297 research outputs found

    New Research in the Military History of the Late Rome and Early Byzantium

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    Submitted: 08.07.2020. Accepted: 15.10.2020.ΠŸΠΎΡΡ‚ΡƒΠΏΠΈΠ»Π° 08.07.2020. ΠŸΡ€ΠΈΠ½ΡΡ‚Π° 15.10.2020.A review of: Mekhamadiev, E. A. (2019). Voennaia organizatsiia pozdnei Rimskoi imperii v 253–353 gg.: ot reform imperatora Galliena do perioda Tetrarkhii (253–305) [A Military Organization of the Later Roman Empire in 253–353 AD: From Emperor Gallienus’ Reforms to the Age of the Tetrarchy (253–305)]. St Petersburg: Peterburgskoe Vostokovedenie Publishers. 406 p. This paper states that the monograph published E. A. Mekhamadiev, a researcher from St. Petersburg, is a fundamental study of the Later Roman military organization, with especial attention to the epigraphic and papyrological accounts. The use of these sources allows the author to reconstruct the history of specific military units, their spatial movements, participation in various military campaigns and wars, and changes in their ranks. Important is that Mekhamadiev examined the internal (organizational) structure of all regional armies of the Roman empire from 253 to 305 and not restricted himself to specific and narrow aspects of history of a particular province or country. The author of the book under present review has analysed the data related to both the eastern and the western imperial provinces, discovered close interrelations of the western and eastern provinces, and indicated permanent movements of the military units from the west to east and in the opposite direction depending on the geopolitical and home political situation.