[Emergency laparoscopy in the treatment of perforated gastroduodenal ulcers]. / Ekstrennaya laparoskopiya pri lechenii perforativnykh gastroduodenal'nykh yazv.

OBJECTIVE: To compare the results of endoscopic and open treatment of perforated gastroduodenal ulcers. MATERIAL AND METHODS: There were 445 patients with perforated gastroduodenal ulcers between 2013 and 2021. Endoscopic suturing of perforation was performed in 172 patients (38.7%), 273 ones underwent open surgery. RESULTS: Among 172 patients scheduled for endoscopy, 160 (93.6%) ones underwent laparoscopic suturing of perforation. Morbidity rate was 5.0% (n=8), postoperative mortality rate - 1.3% (n=2). Comparison of the outcomes after laparoscopic suturing of ulcers in 160 patients and open surgery in 134 patients showed that laparoscopy was followed by 2.5 times lower incidence of complications and 3 times lower postoperative mortality. CONCLUSION: Diagnostic laparoscopy is advisable in patients with perforated ulcers and no contraindications. In most cases, surgery can be successfully and effectively completed without conversion to laparotomy. Endoscopic closure of ulcerative defect is preferable since this procedure has certain advantages over traditional intervention, contributes to significant reduction in morbidity, mortality and hospital-stay.

Screening of familial hypercholesterolemia among patients in age under 40 years old exposed by duplex scanning of carotid arteries, by the local registry data.

AIM: To identify patients with probable FH among Duplex-2013 registry patients under the age of 40 years, to analyze their lipid spectrum and duplex carotid artery data, to evaluate the changes of their lipid spectrum parameters. MATERIALS AND METHODS: The Duplex-2013 registry database was used for this study (n=2550). Patients under the age of 40 years were selected for follow-up analysis (n=192). RESULTS: 20 of them were selected on the basis of Simon Broome criteria as patients with possible FH. The FH group (n=20) and the control group (n=172) had significant differences in age (35.1 ± 4.01 vs. 32.62 ± 5.29, p=0.044), male gender (18 of 20 (90%) vs 92 of 172 (53%), p=0.003), TC (7.64 ± 0.63 vs 5.34 ± 0.91, p=0.0001) and LDL-C cholesterol (5.45 ± 0.62 vs 3.28 ± 0.78, p=0.00001). When comparing the groups by the combined criterion of atherosclerosis (IMT > 1.0 mm and / or atherosclerotic plaque in the carotid artery >20%), it was noted that signs of carotid atherosclerosis were more often recorded in the FH group compared with the control group (40% vs 26%). Repeated laboratory studies of TC and LDL-C in the FH group after 2.5 years showed their significant dynamics (7.64 ± 0.63 vs 6.03 ± 1.04, p=0.007, 5.45 ± 0.63 vs 3.84 ± 1.24, p=0.035). CONCLUSION: The frequency of detection of FH in the cohort study was 1:10 (11% of all patients). Thus, patients referred for duplex scanning of carotid arteries can be a potential target for screening for FH.

Chiral Surface Twists and Skyrmion Stability in Nanolayers of Cubic Helimagnets.

Theoretical analysis and Lorentz transmission electron microscopy (LTEM) investigations in an FeGe wedge demonstrate that chiral twists arising near the surfaces of noncentrosymmetric ferromagnets [Meynell et al., Phys. Rev. B 90, 014406 (2014)] provide a stabilization mechanism for magnetic Skyrmion lattices and helicoids in cubic helimagnet nanolayers. The magnetic phase diagram obtained for freestanding cubic helimagnet nanolayers shows that magnetization processes differ fundamentally from those in bulk cubic helimagnets and are characterized by the first-order transitions between modulated phases. LTEM investigations exhibit a series of hysteretic transformation processes among the modulated phases, which results in the formation of the multidomain patterns.

Time Dependence of the Electron and Positron Components of the Cosmic Radiation Measured by the PAMELA Experiment between July 2006 and December 2015.

