<<
Cosmo
ToK Warszawa meeting - Rough Notes Thu 16 Feb 2007
Langlois - Non-linear cosmological perturbations
zeta
Evolution equation
covariant approach
Thomas Flacke: QCD axions from a 5D gauge field
I.W. Kim Gauge messenger model
Krzysztof Turzyński - multi-field inflation
ToK
Warszawa meeting - Rough Notes Thu 16 Feb 2007
These are just rough notes - feel free to correct them, add links, etc.
Langlois - Non-linear cosmological perturbations
David Langlois + Vernizzi
AstroPh:0503416
Evolution of non-linear cosmological perturbations
AstroPh:0509078
Conserved non-linear quantities in cosmology
zeta
contours of constant density are not equal to contours of constant time
Evolution equation
linear case:
perfect fluid
large scales -
- adiabatic
conserved
covariant approach
generalised H parameter circle{H} = \Del_a u^a
Hawking; Ellis & Bruni
h_a^b \Del_a \rho
= 0 FLRW \not= 0 perturbed FLRW
Thomas Flacke: QCD axions from a 5D gauge field
HepPh:0612126
I.W. Kim Gauge messenger model
HepPh:0607169
HepPh:0702041
...bino-wino-higgsino mixing neutralino as a nbDM candiate
Krzysztof Turzyński - multi-field inflation
[earlier work:
HepPh:0606133
The Price of WMAP Inflation in Supergravity]
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Topic revision:
16 Feb 2007,
BoudRoukema
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