159 research outputs found

    Tunka Advanced Instrument for cosmic rays and Gamma Astronomy

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    The paper is a script of a lecture given at the ISAPP-Baikal summer school in 2018. The lecture gives an overview of the Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA) facility including historical introduction, description of existing and future setups, and outreach and open data activities.Comment: Lectures given at the ISAPP-Baikal Summer School 2018: Exploring the Universe through multiple messengers, 12-21 July 2018, Bol'shie Koty, Russi

    Charm CP Violation and the Electric Dipole Moments from the Charm Scale

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    The reported CP asymmetry in D->K^+K^- / pi^+pi^- is argued to be too large to naturally fit the SM. If so, a new source of CP violation is implied in the Delta C=1 sector with a milliweak strength. CP-odd interactions in the flavor-diagonal sector are strongly constrained by the EDMs placing severe limitations on the underlying theory. While the largest effects usually come from the New Physics energy scale, they are strongly model-dependent. Yet the interference of the CP-odd forces manifested in D decays with the conventional CP-even Delta C=1 weak interaction generates at the charm scale a background level. It has been argued that the d_n in the SM is largely generated via such an interference, with mild KM-specific additional suppression. The reported CP asymmetry is expected to generate d_n of 30 to 100 times larger than in the SM, or even higher in certain model yet not quite natural examples. In the SM the charm-induced loop-less |d_n| is expected around 10^{-31}e*cm. On the technical side, we present a compact Ward-identity--based derivation of the induced scalar pion-nucleon coupling in the presence of the CP-odd interactions, which appears once the latter include the right-handed light quarks.Comment: 29pages, 5 figure

    Π€Π°ΠΊΡ‚ΠΎΡ€Ρ‹ риска, ΠΊΡ€ΠΈΡ‚Π΅Ρ€ΠΈΠΈ ΠΈ Π±ΠΈΠΎΠΌΠ°Ρ€ΠΊΠ΅Ρ€Ρ‹ острого поврСТдСния ΠΏΠΎΡ‡Π΅ΠΊ Π² ΠΏΠ΅Ρ€ΠΈΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½ΠΎΠΌ ΠΏΠ΅Ρ€ΠΈΠΎΠ΄Π΅

