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Vacuum oscillations

We shall develop the theory necessary to understand quasioptics, but before that, it will be useful to consider factors that influence the choice of spectrometer components such as the magnet, the source, and the detector. In Section II we will give a brief review of the performance and characteristics of homodyne detectors. In our discussion of sources, we will discuss vacuum oscillators, such as the reflex klystron and backward wave oscillator, and solid-state sources, such as the Gunn diode. We will also discuss useful criteria for selecting a magnet. [Pg.255]

It is possible to build pulsed versions of the vacuum oscillators that can have variable pulsewidths and separations. The difficulty is in maintaining phase coherence between pulses. Solid-state sources may be switched to provide pulses, but the lower output powers limit the spectroscopist to selective pulses in many cases. As techniques become more advanced, pulse generation will become more and more common in near-millimeter band spectrometers. For the purposes of this chapter, however, we will limit our attention to CW sources. [Pg.262]

H. de Kerret et al, Eroposal to Search for Neutrino Vacuum Oscillations Using a 1 Km Baseline Reactor Neutrino Experiment, 1993, http //www.hep.anl.gov/NDK/Hypertext/chooz.html, p. 74. [Pg.40]

The results from the astroneutrino experiments in Tables V and VI are consistent with different numerical descriptions of neutrino oscillations. One finds solutions in which Am is of the order of 10 eV from two MSW solutions and 10 eV from the so-called solar neutrino vacuum oscillation solution, nominally representing a Ve -o- oscillation. A fourth solution yields 10 eV ... [Pg.208]

In equation (Cl.4.14) the saturation parameter essentially defines a criterion to compare the time required for stimulated and spontaneous processes. If I then spontaneous coupling of the atom to the vacuum modes of the field is fast compared to the stimulated Rabi coupling and the field is considered weak. If s" 1 then the Rabi oscillation is fast compared to spontaneous emission and the field is said to be strong. Setting s equal to unity defines the saturation condition... [Pg.2460]

Note that the wavelength in vacuum has been replaced by the wavelength in the medium, since it is the latter that drives the oscillations in the fluctuation domain. Now what can we say about 6a ... [Pg.680]

Acoustic Wave Sensors. Another emerging physical transduction technique involves the use of acoustic waves to detect the accumulation of species in or on a chemically sensitive film. This technique originated with the use of quartz resonators excited into thickness-shear resonance to monitor vacuum deposition of metals (11). The device is operated in an oscillator configuration. Changes in resonant frequency are simply related to the areal mass density accumulated on the crystal face. These sensors, often referred to as quartz crystal microbalances (QCMs), have been coated with chemically sensitive films to produce gas and vapor detectors (12), and have been operated in solution as Hquid-phase microbalances (13). A dual QCM that has one smooth surface and one textured surface can be used to measure both the density and viscosity of many Hquids in real time (14). [Pg.391]

These fluctuations will affect the motion of charged particles. A major part of the Lamb shift in a hydrogen atom can be understood as the contribution to the energy from the interaction of the electron with these zero point oscillations of the electromagnetic field. The qualitative explanation runs as follows the mean square of the electric and magnetic field intensities in the vacuum state is equal to... [Pg.486]

The main source of noise of such a heterodyne detector is the photon noise that takes place at the splitting of the local oscillator. Quantum physicists see this noise as originating from vacuum fluctuation on the input arm. This gives directly the spectral density of noise at input hv/2. [Pg.368]

Heterodyne is a very efficient tool for detecting the phase of a "coherent" signal i.e. a signal which has a stable phase relation to the local oscillator. The detector is only limited by the quantum fluctuation of vacuum. This property is common use in coherent lidar. Satellite to satellite optical communications using laser as a local oscillator are under development (Fig. 3). [Pg.370]

Changes in thermal stability and mass due to the formation of CdS nanoparticles in LB films were examined [180]. The LB films were formed onto gold-coated quartz oscillators from monolayers of arachidic acid or nonacosa-10,12-diynoic acid on CdCH containing subphases. The films were exposed to H2S gas until the mass change indicated complete conversion of Cd to CdS. The thermal stability of the H2S-treated films was reduced, with significant mass loss initiating at 55°C, compared to minimal mass loss in the untreated films up to at least 80°C under mild vacuum. The average CdS-particle size... [Pg.91]

Absorption of X-ray radiation of energy well above the threshold for an X-ray transition will result in the ejection of a photoelectron since the initial unoccupied band stale to which the transition takes place will be above the vacuum level. The Kronig fine structure is due to oscillations induced in the absorption cross-section of the absorbing atom as a result of interference... [Pg.148]

This effect resembles the traditional Casimir effect, which describes the attraction between two parallel metallic mirrors in vacuum. Here, however, the fluctuating (bosonic) electromagnetic fields are replaced by fermionic matter fields. Furthermore, the Casimir energy is inferred from the geometry-dependent part of the density of states, and its sign is not fixed, but oscillates according to the relative arrangement and distances of the cavities. [Pg.231]

The free theory for the quench models is provided by the potential (4), where A = 0 and m2(t) changes signs either instantaneously or for a finite period. In the Minkowski spacetime, we can apply the LvN method simply by letting R = 1. Before the phase transition (rrii = (mg + m2)1/2), all the modes are stable and oscillate around the true vacuum ... [Pg.285]

Either in the instantaneous quench or in the finite quench, short wavelength modes with k > rrif = (mg — m )1/2 are still stable even after the phase transition and oscillate around the false vacuum as... [Pg.285]


See other pages where Vacuum oscillations is mentioned: [Pg.261]    [Pg.262]    [Pg.296]    [Pg.59]    [Pg.461]    [Pg.261]    [Pg.262]    [Pg.296]    [Pg.59]    [Pg.461]    [Pg.1179]    [Pg.1385]    [Pg.1559]    [Pg.1879]    [Pg.369]    [Pg.665]    [Pg.383]    [Pg.516]    [Pg.332]    [Pg.331]    [Pg.663]    [Pg.32]    [Pg.398]    [Pg.52]    [Pg.486]    [Pg.353]    [Pg.40]    [Pg.116]    [Pg.368]    [Pg.34]    [Pg.503]    [Pg.655]    [Pg.114]    [Pg.286]    [Pg.42]    [Pg.220]    [Pg.99]    [Pg.6]    [Pg.6]    [Pg.338]   


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