<?xml version="1.0" encoding="utf-8"?>
<journal>
  <titleid/>
  <issn>2304-9782, 2618-8686, 2405-7223</issn>
  <journalInfo lang="ENG">
    <title>St. Petersburg Polytechnic University Journal: Physics and Mathematics</title>
  </journalInfo>
  <issue>
    <volume>14</volume>
    <number>3</number>
    <altNumber> </altNumber>
    <dateUni>2021</dateUni>
    <pages>1-187</pages>
    <articles>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>8-20</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Herzen State Pedagogical University of Russia</orgName>
              <surname>Gorokhovatskiy</surname>
              <initials>Yuriy</initials>
              <email>yurig@fromru.com</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Herzen State Pedagogical University of Russia</orgName>
              <surname>Temnov </surname>
              <initials>Dmitry</initials>
              <email>tde@herzen.spb.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Herzen State Pedagogical University of Russia</orgName>
              <surname>Shabanova </surname>
              <initials>Natalya</initials>
              <email>natashshabanov@yandex.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Joint Institute for Nuclear Research</orgName>
              <surname>Rossouw </surname>
              <initials>Arnoux </initials>
              <email>arnoux.rossouw@gmail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Thermoactivated current spectroscopy of polyethylene terephthalate films irradiated by heavy xenon ions</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The paper analyzes the electret state of polyethylene terephthalate (PET) films irradiated on the IC-100 cyclotron (JINR LAR) using thermostimulated spectroscopy methods. Thermally stimulated discharge currents (thermally stimulated depolarization) of PET film samples obtained at different technological stages of track membrane manufacturing are studied. The results of the analysis of thermally stimulated depolarization currents indicate a significant change in the spectra of the energy states of the electric charge accumulated during the polarization of PET films, during irradiation with accelerated heavy Xe ions, ultraviolet treatment, and alkaline etching of latent tracks. The parameters of relaxation processes (activation energy and effective frequency factor) occurring in track membranes are calculated using the Eyring method. A significant change in the energy state spectra of the electric charge accumulated during the polarization of PET films as a result of ion-track processes in them indicates the possibility of creating an electret state in PET films and track membranes irradiated with heavy ions on their basis.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14301</doi>
          <udk>53.08</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>electret</keyword>
            <keyword>track membrane</keyword>
            <keyword>polyethylene terephthalate</keyword>
            <keyword>thermal-stimulated discharge current</keyword>
            <keyword>Eyring method</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.1/</furl>
          <file>01_8-20_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>21-35</pages>
        <authors>
          <author num="001">
            <authorCodes>
              <researcherid>E-5484-2014</researcherid>
              <scopusid>56020596900</scopusid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Smirnov</surname>
              <initials>Evgeny</initials>
              <email>aero@phmf.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="002">
            <authorCodes>
              <orcid>0000-0002-3972-9259</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Northern Water Problems Institute of Karelian Research Centre of RAS</orgName>
              <surname>Smirnov</surname>
              <initials>Sergei</initials>
              <email>sergeysmirnov92@mail.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Abramov</surname>
              <initials>Alexei</initials>
              <email>abramov@runnet.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Galaev </surname>
              <initials>Sergey</initials>
              <email>galaev@spbstu.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Turbulent mixed convection within rapidly rotating heated annular cavities with an axial throughflow</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The results of eddy-resolving numerical simulation of a turbulent mixed convection in a system of three identical, rapidly rotating annular cavities are presented. The cavities are heated from the side of the disk surfaces and from the periphery (the same distribution of the surface temperature is set for all the cavities), and heat removal proceeds by an axial air throughflow in the narrow channel, annular within the cavity system. The computations based on the Implicit LES method have been carried out in view of the conditions close to the experiments known from the literature for a single cavity; the rotational Reynolds number was 200,000, the grid dimension was 17 million cells. The complex multiscale flow structure and the influence of the input aerodynamic and thermal conditions, which are not identical for the cavities included in the system, on the local heat transfer from disk surfaces are discussed.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14302</doi>
          <udk>536.25, 532.517</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>mixed convection</keyword>
            <keyword>rapidly rotating annular cavity</keyword>
            <keyword>axial throughflow</keyword>
            <keyword>global circulation</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.2/</furl>
          <file>02_21-35_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>36-48</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Bulovich</surname>
              <initials>Sergei</initials>
              <email>bulovic@yandex.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Numerical simulation of thermoacoustic gas oscillations in a pipe with toroidal heat exchange elements</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The paper simulates the modes of a gas flow in a pipe closed at one end and open to the atmosphere at the other end; for this purpose, a numerical solution of the system of Navier – Stokes equations in a two-dimensional axisymmetric formulation has been used. The excitation of oscillations of gas-dynamic functions is caused by the temperature gradient in the pipe section resulting from the contact of the gas with differently heated toroidal elements inside the pipe, their temperature being maintained constant. When the specified gradient reaches the threshold value, a stable thermoacoustic oscillation of the gas column is observed in the pipe. The time dependences of the pressure and the axial component of the gas velocity, as well as the heat flows in the heat exchange unit of the resonator, were calculated. The obtained results were in good agreement with the experimental data.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14303</doi>
          <udk>621.486</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>thermoacoustics</keyword>
            <keyword>Sondhauss effect</keyword>
            <keyword>mathematical simulation</keyword>
            <keyword>numerical solution of Navier – Stokes equations</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.3/</furl>
          <file>03_36-48_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>49-62</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Borisenko </surname>
              <initials>Vladislav</initials>
              <email>vladborisenko1995@gmail.com</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Semenov</surname>
              <initials>Artem</initials>
              <email>semenov.artem@googlemail.com</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Dresden University of Technology</orgName>
              <surname>Wallmersperger </surname>
              <initials>Thomas</initials>
              <email>servicecenter.studium@tu-dresden.de</email>
              <address>Germany</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An influence analysis of creep and plasticity characteristics on the spark plasma sintering process</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In the paper, the spark plasma sintering (SPS) process for metal particles has been simulated based on experimental data and using the finite element method in the thermo-electro-mechanical formulation with taking into account the temperature influence on parameters of materials (nickel and copper). A comparison of obtained results with experimental data made it possible to create a computational model of the SPS process, the model being convenient to evaluate the influence of creep and plasticity parameters on the size of the interparticle neck forming in SPS. It was found that the creep effect significantly dominated over the plasticity influence on the process of forming the sintering neck at high temperatures. In this case, the variation of creep parameters in simulation also actively affects the formation of the neck.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14304</doi>
          <udk>004.94</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>spark plasma sintering</keyword>
            <keyword>metal</keyword>
            <keyword>finite-element modelling</keyword>
            <keyword>plasticity</keyword>
            <keyword>creep</keyword>
            <keyword>coupled fields</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.4/</furl>
          <file>04_49-62_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>63-78</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Dudoladov </surname>
              <initials>Savelii</initials>
              <email>sava2312@yandex.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Larionov</surname>
              <initials>Nikolay</initials>
              <email>larionov.nickolay@gmail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The condition for application of the Crocco integral in the mathematical description of a laser welding plasma plume</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">Based on the theoretical approach developed in the article by G.A. Turichin et al. (High Temperature. 2006. Vol. 44. No. 5. Pp. 647–655), the characteristics of the plasma plume forming in the keyhole laser welding have been investigated. A condition corresponding to the existence of the Crocco integral was defined, making it possible to simplify the system of gas dynamics equations and obtain analytical solutions for a plasma plume in the form of a classical submerged jet. These solutions were analyzed for a wide range of metal vapor velocities and temperatures at the keyhole top. For some of the selected values, an agreement with the numerical calculations of other authors was found.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14305</doi>
          <udk>533.1; 621.791</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>gas dynamics equations</keyword>
            <keyword>plasma plume</keyword>
            <keyword>laser welding</keyword>
            <keyword>shear layer</keyword>
            <keyword>submerged jet</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.5/</furl>
          <file>05_63-78_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>79-93</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Voronezh State University</orgName>
              <surname>Kutsova </surname>
              <initials>Daria </initials>
              <email>potanina.ds@gmail.com</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Voronezh State University</orgName>
              <surname>Bogatikov </surname>
              <initials>Evgenii</initials>
              <email>evbogatikov@yandex.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Voronezh State University</orgName>
              <surname>Shebanov </surname>
              <initials>Alexandr</initials>
              <email>anshebanov@hotmail.com</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Voronezh State University</orgName>
              <surname>Bormontov </surname>
              <initials>Evgenii </initials>
