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Radiated fields

To this point, we have considered only the radiation field. We now turn to the interaction between the matter and the field. According to classical electromagnetic theory, the force on a particle with charge e due to the electric and magnetic fields is... [Pg.221]

From these equations one also finds the rate coefficient matrix for themial radiative transitions including absorption, induced and spontaneous emission in a themial radiation field following Planck s law [35] ... [Pg.1048]

In order to illustrate some of the basic aspects of the nonlinear optical response of materials, we first discuss the anliannonic oscillator model. This treatment may be viewed as the extension of the classical Lorentz model of the response of an atom or molecule to include nonlinear effects. In such models, the medium is treated as a collection of electrons bound about ion cores. Under the influence of the electric field associated with an optical wave, the ion cores move in the direction of the applied field, while the electrons are displaced in the opposite direction. These motions induce an oscillating dipole moment, which then couples back to the radiation fields. Since the ions are significantly more massive than the electrons, their motion is of secondary importance for optical frequencies and is neglected. [Pg.1266]

Up to this point, we have calculated the linear response of the medium, a polarization oscillating at the frequency m of the applied field. This polarization produces its own radiation field that interferes with the applied optical field. Two familiar effects result a change in tlie speed of the light wave and its attenuation as it propagates. These properties may be related directly to the linear susceptibility The index of... [Pg.1267]

The polarization P is given in tenns of E by the constitutive relation of the material. For the present discussion, we assume that the polarization P r) depends only on the field E evaluated at the same position r. This is the so-called dipole approximation. In later discussions, however, we will consider, in some specific cases, the contribution of a polarization that has a non-local spatial dependence on the optical field. Once we have augmented the system of equation B 1.5.16. equation B 1.5.17. equation B 1.5.18. equation B 1.5.19 and equation B 1.5.20 with the constitutive relation for the dependence of Pon E, we may solve for the radiation fields. This relation is generally characterized tlirough the use of linear and nonlinear susceptibility tensors, the subject to which we now turn. [Pg.1271]

The linear and nonlinear optical responses for this problem are defined by e, 2, e and respectively, as indicated in figure Bl.5.5. In order to detemiine the nonlinear radiation, we need to introduce appropriate pump radiation fields E(m ) and (co2)- If these pump beams are well-collimated, they will give rise to well-collimated radiation emitted tlirough the surface nonlmear response. Because the nonlinear response is present only in a thin layer, phase matching [37] considerations are unimportant and nonlinear emission will be present in both transmitted and reflected directions. [Pg.1277]

In the previous chapters experiments have been discussed in which one frequency is applied to excite and detect an EPR transition. In multiple resonance experiments two or more radiation fields are used to induce different transitions simultaneously [19, 20, 21, 22 and 23], These experiments represent elaborations of standard CW and pulsed EPR spectroscopy, and are often carried out to complement conventional EPR studies, or to refine the infonnation which can in principle be obtained from them. [Pg.1567]

Figure Cl.4.5. Population modulation as the atom moves through the standing wave in the Tin-periD-lin one dimensional optical molasses. The population lags the light shift such that kinetic is converted to potential energy then dissipated into the empty modes of the radiation field by spontaneous emission (after 1171). Figure Cl.4.5. Population modulation as the atom moves through the standing wave in the Tin-periD-lin one dimensional optical molasses. The population lags the light shift such that kinetic is converted to potential energy then dissipated into the empty modes of the radiation field by spontaneous emission (after 1171).
The high-field output of laser devices allows for a wide variety of nonlinear interactions [17] between tire radiation field and tire matter. Many of tire initial relationships can be derived using engineering principles by simply expanding tire media polarizability in a Taylor series in powers of tire electric field ... [Pg.2863]

When reactor-grade plutonium is left in spent fuel, the large size of the fuel assembhes and the lethal radiation fields make it extremely difficult to divert the material covertly. Once the reactor-grade plutonium is separated in the commercial reprocessing option, however, the radiation barrier is almost eliminated, and in certain steps of the process the plutonium is in powder or Hquid form, which is much more easily diverted than large, bulky fuel... [Pg.242]

