activity
20152020
most citedPrecision reconstruction of the dark matter-neutrino relative velocity from N-body simulations

55 citations · 67 across the 5 of their papers we have counts for

collaborators

15 papers

astro-ph.CO20207 cited

Spin Mode Reconstruction in Lagrangian Space

Qiaoya Wu, Hao-Ran Yu, Shihong Liao +1

Galaxy angular momentum directions (spins) are observable, well described by the Lagrangian tidal torque theory, and proposed to probe the primordial universe. They trace the spins…

math.QA2020

A Very Simple Estimate Of Rational Homological Dimension Of Moduli Spaces Of Riemann Surfaces With Boundary And Marked Points

Hao Yu

The moduli spaces of compact and connected Riemann surfaces has been a central topic in modern mathematics in recent years. Thus their homological dimensions become important invar…

astro-ph.CO2020

Neutrino effects on the morphology of cosmic large-scale structure

Yu Liu, Yu Yu, Hao-Ran Yu +1

In this work, we propose a powerful probe of neutrino effects on the large-scale structure (LSS) of the Universe, i.e., Minkowski functionals (MFs). The morphology of LSS can be fu…

astro-ph.CO2020

Observational detection of correlation between galaxy spins and initial conditions

Pavel Motloch, Hao-Ran Yu, Ue-Li Pen +1

Galaxy spins can be predicted from the initial conditions in the early Universe through the tidal tensor twist. In simulations, their directions are well preserved through cosmic t…

physics.comp-ph2020

CUBE -- Towards an Optimal Scaling of Cosmological N-body Simulations

Shenggan Cheng, Hao-Ran Yu, Derek Inman +3

N-body simulations are essential tools in physical cosmology to understand the large-scale structure (LSS) formation of the Universe. Large-scale simulations with high resolution a…

astro-ph.CO20201 cited

Simulating the Cosmic Neutrino Background using Collisionless Hydrodynamics

Derek Inman, Hao-ran Yu

The cosmic neutrino background is an important component of the Universe that is difficult to include in cosmological simulations due to the extremely large velocity dispersion of…