Evolution of energy, momentum, and spin parameter in dark matter flow and integral constants of motion

preprint2022arXivOpen access

Abstract

N-body equations of motion in comoving system and expanding background are reformulated in a transformed system with static background and fixed damping. The energy and momentum evolution in dark matter flow are rigorously formulated for both systems. The energy evolution in transformed system has a simple form that is identical to the damped harmonic oscillator. The cosmic energy equation can be easily derived in both systems. For entire N-body system, 1) combined with the two-body collapse model (TBCM), kinetic and potential energy increase linearly with time tt such that Kp=εutK_p=\varepsilon_ut and Py=−7εut/5P_y=-7\varepsilon_ut/5, where εu\varepsilon_u is a constant rate of energy cascade; 2) an effective gravitational potential exponent ne=−10/7≠−1n_e=-10/7\ne-1 (ne=−1.38n_e=-1.38 from simulation) can be identified due to surface energy of fast growing halos; 3) the radial momentum G∝a3/2G\propto a^{3/2} and angular momentum H∝a5/2H\propto a^{5/2}, where aa is the scale factor. On halo scale, 1) halo kinetic and potential energy can be modelled by two dimensionless constants αs∗α_s^* and βs∗β_s^*. Both constants are independent of time and halo mass; 2) both halo radial and angular momentum ∝a3/2\propto a^{3/2} and can be modeled by two mass-dependent coefficients τs∗τ_s^* and ηs∗η_s^*; 3) halo spin parameter is determined by αs∗α_s^* and ηs∗η_s^* and decreases with halo mass with derived values of 0.09 and 0.031 for small and large halos. Finally, the radial and angular momentum are closely related to the integral constants of motion ImI_m, i.e. the integral of velocity correlation or the mmth derivative of energy spectrum at long wavelength limit. On large scale, angular momentum is negligible, I2I_2=0 reflects the conservation of linear momentum, while I4I_4 reflects the fluctuation of radial momentum GG. On halo scale, I4I_4 is determined by both momentum that are comparable with each other.

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