683 research outputs found
Influence of intermartensitic transitions on transport properties of Ni2.16Mn0.84Ga alloy
Magnetic, transport, and x-ray diffraction measurements of ferromagnetic
shape memory alloy NiMnGa revealed that this alloy undergoes
an intermartensitic transition upon cooling, whereas no such a transition is
observed upon subsequent heating. The difference in the modulation of the
martensite forming upon cooling from the high-temperature austenitic state
[5-layered (5M) martensite], and the martensite forming upon the
intermartensitic transition [7-layered (7M) martensite] strongly affects the
magnetic and transport properties of the alloy and results in a large thermal
hysteresis of the resistivity and magnetization . The
intermartensitic transition has an especially marked influence on the transport
properties, as is evident from a large difference in the resistivity of the 5M
and 7M martensite, , which is larger than the jump of resistivity at
the martensitic transition from the cubic austenitic phase to the monoclinic 5M
martensitic phase. We assume that this significant difference in between
the martensitic phases is accounted for by nesting features of the Fermi
surface. It is also suggested that the nesting hypothesis can explain the
uncommon behavior of the resistivity at the martensitic transition, observed in
stoichiometric and near-stoichiometric Ni-Mn-Ga alloys.Comment: 7 pages, 6 figures, REVTEX
Novel Scintillation Material - ZnO Transparent Ceramics
ZnO-based scintillation ceramics for application in HENPA LENPA analyzers
have been investigated. The following ceramic samples have been prepared:
undoped ones (ZnO), an excess of zinc in stoichiometry (ZnO:Zn), doped with
gallium (ZnO:Ga) and lithium (ZnO:Li). Optical transmission, x-ray excited
emission, scintillation decay and pulse height spectra were measured and
analyzed. Ceramics have reasonable transparency in visible range (up to 60% for
0.4 mm thickness) and energy resolution (14.9% at 662 keV Cs137 gamma
excitation). Undoped ZnO shows slow (1.6 {\mu}s) luminescence with maximum at
2.37 eV and light yield about 57% of CsI:Tl. ZnO:Ga ceramics show relatively
low light yield with ultra fast decay time (1 ns). Lithium doped ceramics
ZnO:Li have better decay time than undoped ZnO with fair light yield. ZnO:Li
ceramics show good characteristics under alpha-particle excitation and can be
applied for the neutral particle analyzers.Comment: 4 pages, 8 figures, research covered in this paper was presented at
SCINT2011 conference as a poster, submitted for publication at IEEE Trans.
Nucl. Sc
Strongly nonlinear dynamics of electrolytes in large ac voltages
We study the response of a model micro-electrochemical cell to a large ac
voltage of frequency comparable to the inverse cell relaxation time. To bring
out the basic physics, we consider the simplest possible model of a symmetric
binary electrolyte confined between parallel-plate blocking electrodes,
ignoring any transverse instability or fluid flow. We analyze the resulting
one-dimensional problem by matched asymptotic expansions in the limit of thin
double layers and extend previous work into the strongly nonlinear regime,
which is characterized by two novel features - significant salt depletion in
the electrolyte near the electrodes and, at very large voltage, the breakdown
of the quasi-equilibrium structure of the double layers. The former leads to
the prediction of "ac capacitive desalination", since there is a time-averaged
transfer of salt from the bulk to the double layers, via oscillating diffusion
layers. The latter is associated with transient diffusion limitation, which
drives the formation and collapse of space-charge layers, even in the absence
of any net Faradaic current through the cell. We also predict that steric
effects of finite ion sizes (going beyond dilute solution theory) act to
suppress the strongly nonlinear regime in the limit of concentrated
electrolytes, ionic liquids and molten salts. Beyond the model problem, our
reduced equations for thin double layers, based on uniformly valid matched
asymptotic expansions, provide a useful mathematical framework to describe
additional nonlinear responses to large ac voltages, such as Faradaic
reactions, electro-osmotic instabilities, and induced-charge electrokinetic
phenomena.Comment: 30 pages, 17 eps-figures, RevTe
Resonant Cyclotron Radiation Transfer Model Fits to Spectra from Gamma-Ray Burst GRB870303
We demonstrate that models of resonant cyclotron radiation transfer in a
strong field (i.e. cyclotron scattering) can account for spectral lines seen at
two epochs, denoted S1 and S2, in the Ginga data for GRB870303. Using a
generalized version of the Monte Carlo code of Wang et al. (1988,1989b), we
model line formation by injecting continuum photons into a static
plane-parallel slab of electrons threaded by a strong neutron star magnetic
field (~ 10^12 G) which may be oriented at an arbitrary angle relative to the
slab normal. We examine two source geometries, which we denote "1-0" and "1-1,"
with the numbers representing the relative electron column densities above and
below the continuum photon source plane. We compare azimuthally symmetric
models, i.e. models in which the magnetic field is parallel to the slab normal,
with models having more general magnetic field orientations. If the bursting
source has a simple dipole field, these two model classes represent line
formation at the magnetic pole, or elsewhere on the stellar surface. We find
that the data of S1 and S2, considered individually, are consistent with both
geometries, and with all magnetic field orientations, with the exception that
the S1 data clearly favor line formation away from a polar cap in the 1-1
geometry, with the best-fit model placing the line-forming region at the
magnetic equator. Within both geometries, fits to the combined (S1+S2) data
marginally favor models which feature equatorial line formation, and in which
the observer's orientation with respect to the slab changes between the two
