Pages (6)
RSS
With the downscaling of silicon transistors into sub 5 nm size, quantum effects in conductivity start to play a major role, making the transistors increasingly unreliable. Emerging technologies in this field rely on crystalline oxides such as LiNbO3 or BaTiO3.
The project outlined here aims to uncover firstly the formation pathways of MBHs and secondly to track the evolution and growth of MBHs in very early galaxies as the MBHs grow, merge and settle towards their host galaxy's centre.
A computational method able to quantitatively predict spin relaxation in magnetic molecules and individuated the main physical ingredients that can potentially lead to room temperature spin operations
The team proposes DiffMark, a differentiable multi-bit watermarking framework that resolves all three limitations by leveraging Latent Consistency Models.
Massive Black Holes (MBHs) populate the centres of most, if not all, galaxies with total masses greater than approximately 1e12 solar masses.
Ammonia (NH3) is widely used in agriculture, fertilizer production and chemical industry. The process of commercial NH3 production relies on the Haber-Bosch process that is energy-intensive and highly dependent on fossil fuels, and has with significant greenhouse gas emissions.