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Microwave radiation spectrum

Figure 6.2. (I) Conventional phosphorescence spectrum of 2,3-dichloroquinoxa-line in durene at 1.6°K. (II) am-PMDR spectrum, obtained by amplitude modulation of microwave radiation that pumps the tv-t, (1.055 GHz) zf transition with the detection at the modulation frequency. Only bands whose intensities change upon microwave radiation (1.055 GHz) and thus originate from tv or rz appear in the am-PMDR spectrum. Transitions from r and rv appear with opposite sign (phase-shifted by 180°). (Hb, lie ) Polarization of the am-PMDR spectral transitions, relative to the crystal axes. The band at 0,0-490 cm-1 originates from both the r and t spin states its intensity does not change upon the 1.055-GHz saturation (no band in II) however, its polarization does rhanp. (bands in Hb and IIc ). (Reproduced with permission from M. A. El-Sayed.tt7W)... Figure 6.2. (I) Conventional phosphorescence spectrum of 2,3-dichloroquinoxa-line in durene at 1.6°K. (II) am-PMDR spectrum, obtained by amplitude modulation of microwave radiation that pumps the tv-t, (1.055 GHz) zf transition with the detection at the modulation frequency. Only bands whose intensities change upon microwave radiation (1.055 GHz) and thus originate from tv or rz appear in the am-PMDR spectrum. Transitions from r and rv appear with opposite sign (phase-shifted by 180°). (Hb, lie ) Polarization of the am-PMDR spectral transitions, relative to the crystal axes. The band at 0,0-490 cm-1 originates from both the r and t spin states its intensity does not change upon the 1.055-GHz saturation (no band in II) however, its polarization does rhanp. (bands in Hb and IIc ). (Reproduced with permission from M. A. El-Sayed.tt7W)...
It should be also noted that, in a very recent publication, Liu and coworkers were successful in applying microwave radiation within their domino approach towards the synthesis of pyrrolo[2,l-fc]quinazoline alkaloids such as deoxyvasicinone, 8-hy-droxydeoxyvasicinone, mackinazolinone and isaindigotone, which exhibit a promising broad spectrum of biological activities. In the case of isaindigotone, the authors were able to extend their strategy to a three-component procedure, which comprises the domino conversion of anthranilic acids and Boc-protected amino acids into the tricyclic core skeleton [43]. [Pg.584]

In the electromagnetic spectrum, microwave radiation occurs in an area of transition between infrared radiation and radiofrequency waves, as shown in Fig. 1.1. The wavelengths are between 1 cm and 1 m and frequencies between 30 GHz and 300 MHz. [Pg.3]

Microwave spectroscopy The study of the interaction of microwave radiation with the rotational motion of a molecule. Microwave transitions are not restricted to molecules and can occur in atoms whenever the separation between the energy levels is in the microwave region of the spectrum. [Pg.313]

To complicate matters, the spectrum cannot be determined by placing a sample cell in the path of a beam of microwave radiation. Like NMR, the EPR sample must first be placed within a strong magnetic field (conventionally symbolized as B). ... [Pg.248]

The setup for ESR spectroscopy is a cross between NMR and micro-wave techniques (Section 5.8). The source is a frequency-stabilized klystron, whose frequency is measured as in microwave spectroscopy. The microwave radiation is transmitted down a waveguide to a resonant cavity (a hollow metal enclosure), which contains the sample. The cavity is between the poles of an electromagnet, whose field is varied until resonance is achieved. Absorption of microwave power at resonance is observed using the same kind of crystal detector as in microwave spectroscopy. Sensitivity is enhanced, as in microwave spectroscopy, by the use of modulation The magnetic field applied to the sample is modulated at, say, 100 kHz, thus producing a 100-kHz signal at the crystal when an absorption is reached. The spectrum is recorded on chart paper. [Pg.189]

As far as we can see into the Universe, we don t observe any primordial antimatter. Within the limits of our present observational horizon the Universe is seen to contain only matter and no antimatter. The presence of cosmic antimatter would lead to observable traces of annihilation however the measurements of the extragalactic 7 ray flux indicate an absence of annihilation radiation, and the microwave background spectrum lacks a corresponding distortion. These findings preclude the existence of a significant amount of antimatter within tens of Megaparsecs, which is the scale of super-clusters of galaxies. [Pg.188]

