161 research outputs found
Tunka Advanced Instrument for cosmic rays and Gamma Astronomy
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
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°ΠΊΡΠΎΡΡ ΡΠΈΡΠΊΠ°, ΠΊΡΠΈΡΠ΅ΡΠΈΠΈ ΠΈ Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΡ ΠΎΡΡΡΠΎΠ³ΠΎ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΠΏΠΎΡΠ΅ΠΊ Π² ΠΏΠ΅ΡΠΈΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠΌ ΠΏΠ΅ΡΠΈΠΎΠ΄Π΅
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 studΡ 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‘ ΡΠ²Π΅Π»ΠΈΡΠ΅Π½ΠΈΠ΅ΠΌ ΠΏΡΠΎΠ΄ΠΎΠ»ΠΆΠΈΡΠ΅Π»ΡΠ½ΠΎΡΡΠΈ ΠΆΠΈΠ·Π½ΠΈ ΠΈ ΡΠ²ΡΠ·Π°Π½Π½ΠΎΠΉ Ρ Π²ΠΎΠ·ΡΠ°ΡΡΠΎΠΌ ΠΌΡΠ»ΡΡΠΈΠΊΠΎΠΌΠΎΡΠ±ΠΈΠ΄Π½ΠΎΡΡΡΡ Π²ΡΠ΅ Π±ΠΎΠ»ΡΡΡΡ Π°ΠΊΡΡΠ°Π»ΡΠ½ΠΎΡΡΡ ΠΏΡΠΈΠΎΠ±ΡΠ΅ΡΠ°Π΅Ρ ΠΏΡΠ΅Π΄ΠΎΡΠ²ΡΠ°ΡΠ΅Π½ΠΈΠ΅ ΠΎΡΠ»ΠΎΠΆΠ½Π΅Π½ΠΈΠΉ Ρ
ΠΈΡΡΡΠ³ΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ Π»Π΅ΡΠ΅Π½ΠΈΡ, Π² ΡΠΎΠΌ ΡΠΈΡΠ»Π΅ ΠΏΠ΅ΡΠΈΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ ΠΎΡΡΡΠΎΠ³ΠΎ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΠΏΠΎΡΠ΅ΠΊ.Β Π¦Π΅Π»Ρ β Π°Π½Π°Π»ΠΈΡΠΈΡΠ΅ΡΠΊΠΈΠΉ ΠΎΠ±Π·ΠΎΡ ΡΠ΅ΠΊΠΎΠΌΠ΅Π½Π΄Π°ΡΠΈΠΉ ΡΠΊΡΠΏΠ΅ΡΡΠ½ΡΡ
Π³ΡΡΠΏΠΏ ΠΈ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΠΎΠ² ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠΉ ΠΏΠΎ ΡΠ°ΠΊΡΠΎΡΠ°ΠΌ ΡΠΈΡΠΊΠ°, ΠΊΡΠΈΡΠ΅ΡΠΈΡΠΌ ΠΈ Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΠ°ΠΌ ΠΏΠΎΡΠ»Π΅ΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΠΏΠΎΡΠ΅ΠΊ. ΠΠ°ΡΠ΅ΡΠΈΠ°Π»Ρ ΠΈ ΠΌΠ΅ΡΠΎΠ΄Ρ. ΠΡΠ±Π»ΠΈΠΊΠ°ΡΠΈΠΈ Π·Π° ΠΏΠΎΡΠ»Π΅Π΄Π½ΠΈΠ΅ 15 Π»Π΅Ρ, ΠΏΠΎΠ»ΡΡΠ΅Π½Π½ΡΠ΅ ΠΏΠΎΠΈΡΠΊΠΎΠΌ Π½Π° Π΄Π°ΡΡ 15 ΠΌΠ°Ρ 2023Β Π³. Π² Π±Π°Π·Π°Ρ
