Spin mode reconstruction in Lagrangian space

نویسندگان

چکیده

Galaxy angular momentum directions (spins) are observable, well described by the Lagrangian tidal torque theory, and proposed to probe primordial universe. They trace spins of dark matter halos, indicators protohalos properties in space. We define a spin parameter twist parameters quantify their influence on conservation predictability mode reconstruction $N$-body simulations. conclude that more twisting environments preferentially rotation-supported, likely conserve direction through cosmic evolution. These magnitudes predictable density space, such predictions can improve correlation between galaxy initial conditions study constraining universe reconstruction.

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ژورنال

عنوان ژورنال: Physical review

سال: 2021

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.103.063522