band. We prove that interband transitions are suppressed to any order in ε. As a cons...

متن کامل

Duality in Cosmological Perturbation Theory

Cosmological perturbation equations derived from low-energy effective actions are shown to be invariant under a duality transformation reminiscent of electric-magnetic, strong-weak coupling, S-duality. A manifestly dualityinvariant approximation for perturbations far outside the horizon is introduced, and it is argued to be useful even during a high curvature epoch. Duality manifests itself thr...

متن کامل

Hamiltonian cosmological perturbation theory with loop quantum gravity corrections

Cosmological perturbation equations are derived systematically in a canonical scheme based on Ashtekar variables. A comparison with the covariant derivation and various subtleties in the calculation and choice of gauges are pointed out. Nevertheless, the treatment is more systematic when correction terms of canonical quantum gravity are to be included. This is done throughout the paper for one ...

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

سال: 2022

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.105.106009