HPC Resources for Theoretical Astrophysics at the University of Leicester
Lead Research Organisation:
University of Leicester
Department Name: Physics and Astronomy
Abstract
Accretion on to a black hole is the most efficient way of extracting energy from conventional matter. Gravitational energy thus powers the most luminous objects in the Universe. At the same time, gravity's cumulative nature gives it a decisive role in determining the structure and evolution of matter at all scales. The theoretical understanding of these twin aspects -- accretion, and the structure and evolution of the parent systems -- are the key theme of our research, in various cosmic contexts. On the smallest scale, close binary systems containing black holes offer a highly tractable route to studying accretion processes such as disc formation and stability. But it is important also to understand the long--term evolution of these binaries themselves, and the standard and ultraluminous X--ray populations of other galaxies. Similarly, astronomers want to understand how accretion on to supermassive black holes (SMBH) powers active galactic nuclei (AGN). But they also wish to know how these objects fit into the general picture of galaxy structure and formation. Gamma--ray bursts (GRBs) offer another example where the study of accretion processes is closely linked to understanding the host galaxy, and stellar and binary evolution within it. Dark matter provides the potential wells within which structures form and evolve and we therefore need to understand its physical properties in order to have a complete theory of structure formation in the Universe. We study all of these objects theoretically, and our emphasis has shifted strongly towards supermassive/extra\-galactic systems over the last decade.
Organisations
Publications
Zubovas K
(2013)
Outflows of stars due to quasar feedback
in Monthly Notices of the Royal Astronomical Society
Fletcher M
(2016)
Planets, debris and their host metallicity correlations
in Monthly Notices of the Royal Astronomical Society
Dunhill A
(2015)
Precession and accretion in circumbinary discs: the case of HD 104237
in Monthly Notices of the Royal Astronomical Society
Belokurov V
(2014)
Precession of the Sagittarius stream
in Monthly Notices of the Royal Astronomical Society
Dhanoa H
(2014)
Pressure-driven fragmentation of multiphase clouds at high redshift
in Monthly Notices of the Royal Astronomical Society
Power C
(2009)
Primordial globular clusters, X-ray binaries and cosmological reionization
in Monthly Notices of the Royal Astronomical Society
Kacharov N
(2017)
Prolate rotation and metallicity gradient in the transforming dwarf galaxy Phoenix
in Monthly Notices of the Royal Astronomical Society
Nayakshin S
(2013)
Radiative feedback from protoplanets in self-gravitating protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Katz H
(2015)
Seeding high-redshift QSOs by collisional runaway in primordial star clusters
in Monthly Notices of the Royal Astronomical Society
Assmann P
(2011)
Star cluster collisions - a formation scenario for the extended globular cluster Scl-dE1 GC1 Formation scenario for Scl-dE1 GC1
in Monthly Notices of the Royal Astronomical Society
Frank M
(2015)
Strömgren uvby photometry of the peculiar globular cluster NGC 2419
in Astronomy & Astrophysics
Zubovas K
(2013)
SUPERNOVAE IN THE CENTRAL PARSEC: A MECHANISM FOR PRODUCING SPATIALLY ANISOTROPIC HYPERVELOCITY STARS
in The Astrophysical Journal
Nixon C
(2012)
TEARING UP THE DISK: HOW BLACK HOLES ACCRETE
in The Astrophysical Journal
Dunhill A
(2013)
The curiously circular orbit of Kepler-16b
in Monthly Notices of the Royal Astronomical Society
Hague P
(2015)
THE DEGENERACY OF M33 MASS MODELING AND ITS PHYSICAL IMPLICATIONS
in The Astrophysical Journal
Alexander R
(2012)
THE DISPERSAL OF PROTOPLANETARY DISKS AROUND BINARY STARS
in The Astrophysical Journal
Gingell P
(2015)
The impact of a hot sodium ion population on the growth of the Kelvin-Helmholtz instability in Mercury's magnetotail
in Journal of Geophysical Research: Space Physics
Martin R
(2014)
THE KOZAI-LIDOV MECHANISM IN HYDRODYNAMICAL DISKS
in The Astrophysical Journal
Cole D
(2012)
The mass distribution of the Fornax dSph: constraints from its globular cluster distribution The mass distribution of the Fornax dSph
in Monthly Notices of the Royal Astronomical Society
Nayakshin S
(2012)
THE OBSERVED M -s RELATIONS IMPLY THAT SUPER-MASSIVE BLACK HOLES GROW BY COLD CHAOTIC ACCRETION
in The Astrophysical Journal
Nayakshin S.
