CMBR DIPOLE FROM ULTRA LARGE-SCALE ISOCURVATURE PERTURBATIONS

Authors
Citation
D. Langlois, CMBR DIPOLE FROM ULTRA LARGE-SCALE ISOCURVATURE PERTURBATIONS, Helvetica Physica Acta, 69(3), 1996, pp. 229-232
Citations number
8
Categorie Soggetti
Physics
Journal title
ISSN journal
00180238
Volume
69
Issue
3
Year of publication
1996
Pages
229 - 232
Database
ISI
SICI code
0018-0238(1996)69:3<229:CDFULI>2.0.ZU;2-L
Abstract
The observed CMBR dipole, generally interpreted as the consequence of the peculiar motion of the Sun with respect to the reference frame of the CMBR, can also be explained by the presence of ultra large scale ( of the order of 100H(0)(-1)) isocurvature perturbations. Moreover, the simplest model of inflation with several scalar fields, namely that o f double inflation, with appropriate parameters, can produce such pert urbations.