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    Β It is becoming increasingly important to prevent complications of surgical treatment, including perioperative acute kidney injury due to prolongation of life expectancy and age-related multicomorbidity.Β The objective was to review the recommendations of the expert groups and the studΡƒ results on risk factors, criteria and biomarkers of perioperative acute kidney injury.Materials and methods. Reports on search results for the last 15 years as of May 15, 2023 in the eLibrary, PubMed databases for the keywords Β«acute Β kidney injuryΒ», Β«biomarkerΒ», Β«perioperative periodΒ». The inclusion of reports in the review and their evaluation are based on the authors consensus. Β Results. In the perioperative period, acute kidney injury without a decrease in diuresis and/or an increase in serum creatinine levels up to a certain time Β may occur. This condition, which varies in causes and mechanisms of development, is potentially reversible with timely detection and treatment. The Β study of both biomarkers that surpass creatinine and diuresis in the timing and accuracy of detecting kidney damage/dysfunction, as well as tools for Β a comprehensive assessment and risk stratification of perioperative acute kidney injury, have not yet been completed with evidence-based conclusions. Β Conclusion. The strategy of using laboratory biomarkers in combination with the clinical context and risk factors for the prevention, diagnosis and Β treatment of subclinical acute kidney injury of various origins, supported by the Acute Disease Quality Initiative (2020), could be implemented Β based on additional evidence from future clinical studies.Π‘ ΡƒΠ²Π΅Π»ΠΈΡ‡Π΅Π½ΠΈΠ΅ΠΌ ΠΏΡ€ΠΎΠ΄ΠΎΠ»ΠΆΠΈΡ‚Π΅Π»ΡŒΠ½ΠΎΡΡ‚ΠΈ ΠΆΠΈΠ·Π½ΠΈ ΠΈ связанной с возрастом ΠΌΡƒΠ»ΡŒΡ‚ΠΈΠΊΠΎΠΌΠΎΡ€Π±ΠΈΠ΄Π½ΠΎΡΡ‚ΡŒΡŽ всС Π±ΠΎΠ»ΡŒΡˆΡƒΡŽ Π°ΠΊΡ‚ΡƒΠ°Π»ΡŒΠ½ΠΎΡΡ‚ΡŒ ΠΏΡ€ΠΈΠΎΠ±Ρ€Π΅Ρ‚Π°Π΅Ρ‚ ΠΏΡ€Π΅Π΄ΠΎΡ‚Π²Ρ€Π°Ρ‰Π΅Π½ΠΈΠ΅ ослоТнСний хирургичСского лСчСния, Π² Ρ‚ΠΎΠΌ числС ΠΏΠ΅Ρ€ΠΈΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ острого поврСТдСния ΠΏΠΎΡ‡Π΅ΠΊ. ЦСль – аналитичСский ΠΎΠ±Π·ΠΎΡ€ Ρ€Π΅ΠΊΠΎΠΌΠ΅Π½Π΄Π°Ρ†ΠΈΠΉ экспСртных Π³Ρ€ΡƒΠΏΠΏ ΠΈ Ρ€Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚ΠΎΠ² исслСдований