Quota Studentship 2012
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
Doctoral Training Partnerships: a range of postgraduate training is funded by the Research Councils. For information on current funding routes, see the common terminology at https://www.ukri.org/apply-for-funding/how-we-fund-studentships/. Training grants may be to one organisation or to a consortia of research organisations. This portal will show the lead organisation only.
Organisations
People |
ORCID iD |
Martin Ward (Training Grant Holder) |
Publications
Winther H
(2015)
Modified gravity N -body code comparison project
in Monthly Notices of the Royal Astronomical Society
Wilson J
(2015)
Evidence for explosive silicic volcanism on the Moon from the extended distribution of thorium near the Compton-Belkovich Volcanic Complex
in Journal of Geophysical Research: Planets
Wilkinson R
(2014)
Using the CMB angular power spectrum to study Dark Matter-photon interactions
in Journal of Cosmology and Astroparticle Physics
Townson M
(2018)
Generating artificial reference images for open loop correlation wavefront sensors
in Monthly Notices of the Royal Astronomical Society
Townson M
(2015)
Improved shift estimates on extended Shack-Hartmann wavefront sensor images
in Monthly Notices of the Royal Astronomical Society
Stern D
(2014)
NuSTAR AND XMM-NEWTON OBSERVATIONS OF LUMINOUS, HEAVILY OBSCURED, WISE -SELECTED QUASARS AT Z ~ 2
in The Astrophysical Journal
Springel V
(2019)
No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
in Monthly Notices of the Royal Astronomical Society
Schewtschenko J
(2015)
Dark matter-radiation interactions: the impact on dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Schewtschenko J
(2016)
Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
in Monthly Notices of the Royal Astronomical Society
Schewtschenko J
(2014)
Dark matter-radiation interactions: the impact on dark matter haloes
Schewtschenko J
(2015)
Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
Robertson A
(2016)
What does the Bullet Cluster tell us about self-interacting dark matter?
Robertson A
(2015)
Self-interacting dark matter scattering rates through cosmic time
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2015)
Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
Robertson A
(2017)
What does the Bullet Cluster tell us about self-interacting dark matter?
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2017)
Cosmic particle colliders: simulations of self-interacting dark matter with anisotropic scattering
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2018)
The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons
in Monthly Notices of the Royal Astronomical Society: Letters
Description | Celebrate Science 2013 |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Type Of Presentation | Workshop Facilitator |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Durham astronomy hosted a large stall, with lots of interactive exhibitions intended to teach young people about the role of dark matter in the Universe. Over 6500 people attended the event N/A |
Year(s) Of Engagement Activity | 2013 |
Description | Physicist of the Year Ceremony |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Type Of Presentation | Workshop Facilitator |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | This was an event funded by the Ogden Trust where all the local schools nominated a pupil who excelled in Physics to be awarded 'Physicist of the Year'. Before the award giving we had an hour to demonstrate some of the research going on in Durham University Physics. We had various demonstrations, including a hands-on demonstration of a pair of scales showing that the Universe does not weigh enough if we just use what we see. We had a gravitational lensing demonstration where the visitors were the mass bending the light (this used a Xbox kinect and Wii controller). We also had a 3D interactive simulation where you can scan around the dark matter Universe. N/A |
Year(s) Of Engagement Activity | 2013 |