6,619 research outputs found
Dynamical Franz-Keldysh effect
We introduce and analyze the properties of dynamical Franz-Keldysh effect,
i.e. the change of density-of-states, or absorption spectra, of semiconductors
under the influence of {\it time-dependent} electric fields. In the case of a
harmonic time-dependence, we predict the occurence of significant fine
structure, both below and above the zero-field band-gap, which should be
experimentally observable.Comment: 4 pages, REVTEX 3.0, uses epsf, 5 figures attached as Z-compressed
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Measurements of ion-molecule reactions of He plus, H plus, HeH plus with H sub 2 and D sub 2
A drift tube mass spectrometer apparatus has been used to determine the rate coefficient, energy dependence and product ions of the reaction He(+) +H2. The total rate coefficient at 300 K is 1.1 plus or minus 0.1) 10 to minus 13th power cu cm/sec. The reaction proceeds principally by dissociative charge transfer to produce H(+), with the small remainder going by charge transfer to produce H2(+) and by atom rearrangement to produce HeH(+). The rate coefficient increases slowly with increasing ion mean energy, reaching a value of 2.8 x ten to the minus 13th power cu cm sec at 0.18 eV. The corresponding reaction with deuterium, He(+) + D2, exhibits a value (5 plus or minus 1) x 10 to the minus 14th cu cm/sec at 300K. The reaction rates for conversion of H(+) and HeH(+) to H3(+) on collisions with H2 molecules are found to agree well with results of previous investigations
Mobilities of uranium and mercury ions in helium
The mobilities of mass-identified U(+) and Hg (+) ions in helium were determined in a drift tube-mass spectrometer. For uranium ions, a reduced mobility value is obtained at 305 K and a standard gas density of 2.69 x 10 to the 19th power/cu cm. The mobility of mercury ions is in agreement with two previous determinations. The effect of fast ion injection in drift mobility measurements is discussed, and a technique to circumvent these problems is described. The results are compared with existing theories of ion mobilities
Exposure to Sexualized Images of Athletes Negatively Affects Adolescent Male Athletes’ Appraisals of Self and Others
This study used a between-subjects experimental design to examine the effects of viewing sexualized versus performance images of male athletes on male adolescent athletes perceptions of self and other. Participants (n = 83, mean age = 15.4) viewed sexualized or performance images (n = 5) of male celebrity athletes and then completed explicit and implicit measures of self-perceptions. They also judged the athletic competence and respectability of the athletes in the images. Results indicated that viewing sexualized images resulted in lower self-esteem and lower ratings of the athletic competence and respectability of the athletes in the photos compared to viewing performance images. These findings are among the first to demonstrate the negative effects of viewing sexualized images of male athletes on adolescent males
Measurements of the O+ plus N2 and O+ plus O2 reaction rates from 300 to 900 K
Rate coefficients for the O(+) + N2 atom transfer and O(+) + O2 charge transfer reactions are determined at thermal energies between 300 K and 900 K difference in a heated drift tube mass spectrometer apparatus. At 300 K the values K(O(+) + N2) = (1.2 plus or minus 0.1) x 10 to the negative 12 power cubic cm/sec and k(O(+) + O2) = (2.1 plus or minus 0.2) x 10 to the negative 11 power cubic cm/sec were obtained, with a 50% difference decrease in the reaction rates upon heating to 700 K. These results are in good agreement with heated flowing afterglow results, but the O(+) + O2 thermal rate coefficients are systematically lower than equivalent Maxwellian rates inferred by conversion of nonthermal drift tube and flow drift data
Electron-temperature dependence of dissociative recombination of electrons with CO(+)-(CO)n-series ions
A microwave afterglow mass spectrometer apparatus is used to determine the dependence on electron temperature T sub e of the recombination coefficients alpha sub n of the dimer and trimer ions of the series CO+.(CO) sub n. It is found that alpha sub 1 = (1.3 + or - 0.3)x 0.000001 (T sub e(K)/300) to the -0.34; and alpha sub 2 = (1.9 + or - 0.4)x 0.000001 (T sub e(K)/300) to the -0.33 cu cm/sec. These dependences on T sub e are quite different from those obtained previously for polar-cluster ions of the hydronium and ammonium series but are similar to that for simple diatomic ions
Reactions of Na/plus/, K/plus/, and Ba/plus/ ions with O2, NO, and H2O molecules
Investigating ion molecule reactions of sodium, potassium, and barium ions with oxygen, nitric oxide, and water in drift tube mass spectromete
Measurements of recombination of electrons with H3(plus) and H5(plus) ions
The electron-ion recombination coefficients for H3(+) and H5(+) ions were determined by means of a microwave afterglow/mass spectrometer apparatus. Measurements of electron density decays in helium-hydrogen mixtures are correlated with the decay of mass-identified ion currents to the wall of the microwave cavity. At low partial pressures of hydrogen in the mixture, the ion H3(+) dominates the ion composition and the ion wall current tracks the electron density decay curves. From recombination controlled electron density decay curves, the values alpha (H3(+)) = (2.9 + or - 0.3), (2.3 + or - 0.3), and (2.0 + or - 0.2) x 0.0000001 cu cm per sec, are obtained at 205, 300 and 450 K, respectively. At higher partial pressures of hydrogen and low temperatures, where (H5(+)) is the dominant ion, the value alpha (H5(+)) = (3.6 + or - 1.0) x 0.0000001 cu cm per sec is obtained at 205 K. The implications of these results concerning ionization levels in the atmospheres of the outer planets and in the interstellar medium are discussed
On the contribution of thermal excitation to the total 630.0 nm emissions in the northern cusp ionosphere
Direct impact excitation by precipitating electrons is believed to be the
main source of 630.0 nm emissions in the cusp ionosphere. However, this paper
investigates a different source, 630.0 emissions caused by thermally excited
atomic oxygen OD) when high electron temperature prevail in the cusp. On
22 January 2012 and 14 January 2013, the European Incoherent Scatter Scientific
Association (EISCAT) radar on Svalbard measured electron temperature
enhancements exceeding 3000 K near magnetic noon in the cusp ionosphere over
Svalbard. The electron temperature enhancements corresponded to electron
density enhancements exceeding m accompanied by intense 630.0
nm emissions in a field of view common to both the EISCAT Svalbard radar and a
meridian scanning photometer. This offered an excellent opportunity to
investigate the role of thermally excited OD) 630.0 nm emissions in the
cusp ionosphere. The thermal component was derived from the EISCAT Radar
measurements and compared with optical data. For both events the calculated
thermal component had a correlation coefficient greater than 0.8 to the total
observed 630.0 nm intensity which contains both thermal and particle impact
components. Despite fairly constant solar wind, the calculated thermal
component intensity fluctuated possibly due to dayside transients in the
aurora
A class of well-posed parabolic final value problems
This paper focuses on parabolic final value problems, and well-posedness is
proved for a large class of these. The clarification is obtained from Hilbert
spaces that characterise data that give existence, uniqueness and stability of
the solutions. The data space is the graph normed domain of an unbounded
operator that maps final states to the corresponding initial states. It induces
a new compatibility condition, depending crucially on the fact that analytic
semigroups always are invertible in the class of closed operators. Lax--Milgram
operators in vector distribution spaces constitute the main framework. The
final value heat conduction problem on a smooth open set is also proved to be
well posed, and non-zero Dirichlet data are shown to require an extended
compatibility condition obtained by adding an improper Bochner integral.Comment: 16 pages. To appear in "Applied and numerical harmonic analysis"; a
reference update. Conference contribution, based on arXiv:1707.02136, with
some further development
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