(2020)
The paradox of youth for ALMA planet candidates
in Monthly Notices of the Royal Astronomical Society
Pascucci I
(2011)
THE PHOTOEVAPORATIVE WIND FROM THE DISK OF TW Hya
in The Astrophysical Journal
Tanvir N
(2012)
The structure of star clusters in the outer halo of M31 Halo star clusters of M31
in Monthly Notices of the Royal Astronomical Society
Gingell P
(2015)
THE THREE-DIMENSIONAL EVOLUTION OF ION-SCALE CURRENT SHEETS: TEARING AND DRIFT-KINK INSTABILITIES IN THE PRESENCE OF PROTON TEMPERATURE ANISOTROPY
in The Astrophysical Journal
Cioni M
(2011)
The VMC survey I. Strategy and first data
in Astronomy & Astrophysics
Nayakshin S
(2015)
Tidal Downsizing model - III. Planets from sub-Earths to brown dwarfs: structure and metallicity preferences
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
Nayakshin S
(2014)
Two-phase model for black hole feeding and feedback
in Monthly Notices of the Royal Astronomical Society
Hands T
(2014)
Understanding the assembly of Kepler's compact planetary systems
in Monthly Notices of the Royal Astronomical Society
Cole D
(2011)
Weakening dark matter cusps by clumpy baryonic infall Weakening dark matter cusps by baryonic infall
in Monthly Notices of the Royal Astronomical Society
Muldrew S
(2015)
What are protoclusters? - Defining high-redshift galaxy clusters and protoclusters
in Monthly Notices of the Royal Astronomical Society
Description | DiRAC2: Recurrent Costs for 100 Tflop/s HPC cluster |
Amount | £391,000 (GBP) |
Funding ID | ST/K003259/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 05/2012 |
End | 01/2016 |
Description | Astronomy Ireland |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Type Of Presentation | Keynote/Invited Speaker |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | I spoke to about 100 people at the Astronomy Ireland meeting in November 2013 in Trinity College Dublin. My talk was very well received and I have been invited to give another talk to this audience at a later date. |
Year(s) Of Engagement Activity | 2013 |
URL | http://www.astronomy.ie/lecture201311.php |
Description | BBC Stargazing Live |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Type Of Presentation | Keynote/Invited Speaker |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Presentations as part of the BBC Stargazing Live at the National Space Centre and at the University of Leicester, attended by approximately 50 people (2011), 50 people (2012), 300 people (2013), 100 people (2014). The presentation generated lots of questions and discussion from the audience. Local schools had an opportunity to visit the University which is good for inclusivity. |
Year(s) Of Engagement Activity | 2011,2012,2013,2014 |
Description | Cafe Scientifique |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Type Of Presentation | Keynote/Invited Speaker |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | I spoke to the Nottingham Cafe Scientifique about various aspects of the research that myself and others are doing with DiRAC. About 40 people attended. I gave a 25 minute presentation which was followed by more than an hour of questions and discussion. One audience member wrote a blog piece about my talk. |
Year(s) Of Engagement Activity | 2014 |
URL | http://nottinghamscience.blogspot.co.uk/2014/02/talk-building-galaxies-in-office.html |
Description | Royal Society Summer Exhibition |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | Yes |
Geographic Reach | National |
Primary Audience | Schools |
Results and Impact | Over the course of the four day, more than 600 people attended my talks. The Friday evening presentation was followed by more than an hour of audience questions. Several audience members contacted me to ask additional questions. |
Year(s) Of Engagement Activity | 2014 |
Description | School Visit (Dublin) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Type Of Presentation | Keynote/Invited Speaker |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | Approximately 90 primary school students (3 classes) aged 8-12 years old attended my talks in Rathfarnham Parish National School. Following my visit, a number of students expressed interest in pursuing a career in science. |
Year(s) Of Engagement Activity | 2013 |
Description | Secular Society |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Type Of Presentation | Keynote/Invited Speaker |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Spoke to about 50 members of the Leicester Secular Society. My talk generated considerable discussion among the members of the LSS. |
Year(s) Of Engagement Activity | 2012 |
URL | http://www.leicestersecularsociety.org.uk/calendar/view_entry.php?id=1145&date=20121209 |