Semantic Scholar Open Access 1998 2 sitasi

Where do all the Supercurvature Modes Go

J. Cohn D. Kaiser

Abstrak

(1) Departments of Physics and Astronomy, University of IllinoisUrbana-Champaign, IL 61801jdc@uiuc.edu(2) Department of Physics, Harvard UniversityCambridge, MA 02138dkaiser@fas.harvard.edu(March 1998)In the hyperbolic slicing of de Sitter space appropriate for open universe models, a curvaturescale is present and supercurvature fluctuations are possible. In some cases, the expansion of a scalarfield in the Bunch-Davies vacuum includes supercurvature modes, as shown by Sasaki, Tanaka andYamamoto. We express the normalizable vacuum supercurvature modes for a massless scalar fieldin terms of the basis modes for the spatially-flat slicing of de Sitter space.Preprint UIUC-98/2; HUTP-98/A010; gr-qc/9803073I. INTRODUCTION

Topik & Kata Kunci

Penulis (2)

J

J. Cohn

D

D. Kaiser

Format Sitasi

Cohn, J., Kaiser, D. (1998). Where do all the Supercurvature Modes Go. https://doi.org/10.1103/PhysRevD.58.083515

Akses Cepat

Lihat di Sumber doi.org/10.1103/PhysRevD.58.083515
Informasi Jurnal
Tahun Terbit
1998
Bahasa
en
Total Sitasi
Sumber Database
Semantic Scholar
DOI
10.1103/PhysRevD.58.083515
Akses
Open Access ✓