main page: GrassmannCosmoFun2009These are just rough notes - feel free to correct them, add links, etc. from the Grassmann ian Conference in Fundamental Cosmology (Grasscosmofun'09). These are not official proceedings. The speakers might even disagree that they said anything even vaguely related to what are in these online notes! Don't say you weren't warned.
Tues 15 Sep 2009
KOWALSKI - some recent SNe Ia results
John BARROW - varying alpha results:
Chand, Srianand et al. 2004 results wrong because started from assuming alpha = constant (instead of free parameter) and then seeing if it can be varied; and because their best fit chi^2 is not a nice parabola and they missed fitting many lines; someone has reanalysed the data and got back to the varying alpha result;
varying alpha for various absorption lines (Fe II(?), ...)
results from 3 groups agree dalpha/alpha \approx -0.6 \times 10^{-5}
varying alpha model BSBM - scalar field model - interpret Webb et al. results
BSBM => violation of weak equivalence principle
present bounds = 10^{-12} - probably need to go to space to get stronger constraints, e.g. 10^{-18}
... bouncing BSBM models....
Pouria PEDRAM
Wheeler de Witt equation
Piotr DZIERZAK
Bianchi I type model and LQC
T^3 model !!!
... Big Bounce at classical level
algebra of observables:
aim: singularity aspects of the model in terms of observables
E. MELAS
canonical QQ for geometries admitting maximally symmetric 2D surfaces
final expression for WDW eqn
Conclusion:
TODO:
(1) render finite the 3 smooth functionals y^1, y^2, y^3
(2) select an appropriate inner product
requires only first derivatives, cf. Cartan-Karlhede which requires up to the 7th derivatives
Mariusz DABROWSKI
Big Rip, SFS (Sudden Future Singularity), TLB, radially inhomogeneous pressure models, possible solutions to DE with sudden singularity (in future(?))
Przemyslaw MALKIEWICZ
see papers with Piechocki - strings, membranes, in time-dependent orbifold
Ghodsi HODA
working with Martin Hendry
q = fn(z), differs for SFS model vs standard concordance model
with m=constant, SFS fails to fit all fashionable data sets simultaneously
Boguslaw BRODA (Lodz)
DE from quantum flucutations
... get rho approx rho_experimental where rho_experimental = rho_Lambda (?)
other interesting approaches: holographic DE e.g. Ricci DE which is similar to Broda's approach