              <email>me144@phys.vsu.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">A comparison of potential functions for molecular dynamic simulation of methane sorption in the silicalite</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In order to make the best choice, two types of a force field have been studied to access a possibility of application of one of them to simulation of adsorption and transport processes in the silicalite (synthetic zeolite)-methane system. To accomplish this, the molecular dynamic technique implemented in the LAMMPS package was used. Priority criteria of the choice were retention of the structure completeness during long simulation runs, the system’s stability, the possibility of simulation of a separate good-sized zeolite cluster without using periodic boundary conditions for multiplying zeolite’s lattice in space. For the force-field, which met these requirements, some structural, thermodynamic and transport characteristics of the system were calculated. Radial and angular distribution functions for different atom pairs and triplets were obtained for both the pure zeolite and the silicalite-methane system. A good agreement of all obtained characteristics with literature data of numerical and natural experiments was achieved.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14306</doi>
          <udk>538.913</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>silicalite</keyword>
            <keyword>ZSM-5 zeolite</keyword>
            <keyword>methane</keyword>
            <keyword>molecular dynamic</keyword>
            <keyword>sorption</keyword>
            <keyword>potential function</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.6/</furl>
          <file>06_79-93_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>94-111</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Stepasheva </surname>
              <initials>Ekaterina</initials>
              <email>momoirin@yandex.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University </orgName>
              <surname>Zasimova</surname>
              <initials>Marina </initials>
              <email>zasimova_ma@spbstu.ru </email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University </orgName>
              <surname>Ivanov </surname>
              <initials>Nikolay </initials>
              <email>ivanov_ng@spbstu.ru </email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Thermal manikin shape influence on airflow and heat transfer in the model room with displacement ventilation</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The paper presents the results of numerical modeling of turbulent flow and heat transfer in the model room with displacement ventilation. The goal of the study is to assess the shape influence of the thermal manikin placed in the room on the computed airflow structure. Three manikin shapes have been considered: a detailed one (close to a human shape) and ones simplified partially and completely. The problem formulation was close to the test conditions of P.V. Nielsen et al. (2003). The RANS approach based on the standard k-ε turbulence model was applied. The study revealed solution sensitivity to the dimension and topology of the mesh used, as well as the solution dependence on the uncertainty of the inlet velocity distribution. The calculated results were shown to agree generally with the experimental data. The simplification of the manikin shape had a significant impact on the local parameter prediction accuracy.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14307</doi>
          <udk>532.517</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>ventilation</keyword>
            <keyword>thermal manikin</keyword>
            <keyword>turbulent airflow and heat transfer</keyword>
            <keyword>natural convection</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.7/</furl>
          <file>07_94-111_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>112-121</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Petrov</surname>
              <initials>Vladimir</initials>
              <email>petrov@physics.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="002">
            <authorCodes>
              <orcid>0000-0002-2519-2577</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Gabdullin</surname>
              <initials>Pavel</initials>
              <email>gabdullin_pg@spbstu.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Pavlov </surname>
              <initials>Alexander </initials>
              <email>a.pavlov@physics.spbstu.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Ustinov</surname>
              <initials>Alexander</initials>
              <email>ustinov@physics.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <orgName>Paul Scherrer Institute</orgName>
              <surname>Strocov </surname>
              <initials>Vladimir</initials>
              <email>vladimir.strocov@psi.ch</email>
              <address>Switzerland</address>
            </individInfo>
          </author>
          <author num="006">
            <individInfo lang="ENG">
              <orgName>Paul Scherrer Institute</orgName>
              <surname>Dil Jan </surname>
              <initials>Hugo</initials>
              <email>jan-hugo.dil@psi.ch</email>
              <address>Switzerland</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Projecting classical Mott polarimeter</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In this paper we describe a new spin detector designed and manufactured at SPbPU. This device makes it possible to analyze the polarization of the secondary electron flux conserving the information about the electrons' spatial distribution. The main stages of development, construction and testing the detector are discussed in details. As a result, the possibility of implementing such devices has been proved in principle. At the same time, both high spatial resolution of this device and its efficiency were demonstrated. Combining such detectors with hemispherical energy analyzers will make it possible to obtain spin-resolved dispersion images of the structure under study.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14308</doi>
          <udk>53.07, 538.9</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>Mott detector</keyword>
            <keyword>spin</keyword>
            <keyword>electron spectroscopy</keyword>
            <keyword>secondary electron polarization</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.8/</furl>
          <file>08_112-121_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>122-132</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Dyubo</surname>
              <initials>Dmitry</initials>
              <email>doobinator@rambler.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Makarov </surname>
              <initials>Sergey </initials>
              <email>makarov@cee.spbstu.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Military Space Academy named after A.F. Mozhaysky</orgName>
