Tuesday, 30 November 2010

Journal Club: 30/11/10

The cosmology journal club will meet again today (Tuesday 30th Novemeber 2010) at 11:30am (after coffee) in the Pavillion B common room (B1.19).

This week has a modified gravity / `new physics' feel with Jeremy Sakstein  leading the discussion on:

Stellar Structure and Tests of Modified Gravity
Philip Chang, Lam Hui
arXiv:1011.4107

and me (Douglas Shaw) leading the discussion on the ambitous and controversial Penrose & Gurzadyan preprint:

Concentric circles in WMAP data may provide evident of violent pre-Big-Bang activity
V. G. Gurzadyan, R. Penrose

Full paper details follow:


Stellar Structure and Tests of Modified Gravity
Philip Chang, Lam Hui
arXiv:1011.4107
Theories that attempt to explain cosmic acceleration by modifying gravity typically introduces a long-range scalar force that needs to be screened on small scales. One common screening mechanism is the chameleon, where the scalar force is screened in environments with a sufficiently deep gravitational potential, but acts unimpeded in regions with a shallow gravitational potential. This leads to a variation in the overall gravitational G with environment. We show such a variation can occur within a star itself, significantly affecting its evolution and structure, provided that the host galaxy is unscreened. The effect is most pronounced for red giants, which would be smaller by a factor of tens of percent and thus hotter by 100's of K, depending on the parameters of the underlying scalar-tensor theory. Careful measurements of these stars in suitable environments (nearby dwarf galaxies not associated with groups or clusters) would provide constraints on the chameleon mechanism that are four orders of magnitude better than current large scale structure limits, and two orders of magnitude better than present solar system tests. 

Concentric circles in WMAP data may provide evident of violent pre-Big-Bang activity
V. G. Gurzadyan, R. Penrose
arXiv:1011.3706
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. 

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