activity
20182022
most citedSimulating the effect of photoheating feedback during reionization

32 citations · 57 across the 4 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2020

Arepo-MCRT: Monte Carlo Radiation Hydrodynamics on a Moving Mesh

Aaron Smith, Rahul Kannan, Benny T. -H. Tsang +2

We present Arepo-MCRT, a novel Monte Carlo radiative transfer (MCRT) radiation-hydrodynamics (RHD) solver for the unstructured moving-mesh code Arepo. Our method is designed for ge…

astro-ph.GA2020

Dust entrainment in galactic winds

Rahul Kannan, Mark Vogelsberger, Federico Marinacci +3

Winds driven by stellar feedback are an essential part of the galactic ecosystem and are the main mechanism through which low-mass galaxies regulate their star formation. These win…

astro-ph.GA20196 cited

Simulating dust grain-radiation coupling on a moving mesh

Ryan McKinnon, Rahul Kannan, Mark Vogelsberger +3

We present a model for the interaction between dust and radiation fields in the radiation hydrodynamic code AREPO-RT, which solves the moment-based radiative transfer equations on…

astro-ph.GA2019

Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust

Rahul Kannan, Federico Marinacci, Mark Vogelsberger +4

We present a novel framework to self-consistently model the effects of radiation fields, dust physics and molecular chemistry (H) in the interstellar medium (ISM) of galaxies.…

astro-ph.GA2019

Local photoionization feedback effects on galaxies

Aura Obreja, Andrea V. Macciò, Benjamin Moster +5

We implement an optically thin approximation for the effects of the local radiation field from stars and hot gas on the gas heating and cooling in the N-body SPH code GASOLINE2. We…

astro-ph.CO2019

Imprints of temperature fluctuations on the Lyman- forest: a view from radiation-hydrodynamic simulations of reionization

Xiaohan Wu, Matthew McQuinn, Rahul Kannan +5

Reionization leads to large spatial fluctuations in the intergalactic temperature that can persist well after its completion. We study the imprints of such fluctuations on the $z\s…