Results for Technology
53,864 grants found
Showing 3,741 – 3,760 of 53,864 grants for "Technology"
What lies beneath the surface of Mars? Advanced Numerical Modelling and Data Intensive Processing for Large and Complex Ground Penetrating Radar Data
Planetary subsurface exploration is a rapidly growing international scientific endeavour and a key part of the UK's Space Science Programme. The primary tool for surface and subsur...
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Edinburgh Nuclear Physics Consolidated Grant 2024-27
Our research program seeks to answer key open questions on the origin of the elements in stars, the processes responsible for stellar explosions, and the behaviour of nuclei at the...
Liquid sunshine - Modelling of coronal rain in the quiescent and flaring solar corona
The solar corona, the most extended layer of the solar atmosphere, is home to extremely energetic processes like magnetic reconnection that can dramatically heat up the gas to tens...
Particle Physics
Investigation into the properties of elementary particles and the fundamental forces of nature. Precision tests of the Standard Model (SM); searches for new phenomena and extension...
Neutrinos as evidence for dark matter and noevl detector technologies with Liquid0
Explaining the dark matter content of the universe is one of the major challenges in Particle Physics today. Neutrino detectors provide the exciting possibility of detecting neutri...
Electromagnetic Sounding of Ocean Worlds
If we eventually find extra-terrestrial life in the Solar System it will probably be found inside an ocean world. These are a handful of large, almost planet-sized moons orbiting J...
Deep learning for dark matter and dark sirens
In this project we will apply machine learning and data science techniques, such as data compression via geometric deep learning and inference via neural density estimation, to con...
UofG Nuclear Physics Consolidated Grant
The overarching goal of our research programme is to address aspects of the broad science challenge: "What are the basic constituents of matter and how do they interact?"...
WIMP dark matter searches with the LZ experiment
Searches for WIMP dark matter with LZ
Measuring the size of the Universe with type Ia supernova
The Universe is currently undergoing a period of rapid accelerated expansion. This discovery, suggesting that 75% of the energy budget of the Universe is unexplained represents the...
Axion Miniclusters, Radio Telescopes, and other observations
We will study the transient radio signature produced when dark matter clumps known as axion miniclusters encounter neutron stars. We will statistically model the population of both...
Modelling the destructive formation of moons and rings
We do not know where Mars's moons came from, nor how Saturn's rings and icy moons formed. Their origins are among the longest-running unsolved problems in planetary science, and ar...
Unusual planetary systems with massive debris disks
Debris disks are dusty disks of material around main sequence stars, revealed by their far-infrared excess emission. Collisions between asteroids or Kuiper Belt Objects generate sm...
X-Ray Emissions from the Uranian System
The project involves modelling potential x-ray emissions from Uranus's magnetosheath. The x-rays are created through solar wind charge exchange between neutral particles from Uranu...
Neutrino physics and astrophysics with the P-ONE neutrino telescope
The research supported by this scholarship will concentrate on the development of hardware, software, and analysis techniques for the Pacific Ocean Neutrino Experiment (P-ONE), wit...
Radiation damage in detectors: what really happens to silicon imaging detectors in orbit?
The Euclid mission, launched in July 2023, is an ESA space mission with the objective of mapping the geometry of the Universe to better understand dark matter and dark energy. Whil...
Probabilistic deep learning for cosmology and beyond
The current evolution of our Universe is dominated by the influence of dark energy and dark matter, which constitute 95% of its content. However, an understanding of the fundamenta...
The magnetic and thermodynamic properties of small-scale solar magnetic structures
"Magnetic flux emerges from the convection zone to the solar surface over an enormous range of spatial (100 km - 100,000 km) and temporal (seconds to months) scales. The turbu...
Supermassive black holes: Engines of the Universe
Our Universe developed hierarchically: small perturbations led to stars, then galaxies, which clustered into 'galaxy-groups' and 'galaxy-clusters', regions where the galaxy density...