866 research outputs found
Tycho's SNR as the source of cosmic rays and gamma-quanta with energy of 1 - 30 TeV in Galaxy
The TeV gamma emission of the far active galaxies 1739+522 (z=1.375), 3c454.3 (z=0.859) and Markarian 501 (z=0.034), Markarian 421 (z=0.031)
Periodically modulated geometric and electronic structure of graphene on Ru(0001)
We report here on a method to fabricate and characterize highly perfect,
periodically rippled graphene monolayers and islands, epitaxially grown on
single crystal metallic substrates under controlled UHV conditions. The
periodicity of the ripples is dictated by the difference in lattice parameters
of graphene and substrate, and, thus, it is adjustable. We characterize its
perfection at the atomic scale by means of STM and determine its electronic
structure in the real space by local tunnelling spectroscopy. There are
periodic variations in the geometric and electronic structure of the graphene
monolayer. We observe inhomogeneities in the charge distribution, i.e a larger
occupied Density Of States at the higher parts of the ripples. Periodically
rippled graphene might represent the physical realization of an ordered array
of coupled graphene quantum dots. The data show, however, that for rippled
graphene on Ru(0001) both the low and the high parts of the ripples are
metallic. The fabrication of periodically rippled graphene layers with
controllable characteristic length and different bonding interactions with the
substrate will allow a systematic experimental test of this fundamental
problem.Comment: 12 pages. Contribution to the topical issue on graphene of
Semiconductor Science and Technolog
Extragalactic Background Light expected from photon-photon absorption on spectra of distant Active Galactic Nuclei
Extragalactic background radiation blocks the propagation of TeV gamma-ray over large distances by producing e+e− pairs. As a result, primary spectrum of gamma-source is changed, depending on spectrum of background light. So, hard spectra of Active Galactic Nuclei with high red shifts allow the determination of a EBL spectrum. The redshifts of SHALON TeV gamma-ray sources range from 0.018 to 1.375 those spectra are resolved at the energies from 800GeV to 30 TeV. Spectral energy distribution of EBL constrained from observations of Mkn421 (z=0.031), Mkn501 (z=0.034), Mkn180 (z=0.046), OJ287 (z=0.306), 3c454.3 (z=0.859) and 1739+5220(z=1.375) together with models and measurements are presented
Selection of the optimal frequency of the signal exciting winding of u-shaped eddy-current probe with ferromagnetic core
The paper presents the results of the investigations of eddy current parameters of the U-shaped probe. Optimalfrequencies of NDTsolderingwere foundfor the two groups of samples –nonferromagnetic busbars and cylindrical conductors with diameter 9 and 5.5 mm.В работе представлены результаты измеренийвихретоковых параметров П-образного вихретокового преобразователя. Экспериментально были установлены оптимальные частоты контроля степени пропаянности для двух групп образцов – неферромагнитных токопроводящих шин и цилиндрических токопроводов диаметром 9 мм и 5,5 мм
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