no code implementations • 9 May 2022 • Luisa Lucie-Smith, Susmita Adhikari, Risa H. Wechsler
We find two primary scales in the initial conditions (ICs) that impact the final mass profile: the density at approximately the scale of the haloes' Lagrangian patch $R_L$ ($R\sim 0. 7\, R_L$) and that in the large-scale environment ($R\sim 1. 7~R_L$).
1 code implementation • 6 Feb 2017 • Eric Baxter, Chihway Chang, Bhuvnesh Jain, Susmita Adhikari, Neal Dalal, Andrey Kravtsov, Surhud More, Eduardo Rozo, Eli Rykoff, Ravi K. Sheth
Using data from SDSS, we explore the evidence for such a feature in the density profiles of galaxy clusters and investigate the connection between this feature and a possible phase space boundary.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies