if the answer to a physical question depends partially on
the unknown, then to elaborate hypotheses concerning its incidence on the
observable world is a legitimate logical exercise which allows one to explore
these hypotheses as a guide towards a more fundamental theory.

Armed thus with the experience of the 2-fluid approach applied to black
hole evaporation, it is then natural to inquire into what it can offer for
cosmogenesis and inflation. It is in this spirit that we explore the possibility of identifying the inflaton with mode density.

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вооооот, про комплексную это интересно, спасибо

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вооооот, копипашка, вооооот

(Reply to this) (Parent)

не лень же копипастить какую-то хуету пустую

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