Universe as Klein–Gordon eigenstates
Abstract We formulate Friedmann’s equations as second-order linear differential equations. This is done using techniques related to the Schwarzian derivative that selects the $$\beta $$ β -times $$t_\beta :=\int ^t a^{-2\beta }$$ t β : = ∫ t a - 2 β , where a is the scale factor. In particular, it t...
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| Formato: | article |
| Lenguaje: | EN |
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SpringerOpen
2021
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| Materias: | |
| Acceso en línea: | https://doaj.org/article/c445670e1eda45c2b0767ed5c2ddd36c |
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