From the 1 of 14 linked papers with an AI index.
14 papers
RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime
Ruby J. Wright, Roosa Heiskanen, Shihong Liao +5
The authors run high‑resolution galaxy merger simulations to examine how the strength of stellar feedback influences the delay between galaxy coalescence and the merger of supermas…
First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation
Paurush Punyasheel, Aswin P. Vijayan, William J. Roper +8
Recent observations have revealed intriguing offsets between the UV and FIR emission in high redshift galaxies. In this study, we use the First Light And Reionisation Epoch Simulat…
Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity
Wangzheng Zhang, Ming-chung Chu, Shihong Liao
Cosmic neutrinos are among the most abundant fermions in the Universe, yet the values of their masses and chemical potentials remain uncertain. In this Letter, we present the first…
The Quenching Mechanisms of Field Dwarf Galaxies
Zuoyu Wu, Yougang Wang, Shihong Liao
Isolated dwarf galaxies are intrinsically faint and difficult to detect. The limited sample size makes it challenging to observationally constrain the physical mechanisms that quen…
RABBITS - III. Modelling relativistic accretion discs around spinning black holes in galaxy formation simulations
Dimitrios Irodotou, Shihong Liao, Theodoros Nakas +6
In this third study of the 'Resolving supermAssive Black hole Binaries In galacTic hydrodynamical Simulations' (RABBITS) series we develop and implement a geometrically thin relati…
Halo abundance and clustering in cosmologies with massive and asymmetric neutrinos
Yizhou Liu, Wangzheng Zhang, Shihong Liao +1
Neutrinos are the most abundant fermions in the Universe and influence the formation of large-scale structure through both their non-zero masses and a possible chemical potential w…