缅北轮奸

缅北轮奸 the Project

Reconfigurable Hardware for Thermodynamic Computing

Federico's current research focuses on developing novel quantum devices for thermodynamic computing, an emerging computing paradigm that seeks to harness noise and thermal dissipation as computational resources to improve efficiency and enable new forms of information processing.

缅北轮奸 the Project

MC PDF: Mapping the diversity of Type Ia supernovae explosions

Type Ia supernovae (SNe Ia) are powerful white dwarf explosions that astronomers use to measure the expansion of the universe. They’ve been essential in discovering dark energy, but not all of them behave the same way, with some “peculiar” ones showing unexpected brightness and evolution. The project aims to understand these unusual explosions by studying the galaxies they occur in and estimating how old their parent star systems are. Using data from the Zwicky Transient Facility (), it will build the largest consistent sample of these peculiar events and compare them to theoretical models of how white dwarfs explode. The goal is to map out the full diversity of these supernovae, figure out their origins, and help ensure that future surveys like the Vera Rubin, Legacy Survey of Space and Time () can use only the most reliable ones for studying the universe.

缅北轮奸 the Project

Understanding the Energy Pathways of Earth's Magnetosphere

Electronic devices are part of our everyday lives. They allow us to message each other, provide energy for our homes, and control critical systems like air traffic, but they are vulnerable. Space Weather describes how electric and magnetic fields change around Earth. Just like normal weather, there are storms in space and when a Space Weather "geomagnetic storm" happens, our electronic devices can be damaged so it is extremely important that we can predict when these storms will happen. Maria's fellowship aims to gain new insights into space weather events, specifically looking into how energy unloading occurs during geomagnetic storms, using a combination of data from spacecraft and ground-based observatories to understand the amount of energy that is put into the magnetosphere and how this changes over time.

缅北轮奸 the Project

ECF: Towards Energy-efficient Nanodevices based on Quantum Interference (ENano)

The ENano project (Towards Energy-efficient Nanodevices based on Quantum Interference) aims to explore the use of individual molecules as functional components in electronic devices, particularly memristors. By leveraging quantum interference effects, the project seeks to design molecular-scale devices with tunable electrical properties, offering a potential pathway toward ultra-low-power computing technologies. This is especially relevant in the context of the rapidly increasing energy demands of artificial intelligence, where new device paradigms are needed to improve efficiency beyond conventional silicon-based electronics.

缅北轮奸 the Project

Pushing the boundaries of superfluid vacuum and coherence

Samuli's EPSRC fellowship supports investigations of the interfaces between classical and quantum physics in superfluid 3He, aiming to answer questions such as “what does it feel like to touch a quantum fluid” and “can we melt a time crystal”. He is also working on a superfluid-based dark matter detector, laboratory simulations of phase transitions in the early universe, and neutron star superfluid and vortex dynamics.

缅北轮奸 the Project

Quantum-Interference-Enhanced Thermolectric Materials

This research addresses the climate crisis by developing technologies to reclaim low-level waste heat from data centres, industry, and the human body. By exploiting room-temperature quantum effects, the project aims to design molecular-scale materials with a high dimensionless figure of merit (ZT). These materials will enable efficient, solid-state energy harvesting via the Seebeck effect and advanced on-chip Peltier-cooling for CMOS devices, providing a silent and sustainable alternative to traditional energy management.

缅北轮奸 the Project

MSI: ERC:MesoPhone

Edward's ERC project studied some the smallest moving objects that can be fabricated – carbon nanotubes, which vibrate like tiny guitar strings. Because they are so small and so light, they are ideal for measuring tiny forces, such as those due to quantum tunnelling by electrons, or due to residual damping in superfluids. As well as being a fascinating way to study quantum effects in electronics, they may one day allow for new types of microscope. The project allowed Professor Laird to establish his lab in the low-temperature group.

