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SUMMARY:Sebastian Cespedes (IFT)
DTSTART:20201008T140000Z
DTEND:20201008T150000Z
DTSTAMP:20260423T003258Z
UID:IFTWeb/9
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/IFTWeb/9/">O
 n the time evolution of cosmological correlation functions</a>\nby Sebasti
 an Cespedes (IFT) as part of IFT-Madrid Webinars\n\n\nAbstract\nDeveloping
  our understanding of how correlations evolve during inflation is crucial 
 if we are to extract information about the early Universe from our late-ti
 me observables. To that end\, we’ll revisit the time evolution of scalar
  field correlators on de Sitter spacetime in the Schrodinger picture. By d
 irect manipulation of the Schrodinger equation\, it is possible to  write 
 down simple “equations of motion” for the coefficients which determine
  the wavefunction. Rather than specify a particular interaction Hamiltonia
 n\, we assume only very basic properties (unitarity\, de Sitter invariance
  and locality) to derive general consequences for the wavefunction’s evo
 lution. In particular\, we identify a number of “constants of motion”:
  properties of the initial state which are conserved by any unitary dynami
 cs. We further constrain the time evolution by deriving constraints from t
 he de Sitter isometries and show that these reduce to the familiar conform
 al Ward identities at late times. Finally\, we show how the evolution of a
  state from the conformal boundary into the bulk can be described via a nu
 mber of “transfer functions” which are analytic outside the horizon fo
 r any local interaction. These objects exhibit divergences for particular 
 values of the scalar mass\, and we show how such divergences can be remove
 d by a renormalisation of the boundary wavefunction—this is equivalent t
 o performing a “Boundary Operator Expansion” which expresses the bulk 
 operators in terms of regulated boundary operators. Altogether\, this impr
 oved understanding of the wavefunction in the bulk of de Sitter complement
 s recent advances from a purely boundary perspective\, and reveals new str
 ucture in cosmological correlators.\n
LOCATION:https://researchseminars.org/talk/IFTWeb/9/
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