Reference : Mapping extreme-scale alignments of quasar polarization vectors
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/1782
Mapping extreme-scale alignments of quasar polarization vectors
English
Hutsemekers, Damien mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Cabanac, R. [Canada France Hawaii Telescope, 65-1238 Mamalahoa Highway, Kamuela, Hawaii 96743, USA]
Lamy, H. [BIRA-IASB, Avenue Circulaire 3, 1180 Bruxelles, Belgium]
Sluse, D. [Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 17, B5c, 4000 Liège, Belgium]
1-Oct-2005
Astronomy and Astrophysics
EDP Sciences
441
915-930
Yes (verified by ORBi)
International
0004-6361
1432-0746
Les Ulis
France
[en] quasars: general ; polarization ; large-scale structure of Universe ; dark matter ; cosmology: observations
[en] Based on a new sample of 355 quasars with significant optical polarization and using complementary statistical methods, we confirm that quasar polarization vectors are not randomly oriented over the sky with a probability often in excess of 99.9%. The polarization vectors appear coherently oriented or aligned over huge ( 1 Gpc) regions of the sky located at both low (z Ë 0.5) and high (z Ë 1.5) redshifts and characterized by different preferred directions of the quasar polarization. In fact, there seems to exist a regular alternance along the line of sight of regions of randomly and aligned polarization vectors with a typical comoving length scale of 1.5 Gpc. Furthermore, the mean polarization angle bartheta appears to rotate with redshift at the rate of 30° per Gpc. The symmetry of the the bartheta -z relation is mirror-like, the mean polarization angle rotating clockwise with increasing redshift in North Galactic hemisphere and counter-clockwise in the South Galactic one. These characteristics make the alignment effect difficult to explain in terms of local mechanisms, namely a contamination by interstellar polarization in our Galaxy. While interpretations like a global rotation of the Universe can potentially explain the effect, the properties we observe qualitatively correspond to the dichroism and birefringence predicted by photon-pseudoscalar oscillation within a magnetic field. Interestingly, the alignment effect seems to be prominent along an axis not far from preferred directions tentatively identified in the Cosmic Microwave Background maps. Although many questions and more particularly the interpretation of the effect remain open, alignments of quasar polarization vectors appear as a promising new way to probe the Universe and its dark components at extremely large scales.
http://hdl.handle.net/2268/1782
10.1051/0004-6361:20053337
http://adsabs.harvard.edu/abs/2005A%26A...441..915H
http://de.arxiv.org/abs/astro-ph/0507274

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Open access
2005A&A...441..915H.pdfPublisher postprint1.25 MBView/Open

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.