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- W1998207918 abstract "The inhomogeneous fluctuations that underlie structure formation - galaxies and CMB hotspots - might have been seeded by quantum cosmological fluctuations, as magnified by some inflationary mechanism. The Halliwell-Hawking model for these, as a lower-energy semiclassical limit, is expected to be shared by many theories. E.g. an O((H/m_pl)^2) suppression of power at large scales results from this. This model contains/suppresses very many terms; we want a qualitative understanding of the meaning of these terms and of different regimes resulting from different combinations of them. I study this with toy models that have tractable mathematics: minisuperspace and, especially, relational particle mechanics. In the present Seminar, I consider in particular averaged terms with some lessons from Hartree-Fock approach to Atomic and Molecular Physics. One needs to anchor this on variational principles; treating the subsequent equations is a numerical venture." @default.
- W1998207918 created "2016-06-24" @default.
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- W1998207918 date "2014-03-25" @default.
- W1998207918 modified "2023-09-23" @default.
- W1998207918 title "QUANTUM COSMOLOGY WILL NEED TO BECOME A NUMERICAL SUBJECT" @default.
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- W1998207918 doi "https://doi.org/10.1142/9789814578745_0024" @default.
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