Inelastic scattering and local heating in atomic gold wires
We present a method for including inelastic scattering in a first-principles density-functional computational scheme for molecular electronics. As an application,
355 indexed results
We present a method for including inelastic scattering in a first-principles density-functional computational scheme for molecular electronics. As an application,
Collisionless shocks play a role in many astrophysical phenomena, from coronal mass ejections (CMEs) in the heliosphere to supernova remnants.
Using both a recent calculation by Bruch of the damping of the motion of a monolayer nitrogen film oscillating harmonically
Formation of luminous matter in the Universe is a complicated process, which includes many processes and components. It is the
The lack of our knowledge on how angular momentum is transported in accretion disks around black holes has prevented us
Using recent data for the photosphere-chromosphere region of the solar atmosphere the magnetic reconnection in tripolar geometry has been investigated
I review particle heating by MHD turbulence in collisionless plasmas appropriate to advection-dominated accretion flows. These considerations suggest that the
We have developed a numerical code with which we study the effects of 2D perturbations on stellar structure. We present
Modeling the dynamics of the quantum fluids within a spinning-down neutron star gives a description consistent with observed pulsar magnetic
Effects of microwave radiation on magnetoresistance are analyzed in a balance-equation scheme that covers regimes of inter- and intra-Landau level
We have performed 3-D numerical magnetohydrodynamic (MHD) jet experiments to study the instabilities associated with strongly toroidal magnetic fields and
Most supernovae are expected to explode in low-density hot media, particularly in galactic bulges and elliptical galaxies. The remnants of
We study the chemodynamical evolution of elliptical galaxies and their X-ray and optical properties using high-resolution cosmological simulations. Our Tree
We present results of including heating and cooling in cosmological simulations of the $Λ$CDM cosmology and demonstrate their effects on
We present a model for the compression and heating of the ICM by powerful radio galaxies and quasars. Based on
X-ray observations indicate that non-gravitational processes play a key role in the thermodynamics of the Intra Cluster Medium (ICM). The
X-ray observations indicate that non-gravitational processes play a key role in determining the distribution of the diffuse, X-ray emitting gas
Based on simultaneous observations of solar flares in hard and soft X-rays we studied several aspects of the Neupert effect.
By making spectral absorption-line observations of disk galaxies at intermediate inclinations, we have been able to determine the amplitude of
We re-examine the age-velocity dispersion relation in the solar neighborhood using improved stellar age estimates that are based on Hipparcos
I study the time evolution of the density matrices of quantum Fermi systems interacting with classic external Fermi fields. This
Nine lectures reviewing the astrophysics of dust in interstellar clouds. Topics include: (1) Summary of observational evidence concerning interstellar dust:
The heating of the solar corona and the puzzle of the slender high reaching magnetic loops seen in observations from
We present tight-binding molecular dynamics simulations of the structural modifications that result from the "thermal spike" that occurs during the