ΠΏΠΎ Ρ„Π°ΠΊΡ‚ΠΎΡ€Π°ΠΌ риска, критСриям ΠΈ Π±ΠΈΠΎΠΌΠ°Ρ€ΠΊΠ΅Ρ€Π°ΠΌ послСопСрационного поврСТдСния ΠΏΠΎΡ‡Π΅ΠΊ. ΠœΠ°Ρ‚Π΅Ρ€ΠΈΠ°Π»Ρ‹ ΠΈ ΠΌΠ΅Ρ‚ΠΎΠ΄Ρ‹. ΠŸΡƒΠ±Π»ΠΈΠΊΠ°Ρ†ΠΈΠΈ Π·Π° послСдниС 15 Π»Π΅Ρ‚, ΠΏΠΎΠ»ΡƒΡ‡Π΅Π½Π½Ρ‹Π΅ поиском Π½Π° Π΄Π°Ρ‚Ρƒ 15 мая 2023Β Π³. Π² Π±Π°Π·Π°Ρ… eLibrary, PubMed ΠΏΠΎ ΠΊΠ»ΡŽΡ‡Π΅Π²Ρ‹ΠΌ словам «остроС ΠΏΠΎΠ²Ρ€Π΅ΠΆΠ΄Π΅Π½ΠΈΠ΅ ΠΏΠΎΡ‡Π΅ΠΊΒ», Β«Π±ΠΈΠΎΠΌΠ°Ρ€ΠΊΠ΅Ρ€Β», Β«ΠΏΠ΅Ρ€ΠΈΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½Ρ‹ΠΉ ΠΏΠ΅Ρ€ΠΈΠΎΠ΄Β». Π’ΠΊΠ»ΡŽΡ‡Π΅Π½ΠΈΠ΅ ΠΏΡƒΠ±Π»ΠΈΠΊΠ°Ρ†ΠΈΠΉ Π² ΠΎΠ±Π·ΠΎΡ€ ΠΈ ΠΈΡ… ΠΎΡ†Π΅Π½ΠΊΠ° основаны Π½Π° согласованном ΠΌΠ½Π΅Π½ΠΈΠΈ Π°Π²Ρ‚ΠΎΡ€ΠΎΠ².Β Π Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹. Π’ ΠΏΠ΅Ρ€ΠΈΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½ΠΎΠΌ ΠΏΠ΅Ρ€ΠΈΠΎΠ΄Π΅ ΠΌΠΎΠΆΠ΅Ρ‚ ΠΈΠΌΠ΅Ρ‚ΡŒ мСсто остроС ΠΏΠΎΡ‡Π΅Ρ‡Π½ΠΎΠ΅ ΠΏΠΎΠ²Ρ€Π΅ΠΆΠ΄Π΅Π½ΠΈΠ΅, Π΄ΠΎ ΠΎΠΏΡ€Π΅Π΄Π΅Π»Π΅Π½Π½ΠΎΠ³ΠΎ Π²Ρ€Π΅ΠΌΠ΅Π½ΠΈ Π½Π΅ ΠΏΡ€ΠΎΡΠ²Π»ΡΡŽΡ‰Π΅Π΅ΡΡ сниТСниСм Π΄ΠΈΡƒΡ€Π΅Π·Π° ΠΈ/ΠΈΠ»ΠΈ нарастаниСм уровня ΠΊΡ€Π΅Π°Ρ‚ΠΈΠ½ΠΈΠ½Π° Π² сывороткС ΠΊΡ€ΠΎΠ²ΠΈ. Π­Ρ‚ΠΎ Π²Π°Ρ€ΡŒΠΈΡ€ΡƒΡŽΡ‰Π΅Π΅ ΠΏΠΎ ΠΏΡ€ΠΈΡ‡ΠΈΠ½Π°ΠΌ ΠΈ ΠΌΠ΅Ρ…Π°Π½ΠΈΠ·ΠΌΠ°ΠΌ развития состояниС ΠΏΠΎΡ‚Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½ΠΎ ΠΎΠ±Ρ€Π°Ρ‚ΠΈΠΌΠΎ ΠΏΡ€ΠΈ своСврСмСнном выявлСнии ΠΈ Π»Π΅Ρ‡Π΅Π½ΠΈΠΈ. Π˜Π·ΡƒΡ‡Π΅Π½ΠΈΠ΅ Π±ΠΈΠΎΠΌΠ°Ρ€ΠΊΠ΅Ρ€ΠΎΠ², прСвосходящих ΡƒΡ€ΠΎΠ²Π΅Π½ΡŒ ΠΊΡ€Π΅Π°Ρ‚ΠΈΠ½ΠΈΠ½Π° ΠΈ Π΄ΠΈΡƒΡ€Π΅Π· Π² сроках ΠΈ точности выявлСния поврСТдСния/дисфункции ΠΏΠΎΡ‡Π΅ΠΊ, Π° Ρ‚Π°ΠΊΠΆΠ΅ инструмСнтов комплСксной ΠΎΡ†Π΅Π½ΠΊΠΈ ΠΈ стратификации риска послСопСрационного поврСТдСния ΠΏΠΎΡ‡Π΅ΠΊ ΠΏΠΎΠΊΠ° Π½Π΅ Π·Π°Π²Π΅Ρ€ΡˆΠΈΠ»ΠΈΡΡŒ Π΄ΠΎΠΊΠ°Π·Π°Ρ‚Π΅Π»ΡŒΠ½Ρ‹ΠΌΠΈ Π·Π°ΠΊΠ»ΡŽΡ‡Π΅Π½ΠΈΡΠΌΠΈ. Π—Π°ΠΊΠ»ΡŽΡ‡Π΅Π½ΠΈΠ΅. ΠŸΠΎΠ΄Π΄Π΅Ρ€ΠΆΠΈΠ²Π°Π΅ΠΌΠ°Ρ Π˜Π½ΠΈΡ†ΠΈΠ°Ρ‚ΠΈΠ²ΠΎΠΉ ΠΏΠΎ ΠΎΠ±Π΅ΡΠΏΠ΅Ρ‡Π΅Π½ΠΈΡŽ качСства ΠΏΡ€ΠΈ острых заболСваниях (2020) стратСгия использования Π»Π°Π±ΠΎΡ€Π°Ρ‚ΠΎΡ€Π½Ρ‹Ρ… Π±ΠΈΠΎΠΌΠ°Ρ€ΠΊΠ΅Ρ€ΠΎΠ² Π² сочСтании с клиничСским контСкстом ΠΈ Ρ„Π°ΠΊΡ‚ΠΎΡ€Π°ΠΌΠΈ риска для ΠΏΡ€ΠΎΡ„ΠΈΠ»Π°ΠΊΡ‚ΠΈΠΊΠΈ, диагностики ΠΈ лСчСния субклиничСского острого ΠΏΠΎΡ‡Π΅Ρ‡Π½ΠΎΠ³ΠΎ поврСТдСния Ρ€Π°Π·Π»ΠΈΡ‡Π½ΠΎΠ³ΠΎ Π³Π΅Π½Π΅Π·Π° ΠΌΠΎΠΆΠ΅Ρ‚ Π±Ρ‹Ρ‚ΡŒ Ρ€Π΅Π°Π»ΠΈΠ·ΠΎΠ²Π°Π½Π° Π½Π° основС Π΄ΠΎΠΏΠΎΠ»Π½ΠΈΡ‚Π΅Π»ΡŒΠ½Ρ‹Ρ… Π΄ΠΎΠΊΠ°Π·Π°Ρ‚Π΅Π»ΡŒΡΡ‚Π² Π±ΡƒΠ΄ΡƒΡ‰ΠΈΡ… клиничСских исслСдований

