CMB中的同心圆可以用来探测大爆炸前的宇宙活动

宇宙微波背景辐射中的同心圆可以用来探测大爆炸前的宇宙?niubility

-------------------------------

Concentric circles in WMAP data may provide evidence of violent pre-Big-Bang activity

 

Abstract: Conformal cyclic cosmology (CCC) posits the existence of an aeon preceding
our Big Bang 'B', whose conformal infinity 'I' is identified, conformally, with
'B', now regarded as a spacelike 3-surface. Black-hole encounters, within bound
galactic clusters in that previous aeon, would have the observable effect, in
our CMB sky, of families of concentric circles over which the temperature
variance is anomalously low, the centre of each such family representing the
point of 'I' at which the cluster converges. These centres appear as fairly
randomly distributed fixed points in our CMB sky. The analysis of Wilkinson
Microwave Background Probe's (WMAP) cosmic microwave background 7-year maps
does indeed reveal such concentric circles, of up to 6{\sigma} significance.
This is confirmed when the same analysis is applied to BOOMERanG98 data,
eliminating the possibility of an instrumental cause for the effects. These
observational predictions of CCC would not be easily explained within standard
inflationary cosmology.

Comments: 8 pages, 6 figs
Subjects: Cosmology and Extragalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:1011.3706v1 [astro-ph.CO]

 

评论

yet another

yet another follow-up,对CMB中的圈圈做了进一步的理论扩展

Pre-Big-Bang Cosmology and Circles in the Cosmic Microwave Background

Abstract: We examine the possibility that circles in the cosmic microwave background
could be formed by the interaction of a gravitational wave pulse emitted in
some pre-big-bang phase of the universe with the last scattering surface. We
derive the expected size distribution of such circles, as well as their typical
width and (for concentric circles) angular separation. We apply these results
in particular to conformal cyclic cosmology, ekpyrotic cosmology as well as
loop quantum cosmology with and without inflation in order to determine how the
predicted geometric properties of these circles would vary from one model to
the other, and thus, if detected, could allow us to differentiate between
various pre-big-bang cosmological models. We also show that the angular width
and the sine of the angular radius of such circles are inversely proportional.
This relation can be used in order to determine whether or not circles observed
in the cosmic microwave background are due to energetic pre-big-bang events.

Comments: 21 pages, 3 figures
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Extragalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:1104.3688v1 [gr-qc]