Cosmic-ray electrons and positrons are a unique probe of the propagation of cosmic rays as well as of the nature and distribution of particle sources in our Galaxy. Recent measurements of these particles are challenging our basic understanding of the mechanisms of production, acceleration, and propagation of cosmic rays. Particularly striking are the differences between the low energy results collected by the space-borne PAMELA and AMS-02 experiments and older measurements pointing to sign-charge dependence of the solar modulation of cosmic-ray spectra. The PAMELA experiment has been measuring the time variation of the positron and electron intensity at Earth from July 2006 to December 2015 covering the period for the minimum of solar cycle 23 (2006-2009) until the middle of the maximum of solar cycle 24, through the polarity reversal of the heliospheric magnetic field which took place between 2013 and 2014. The positron to electron ratio measured in this time period clearly shows a sign-charge dependence of the solar modulation introduced by particle drifts. These results provide the first clear and continuous observation of how drift effects on solar modulation have unfolded with time from solar minimum to solar maximum and their dependence on the particle rigidity and the cyclic polarity of the solar magnetic field.

[[Morpho-functional peculiarities of course of purulent-septic wound process while impact of a low-dosed vacuum].]

Morpho-functional peculiarities of course of the purulent-septic wound process, while vacuum-therapy method application for local treatment of the wounds, were studied. High reparative effect of vacuum-therapy, caused by activation of the wound proliferative processes, was noted, It had permitted to improve the patients treatment results for purulent surgical diseases of soft tissues, to lower the rate of complications and reoperations and to improve their quality of life.

[CHANGES IN THE AREA OF THE WOUND SURFACE ON EXPOSURE LOW­DOSE VACUUM].

Results of treatment of were analysed 30 patients over a long non­healing wounds and trophic ulcers, in which as a topical treatment, the method of vacuum therapy was applied. To study the activity of reparative regeneration in the wound using a dynamic method of determining the area of wounds using lqSquare computer program and immunohistochemical method for determining the Ki 67 positive cells in tissues of near wound area. It was found that low­dose exposure to vacuum at the wound contributed to increase the proliferative activity of tissues of near wound area and reduce the area of wound defect. Assessment of changes in the area of the wound surface is an important predictor of treatment efficacy, prevention of complications.

New upper limit on strange quark matter abundance in cosmic rays with the PAMELA space experiment.

In this work we present results of a direct search for strange quark matter (SQM) in cosmic rays with the PAMELA space spectrometer. If this state of matter exists it may be present in cosmic rays as particles, called strangelets, having a high density and an anomalously high mass-to-charge (A/Z) ratio. A direct search in space is complementary to those from ground-based spectrometers. Furthermore, it has the advantage of being potentially capable of directly identifying these particles, without any assumption on their interaction model with Earth's atmosphere and the long-term stability in terrestrial and lunar rocks. In the rigidity range from 1.0 to ∼1.0×10^{3} GV, no such particles were found in the data collected by PAMELA between 2006 and 2009. An upper limit on the strangelet flux in cosmic rays was therefore set for particles with charge 1≤Z≤8 and mass 4≤A≤1.2×10^{5}. This limit as a function of mass and as a function of magnetic rigidity allows us to constrain models of SQM production and propagation in the Galaxy.

An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV.

Antiparticles account for a small fraction of cosmic rays and are known to be produced in interactions between cosmic-ray nuclei and atoms in the interstellar medium, which is referred to as a 'secondary source'. Positrons might also originate in objects such as pulsars and microquasars or through dark matter annihilation, which would be 'primary sources'. Previous statistically limited measurements of the ratio of positron and electron fluxes have been interpreted as evidence for a primary source for the positrons, as has an increase in the total electron+positron flux at energies between 300 and 600 GeV (ref. 8). Here we report a measurement of the positron fraction in the energy range 1.5-100 GeV. We find that the positron fraction increases sharply over much of that range, in a way that appears to be completely inconsistent with secondary sources. We therefore conclude that a primary source, be it an astrophysical object or dark matter annihilation, is necessary.

Cosmic-ray positron energy spectrum measured by PAMELA.

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray positron flux and fraction that extends previously published measurements up to 300 GeV in kinetic energy. The combined measurements of the cosmic-ray positron energy spectrum and fraction provide a unique tool to constrain interpretation models. During the recent solar minimum activity period from July 2006 to December 2009, approximately 24,500 positrons were observed. The results cannot be easily reconciled with purely secondary production, and additional sources of either astrophysical or exotic origin may be required.