Semiconductor devices ate affected by three kinds of noise. Thermal or Johnson noise is a consequence of the equihbtium between a resistance and its surrounding radiation field. It results in a mean-square noise voltage which is proportional to resistance and temperature. Shot noise, which is the principal noise component in most semiconductor devices, is caused by the random passage of individual electrons through a semiconductor junction. Thermal and shot noise ate both called white noise since their noise power is frequency-independent at low and intermediate frequencies. This is unlike flicker or ///noise which is most troublesome at lower frequencies because its noise power is approximately proportional to /// In MOSFETs there is a strong correlation between ///noise and the charging and discharging of surface states or traps. Nevertheless, the universal nature of ///noise in various materials and at phase transitions is not well understood. [Pg.346]

No object can radiate more energy than can a blackbody at the same temperature, because a blackbody ia equiUbrium with a radiation field at temperature T radiates exacdy as much energy as it absorbs. Any object exhibiting surface reflection must have emissivity of less than 1. Pyrometers are usually caUbrated with respect to blackbodies. This can cause a serious problem ia use. The emissivities of some common materials are fisted ia Table 4. [Pg.404]

Electronic conductivity Flexible conductor of electricity heating elements (resistance heating), shielding of electromagnetic radiation field flattening (high-voltage cables), materials with antistatic capability... [Pg.888]

Hot Work - Work involving welding, cutting, brazing or other spark-producing operations. It also means work in a radiation field. [Pg.462]

Here the sum runs over all possible initial states and the operator describes the interaction of the electrons and the radiation field with wave vector q and polarization A. In Eq. (1) it has been assumed that the detector selectively counts photo electrons with energy E, wave vector k, and spin polarization The corresponding final... [Pg.188]

The quantum mechanical view of Raman scatering sees a radiation field hvo inducing a transition from a lower level A to a level n. If vnlc is the transition frequency, then the inelastically scattered light has frequency v0 — v t. That is, the molecule removes energy hv k from an incident photon. This process corresponds to Stokes scattering. Alternatively, a molecule under-... [Pg.296]


See other pages where Radiated fields is mentioned: [Pg.163]    [Pg.2]    [Pg.221]    [Pg.221]    [Pg.222]    [Pg.223]    [Pg.1029]    [Pg.1047]    [Pg.1061]    [Pg.1061]    [Pg.1062]    [Pg.1067]    [Pg.1069]    [Pg.1197]    [Pg.1552]    [Pg.1565]    [Pg.1565]    [Pg.2455]    [Pg.2462]    [Pg.2863]    [Pg.377]    [Pg.133]    [Pg.192]    [Pg.192]    [Pg.193]    [Pg.197]    [Pg.424]    [Pg.111]    [Pg.482]    [Pg.489]    [Pg.509]    [Pg.1033]    [Pg.226]    [Pg.666]    [Pg.297]   


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An Overview of Quantum Electrodynamics and Matter-Radiation Field Interaction

Chaotic radiation field

Circularly polarized radiation electric fields

Coherence Properties of Radiation Fields

Decomposition of the radiation field

Dipole operator interaction with radiation field

Dust and Stellar Radiation Field

Electric field radiation

Electromagnetic field radiation

Electromagnetic radiation electric field

Electromagnetic radiation magnetic field

Electromagnetism radiation fields

Excitation radiation field

External radiation field coupling

External radiation field coupling techniques

Field radiation

Field radiation

Hamiltonian including radiation field

Induced Dipole Forces in a Radiation Field

Instruments to measure the radiation field

Involved field radiation therapy

Magnetic field radiation

Magnetic field, plane-polarized electromagnetic radiation

Matter-radiation field interactions

Matter-radiation field interactions electrodynamics

Mixed radiation fields

Multipole radiation field

Overlapping radiation fields

Quantization of the radiation field

Radiated fields boundary condition

Radiated fields polarizability tensor

Radiated fields semiclassical theory

Radiation field Subject

Radiation field coupling with

Radiation field decomposition

Radiation field integral representation

Radiation field leaky mode contribution

Radiation field space wave contribution

Radiation field states

Radiation field theory

Radiation field total power

Radiation field, interaction with molecules

Radiation fields susceptibility

Radiation fields, electromagnetic topology

Radiation-induced conductivity high field

The Radiation Field Theory

The emerging radiation field

The quantum radiation field

The radiation field

The solar radiation field

Thermokinetic coupling with radiation field

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