РСцСнзия Π½Π° ΠΊΠ½ΠΈΠ³Ρƒ: ΠœΠ΅Ρ…Π°ΠΌΠ°Π΄ΠΈΠ΅Π² Π•. А. ВоСнная организация ΠΏΠΎΠ·Π΄Π½Π΅ΠΉ Римской ΠΈΠΌΠΏΠ΅Ρ€ΠΈΠΈ Π² 253–353 Π³Π³.: ΠΎΡ‚ Ρ€Π΅Ρ„ΠΎΡ€ΠΌ ΠΈΠΌΠΏΠ΅Ρ€Π°Ρ‚ΠΎΡ€Π° Π“Π°Π»Π»ΠΈΠ΅Π½Π° Π΄ΠΎ ΠΏΠ΅Ρ€ΠΈΠΎΠ΄Π° Π’Π΅Ρ‚Ρ€Π°Ρ€Ρ…ΠΈΠΈ (253–305). БПб. : ΠŸΠ΅Ρ‚Π΅Ρ€Π±ΡƒΡ€Π³ΡΠΊΠΎΠ΅ востоковСдСниС, 2019. 406 с. Π’ ΡΡ‚Π°Ρ‚ΡŒΠ΅ отмСчаСтся, Ρ‡Ρ‚ΠΎ рСцСнзируСмая ΠΊΠ½ΠΈΠ³Π° пСтСрбургского исслСдоватСля Π•. А. ΠœΠ΅Ρ…Π°ΠΌΠ°Π΄ΠΈΠ΅Π²Π° являСтся Ρ„ΡƒΠ½Π΄Π°ΠΌΠ΅Π½Ρ‚Π°Π»ΡŒΠ½Ρ‹ΠΌ исслСдованиСм ΠΏΠΎ Π²ΠΎΠ΅Π½Π½ΠΎΠΉ ΠΎΡ€Π³Π°Π½ΠΈΠ·Π°Ρ†ΠΈΠΈ ΠΏΠΎΠ·Π΄Π½Π΅Π³ΠΎ Π ΠΈΠΌΠ°, Π² ΠΊΠΎΡ‚ΠΎΡ€ΠΎΠΌ сдСлан особый Π°ΠΊΡ†Π΅Π½Ρ‚ Π½Π° Π΄Π°Π½Π½Ρ‹Π΅ эпиграфики ΠΈ ΠΏΠ°ΠΏΠΈΡ€ΠΎΠ»ΠΎΠ³ΠΈΠΈ. Π˜Ρ… ΠΏΡ€ΠΈΠ²Π»Π΅Ρ‡Π΅Π½ΠΈΠ΅ ΠΏΠΎΠ·Π²ΠΎΠ»ΠΈΠ»ΠΈ Π°Π²Ρ‚ΠΎΡ€Ρƒ Ρ€Π΅ΠΊΠΎΠ½ΡΡ‚Ρ€ΡƒΠΈΡ€ΠΎΠ²Π°Ρ‚ΡŒ ΠΈΡΡ‚ΠΎΡ€ΠΈΡŽ ΠΎΡ‚Π΄Π΅Π»ΡŒΠ½Ρ‹Ρ… войсковых ΠΏΠΎΠ΄Ρ€Π°Π·Π΄Π΅Π»Π΅Π½ΠΈΠΉ, ΠΈΡ… Ρ‚Π΅Ρ€Ρ€ΠΈΡ‚ΠΎΡ€ΠΈΠ°Π»ΡŒΠ½Ρ‹Π΅ пСрСмСщСния, участиС Π² Ρ€Π°Π·Π»ΠΈΡ‡Π½Ρ‹Ρ… Π²ΠΎΠ΅Π½Π½Ρ‹Ρ… кампаниях ΠΈ ΠΏΠΎΡ…ΠΎΠ΄Π°Ρ…, измСнСния Ρ€Π°Π½Π³ΠΎΠ². УказываСтся, Ρ‡Ρ‚ΠΎ Π•. А. ΠœΠ΅Ρ…Π°ΠΌΠ°Π΄ΠΈΠ΅Π² рассмотрСл Π²Π½ΡƒΡ‚Ρ€Π΅Π½Π½ΡŽΡŽ (ΠΎΡ€Π³Π°Π½ΠΈΠ·Π°Ρ†ΠΈΠΎΠ½Π½ΡƒΡŽ) структуру всСх Ρ€Π΅Π³ΠΈΠΎΠ½Π°Π»ΡŒΠ½Ρ‹Ρ… Π°Ρ€ΠΌΠΈΠΉ Π ΠΈΠΌΠ° с 253 ΠΏΠΎ 305 Π³., Π½Π΅ ограничился исслСдованиСм ΠΎΡ‚Π΄Π΅Π»ΡŒΠ½Ρ‹Ρ… ΠΈ ΡƒΠ·ΠΊΠΈΡ… ΡΡŽΠΆΠ΅Ρ‚ΠΎΠ², связанных с историСй ΠΎΡ‚Π΄Π΅Π»ΡŒΠ½ΠΎ взятой импСрской ΠΏΡ€ΠΎΠ²ΠΈΠ½Ρ†ΠΈΠΈ ΠΈΠ»ΠΈ Ρ€Π΅Π³ΠΈΠΎΠ½Π°. Автор Ρ€Π΅Ρ†Π΅Π½Π·ΠΈΡ€ΡƒΠ΅ΠΌΠΎΠΉ ΠΊΠ½ΠΈΠ³ΠΈ ΠΏΡ€ΠΎΠ°Π½Π°Π»ΠΈΠ·ΠΈΡ€ΠΎΠ²Π°Π» Π΄Π°Π½Π½Ρ‹Π΅ ΠΊΠ°ΠΊ ΠΏΠΎ восточным, Ρ‚Π°ΠΊ ΠΈ ΠΏΠΎ Π·Π°ΠΏΠ°Π΄Π½Ρ‹ΠΌ провинциям ΠΈΠΌΠΏΠ΅Ρ€ΠΈΠΈ, выявил Ρ‚Π΅ΡΠ½ΡƒΡŽ взаимосвязь Π·Π°ΠΏΠ°Π΄Π½Ρ‹Ρ… ΠΈ восточных ΠΏΡ€ΠΎΠ²ΠΈΠ½Ρ†ΠΈΠΉ, ΡƒΠΊΠ°Π·Π°Π» Π½Π° постоянныС пСрСмСщСния войсковых ΠΏΠΎΠ΄Ρ€Π°Π·Π΄Π΅Π»Π΅Π½ΠΈΠΉ с Π·Π°ΠΏΠ°Π΄Π° Π½Π° восток ΠΈ Π² ΠΎΠ±Ρ€Π°Ρ‚Π½ΡƒΡŽ сторону Π² зависимости ΠΎΡ‚ гСополитичСской ΠΈ внутриполитичСской ситуации