    First metatarsophalangeal hemiarthroplasty for hallux rigidus

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    There is a paucity of objective information in the literature about first metatarsophalangeal (MTP) hemiarthroplasty. The authors postulate that it is a reasonable treatment option for severe hallux rigidus in selected patients. Twenty-two elective first MTP hemiarthroplasties were performed on 20 patients that met the inclusion criteria. Pre- and postoperative evaluations were done using the American Orthopaedic Foot and Ankle Society (AOFAS) forefoot score, visual analogue scale (VAS) pain score, range of motion (ROM) measurements, and radiographs. Average ROM and dorsiflexion improved by 15Β° and 8Β°, respectively. VAS pain scores improved from 5 to 2.5 after sixΒ weeks. Painless ambulation occurred after sixΒ weeks, with maximum improvement by sixΒ months. After 24Β months, two patients had pain at the surgical site interfering with function, leading to an unsatisfactory result that required conversion to arthrodesis. First MTP hemiarthroplasty for severe hallux rigidus can be considered an alternative to fusion in properly selected patients who wish to maintain a functional range of motion

    Novel metallic implantation technique for osteochondral defects of the medial talar dome: A cadaver study

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    BACKGROUND AND PURPOSE: A metallic inlay implant (HemiCAP) with 15 offset sizes has been developed for the treatment of localized osteochondral defects of the medial talar dome. The aim of this study was to test the following hypotheses: (1) a matching offset size is available for each talus, (2) the prosthetic device can be reproducibly implanted slightly recessed in relation to the talar cartilage level, and (3) with this implantation level, excessive contact pressures on the opposite tibial cartilage are avoided. METHODS: The prosthetic device was implanted in 11 intact fresh-frozen human cadaver ankles, aiming its surface 0.5 mm below cartilage level. The implantation level was measured at 4 margins of each implant. Intraarticular contact pressures were measured before and after implantation, with compressive forces of 1,000-2,000 N and the ankle joint in plantigrade position, 10 dorsiflexion, and 14 plantar flexion. RESULTS: There was a matching offset size available for each specimen. The mean implantation level was 0.45 (SD 0.18) mm below the cartilage surface. The defect area accounted for a median of 3% (0.02-18) of the total ankle contact pressure before implantation. This was reduced to 0.1% (0.02-13) after prosthetic implantation. INTERPRETATION: These results suggest that the implant can be applied clinically in a safe way, with appropriate offset sizes for various talar domes and without excessive pressure on the opposite cartilag

    TAIGA -- an advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy

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    The physical motivations, present status, main results in study of cosmic rays and in the field of gamma-ray astronomy as well future plans of the TAIGA-1 (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA observatory addresses ground-based gamma-ray astronomy and astroparticle physics at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west from the southern tip of the lake Baikal.Comment: Submission to SciPost Phys. Proc., 10 pages, 2 figure

    Primary Cosmic Rays Energy Spectrum and Mean Mass Composition by the Data of the TAIGA Astrophysical Complex

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    The corrected dependence of the mean depth of the EAS maximum XmaxX_{max} on the energy was obtained from the data of the Tunka-133 array for 7 years and the TAIGA-HiSCORE array for 2 year. The parameter ⟨ln⁑A⟩\langle\ln A\rangle, characterizing the mean mass compositon was derived from these results. The differential energy spectrum of primary cosmic rays in the energy range of 2β‹…10142\cdot 10^{14} - 2β‹…10162\cdot 10^{16}\,eV was reconstructed using the new parameter Q100Q_{100} the Cherenkov light flux at the core distance 100 m.}Comment: 6 pages, 3 figures, Submitted to SciPost Phys.Pro
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