              <surname>Kuleshov </surname>
              <initials>Yuri</initials>
              <email>vka@mil.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Military Space Academy named after A.F. Mozhaysky</orgName>
              <surname>Goncharov </surname>
              <initials>Pavel </initials>
              <email>vka@mil.ru</email>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <orgName>Military Space Academy named after A.F. Mozhaysky</orgName>
              <surname>Shunevich </surname>
              <initials>Nikolay</initials>
              <email>vka@mil.ru</email>
            </individInfo>
          </author>
          <author num="006">
            <individInfo lang="ENG">
              <orgName>Military Space Academy named after A.F. Mozhaysky</orgName>
              <surname>Martynov </surname>
              <initials>Viktor </initials>
              <email>vka@mil.ru</email>
            </individInfo>
          </author>
          <author num="007">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Tsybin</surname>
              <initials>Oleg</initials>
              <email>otsybin@rphf.spbstu.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">A model of an ion plasma electrically powered spacecraft propulsion with a remote monitoring and a control system</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">This paper continues the publication cycle on developing the ion plasma electrically powered spacecraft propulsion (EPSP) of the spacecraft. For monitoring and control of the EPSP operation, a feedback system based on a signal proportional to the EPSP plasma radiation intensity has been proposed to be used. It was assumed that the radiation intensity in the ultraviolet, visible and infrared ranges being proportional to the instantaneous thrust value of the EPSP. Accordingly, the introduction of a signal from the radiation registration detector into the feedback loop should allow to create an onboard closed system for monitoring and control of the EPSP operation. A photodetector based on a dynamic pin-diode integrator was considered for use in this system.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14309</doi>
          <udk>621.455.4; 621.455.34</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>ion plasma thruster</keyword>
            <keyword>acceleration</keyword>
            <keyword>neutralization</keyword>
            <keyword>plasma radiation</keyword>
            <keyword>photodetector</keyword>
            <keyword>automatic control</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.9/</furl>
          <file>09_122-132_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>133-145</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Kozhevnikov</surname>
              <initials>Vadim</initials>
              <email>vadim.kozhevnikov@gmail.com</email>
            </individInfo>
          </author>
          <author num="002">
            <authorCodes>
              <scopusid>7006335646</scopusid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Privalov</surname>
              <initials>Vadim</initials>
              <email>kafedra@physics.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="003">
            <authorCodes>
              <researcherid>AAD-9657-2019</researcherid>
              <scopusid>57197390995</scopusid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Fotiadi</surname>
              <initials>Alexander</initials>
              <email>fotiadi@rphf.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">A new approach to the assessment of the output power for a helium-neon gas laser with different cross-sectional geometry of the active element</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The proposed study continues a series of articles devoted to design methods for the key energy parameters of a helium-neon (He-Ne) gas laser. An application of the previously proposed method for designing the emission power to lasers with the rectangle- and ellipse-shaped cross sections of active elements has been considered. An idea of effective mode volume was used, a calculation algorithm was presented, and a procedure reducing unwieldy calculations was put forward. Varying the parameter values made it possible to get a detailed picture of dependencies of the output laser energy on the geometrical parameters of objects under study. A comparison of the obtained results permitted to find optimal laser parameters for maximum output power. The calculation results of the radiation energy were established to agree well both with those of the laser gain for the given cross sections and those of the experimental data.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14310</doi>
          <udk>621.373.8</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>helium-neon laser</keyword>
            <keyword>laser power</keyword>
            <keyword>tube geometry</keyword>
            <keyword>rectangular and elliptical cross sections</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.10/</furl>
          <file>10_133-145_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>146-157</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Institute for Analytical Instrumentation  of the Russian Academy of Sciences</orgName>
              <surname>Manoilov</surname>
              <initials>Vladimir</initials>
              <email>manoilov_vv@mail.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Institute for Analytical Instrumentation of the Russian Academy of Sciences</orgName>
              <surname>Novikov</surname>
              <initials>Lev</initials>
              <email>novik38@mail.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Institute for Analytical Instrumentation</orgName>
              <surname>Kuzmin </surname>
              <initials>Alexey</initials>
              <email>agqz55@rambler.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>Institute for Analytical Instrumentation</orgName>
              <surname>Titov </surname>
              <initials>Yuriy </initials>
              <email>titov.uriy@gmail.com</email>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <orgName>Institute for Analytical Instrumentation of the Russian Academy of Sciences</orgName>
              <surname>Zarutskiy </surname>
              <initials>Igor</initials>