Topological structures in chiral media: Effects of confined geometry.

We theoretically study orientational structures in chiral magnetics and cholesteric liquid crystal (CLC) nanosystems confined in the slab geometry. Our analysis is based on the model that, in addition to the exchange and the Dzyaloshinskii-Moriya interactions, takes into account the bulk and surface anisotropies. In CLC films, these anisotropies describe the energy of interaction with external magnetic/electric field and the anchoring energy assuming that magnetic/electric anisotropy is negative and the boundary conditions are homeotropic. We have computed the phase diagram and found that the ground state of the film is represented by various delocalized structures depending on the bulk and surface anisotropy parameters, κ^{b} and κ^{s}. These include the z helix and the z cone states, the oblique, and the x helicoids. The minimum energy paths connecting the ground state and metastable helicoids and the energy barriers separating these states are evaluated. We have shown that there is a variety of localized topological structures such as the skyrmion tube, the toron, and the bobber that can be embedded in different ground states including the z cone (conical phase) and tilted fingerprint states. We have also found the structure called the leech that can be viewed as an intermediate state between the toron and the skyrmion tube.

Quantitative genetic study of amphiregulin and fractalkine circulating levels--potential markers of arthropathies.

OBJECTIVE: Amphiregulin (AREG) and Fractalkine (FRACT), are involved in a variety of normal and pathological processes, and are both suggested to be relevant to joint degeneration. The aims of the present study included (1) testing association between circulating levels of these biomarkers and joint pathologies, (2) evaluation of the putative genetic and familial factors' effect on AREG and FRACT variability. DESIGN: The study was conducted in the family-based sample of 923 Caucasian individuals. Variance component analysis was used to assess contribution of genetic and environmental factors to variability of AREG and FRACT concentration. RESULTS: The mean levels of FRACT were significantly higher in the affected group with arthropathies (synovial joints osteoarthritis (OA) and disc degenerative disease, DDD) then in the control group (P<0.0004). Circulating AREG levels were higher in DDD (P=0.0272). Genetic factors constituted the main source of the interindividual differences of the AREG and FRACT levels in our sample, and explained 29.68% and 41.68% of the total variation, respectively. The phenotypic correlation between AREG and FRACT was substantial (r=0.55, P=0.0001) and was associated with both common genetic and environmental factors. Specifically, 30% of the phenotypic correlation between AREG and FRACT was due to common genetic effects. CONCLUSIONS: Further studies are required to assess relevancy of FRACT to clinical diagnosis and prognosis of arthropathies, to investigate the mechanisms behind the observed phenotypic and genetic covariation among the studied biomarkers, and to explore specific genetic polymorphisms affecting AREG and FRACT variation.

Quantitative genetic study of the circulating osteopontin in community-selected families.

UNLABELLED: The study assessed contribution of genetic factors to variability of osteopontin (OPN) levels. Evidence of association of OPN levels with polymorphisms in its structural gene and integrin-binding sialoprotein gene loci was obtained. The results motivate research of OPN-related proteins and genes with respect to biomineralization and other biological processes. INTRODUCTION: OPN is a major phosphoprotein in bone, which plays key role in regulation of bone mineralization process. It is considered as a promising biomarker for osteoarthritis and osteoporosis, and various other pathological conditions. However, the contribution of genetics and other confounding factors to OPN circulating levels variation in general population has never been specifically determined. The main aims of the present study included (1) evaluation of the putative genetic and familial factors' effect on OPN variability and (2) testing the hypothesis that OPN plasma levels are associated with the genetic polymorphisms in its structural gene locus (SPP1) and in integrin-binding sialoprotein gene locus (IBSP). METHODS: To address these questions, we used a family-based sample of 925 apparently healthy Caucasian individuals. Association of OPN levels with three SNPs in each of the two selected gene loci was explored using pedigree disequilibrium tests. RESULTS: Some 58% and 13% of the OPN levels variability were attributable to genetic factors and common spouse environment, respectively. Three SNPs showed nominally significant association with OPN (p < 0.05). Of these, rs2616262 linked to IBSP promoter region remained significant after correction for multiple testing (p = 0.003). Significant association of this SNP and rs10516799 (distal segment of SPP1) with OPN was confirmed in several statistical tests. Using a special modification of variance component analysis, we examined gene-gene and gene-sex interaction effects, but found non-significant confirmation for these hypotheses. CONCLUSIONS: Further studies are required to confirm the observed results and to explore the underlying molecular and physiological mechanisms.

