Supercomputer support for the Astrophysics Group at the University of Exeter
Lead Research Organisation:
UNIVERSITY OF EXETER
Department Name: Physics
Abstract
The Astrophysics Group in the School of Physics at the University of Exeter urgently requires access to supercomputer time in order to conduct its numerical research. This research includes magnetohydrodynamical and radiation hydrodynamical modelling of star and planet formation and the interstellar medium and radiative transfer modelling of young stars and protoplanetary discs. In this application, we request STFC funding to purchase three years of computing resource on the Exeter supercomputer. We believe that providing funding for access charges to Exeter's local machine is the most cost-effective and rapid way for STFC to provide the Astrophysics Group with the supercomputer access and programming support it requires.
Organisations
Publications

Meru F
(2010)
Exploring the conditions required to form giant planets via gravitational instability in massive protoplanetary discs Giant planet formation in self-gravitating discs
in Monthly Notices of the Royal Astronomical Society

Lewis B
(2017)
The dependence of protostar formation on the geometry and strength of the initial magnetic field
in Monthly Notices of the Royal Astronomical Society

Meru F
(2012)
On the convergence of the critical cooling time-scale for the fragmentation of self-gravitating discs Convergence of fragmenting discs
in Monthly Notices of the Royal Astronomical Society

Bate M
(2012)
Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation Stellar and multiple star properties
in Monthly Notices of the Royal Astronomical Society

Duarte-Cabral A
(2017)
The evolution of giant molecular filaments
in Monthly Notices of the Royal Astronomical Society

Acreman D
(2015)
Modelling multiwavelength observational characteristics of bow shocks from runaway early-type stars
in Monthly Notices of the Royal Astronomical Society

Lorén-Aguilar P
(2015)
Two-fluid dust and gas mixtures in smoothed particle hydrodynamics II: an improved semi-implicit approach
in Monthly Notices of the Royal Astronomical Society

Harries T
(2011)
An algorithm for Monte Carlo time-dependent radiation transfer Time-dependent radiative transfer
in Monthly Notices of the Royal Astronomical Society

Ayliffe B
(2011)
Migration of protoplanets with surfaces through discs with steep temperature gradients Migration with steep temperature gradients
in Monthly Notices of the Royal Astronomical Society

Pettitt A
(2014)
The morphology of the Milky Way - I. Reconstructing CO maps from simulations in fixed potentials
in Monthly Notices of the Royal Astronomical Society

Bate M
(2011)
Collapse of a molecular cloud core to stellar densities: the formation and evolution of pre-stellar discs Formation and evolution of pre-stellar discs
in Monthly Notices of the Royal Astronomical Society

Pettitt A
(2015)
The morphology of the Milky Way - II. Reconstructing CO maps from disc galaxies with live stellar distributions
in Monthly Notices of the Royal Astronomical Society

Wurster J
(2017)
The impact of non-ideal magnetohydrodynamics on binary star formation
in Monthly Notices of the Royal Astronomical Society

Haworth T
(2013)
Assessing molecular line diagnostics of triggered star formation using synthetic observations
in Monthly Notices of the Royal Astronomical Society

Rey-Raposo R
(2017)
The roles of stellar feedback and galactic environment in star-forming molecular clouds
in Monthly Notices of the Royal Astronomical Society

Duarte-Cabral A
(2016)
What can simulated molecular clouds tell us about real molecular clouds?
in Monthly Notices of the Royal Astronomical Society

Acreman D
(2010)
Synthetic H i observations of a simulated spiral galaxy Synthetic observations of a spiral galaxy
in Monthly Notices of the Royal Astronomical Society

Bate M
(2018)
On the diversity and statistical properties of protostellar discs
in Monthly Notices of the Royal Astronomical Society

Lorén-Aguilar P
(2014)
Two-fluid dust and gas mixtures in smoothed particle hydrodynamics: a semi-implicit approach
in Monthly Notices of the Royal Astronomical Society

Harries T
(2015)
Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer - I. Algorithms and numerical methods
in Monthly Notices of the Royal Astronomical Society

Rundle D
(2010)
Three-dimensional molecular line transfer: a simulated star-forming region Three-dimensional molecular line transfer
in Monthly Notices of the Royal Astronomical Society

Dobbs C
(2017)
The properties, origin and evolution of stellar clusters in galaxy simulations and observations
in Monthly Notices of the Royal Astronomical Society

Helling C
(2016)
The mineral clouds on HD 209458b and HD 189733b
in Monthly Notices of the Royal Astronomical Society

Ayliffe B
(2012)
On the accumulation of planetesimals near disc gaps created by protoplanets Planetesimal accumulation near gaps
in Monthly Notices of the Royal Astronomical Society

Bate M
(2014)
Collapse of a molecular cloud core to stellar densities: stellar-core and outflow formation in radiation magnetohydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Description | This grant provided funding for research into star and planet formation. |
Exploitation Route | Via refereed journal articles. |
Sectors | Digital/Communication/Information Technologies (including Software) Education |
Description | Findings were published in refereed journal papers. Animations and images provided at http://www.astro.ex.ac.uk/people/mbate |
First Year Of Impact | 2009 |
Sector | Creative Economy,Education,Culture, Heritage, Museums and Collections |
Impact Types | Cultural |
Description | ERC Advanced Grant |
Amount | € 1,706,418 (EUR) |
Funding ID | No. 339248 |
Organisation | European Research Council (ERC) |
Sector | Public |
Country | Belgium |
Start | 03/2014 |
End | 02/2019 |
Description | STFC Consolidated Grant |
Amount | £1,734,000 (GBP) |
Funding ID | ST/J001627/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2012 |
End | 09/2015 |
Description | Website |
Form Of Engagement Activity | A magazine, newsletter or online publication |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Animations of some of my star formation calculations were placed on the web in 2008. These were used in: a movie to introduce the Nobeyama Observatory in 2009, a public television science programme called Newslight on Vara in the Netherlands in 2009, and a TV series "From the Big Bang to Life" produced in Canada in 2010. Animations placed on the web before 2006 have been used during the period 2006-present in the following ways: 4 different Planetarium shows in France (2), Germany, Newcastle; two books, a presentation at Singleton Hospital, Swansea NHS Trust, the `Universe Awareness' programme of Leiden University, a short documentary film produced by Experimentarium, a Science Centre in Denmark, and the German calendar `Bild der Wissenschaft". My animations were used in the various ways above to inform the general public about star formation. |
Year(s) Of Engagement Activity | 2008,2009,2010,2011,2012,2013,2014 |
URL | http://www.astro.ex.ac.uk/people/mbate |