              <email>igorzv@yandex.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An algorithm for processing mass spectrometric analysis data for initial diagnostics of diseases by exhaled gases</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">An algorithm for processing mass spectra of gases exhaled by patients has been proposed in the paper. The mass spectra are recorded on the MS7-200 quadrupole mass spectrometer, with electronic ionization and with direct capillary injection of the sample. The algorithm is based on transforming an array of spectra (not less than 10) in the space of principal components. The probability of a disease is determined through the Euclidean distance of the patient's coordinates from the centroid. Testing of the algorithm was carried out on the data of mass spectra of gases exhaled by cancer patients. The proposed procedure has several advantages over traditional laboratory methods. The algorithm uses the multidimensional probability density of the distribution of the parameters of the exhaled gases of control groups and the patient being tested and allows to compile an overall picture of the patient's probable diseases in a short time.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14311</doi>
          <udk>543.51+ 681.2–5</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>diagnostics</keyword>
            <keyword>principal component analysis</keyword>
            <keyword>multivariate probability density</keyword>
            <keyword>multivariate data processing</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.11/</furl>
          <file>11_146-157_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>158-167</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University </orgName>
              <surname>Mitrankova </surname>
              <initials>Mariia </initials>
              <email>mashalario@gmail.com </email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Bannikov </surname>
              <initials>Egor </initials>
              <email>bannikov.ev.21@gmail.com</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Berdnikov</surname>
              <initials>Alexander</initials>
              <email>alexber@phmf.spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="004">
            <authorCodes>
              <orcid>0000-0003-0309-5917</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Berdnikov</surname>
              <initials>Yaroslav</initials>
              <email>berdnikov@spbstu.ru</email>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Dubov </surname>
              <initials>Alexander</initials>
              <email>alexanderpolytech@mail.ru</email>
            </individInfo>
          </author>
          <author num="006">
            <authorCodes>
              <orcid>0000-0002-3395-0454</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Kotov</surname>
              <initials>Dmitry</initials>
              <email>dmitriy.kotov@gmail.com</email>
            </individInfo>
          </author>
          <author num="007">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Mitrankov</surname>
              <initials>Yuriy</initials>
              <email>mitrankovy@gmail.com</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An analysis of φ-meson production in the collisions of proton beams with aluminum and gold nuclei at energies of 200 GeV</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In the paper, φ-meson production in the relativistic collisions at energies of 200 GeV measured by the PHENIX experiment (RHIC) has been studied. Phi-mesons’ nuclear modification factors were calculated for the mentioned interactions under conditions identical to the experimental ones, using different theoretical models, the results being compared. The accounting for the formation phase of quark-gluon plasma (QGP) in simulation was established to agree well with experiment for the p + Au collisions and disagree for the p + Al ones. This result could indicate an insufficient size of the interaction system of the latter to form QGP at an energy of 200 GeV and the sufficiency of the created minimum conditions for its formation in the former interaction system.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14312</doi>
          <udk>539.12</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>quark-gluon plasma</keyword>
            <keyword>cold nuclear matter effect</keyword>
            <keyword>nuclear modification factor</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.12/</furl>
          <file>12_158-167_14(3)2021.pdf</file>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>168-184</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Fedosin </surname>
              <initials>Sergey</initials>
              <email>sergey.fedosin@gmail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The relativistic uniform model: the metric of the covariant theory of gravitation inside a body</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In the paper, it has been established that the sum of stress-energy tensors of the electromagnetic and gravitational fields, the acceleration and the pressure ones inside a stationary uniform spherical body vanishes within the framework of relativistic uniform model. This fact significantly simplifies a solution of the equation for the metric in the covariant theory of gravitation (CTG). The metric tensor components inside the body were calculated, and then they were combined with those of external metric tensor on the body’s surface. The latter procedure also allowed us to exactly determine one of two unknown coefficients in the metric outside the body. The comparison between the CTG metric and the Reissner – Nordström one in general theory of relativity clearly demonstrated their difference caused by discrepancy between equations for the metric and a difference in formulations of the cosmological constant.</abstract>
        </abstracts>
        <codes>
          <doi>10.18721/JPM.14313</doi>
          <udk>514.13:531.51</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>metric</keyword>
            <keyword>covariant theory of gravitation</keyword>
            <keyword>scalar curvature</keyword>
            <keyword>cosmological constant</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2021.53.13/</furl>
          <file>13_168-184_14(3)2021.pdf</file>
        </files>
      </article>
    </articles>
  </issue>
</journal>
