Inflation including collapse of the wave function: the quasi-de Sitter case
The precise physical mechanism describing the emergence of the seeds of cosmic structure from a perfect isotropic and homogeneous universe has not been fully explained by the standard version of inflationary models. To handle this shortcoming, D. Sudarsky and collaborators have developed a proposal:...
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| Autores principales: | León, G., Landau, S.J., Piccirilli, M.P. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14346044_v75_n8_p_Leon |
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