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We discuss the kinetic theory of stellar systems and two-dimensional vortices and stress their analogies. We recall the derivation of the Landau and Lenard–Balescu equations from the Klimontovich formalism. These equations take into account two-body correlations and are valid at the order 1/N, where N is the number of particles in the system. They have the structure of a Fokker–Planck equation involving a diffusion term and a drift term. The systematic drift of a vortex is the counterpart of the dynamical friction experienced by a star. At equilibrium, the diffusion and the drift terms balance each other establishing the Boltzmann distribution of statistical mechanics. We discuss the problem of kinetic blocking in certain cases and how it can be solved at the order by the consideration of three-body correlations. We also consider the behaviour of the system close to the critical point following a recent suggestion by Hamilton and Heinemann (2023). We present a simple calculation, valid for spatially homogeneous systems with long-range interactions described by the Cauchy distribution, showing how the consideration of the Landau modes regularizes the divergence of the friction by polarization at the critical point. We mention, however, that fluctuations may be very important close to the critical point and that deterministic kinetic equations for the mean distribution function (such as the Landau and Lenard–Balescu equations) should be replaced by stochastic kinetic equations.
We consider an isothermal self-gravitating system surrounding a central body. This model can represent a galaxy or a globular cluster harboring a central black hole. It can also represent a gaseous atmosphere surrounding a protoplanet. In three dimensions, the Boltzmann-Poisson equation must be solved numerically to obtain the density profile of the gas [Chavanis et al., Phys. Rev. E 109, 014118 (2024)]. In one and two dimensions, we show that the Boltzmann-Poisson equation can be solved analytically. We obtain explicit analytical expressions of the density profile around a central body which generalize the analytical solutions found by Camm (1950) and Ostriker (1964) in the absence of a central body. Our results also have applications for self-gravitating Brownian particles (Smoluchowski-Poisson system), for the chemotaxis of bacterial populations in biology (Keller-Segel model), and for two-dimensional point vortices in hydrodynamics (Onsager's model). In the case of bacterial populations, the central body could represent a supply of “food” that attracts the bacteria (chemoattractant). In the case of two-dimensional vortices, the central body could be a central vortex.
Despite 15 years of extensive investigation, the fabrication and study of nanofluidic devices that incorporate a single carbon nanotube (CNT) still represents a remarkable experimental challenge. In this study, we present the fabrication of nanofluidic devices that integrate an individual single-walled CNT (SWCNT), showcasing a notable reduction in noise by 1 -3 orders of magnitude compared to conventional devices. This achievement was made possible by employing high dielectric constant materials for both the substrate and the CNT-covering layer. Furthermore, we provide a detailed account of the crucial factors contributing to the successful fabrication of SWCNT-based nanofluidic devices that are reliably leak-free, plug-free, and long-lived. Key considerations include the quality of the substrate-layer interface, the nanotube opening, and the effective removal of photoresist residues and trapped microbubbles. We demonstrate that these devices, characterized by a high signal-tonoise ratio, enable spectral noise analysis of ionic transport through an individual SWCNT, thus showing that SWCNTs obey Hooge's law in 1/ f at low frequencies. Beyond advancing our fundamental understanding of ion transport in SWCNTs, these ultralow-noise measurements open avenues for leveraging SWCNTs in nanopore sensing applications for single-molecule detection, offering high sensitivity and identification capabilities.
Current fluctuations for the one-dimensional totally asymmetric exclusion process (TASEP) connected to reservoirs of particles, and their large scale limit to the KPZ fixed point in finite volume, are studied using exact methods. Focusing on the maximal current phase for TASEP, corresponding to infinite boundary slopes for the KPZ height field, we obtain for general initial condition an exact expression for the late time correction to stationarity, involving extreme value statistics of Brownian paths. In the special cases of stationary and narrow wedge initial conditions, a combination of Bethe ansatz and numerical conjectures alternatively provide fully explicit exact expressions.
The Riemann surface associated with counting the current between two states of an underlying Markov process is hyperelliptic. We explore the consequences of this property for the time-dependent probability of that current for Markov processes with generic transition rates. When the system is prepared in its stationary state, the relevant meromorphic differential is in particular fully characterized by the precise identification of all its poles and zeroes.
Sujets
Fermi gas
Turbulence
Cosmological model
Hydrodynamics
Smoluchowski equation
Statistical mechanics
Smoluchowski-Poisson
Thermodynamics
Gravitation
Mesoscale and Nanoscale Physics cond-matmes-hall
Cosmological constant
Gravitation self-force
Collisionless stellar-systems
Gravitational collapse
Equation of state
Computational modelling
Entropy
Black hole
Structure
Current fluctuations
Dark energy
Collective behavior
Cosmology
Energy density
Keller-Segel
Model
Galaxy
Dark matter halo
9880-k
Bose–Einstein condensates
Rotation
Axion star
Mass density
Scattering length
Wisdom of crowds
Pressure
Dark matter
Density
Mouvement brownien
9530Sf
Physique statistique
Collective intelligence
Carbon nanotube
Critical phenomena
Quantum chromodynamics axion
Halo
Dissipation
Catastrophe theory
Axion
Mass
General relativity
Phase separation
Random walker
Nonrelativistic
Denaturation
Quantum mechanics
Condensation Bose-Einstein
Brownian motion
Dark matter fuzzy
Atmosphere
Soft Condensed Matter cond-matsoft
Chemotaxis
Competition
Numerical calculations
9862Gq
9536+x
Fokker-Planck
DNA
Dark matter condensation
Nonlinear
Field theory scalar
TASEP
Expansion acceleration
Kinetic theory
Wave function
Bethe ansatz
Collective behaviour
Fermions
Bose-Einstein
Asymptotic behavior
Scalar field
Marcheur aléatoire
Dark matter density
Nanofiltration
Dark matter theory
Stability
FOS Physical sciences
Computational modeling
Collective motion
Chemotaxie
9535+d
Evaporation
Transition vitreuse
Diffusion
Gas Chaplygin
Collapse
Gravitation collapse
Effondrement gravitationnel
Einstein
Formation