Tuesdays 10:30 - 11:30 | Fridays 11:30 - 12:30
Showing votes from 2017-07-18 11:30 to 2017-07-21 12:30 | Next meeting is Tuesday May 12th, 10:30 am.
We compute the weak lensing convergence power spectrum, $C^{\kappa\kappa}(\theta)$, in a dust-filled universe using fully non-linear general relativistic simulations. The spectrum is then compared to more standard, approximate calculations by computing the Bardeen (Newtonian) potentials in linearized gravity and utilizing the Born approximation. We find corrections to the angular power spectrum amplitude of order ten percent at very large angular scales, $\ell \sim 2-3$, and percent-level corrections at intermediate angular scales of $\ell \sim 20-30$.