transparencies (pdf) - Rencontres du Vietnam

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cosmic strings as seeds of structure formation DX = S for given initial conditions, this eq. can be solved by means of a green’s function: X j (ñ 0 , k) = R ñ in ñ 0 G jm (ñ 0 ,ñ,k) we want to compute quadratic expectation values of the form: hX j (ñ 0 , k)X ? l (ñ 0, k 0 )i = R ñ 0 ñ in dñG jm (ñ, k) R ñ 0 ñ in dñ 0 G ? ln (ñ0 , k 0 )âhS m (ñ, k)S ? n (ñ0 , k 0 )i 1 hindmarsh 1995 unequal time 2-pt correlators heavy numerical simulations ! 1 production of topological defects at the end of inflation mairi sakellariadou vi th rencontres du vietnam
cmb power spectrum from cosmic strings using field 1 evolution simulation of the Abelian Higgs model 1 WMAP cosmic strings global textures a roughly constant slope at low multipoles, rising up to a single peak at ` ù 400 , with decay at small scales ` =10 WMAP normalisation Gö =2â 10 à6 1 ö ø T 2 crit 1 bevis, hindmarsh, kunz & urrestilla 2006 production of topological defects at the end of inflation mairi sakellariadou vi th rencontres de vietnam
Page 1 and 2: production of topological defects a
Page 3 and 4: motivation however the inflationary
Page 5 and 6: topological defect formation and ha
Page 7: cosmic string network evolution lon
Page 11 and 12: 1 compute one-loop radiative correc
Page 13 and 14: D-term hybrid inflation in supergra
Page 15 and 16: how generic is cosmic strings forma
Page 17 and 18: E 6 non-thermal leptogenesis and :
Page 19 and 20: cosmic superstring formation in bra
Page 21 and 22: mixed models: anisotropies in the c
Page 23 and 24: curvaton mechanism: ψ init ô 5 â
Page 25 and 26: consider a curvaton mechanism: Cont
Page 27 and 28: • keep all corrections up to the
Page 29 and 30: spectral index for various values o
Page 31: conclusions cosmic strings/superstr

transparencies (pdf) - Rencontres du Vietnam

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