In a recent publication,
Chiara, Pierre and
Baptiste, together with Vincent
Vennin,
have developed a novel framework to implement stochastic inflation on
random trees. These trees represent dynamically how different
regions of space grow and gradually become causally disconnected.
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The next cosmology seminar takes place on Thursday 30th of January,
room E349 at 4:00pm. Our guest speaker is Anish Ghoshal from Warsaw U. (Poland).
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The next cosmology seminars take place on Friday 13th of December,
seminar room E349 at 9:45am. Our guest speakers are Jibril
Ben Achour from Munich U. (Germany) and Hugo Roussille from
ENS Lyon (France).
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Within the landscape of single-field slow-roll models, and given the
present cosmological data, we show that Cosmic Inflation predicts a
small negative running of the spectral index of the cosmological
fluctuations. This quantity imprints the large scale structures of the
universe and we have just made a prediction for its value. Will it be
measured negative and small?
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Making observable predictions for cosmic inflation requires
determining when the wavenumbers of astrophysical interest today
exited the Hubble radius during the inflationary epoch. These instants
are commonly evaluated using the slow-roll approximation and measured
in e-folds time. Pierre,
Baptiste and Christophe
propose a new analytical method to determine these instants with a
precision reaching the tenth of an e-fold.
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