Precursor phenomena at the magnetic ordering of the cubic helimagnet FeGe.

We report on detailed magnetic measurements on the cubic helimagnet FeGe in external magnetic fields and temperatures near the onset of long-range magnetic order at T(C)=278.2(3) K. Precursor phenomena display a complex succession of temperature-driven crossovers and phase transitions in the vicinity of T(C). The A-phase region, present below T(C) and fields H<0.5 kOe, is split in several pockets. The complexity of the magnetic phase diagram is theoretically explained by the confinement of solitonic kinklike or Skyrmionic units that develop an attractive and oscillatory intersoliton coupling owing to the longitudinal inhomogeneity of the magnetization.

Cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV.

Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy. Here we present new results regarding negatively charged electrons between 1 and 625 GeV performed by the satellite-borne experiment PAMELA. This is the first time that cosmic-ray e⁻ have been identified above 50 GeV. The electron spectrum can be described with a single power-law energy dependence with spectral index -3.18 ± 0.05 above the energy region influenced by the solar wind (> 30 GeV). No significant spectral features are observed and the data can be interpreted in terms of conventional diffusive propagation models. However, the data are also consistent with models including new cosmic-ray sources that could explain the rise in the positron fraction.

[Molecular monitoring of the rotavirus (Reoviridae: Sedoreovirinae: Rotavirus: Rotavirus A) strains circulating in Nizhny Novgorod (2012-2020): detection of the strains with the new genetic features].

INTRODUCTION: The pentavalent rotavirus vaccine has been registered in Russia, however, the vaccination coverage remains low, and an annual increase in the incidence of rotavirus infection is unavoidable. In this regard, molecular monitoring of rotaviruses in order to search for new variants possessing epidemic potential is an urgent task. MATERIAL AND METHODS: PCR genotyping and VP4 and VP7 genes sequencing were used to characterize rotaviruses circulating in Nizhny Novgorod in 2012-2020. The phylogenetic analysis of the strains was carried out using the BEAST software package. RESULTS: The spectrum included 17 genotypes with predominance of G9P[8] (37,4%). Detected in this study genotypes G1P[4], G1P[9], G2P[8], G4P[4], G4P[6], G8P[8], and G9P[4] were not previously identified in Nizhny Novgorod. The circulation of DS-1-like strains possessing genotypes G1P[8], G3P[8], G8P[8], or G9P[8] and a short RNA pattern had been shown. Rotaviruses of the common genotypes were genetically heterogeneous and belonged to different phylogenetic lineages and/or sublineages (P[4]-IV-a; P[4]-IV-b; P[8]-3.1; P[8]-3.3; P[8]-3.4 and P[8]-3.6; G1-I; G1-II; G2-IVa-1; G2-IVa-3; G3-1; G3-3; G4-I-c; G9-III; G9-VI). DISCUSSION: These results extend the available data on the genotypic structure of rotavirus populations in Russia and show the genetic diversity of viral strains. G3P[8] DS-1-like viruses were representatives of the G3-1 lineage, new for the territory of Russia, and had the largest number of amino acid substitutions in the VP7 antigenic epitopes. CONCLUSION: The emergence and spread of strains with new genetic features may allow rotavirus to overcome the immunological pressure formed by natural and vaccine-induced immunity, and maintain or increase the incidence of rotavirus infection.

PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy.

The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio which extends previously published measurements down to 60 MeV and up to 180 GeV in kinetic energy. During 850 days of data acquisition approximately 1500 antiprotons were observed. The measurements are consistent with purely secondary production of antiprotons in the Galaxy. More precise secondary production models are required for a complete interpretation of the results.

Insitu magnesium calcium phosphate cements formation: From one pot powders precursors synthesis to in vitro investigations.