eLibrary, PubMed ΠΏΠΎ ΠΊΠ»ΡΡΠ΅Π²ΡΠΌ ΡΠ»ΠΎΠ²Π°ΠΌ Β«ΠΎΡΡΡΠΎΠ΅ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΠ΅ ΠΏΠΎΡΠ΅ΠΊΒ», Β«Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΒ», Β«ΠΏΠ΅ΡΠΈΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΡΠΉ ΠΏΠ΅ΡΠΈΠΎΠ΄Β». ΠΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅ ΠΏΡΠ±Π»ΠΈΠΊΠ°ΡΠΈΠΉ Π² ΠΎΠ±Π·ΠΎΡ ΠΈ ΠΈΡ
ΠΎΡΠ΅Π½ΠΊΠ° ΠΎΡΠ½ΠΎΠ²Π°Π½Ρ Π½Π° ΡΠΎΠ³Π»Π°ΡΠΎΠ²Π°Π½Π½ΠΎΠΌ ΠΌΠ½Π΅Π½ΠΈΠΈ Π°Π²ΡΠΎΡΠΎΠ².Β Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ. Π ΠΏΠ΅ΡΠΈΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠΌ ΠΏΠ΅ΡΠΈΠΎΠ΄Π΅ ΠΌΠΎΠΆΠ΅Ρ ΠΈΠΌΠ΅ΡΡ ΠΌΠ΅ΡΡΠΎ ΠΎΡΡΡΠΎΠ΅ ΠΏΠΎΡΠ΅ΡΠ½ΠΎΠ΅ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΠ΅, Π΄ΠΎ ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½Π½ΠΎΠ³ΠΎ Π²ΡΠ΅ΠΌΠ΅Π½ΠΈ Π½Π΅ ΠΏΡΠΎΡΠ²Π»ΡΡΡΠ΅Π΅ΡΡ ΡΠ½ΠΈΠΆΠ΅Π½ΠΈΠ΅ΠΌ Π΄ΠΈΡΡΠ΅Π·Π° ΠΈ/ΠΈΠ»ΠΈ Π½Π°ΡΠ°ΡΡΠ°Π½ΠΈΠ΅ΠΌ ΡΡΠΎΠ²Π½Ρ ΠΊΡΠ΅Π°ΡΠΈΠ½ΠΈΠ½Π° Π² ΡΡΠ²ΠΎΡΠΎΡΠΊΠ΅ ΠΊΡΠΎΠ²ΠΈ. ΠΡΠΎ Π²Π°ΡΡΠΈΡΡΡΡΠ΅Π΅ ΠΏΠΎ ΠΏΡΠΈΡΠΈΠ½Π°ΠΌ ΠΈ ΠΌΠ΅Ρ
Π°Π½ΠΈΠ·ΠΌΠ°ΠΌ ΡΠ°Π·Π²ΠΈΡΠΈΡ ΡΠΎΡΡΠΎΡΠ½ΠΈΠ΅ ΠΏΠΎΡΠ΅Π½ΡΠΈΠ°Π»ΡΠ½ΠΎ ΠΎΠ±ΡΠ°ΡΠΈΠΌΠΎ ΠΏΡΠΈ ΡΠ²ΠΎΠ΅Π²ΡΠ΅ΠΌΠ΅Π½Π½ΠΎΠΌ Π²ΡΡΠ²Π»Π΅Π½ΠΈΠΈ ΠΈ Π»Π΅ΡΠ΅Π½ΠΈΠΈ. ΠΠ·ΡΡΠ΅Π½ΠΈΠ΅ Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΠΎΠ², ΠΏΡΠ΅Π²ΠΎΡΡ
ΠΎΠ΄ΡΡΠΈΡ
ΡΡΠΎΠ²Π΅Π½Ρ ΠΊΡΠ΅Π°ΡΠΈΠ½ΠΈΠ½Π° ΠΈ Π΄ΠΈΡΡΠ΅Π· Π² ΡΡΠΎΠΊΠ°Ρ
ΠΈ ΡΠΎΡΠ½ΠΎΡΡΠΈ Π²ΡΡΠ²Π»Π΅Π½ΠΈΡ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ/Π΄ΠΈΡΡΡΠ½ΠΊΡΠΈΠΈ ΠΏΠΎΡΠ΅ΠΊ, Π° ΡΠ°ΠΊΠΆΠ΅ ΠΈΠ½ΡΡΡΡΠΌΠ΅Π½ΡΠΎΠ² ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡΠ½ΠΎΠΉ ΠΎΡΠ΅Π½ΠΊΠΈ ΠΈ ΡΡΡΠ°ΡΠΈΡΠΈΠΊΠ°ΡΠΈΠΈ ΡΠΈΡΠΊΠ° ΠΏΠΎΡΠ»Π΅ΠΎΠΏΠ΅ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΠΏΠΎΡΠ΅ΠΊ ΠΏΠΎΠΊΠ° Π½Π΅ Π·Π°Π²Π΅ΡΡΠΈΠ»ΠΈΡΡ Π΄ΠΎΠΊΠ°Π·Π°ΡΠ΅Π»ΡΠ½ΡΠΌΠΈ Π·Π°ΠΊΠ»ΡΡΠ΅Π½ΠΈΡΠΌΠΈ. ΠΠ°ΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅. ΠΠΎΠ΄Π΄Π΅ΡΠΆΠΈΠ²Π°Π΅ΠΌΠ°Ρ ΠΠ½ΠΈΡΠΈΠ°ΡΠΈΠ²ΠΎΠΉ ΠΏΠΎ ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠ΅Π½ΠΈΡ ΠΊΠ°ΡΠ΅ΡΡΠ²Π° ΠΏΡΠΈ ΠΎΡΡΡΡΡ
Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π½ΠΈΡΡ
(2020) ΡΡΡΠ°ΡΠ΅Π³ΠΈΡ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΡ Π»Π°Π±ΠΎΡΠ°ΡΠΎΡΠ½ΡΡ
Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΠΎΠ² Π² ΡΠΎΡΠ΅ΡΠ°Π½ΠΈΠΈ Ρ ΠΊΠ»ΠΈΠ½ΠΈΡΠ΅ΡΠΊΠΈΠΌ ΠΊΠΎΠ½ΡΠ΅ΠΊΡΡΠΎΠΌ ΠΈ ΡΠ°ΠΊΡΠΎΡΠ°ΠΌΠΈ ΡΠΈΡΠΊΠ° Π΄Π»Ρ ΠΏΡΠΎΡΠΈΠ»Π°ΠΊΡΠΈΠΊΠΈ, Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ ΠΈ Π»Π΅ΡΠ΅Π½ΠΈΡ ΡΡΠ±ΠΊΠ»ΠΈΠ½ΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΠΎΡΡΡΠΎΠ³ΠΎ ΠΏΠΎΡΠ΅ΡΠ½ΠΎΠ³ΠΎ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΡΠ°Π·Π»ΠΈΡΠ½ΠΎΠ³ΠΎ Π³Π΅Π½Π΅Π·Π° ΠΌΠΎΠΆΠ΅Ρ Π±ΡΡΡ ΡΠ΅Π°Π»ΠΈΠ·ΠΎΠ²Π°Π½Π° Π½Π° ΠΎΡΠ½ΠΎΠ²Π΅ Π΄ΠΎΠΏΠΎΠ»Π½ΠΈΡΠ΅Π»ΡΠ½ΡΡ
Π΄ΠΎΠΊΠ°Π·Π°ΡΠ΅Π»ΡΡΡΠ² Π±ΡΠ΄ΡΡΠΈΡ
ΠΊΠ»ΠΈΠ½ΠΈΡΠ΅ΡΠΊΠΈΡ
ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠΉ
First metatarsophalangeal hemiarthroplasty for hallux rigidus
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
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
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
The corrected dependence of the mean depth of the EAS maximum 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 ,
characterizing the mean mass compositon was derived from these results. The
differential energy spectrum of primary cosmic rays in the energy range of
- \,eV was reconstructed using the new
parameter the Cherenkov light flux at the core distance 100 m.}Comment: 6 pages, 3 figures, Submitted to SciPost Phys.Pro
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