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Carlo Cavazzoni

Researcher at Leonardo

Publications -  85
Citations -  29747

Carlo Cavazzoni is an academic researcher from Leonardo. The author has contributed to research in topics: Quantum ESPRESSO & Efficient energy use. The author has an hindex of 26, co-authored 79 publications receiving 22189 citations. Previous affiliations of Carlo Cavazzoni include International School for Advanced Studies & University College London.

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QUANTUM ESPRESSO: a modular and open-source software project for quantum simulations of materials

TL;DR: QUANTUM ESPRESSO as discussed by the authors is an integrated suite of computer codes for electronic-structure calculations and materials modeling, based on density functional theory, plane waves, and pseudopotentials (norm-conserving, ultrasoft, and projector-augmented wave).
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Advanced capabilities for materials modelling with Quantum ESPRESSO.

Paolo Giannozzi, +53 more
TL;DR: Recent extensions and improvements are described, covering new methodologies and property calculators, improved parallelization, code modularization, and extended interoperability both within the distribution and with external software.
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Advanced capabilities for materials modelling with Quantum ESPRESSO

Paolo Giannozzi, +53 more
TL;DR: Quantum ESPRESSO as discussed by the authors is an integrated suite of open-source computer codes for quantum simulations of materials using state-of-the-art electronic-structure techniques, based on density functional theory, density functional perturbation theory, and many-body perturbations theory, within the plane-wave pseudo-potential and projector-augmented-wave approaches.
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Quantum ESPRESSO toward the exascale.

TL;DR: A motivation and brief review of the ongoing effort to port Quantum ESPRESSO onto heterogeneous architectures based on hardware accelerators, which will overcome the energy constraints that are currently hindering the way toward exascale computing are presented.
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Superionic and Metallic States of Water and Ammonia at Giant Planet Conditions

TL;DR: The phase diagrams of water and ammonia were determined by constant pressure ab initio molecular dynamic simulations at pressures (30 to 300 gigapascal) and temperatures (300 to 7000 kelvin) of relevance for the middle ice layers of the giant planets Neptune and Uranus to improve the understanding of the properties of the middle icy layers.