epochs. We interpret this change as being due to neutron star rotation, and we
place limits on the rotation period.Comment: LaTeX2e (aastex.cls included); 45 pages text, 17 figures (on 21
pages); accepted by ApJ (to be published 1 Nov 1999, v. 525
Gamma Ray Bursts from the Evolved Galactic Nuclei
A new cosmological scenario for the origin of gamma ray bursts (GRBs) is
proposed. In our scenario, a highly evolved central core in the dense galactic
nucleus is formed containing a subsystem of compact stellar remnants (CSRs),
such as neutron stars and black holes. Those subsystems result from the
dynamical evolution of dense central stellar clusters in the galactic nuclei
through merging of stars, thereby forming (as has been realized by many
authors) the short-living massive stars and then CSRs. We estimate the rate of
random CSR collisions in the evolved galactic nuclei by taking into account,
similar to Quinlan & Shapiro (1987), the dissipative encounters of CSRs, mainly
due to radiative losses of gravitational waves, which results in the formation
of intermediate short-living binaries, with further coalescence of the
companions to produce GRBs. We also consider how the possible presence of a
central supermassive black hole, formed in a highly evolved galactic nucleus,
influences the CSR binary formation. This scenario does not postulate ad hoc a
required number of tight binary neutron stars in the galaxies. Instead, it
gives, for the most realistic parameters of the evolved nuclei, the expected
rate of GRBs consistent with the observed one, thereby explaining the GRB
appearance in a natural way of the dynamical evolution of galactic nuclei. In
addition, this scenario provides an opportunity for a cosmological GRB
recurrence, previously considered to be a distinctive feature of GRBs of a
local origin only. We also discuss some other observational tests of the
proposed scenario.Comment: 25 pages, LATEX, uses aasms4.sty, accepted by Ap
Mechanisms of Manganese-Assisted Nonradiative Recombination in Cd(Mn)Se/Zn(Mn)Se Quantum Dots
Mechanisms of nonradiative recombination of electron-hole complexes in
Cd(Mn)Se/Zn(Mn)Se quantum dots accompanied by interconfigurational excitations
of Mn ions are analyzed within the framework of single electron model of
deep {\it 3d}-levels in semiconductors. In addition to the mechanisms caused by
Coulomb and exchange interactions, which are related because of the Pauli
principle, another mechanism due to {\it sp-d} mixing is considered. It is
shown that the Coulomb mechanism reduces to long-range dipole-dipole energy
transfer from photoexcited quantum dots to Mn ions. The recombination
due to the Coulomb mechanism is allowed for any states of Mn ions and
{\it e-h} complexes. In contrast, short-range exchange and
recombinations are subject to spin selection rules, which are the result of
strong {\it lh-hh} splitting of hole states in quantum dots. Estimates show
that efficiency of the {\it sp-d} mechanism can considerably exceed that of the
Coulomb mechanism. The phonon-assisted recombination and processes involving
upper excited states of Mn ions are studied. The increase in PL
intensity of an ensemble of quantum dots in a magnetic field perpendicular to
the sample growth plane observed earlier is analyzed as a possible
manifestation of the spin-dependent recombination.Comment: 14 pages, 2 figure
ПОРІВНЯЛЬНИЙ АНАЛІЗ КІРЛІАНОГРАФІЧНОГО СВІТІННЯ БІОЛОГІЧНОЇ ТКАНИНИ З БІОХІМІЧНИМИ ПРОЦЕСАМИ
Kirlian diagram samples Conducted. Achilles tendon dead people with various postmorbidnym period (from 5:0 until 22 days) and optoelectronics is part of the standard terms of the x-ray film developer. The results obtained were compared with biochemical indicators of the level of enzymes and content of degradation products of proteins, trace elements, derived from the investigated samples. For kirlianograficeskih studies used an experimental device, RIVERS 1, developed by Ukrainian Scientific Research Institute of mechanical engineering technologies (Dnepropetrovsk). For mathematical processing of results using Matlab program.The growing shortage of ATP causes the breach and termination of ion exchange, increases reactive oxygen generation, lipid peroxidation destroys cell membranes. The process of self digestion (autoliza) tissue tendons, as shown by the results of the experiments, had cyclical changes metabolism enzyme activity (ALT), carbohydrate (LDH), nucleotides, of total protein and micronutrients.Cравнивали кирлианографические изображения образцов и жидкой части ахиллова сухожилия разного по-стморбидного периода (от 5 часов до 22 суток) с показателями биохимических исследований в процессе аутолиза. Кирлианографию проводили на рентгеновской пленке. Использовали экспериментальный прибор «РЕК 1» (г. Днепропетровск). Процесс самопереваривания (аутолиза) тканей сухожилия, как показали результаты экспериментов, имел циклический характер изменения активности ферментов обмена аминокислот (АЛТ), углеводов (ЛДГ), нукле-отидов (мочевая кислота, мочевина), содержания общего белка и микроэлементов. Изменение площади засветки и фрактальности кирлиановских изображений также имело цикличный характер по давности аутолиза, что ображало характер энергетических изменений по содержанию взаимодействующих веществ.Порівняли кірліанографічне зображення зразків та рідини ахілового сухожилка різного постморбідного періоду (від 5 годин до 22 діб) із показниками біохімічних досліджень в процесі аутолізу. Кірліанографію проводили на рентгенівській плівці. Використовували експериментальний прилад «РЕК 1» (м. Дніпропетровськ). Процес саморуйнування тканин сухожилка, як показали результати експериментів, мав циклічний характер змінення активності ферментів обміну амінокислот (АЛТ), вуглеводів (ЛДГ), нуклеотидів (сечова кислота, сечовина), вмісту загального білка та мікроелементів. Зміни площі засвітки та фрактальності кірліанограм крапель біологічної речовини в процесі аутолізу також мали циклічність з часом, що віддзеркалювало характер енергетичних змін за вмістом речовин взаємодії
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