Tidal alignment and tidal torquing modeling for the cosmic shear three-point correlation function and mass aperture skewness
Rafael C. H. Gomes, Kyle Miller, Sunao Sugiyama, Jonathan Blazek, Thomas Bakx, Bhuvnesh Jain
TL;DR
This work develops a tidal alignment and tidal torquing (TATT) based model for intrinsic alignment contamination of the cosmic shear three-point correlation function (3PCF) and the mass aperture skewness $\langle M_{ap}^3 \rangle$. It connects EFT-based IA bispectra to TATT parameters ($C_1$, $C_2$, $C_{1\delta}$) and includes a velocity-shear extension ($C_t$), with Limber projections to observable convergence statistics. Using DES Year 3 posteriors, they show that higher-order IA terms substantially modify the 3PCF across triangle configurations and that including higher-order IA terms can dampen the two-point signal while boosting the mass aperture skewness, highlighting the value of joint 2PCF+3PCF analyses to break degeneracies and tighten cosmological and IA constraints. The results underscore the importance of incorporating complex IA models for Stage IV surveys and provide an emulator-ready framework for $\langle M_{ap}^3 \rangle$ analyses.
Abstract
We present a model for the intrinsic alignment contamination of the shear three-point correlation function and skewness of the mass aperture statistic using the tidal alignment and tidal torquing (TATT) formalism. We compute the intrinsic alignment bispectra components in terms of the TATT model parameters. We consider two effective field theory approaches in the literature, relate them to the TATT model parameters and an extension to TATT that includes the velocity-shear (VS) parameter. We compare the impact of changing between NLA, TATT, and TATT+VS on the theoretical computation of the 3PCF using the best fit parameters and tomographic redshift distributions from Dark Energy Survey Year 3. We find that the TATT model significantly impacts the skewed triangle configurations of the 3PCF. Additionally, including the higher-order effects from TATT can introduce opposite effects on the two-point function and on the mass aperture skewness, damping the signal of the former while boosting the signal of the latter. We argue that a joint 2PCF+3PCF analysis with the TATT model can help break the degeneracy between its model parameters and provide more robust constraints on both cosmology and intrinsic alignment amplitude parameters. We show that typical values of order unity for the intrinsic alignment parameters introduce differences of around $10\%$ between NLA and TATT predictions.