Calcium phosphate cements are of great interest for researchers and their applications in medical practice expanded. Nevertheless, they have a number of drawbacks including the insufficient level of mechanical properties and low degradation rate. Struvite (MgNH4PO4) -based cements, which grew in popularity in recent years, despite their neutral pH and acceptable mechanical performance, release undesirable NH4 + ions during their resorption. This issue could be avoided by replacement of ammonia ions in the cement liquid with sodium, however, such cements have a pH values of 9-10, leading to cytotoxicity. Thus, the main goal of this investigation is to optimize the composition of cements to achieve the combination of desirable properties: neutral pH, sufficient mechanical properties, and the absence of cytotoxicity, applying Na2HPO4-based cement liquid. For this purpose, cement powders precursors in the CaO-MgO-P2O5 system were synthesized by one-pot process in a wide composition range, and their properties were investigated. The optimal performance was observed for the cements with (Ca + Mg)/P ratio of 1.67, which are characterized by newberyite phase formation during setting reaction, pH values close to 7, sufficient compressive strength up to 22 ± 3 MPa (for 20 mol.% of Mg), dense microstructure and adequate matrix properties of the surface. This set of features make those materials promising candidates for medical applications.

[Interaction of 23S ribosomal RNA helices 89 and 91 of Escherichia coli contributes to the activity of IF2 but is insignificant for elongation factors functioning].

The non-canonical base-pair C2475/G2529 joins helices 89 and 91 of the 23S rRNA in the large subunit of E. coli ribosomes. These nucleotides are located at the "crossroads" between the peptidyl transferase center, the sarcin-ricin loop and the GTPase-associated center. We probed the functional role of nucleotides C2475/G2529 by the mutations C2475G, C2475G/G2529C and deltaA2471/U2479 of 23S rRNA. All these mutations had no influence on the elongation factors activity but had different effects on the cell growth, 23S rRNA conformation and translation initiation. C2475G/G2529C and C2475G mutations led to more or less substantial decrease in IF2.GDPNP binding to the ribosomes, and IF2-assisted initiation complex formation. Ribosome-dependent GTPase activity of IF2 was enhanced by both C2475G/G2529C and C2475G mutations. Mutation deltaA2471/U2479 has no influence on IF2.GDPNP binding to the ribosome, but reduces IF2-dependent formation of initiation complex and the ribosome-dependent GTPase activity. Thus, the contact between helices 89 and 91 is important for efficient IF2 functioning in translation initiation.

Edge states and skyrmion dynamics in nanostripes of frustrated magnets.

Magnetic skyrmions are particle-like topological excitations recently discovered in chiral magnets. Their small size, topological protection and the ease with which they can be manipulated by electric currents generated much interest in using skyrmions for information storage and processing. Recently, it was suggested that skyrmions with additional degrees of freedom can exist in magnetically frustrated materials. Here, we show that dynamics of skyrmions and antiskyrmions in nanostripes of frustrated magnets is strongly affected by complex spin states formed at the stripe edges. These states create multiple edge channels which guide the skyrmion motion. Non-trivial topology of edge states gives rise to complex current-induced dynamics, such as emission of skyrmion-antiskyrmion pairs. The edge-state topology can be controlled with an electric current through the exchange of skyrmions and antiskyrmions between the edges of a magnetic nanostructure.

Equilibrium Skyrmion Lattice Ground State in a Polar Easy-plane Magnet.

The skyrmion lattice state (SkL), a crystal built of mesoscopic spin vortices, gains its stability via thermal fluctuations in all bulk skyrmion host materials known to date. Therefore, its existence is limited to a narrow temperature region below the paramagnetic state. This stability range can drastically increase in systems with restricted geometries, such as thin films, interfaces and nanowires. Thermal quenching can also promote the SkL as a metastable state over extended temperature ranges. Here, we demonstrate more generally that a proper choice of material parameters alone guarantees the thermodynamic stability of the SkL over the full temperature range below the paramagnetic state down to zero kelvin. We found that GaV4Se8, a polar magnet with easy-plane anisotropy, hosts a robust Néel-type SkL even in its ground state. Our supporting theory confirms that polar magnets with weak uniaxial anisotropy are ideal candidates to realize SkLs with wide stability ranges.