Cosmological Neutrino N-Body Simulations of Dark Matter Halo

Author:

Chen Yu12,Lu Chang-Zhi12,Li Juan23,Liu Siqi45,Zhang Tong-Jie126ORCID,Zhang Tingting7

Affiliation:

1. Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China

2. Department of Astronomy, Beijing Normal University, Beijing 100875, China

3. College of Physics and Electronic Engineering, Qilu Normal University, Jinan 250200, China

4. University of Chinese Academy of Sciences, Beijing 100049, China

5. CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Beijing 100101, China

6. Institute for Astronomical Science, Dezhou University, Dezhou 253023, China

7. College of Command and Control Engineering, PLA Army Engineering University, Nanjing 210001, China

Abstract

The study of massive neutrinos and their interactions is a critical aspect of contemporary cosmology. Recent advances in parallel computation and high-performance computing provide new opportunities for accurately constraining Large-Scale Structures (LSS). In this paper, we introduce the TianNu cosmological N-body simulation during the co-evolution of massive neutrino and cold dark matter components via the CUBEP3M code running on the supercomputer Tianhe-2 and TianNu’s connected works. We start by analyzing 2.537×107 dark halos from the scientific data of TianNu simulation, and compare their angular momentum with the matched halos from neutrino-free TianZero, revealing a dependence of angular momentum modulus on neutrino injection at scales below 50 Mpc and around 10 Mpc.

Funder

National Science Foundation of China

Publisher

MDPI AG

Subject

General Physics and Astronomy

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