    Ocular Manifestations In COVID-19: Clinical Case Reports And A Literature (Review)

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    Coronavirus disease 2019 (COVID-19) has affected more than 130 million people as of April 2021. During the current pandemic, SARS-CoV-2 has been found to cause conjunctivitis with anecdotal evidence of a wide range of manifestations from scleritis to retinitis, occlusive vasculitis and optic neuritis. The purpose of this study is to raise awareness about possible COVID-19 related ocular manifestations, including papillophlebitis, anterior ischemic optic neuropathy, uveitis and neuroretinitis. Further detailed analyses will be needed to elucidate the link between SARS-CoV-2 and ocular pathology

    Search for a new gauge boson in the Aβ€²A' Experiment (APEX)

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    We present a search at Jefferson Laboratory for new forces mediated by sub-GeV vector bosons with weak coupling Ξ±β€²\alpha' to electrons. Such a particle Aβ€²A' can be produced in electron-nucleus fixed-target scattering and then decay to an e+eβˆ’e^+e^- pair, producing a narrow resonance in the QED trident spectrum. Using APEX test run data, we searched in the mass range 175--250 MeV, found no evidence for an Aβ€²β†’e+eβˆ’A'\to e^+e^- reaction, and set an upper limit of Ξ±β€²/α≃10βˆ’6\alpha'/\alpha \simeq 10^{-6}. Our findings demonstrate that fixed-target searches can explore a new, wide, and important range of masses and couplings for sub-GeV forces.Comment: 5 pages, 5 figures, references adde

    Evidence for proton acceleration up to TeV energies based on VERITAS and Fermi-LAT observations of the Cas A SNR

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    We present a study of Ξ³\gamma-ray emission from the core-collapse supernova remnant Cas~A in the energy range from 0.1GeV to 10TeV. We used 65 hours of VERITAS data to cover 200 GeV - 10 TeV, and 10.8 years of \textit{Fermi}-LAT data to cover 0.1-500 GeV. The spectral analysis of \textit{Fermi}-LAT data shows a significant spectral curvature around 1.3Β±0.4stat1.3 \pm 0.4_{stat} GeV that is consistent with the expected spectrum from pion decay. Above this energy, the joint spectrum from \textit{Fermi}-LAT and VERITAS deviates significantly from a simple power-law, and is best described by a power-law with spectral index of 2.17Β±0.02stat2.17\pm 0.02_{stat} with a cut-off energy of 2.3Β±0.5stat2.3 \pm 0.5_{stat} TeV. These results, along with radio, X-ray and Ξ³\gamma-ray data, are interpreted in the context of leptonic and hadronic models. Assuming a one-zone model, we exclude a purely leptonic scenario and conclude that proton acceleration up to at least 6 TeV is required to explain the observed Ξ³\gamma-ray spectrum. From modeling of the entire multi-wavelength spectrum, a minimum magnetic field inside the remnant of Bminβ‰ˆ150 μGB_{\mathrm{min}}\approx150\,\mathrm{\mu G} is deduced.Comment: 33 pages, 9 Figures, 6 Table

    New Measurements of the Transverse Beam Asymmetry for Elastic Electron Scattering from Selected Nuclei

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    We have measured the beam-normal single-spin asymmetry An in the elastic scattering of 1-3 GeV transversely polarized electrons from H-1 and for the first time from He-4, C-12, and Pb-208. For H-1, He-4, and C-12, the measurements are in agreement with calculations that relate A(n) to the imaginary part of the two-photon exchange amplitude including inelastic intermediate states. Surprisingly, the Pb-208 result is significantly smaller than the corresponding prediction using the same formalism. These results suggest that a systematic set of new A(n) measurements might emerge as a new and sensitive probe of the structure of heavy nuclei

    Direct measurement of stellar angular diameters by the VERITAS Cherenkov Telescopes

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    The angular size of a star is a critical factor in determining its basic properties. Direct measurement of stellar angular diameters is difficult: at interstellar distances stars are generally too small to resolve by any individual imaging telescope. This fundamental limitation can be overcome by studying the diffraction pattern in the shadow cast when an asteroid occults a star, but only when the photometric uncertainty is smaller than the noise added by atmospheric scintillation. Atmospheric Cherenkov telescopes used for particle astrophysics observations have not generally been exploited for optical astronomy due to the modest optical quality of the mirror surface. However, their large mirror area makes them well suited for such high-time-resolution precision photometry measurements. Here we report two occultations of stars observed by the VERITAS Cherenkov telescopes with millisecond sampling, from which we are able to provide a direct measurement of the occulted stars' angular diameter at the ≀0.1\leq0.1 milliarcsecond scale. This is a resolution never achieved before with optical measurements and represents an order of magnitude improvement over the equivalent lunar occultation method. We compare the resulting stellar radius with empirically derived estimates from temperature and brightness measurements, confirming the latter can be biased for stars with ambiguous stellar classifications.Comment: Accepted for publication in Nature Astronom
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