Peridynamics simulation of the comminution of particles containing
... where σw corresponds to the stress for which 63% of particles are broken and m is the Weibull modulus characterizing the width of the distribution. Figure 6 shows ln(ln(1/PS )) as a function of ln(σt /σth ). If the data collapse on a straight line, the slope equals the Weibull modulus of the distrib ...
... where σw corresponds to the stress for which 63% of particles are broken and m is the Weibull modulus characterizing the width of the distribution. Figure 6 shows ln(ln(1/PS )) as a function of ln(σt /σth ). If the data collapse on a straight line, the slope equals the Weibull modulus of the distrib ...
IC_2012
... EM wave propagation in a plasma with a linear density gradient Consider plane waves at normal incidence. Assume the density gradient is in the propagation direction Z. This ...
... EM wave propagation in a plasma with a linear density gradient Consider plane waves at normal incidence. Assume the density gradient is in the propagation direction Z. This ...
Atomic Theory&Isotopes
... Ionization of an atom involves the loss of an electron to form a positive ion. The first ionization energy is defined as the energy required to remove one mole of electrons from one mole of atoms of a gaseous element. The first ionization energy of an atom can be represented by the following general ...
... Ionization of an atom involves the loss of an electron to form a positive ion. The first ionization energy is defined as the energy required to remove one mole of electrons from one mole of atoms of a gaseous element. The first ionization energy of an atom can be represented by the following general ...
On the consequences of bi-Maxwellian distributions on parallel electric fields.
... because the electrons are more mobile than the ions and do most shielding by creating ...
... because the electrons are more mobile than the ions and do most shielding by creating ...
lecture12
... OK, but wait a minute. Doesn’t this really just mean that there must be at least that much energy in the photon? If there is too much, some of it just won’t get used by the transition. But that does not work. There is no where for the extra energy to go. Since energy must be conserved, absorption of ...
... OK, but wait a minute. Doesn’t this really just mean that there must be at least that much energy in the photon? If there is too much, some of it just won’t get used by the transition. But that does not work. There is no where for the extra energy to go. Since energy must be conserved, absorption of ...
URL - StealthSkater
... descriptions and methodologies that would affect the polarizable vacuum medium as an alternative method for affecting space-time curvature. It began with the assumption that a relationship can be forged between an applied EM field and the local value of gravitational acceleration “g”. ElectroGraviMa ...
... descriptions and methodologies that would affect the polarizable vacuum medium as an alternative method for affecting space-time curvature. It began with the assumption that a relationship can be forged between an applied EM field and the local value of gravitational acceleration “g”. ElectroGraviMa ...
Density of states
In solid-state and condensed matter physics, the density of states (DOS) of a system describes the number of states per interval of energy at each energy level that are available to be occupied. Unlike isolated systems, like atoms or molecules in gas phase, the density distributions are not discrete like a spectral density but continuous. A high DOS at a specific energy level means that there are many states available for occupation. A DOS of zero means that no states can be occupied at that energy level. In general a DOS is an average over the space and time domains occupied by the system. Localvariations, most often due to distortions of the original system, are often called local density of states (LDOS). If the DOS of an undisturbedsystem is zero, the LDOS can locally be non-zero due to the presence of a local potential.