Electromagnetic radiation with a frequency of 0.3-300 GHz (X = 1-0.001 m) is called microwave radiation. The microwave part of the electromagnetic spectrum lies between the more energetic infrared radiation... [Pg.168]

The microwave acoustic effect may be defined as the auditory perception of microwave radiation which is a form of electromagnetic energy which occupies the part of spectrum between ordinary radio waves and infrared and optical waves. This definition may... [Pg.317]

For radiofrequency and microwave radiation there are detectors which can respond sufficiently quickly to the low frequencies (<100 GHz) involved and record the time domain spectrum directly. For infrared, visible and ultraviolet radiation the frequencies involved are so high (>600 GHz) that this is no longer possible. Instead, an interferometer is used and the spectrum is recorded in the length domain rather than the frequency domain. Because the technique has been used mostly in the far-, mid- and near-infrared regions of the spectrum the instrument used is usually called a Fourier transform infrared (FTIR) spectrometer although it can be modified to operate in the visible and ultraviolet regions. [Pg.55]

During the past five years two research disciplines of optical spectroscopy and magnetic resonance have merged when it became evident that at low temperatures, microwave radiation of resonance frequencies with the zero-field (zf) transitions of the lowest triplet state could have observable effects on the phosphorescence intensity as well as the spectrum. Quantitative information can then be obtained from these phosphorescence-microwave multiple-resonance experiments from which the magnetic, the radiative, and the nonradiative as well as the structural properties of the triplet state can be determined. [Pg.313]

It should be pointed out that once the zf origin of the different bands is determined (in particular the true and false origins of the spectrum), a complete description could be given for the spin-orbit perturbations that give the lowest triplet state its radiative properties. A very extensive work was conducted by Tinti and El-Sayed (39) in which different perturbations—e.g., heating, applying a magnetic field, as well as saturation of the zf transitions with microwave radiation-were used to determine the property of the individual zf levels. The effect of these perturbations not only on the phosphorescence spectrum but also on the observed decays and polarizations has been examined. Limits on the importance of the different spin-orbit interactions are obtained. This spectroscopic work represents the type of experiments that can be done and the kind of information that can be obtained from PMDR and other methods. [Pg.343]

Figure 9a (inset) shows the zero-field ODMR spectrum for Pd(2-thpy)2 detected at the electronic origin of the emission spectrum at 18,418 cm Due to the frequency scan of the microwave radiation, one observes a signal at 2886 MHz (0.0962 cm ) with a line width (fwhm) of 20 MHz. No other zero-field ODMR signal could be observed in the frequency range from 300 MHz up to 8000 MHz. However, for a system of three triplet substates, one would expect to... [Pg.109]

Electromagnetic radiation in the microwave frequency spectrum is absorbed most strongly by molecules with permanent dipole moments (4). The relaxation phenomenon of this absorbed power manifests itself in a heatlike reaction. The University of Colorado Oil Shale Project has studied the degradation of the liquid-fuel precursor (kerogen) by micro-wave interaction. Kerogen is a moderately strong absorber of this radia-... [Pg.330]

Where f is the frequency of the incident microwave radiation and Q is the dimensionless cavity quality factor. Thus for a typical cavity Q of 20,000 at 10 GHz the operational bandwidth is on the order of 0.5 MHz. Therefore a typical rotational spectrum that covers 7.5-18.5 GHz must be stepped in 500 kHz step sizes over that spectral range. The result is a recording device that must take 22,000 steps to record an 11 GHz spectral region leading to data acquisition times that can take upwards of 14 hours. This analysis time can be reduced to minutes if spot checks are performed by tuning the cavity only to the rotational transition of a known species, however, in tliis mode of operation, only the species of interest will be detected, i.e., molecular species with transitions outside the spectral window being monitored will not be detected. [Pg.291]

One very recently published result must be mentioned. Petukhov et al. have reported the detection of the EPR spectrum of micron-sized crystals of Fe8 via their magnetization response as a function of apphed magnetic field, using a Hall-probe magnetometer under either continuous wave or pulsed microwave irradiation at 118 GHz and between 1.4 and 50 K [53]. Dips are observed in the magnetization vs. field curves corresponding to resonant absorption - that is, EPR transitions. This method offers potentially extraordinary sensitivity and, furthermore, manipulation of the magnetization data in the absence and presence of the microwave radiation allows determination of the spin temperature. [Pg.82]


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See also in sourсe #XX -- [ Pg.962 , Pg.963 ]




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