DiRAC 2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
University of Cambridge
Department Name: Applied Maths and Theoretical Physics
Abstract
Refer to parent proposal from Leicester - Joint reference: T2414701
Planned Impact
Refer to parent proposal from Leicester - Joint reference: T2414701
Organisations
Publications
Bourne Martin A.
(2019)
AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
in arXiv e-prints
Katz Harley
(2018)
A Census of the LyC Photons that Form the UV Background During Reionization
in ArXiv e-prints
Hu Shaoran
(2017)
Impact of Cosmological Satellites on Stellar Discs: Dissecting One Satellite at a Time
in ArXiv e-prints
Katz Harley
(2016)
Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
in ArXiv e-prints
Fiacconi Davide
(2017)
Galaxy formation simulations with spinning black holes: method and implementation
in ArXiv e-prints
Costa Tiago
(2017)
Quenching star formation with quasar outflows launched by trapped IR radiation
in ArXiv e-prints
Smith Matthew C.
(2017)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in ArXiv e-prints
Davies C
(2018)
Improving the theoretical prediction for the B s - B¯ s width difference: matrix elements of next-to-leading order ? B = 2 operators
in EPJ Web of Conferences
Cheung G
(2017)
Tetraquark operators in lattice QCD and exotic flavour states in the charm sector
in Journal of High Energy Physics
Bourne M
(2017)
AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
in Monthly Notices of the Royal Astronomical Society
Sembolini F
(2016)
nIFTy galaxy cluster simulations - II. Radiative models
in Monthly Notices of the Royal Astronomical Society
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Smith Matthew C.
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Bolton J
(2017)
The Sherwood simulation suite: overview and data comparisons with the Lyman a forest at redshifts 2 = z = 5
in Monthly Notices of the Royal Astronomical Society
Henden N
(2018)
The FABLE simulations: a feedback model for galaxies, groups, and clusters
in Monthly Notices of the Royal Astronomical Society
Fiacconi D
(2018)
Galactic nuclei evolution with spinning black holes: method and implementation
in Monthly Notices of the Royal Astronomical Society
Katz H
(2019)
Tracing the sources of reionization in cosmological radiation hydrodynamics simulations
in Monthly Notices of the Royal Astronomical Society
Henden N
(2018)
The FABLE simulations: a feedback model for galaxies, groups, and clusters
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Quenching star formation with quasar outflows launched by trapped IR radiation
in Monthly Notices of the Royal Astronomical Society
Fiacconi D
(2018)
Galactic nuclei evolution with spinning black holes: method and implementation
in Monthly Notices of the Royal Astronomical Society
Hu S
(2018)
Impact of cosmological satellites on stellar discs: dissecting one satelliteat a time
in Monthly Notices of the Royal Astronomical Society
Cashmore C
(2017)
Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
in Monthly Notices of the Royal Astronomical Society
Rorai A
(2017)
Exploring the thermal state of the low-density intergalactic medium at z = 3 with an ultrahigh signal-to-noise QSO spectrum
in Monthly Notices of the Royal Astronomical Society
Kulkarni G
(2016)
Models of the cosmological 21 cm signal from the epoch of reionization calibrated with Ly a and CMB data
in Monthly Notices of the Royal Astronomical Society
Iršic V
(2016)
The Lyman-alpha forest power spectrum from the XQ-100 Legacy Survey
in Monthly Notices of the Royal Astronomical Society