DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
DiRAC-3 Operations 2019-2022 resubmission; This is an administrative resubmission to replace ST/S003800/1 which has already been peer-reviewed.
Organisations
Publications
Saló L
(2024)
GRFolres: A code for modified gravity simulations in strong gravity
in Journal of Open Source Software
Salvioni G
(2020)
Model nuclear energy density functionals derived from ab initio calculations
in Journal of Physics G: Nuclear and Particle Physics
Salcido J
(2020)
How feedback shapes galaxies: an analytic model
in Monthly Notices of the Royal Astronomical Society
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Saha B
(2024)
Quantifying the impact of AGN feedback on the large-scale matter distribution using two- and three-point statistics
in Monthly Notices of the Royal Astronomical Society
Saavedra-Bastidas J
(2024)
Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
in Astronomy & Astrophysics
Ryczanowski D
(2020)
What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
in Monthly Notices of the Royal Astronomical Society
Ruiz-Bonilla S
(2022)
Dealing with density discontinuities in planetary SPH simulations
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2022)
Towards an accurate model of small-scale redshift-space distortions in modified gravity
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Rowther S
(2024)
The role of drag and gravity on dust concentration in a gravitationally unstable disc
in Monthly Notices of the Royal Astronomical Society
Rowther S
(2024)
Short-lived gravitational instability in isolated irradiated discs
in Monthly Notices of the Royal Astronomical Society
Rouillard A
(2020)
Models and data analysis tools for the Solar Orbiter mission
in Astronomy & Astrophysics
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society
Rosenberg E
(2022)
CMB power spectra and cosmological parameters from Planck PR4 with CamSpec
in Monthly Notices of the Royal Astronomical Society
Roper W
(2022)
First Light And Reionisation Epoch Simulations ( flares ) - IV. The size evolution of galaxies at z = 5
in Monthly Notices of the Royal Astronomical Society
Roper W
(2023)
First light and reionization epoch simulations (FLARES) IX: the physical mechanisms driving compact galaxy formation and evolution
in Monthly Notices of the Royal Astronomical Society
Roper F
(2023)
The diversity of rotation curves of simulated galaxies with cusps and cores
in Monthly Notices of the Royal Astronomical Society
Rogers J
(2024)
Under the light of a new star: evolution of planetary atmospheres through protoplanetary disc dispersal and boil-off
in Monthly Notices of the Royal Astronomical Society
Robson D
(2020)
X-ray emission from hot gas in galaxy groups and clusters in simba
in Monthly Notices of the Royal Astronomical Society
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Robins L
(2020)
Viscous and inviscid strato-rotational instability
in Journal of Fluid Mechanics
Robertson A
(2020)
Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2024)
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award. |
| Exploitation Route | Many international collaborative projects are supported by our results |
| Sectors | Aerospace Defence and Marine Digital/Communication/Information Technologies (including Software) Education |