The development of gravitational instabilities - RESCEU

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Mass of the field at 0.3 Mpc scale Mass of the field at 1 Mpc scale Mass of the field at 3 Mpc scale
Evolution of structure: from GR to modified gravity dynamics log a Mod. Grav. =Cte Horizon GR =0 k = m! log k k"k c k=k c k!k c
Page 1: Francis Bernardeau IPhT Saclay, Fra
Page 4 and 5: Which observables ? 〈δ x (k 1 )
Page 6 and 7: A self-gravitating expanding dust f
Page 8 and 9: ‣Motion equations in Fourier spac
Page 10 and 11: ‣ A lot is known at tree order Th
Page 12 and 13: A field theory reformulation Scocci
Page 14 and 15: Not a standard quantum field theory
Page 16: The closure theory Valageas P., A&A
Page 19 and 20: One key ingredient : the propagator
Page 21 and 22: ‣ RPT (Scoccimarro and Crocce) co
Page 23 and 24: Insights into higher order propagat
Page 25 and 26: ‣ This suggests another scheme :
Page 27 and 28: Comparison with numerical simulatio
Page 29 and 30: • Does it speed up the convergenc
Page 31 and 32: Using large-scale structure to test
Page 33: In presence of a dilaton field Brax
Page 37 and 38: Bispectra (equilateral configuratio

The development of gravitational instabilities - RESCEU

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