2,246 research outputs found

    Cryogenic Magneto-Terahertz Scanning Near-field Optical Microscope (cm-SNOM)

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    We have developed a versatile near-field microscopy platform that can operate at high magnetic fields and below liquid-helium temperatures. We use this platform to demonstrate an extreme terahertz (THz) nanoscope operation and to obtain the first cryogenic magneto-THz time-domain nano-spectroscopy/imaging at temperatures as low as 1.8 K and magnetic fields of up to 5 T simultaneously. Our cryogenic magneto-THz scanning near-field optical microscopy, or cm-SNOM, instrument comprises three main equipment: i) a 5 T split pair magnetic cryostat with a custom made insert for mounting SNOM inside; ii) an atomic force microscope (AFM) unit that accepts ultrafast THz excitation and iii) a MHz repetition rate, femtosecond laser amplifier for high-field THz pulse generation and sensitive detection. We apply the cm-SNOM to obtain proof of principle measurements of superconducting and topological materials. The new capabilities demonstrated break grounds for studying quantum materials that requires extreme environment of cryogenic operation and applied magnetic fields simultaneously in nanometer space, femtosecond time, and terahertz energy scales

    Van der Waals epitaxy of Bi2Se3 on Si(111) vicinal surface: An approach to prepare high-quality thin films of topological insulator

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    Epitaxial growth of topological insulator Bi2Se3 thin films on nominally flat and vicinal Si(111) substrates is studied. In order to achieve planner growth front and better quality epifilms, a two-step growth method is adopted for the van der Waal epitaxy of Bi2Se3 to proceed. By employing vicinal Si(111) substrate surfaces, the in-pane growth rate anisotropy of Bi2Se3 is explored to achieve single crystalline Bi2Se3 epifilms, in which threading defects and twins are effectively suppressed. Optimization of the growth parameters has resulted in vicinal Bi2Se3 films showing a carrier mobility of ~ 2000 cm2V-1s-1 and the background doping of ~ 3 x 1018 cm-3 of the as-grown layers. Such samples not only show relatively high magnetoresistance but also a linear dependence on magnetic field.Comment: 18 pages, 4 figure

    Exact calculation of the skyrmion lifetime in a ferromagnetic Bose condensate

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    The tunneling rate of a skyrmion in ferromagnetic spin-1/2 Bose condensates through an off-centered potential barrier is calculated exactly with the periodic instanton method. The prefactor is shown to depend on the chemical potential of the core atoms, at which level the atom tunnels. Our results can be readily extended to estimate the lifetime of other topological excitations in the condensate, such as vortices and monopoles.Comment: 16 pages, 4 figures, to appear Phys. Rev.

    Detecting massive gravitons using pulsar timing arrays

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    Massive gravitons are features of some alternatives to general relativity. This has motivated experiments and observations that, so far, have been consistent with the zero mass graviton of general relativity, but further tests will be valuable. A basis for new tests may be the high sensitivity gravitational wave experiments that are now being performed, and the higher sensitivity experiments that are being planned. In these experiments it should be feasible to detect low levels of dispersion due to nonzero graviton mass. One of the most promising techniques for such a detection may be the pulsar timing program that is sensitive to nano-Hertz gravitational waves. Here we present some details of such a detection scheme. The pulsar timing response to a gravitational wave background with the massive graviton is calculated, and the algorithm to detect the massive graviton is presented. We conclude that, with 90% probability, massles gravitons can be distinguished from gravitons heavier than 3Γ—10βˆ’223\times 10^{-22} eV (Compton wave length Ξ»g=4.1Γ—1012\lambda_{\rm g}=4.1 \times 10^{12} km), if biweekly observation of 60 pulsars are performed for 5 years with pulsar RMS timing accuracy of 100 ns. If 60 pulsars are observed for 10 years with the same accuracy, the detectable graviton mass is reduced to 5Γ—10βˆ’235\times 10^{-23} eV (Ξ»g=2.5Γ—1013\lambda_{\rm g}=2.5 \times 10^{13} km); for 5-year observations of 100 or 300 pulsars, the sensitivity is respectively 2.5Γ—10βˆ’222.5\times 10^{-22} (Ξ»g=5.0Γ—1012\lambda_{\rm g}=5.0\times 10^{12} km) and 10βˆ’2210^{-22} eV (Ξ»g=1.2Γ—1013\lambda_{\rm g}=1.2\times 10^{13} km). Finally, a 10-year observation of 300 pulsars with 100 ns timing accuracy would probe graviton masses down to 3Γ—10βˆ’233\times 10^{-23} eV (Ξ»g=4.1Γ—1013\lambda_{\rm g}=4.1\times 10^{13} km).Comment: 13 pages, 5 figures, Accepted by Ap

    Π€ΠΎΡ€ΠΌΠΈΡ€ΠΎΠ²Π°Π½ΠΈΠ΅ ΠΈ Ρ€Π°Π·Π²ΠΈΡ‚ΠΈΠ΅ Ρ€Ρ‹Π½ΠΊΠ° экологичСски чистых ΠΏΡ€ΠΎΠ΄ΡƒΠΊΡ‚ΠΎΠ² Π² России

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    Π Π°Π±ΠΎΡ‚Π° Π½Π°ΠΏΡ€Π°Π²Π»Π΅Π½Π° Π½Π° выявлСниС особСнностСй формирования ΠΈ Π½Π°ΠΏΡ€Π°Π²Π»Π΅Π½ΠΈΠΉ развития российского Ρ€Ρ‹Π½ΠΊΠ° экологичСски чистой ΠΏΡ€ΠΎΠ΄ΠΎΠ²ΠΎΠ»ΡŒΡΡ‚Π²Π΅Π½Π½ΠΎΠΉ ΠΏΡ€ΠΎΠ΄ΡƒΠΊΡ†ΠΈΠΈ, Π° Ρ‚Π°ΠΊ ΠΆΠ΅ Π½Π° Ρ€Π°Π·Ρ€Π°Π±ΠΎΡ‚ΠΊΡƒ ΠΏΡ€ΠΎΠ³Ρ€Π°ΠΌΠΌΡ‹ ΠΏΠΎΠ²Ρ‹ΡˆΠ΅Π½ΠΈΡ эффСктивности ΠΈ устойчивости функционирования прСдприятий Π΄Π°Π½Π½ΠΎΠΉ сфСры Π΄Π΅ΡΡ‚Π΅Π»ΡŒΠ½ΠΎΡΡ‚ΠΈ.The work is aimed at identifying the features of formation and directions development of the Russian market of ecologically pure food products, and As well as the development of a program to increase efficiency and sustainability Functioning of enterprises in this field of activity
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