缅北轮奸 the Project

Superfluid 3He Far from Equilibrium

The Fellowship project titled “Superfluid 3He Far from Equilibrium” was aimed at investigating the reason behind unexpectedly fast superfluid flows in 3He. The Fellowship has allowed to build a strong team of physicists who managed to explain this mystery. The project has also allowed the creation of new, precise instruments enabling exploration of other physics phenomena far beyond what was envisaged initially in the proposal.

缅北轮奸 the Project

STFC Ernest Rutherford Fellowship: Illuminating Solar-Planetary Interactions

This project investigated how the Sun affects the space environments of the planets Jupiter and Saturn by studying their aurora. The aurorae are nature’s light show: dancing displays of light near the planet’s northern and southern magnetic poles, caused by charged particles crashing into the atmosphere. Known as the northern and southern lights on Earth, these brilliant emissions have fascinated humans throughout history. The aurora reveals the transfer of energy from the Sun, through the stream of solar particles through the solar system, to the planet’s local environment. The aurora also reveals how the planet connects with its moons, such as Io and Ganymede at Jupiter, and Enceladus at Saturn. This project studied aurora at the outer planets in detail using two space missions: the Cassini Solstice Mission at Saturn and the Juno mission at Jupiter. These spacecraft flew low over their planet’s polar regions, simultaneously taking images of the aurora and measuring their presence in the magnetic field and the charged particles above the atmosphere.

RAS Research Fellowship: Planetary magnetospheres

This research programme aimed to discover the control that a planet’s magnetic field exerts on its magnetospheric dynamics, by probing the different environments of Jupiter and Saturn. It investigated magnetospheric processes driven internally by the planet’s magnetic field and its rotation, and those driven externally through the interaction with the surrounding solar wind. The balance between internally- and externally-driven dynamics concerns the fundamental transfer of energy and momentum through the solar system, from the Sun to planetary atmospheres. It is intrinsic to understanding our local space environment, and leads to discovery and understanding of planetary systems beyond our solar system. Observations of Jupiter show how changes in the inner plasma environment affect the dynamics of its vast magnetosphere and how these are reflected in the auroral emissions from the planet’s polar regions. In situ and remote sensing observations of Saturn’s magnetic field, plasma, and aurora indicate where and how much energy is transferred from the solar wind.

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Probing the mechanical properties of metal-coordinated molecules

This fellowship explored new ways to build and control molecular structures one bond at a time using advanced atomic-scale microscopy techniques. During this project, I explored methods for linking individual molecules together on insulating surfaces, a major challenge in nanotechnology that could help enable future nanoscale electronic devices and molecular circuits. Combining experimental physics and computational modelling, the project pushed the boundaries of single-molecule engineering and provided deeper understanding of chemical reactions at the level of individual atoms and bonds.

缅北轮奸 the Project

A place in the Sun - Taking Solar System Science to the Public

This STFC Science in Society Fellowship focussed on communicating the direct relevance of research into the space environment to the public and policy-makers. For example, society is becoming increasingly reliant upon modern technologies for utilities, communication, commerce, entertainment and security, but many of these technologies are susceptible to the rapid changes and disturbances in the space environment often referred to as “space weather”. Events at the Sun, such as solar flares and coronal mass ejections, can result in disturbed space weather in the near-Earth space environment and potentially disruptive consequences for technologies on the ground and in space. Large disturbances, on the same scale as the enormous solar flare observed by English astronomer Richard Carrington in 1859, could have a massive impact on space- and ground-based technologies such as communications satellites and electricity distribution networks, with obvious economic consequences. Solar system research is also relevant to global climate change, the search for life in our solar system and the hunt for potentially life-sustaining exoplanets – clearly issues of huge societal and cultural importance. This fellowship enabled Prof Wild to build upon his previous outreach activities and engage with public audiences via innovative channels.

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Superfluid Helium-3: an Ideal System for Investigating Fundamental Physics

In the fellowship research, Rich showed that the quantum fluid behaviour of helium-3 could be used to simulate some of the fundamental physics of cosmological phase transitions in the early Universe shortly after the Big Bang.