plasma physics

topic

• Theory of Superconductivity
• Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
• Ordering, metastability and phase transitions in two-dimensional systems
• Unconventional superconductivity in magic-angle graphene superlattices
• Physics-informed machine learning
• Plasma perspective on strong field multiphoton ionization
• FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION
• The cosmological constant and dark energy
• NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
• Simulations of the formation, evolution and clustering of galaxies and quasars
• A fast algorithm for particle simulations
• Unified Schemes for Radio-Loud Active Galactic Nuclei
• Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies
• MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA)
• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• Electronic excitations: density-functional versus many-body Green’s-function approaches
• The Confrontation between General Relativity and Experiment
• Multi-messenger Observations of a Binary Neutron Star Merger *
• The EAGLE project: simulating the evolution and assembly of galaxies and their environments
• Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• The Solar Dynamics Observatory (SDO)
• Experimental and theoretical challenges in the search for the quark–gluon plasma: The STAR Collaboration's critical assessment of the evidence from RHIC collisions
• MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS
• Formation of dense partonic matter in relativistic nucleus–nucleus collisions at RHIC: Experimental evaluation by the PHENIX Collaboration
• Active Particles in Complex and Crowded Environments
• The critical properties of the two-dimensional xy model
• MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
• Machine Learning for Fluid Mechanics
• Global Conservation Laws and Massless Particles
• Scientific Machine Learning Through Physics–Informed Neural Networks: Where we are and What’s Next
• LOFAR: The LOw-Frequency ARray
• Theoretical Modeling of Starburst Galaxies
• The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)
• Theory of Star Formation
• Thermal fluctuations, quenched disorder, phase transitions, and transport in type-II superconductors
• Collapsars: Gamma‐Ray Bursts and Explosions in “Failed Supernovae”
• Quasinormal modes of black holes and black branes
• A compilation of charged-particle induced thermonuclear reaction rates
• Cosmological smoothed particle hydrodynamics simulations: a hybrid multiphase model for star formation
• Quark–gluon plasma and color glass condensate at RHIC? The perspective from the BRAHMS experiment
• Modules for Experiments in Stellar Astrophysics ( ): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• Cosmological hydrodynamics with adaptive mesh refinement
• Axion cosmology
• Zonal flows in plasma—a review
• The order of the quantum chromodynamics transition predicted by the standard model of particle physics
• Optical magnetometry
• Large-amplitude Alfvén waves in the interplanetary medium, 2
• First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
• Phase retrieval and differential phase-contrast imaging with low-brilliance X-ray sources
• Recoil-ion and electron momentum spectroscopy: reaction-microscopes
• PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
• Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)
• The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI)
• Heavy quarkonium: progress, puzzles, and opportunities
• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
• Extremely high-intensity laser interactions with fundamental quantum systems
• FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA
• An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmas
• The Cosmic Microwave Background Spectrum from the FullCOBEFIRAS Data Set
• Grids of stellar models with rotation
• GeV electron beams from a centimetre-scale accelerator
• X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• The ALICE experiment at the CERN LHC
• First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
• Strong coupling between surface plasmon polaritons and emitters: a review
• Lectures on holographic methods for condensed matter physics
• Operation of a free-electron laser from the extreme ultraviolet to the water window
• Contemporary particle-in-cell approach to laser-plasma modelling
• Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
• The Phase Structure of QCD: Fluctuations and Correlations
• Anisotropic particle transport from a pulsar wind nebula revealed by Einstein Probe and LHAASO
• Bifurcations in the Heliosphere: Global-scale Coronal Pseudostreamer Evolution and the Creation of Secondary Heliospheric Current Sheets
• On local and non-local energy transfers in Hall magnetohydrodynamic turbulence
• BlackHoleWeather – Spin-coupled chaotic cold accretion across the meso scale: Morphology and thermodynamics
• Searching for optical pulsations from spider millisecond pulsars with the fast photometer SiFAP2
• Intense but Harmless: Exo-Space Weather around an M Dwarf with a Single-hemisphere Dynamo
• Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones
• Advantages of Pulsed Laser Ion Source ( LIS ) at an Intensity of About 10 10 W/cm 2 for Heavy‐Ion Injection Into High‐Energy Accelerators
• Evidence for plasmoid formation related to a hot UV burst in the solar atmosphere