Orbifold line topology and the cosmic microwave background
We extend our study of a universe with a non-classical stringy topology, and consider an orbifold line topology, R x R super(2)/Z sub()p. This topology has a fixed line and identifies each point in space with p - 1 other points. An observable imprint of an orbifold line on the CMB is the appearance...
Gespeichert in:
Veröffentlicht in: | Journal of cosmology and astroparticle physics 2013-10, Vol.2013 (10), p.I-10, Article JCAP10(2013)45 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | We extend our study of a universe with a non-classical stringy topology, and consider an orbifold line topology, R x R super(2)/Z sub()p. This topology has a fixed line and identifies each point in space with p - 1 other points. An observable imprint of an orbifold line on the CMB is the appearance of up to (p - 1)/2 pairs of matching circles. Searching the WMAP data for matching circles, we can rule out an orbifold line topology with p up to 10, except for p = 8. While the significance of the peak at p = 8 varies between data releases of WMAP, it does not appear in Planck data, enabling us to rule out p = 8 as well. |
---|---|
ISSN: | 1475-7516 1475-7516 |
DOI: | 10.1088/1475-7516/2013/10/045 |