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  <front>
    <journal-meta>
      <journal-id journal-id-type="publisher-id">80</journal-id>
      <journal-id journal-id-type="index">urn:lsid:arphahub.com:pub:3CDB4662-2EEC-55B0-878A-88F876A7F403</journal-id>
      <journal-title-group>
        <journal-title xml:lang="en">Modern Electronic Materials</journal-title>
        <abbrev-journal-title xml:lang="en">MoEM</abbrev-journal-title>
      </journal-title-group>
      <issn pub-type="ppub">2452-2449</issn>
      <issn pub-type="epub">2452-1779</issn>
      <publisher>
        <publisher-name>Modern Electronic Materials</publisher-name>
      </publisher>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.3897/j.moem.12.1.182531</article-id>
      <article-id pub-id-type="publisher-id">182531</article-id>
      <article-categories>
        <subj-group subj-group-type="heading">
          <subject>Research Article</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title>Magnetic properties of hexagonal isotropic polycrystalline SrFe<sub>12</sub>O<sub>19</sub> ferrites obtained by radiation-thermal sintering</article-title>
      </title-group>
      <contrib-group content-type="authors">
        <contrib contrib-type="author" corresp="yes">
          <name name-style="western">
            <surname>Kostishin</surname>
            <given-names>Vladimir G.</given-names>
          </name>
          <email xlink:type="simple">drvgkostishyn@mail.ru</email>
          <uri content-type="orcid">https://orcid.org/0000-0001-5384-6331</uri>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Alekseev</surname>
            <given-names>Albert A.</given-names>
          </name>
          <uri content-type="orcid">https://orcid.org/0009-0007-3031-0164</uri>
          <xref ref-type="aff" rid="A2">2</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Scherbakov</surname>
            <given-names>Sergey V.</given-names>
          </name>
          <xref ref-type="aff" rid="A2">2</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Nalogin</surname>
            <given-names>Aleksey G.</given-names>
          </name>
          <xref ref-type="aff" rid="A2">2</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Turchenko</surname>
            <given-names>Vitaliy A.</given-names>
          </name>
          <uri content-type="orcid">https://orcid.org/0000-0002-4755-3898</uri>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Isaev</surname>
            <given-names>Igor M.</given-names>
          </name>
          <uri content-type="orcid">https://orcid.org/0000-0003-3167-7025</uri>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Savchenko</surname>
            <given-names>Elena S.</given-names>
          </name>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Savchenko</surname>
            <given-names>Alexander G.</given-names>
          </name>
          <uri content-type="orcid">https://orcid.org/0000-0002-8477-0162</uri>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Skibo</surname>
            <given-names>Boris M.</given-names>
          </name>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name name-style="western">
            <surname>Matashneva</surname>
            <given-names>Ekaterina O.</given-names>
          </name>
          <xref ref-type="aff" rid="A1">1</xref>
        </contrib>
      </contrib-group>
      <aff id="A1">
        <label>1</label>
        <addr-line content-type="verbatim">National University of Science and Technology “MISIS”, 4-1 Leninsky Ave., Moscow 119049, Russian Federation</addr-line>
        <institution>National University of Science and Technology “MISIS”</institution>
        <addr-line content-type="city">Moscow</addr-line>
        <country>Russia</country>
        <uri content-type="ror">https://ror.org/019vsm959</uri>
      </aff>
      <aff id="A2">
        <label>2</label>
        <addr-line content-type="verbatim">JSC “NPP “Istok” named after Shokin”, 2A Vokzalnaya Str., Fryazino, Moscow Region 141190, Russian Federation</addr-line>
        <institution>JSC “NPP “Istok” named after Shokin”</institution>
        <addr-line content-type="city">Fryazino</addr-line>
        <country>Russia</country>
      </aff>
      <author-notes>
        <fn fn-type="corresp">
          <p>Corresponding author: Vladimir G. Kostishin (<email xlink:type="simple">drvgkostishyn@mail.ru</email>)</p>
        </fn>
      </author-notes>
      <pub-date pub-type="collection">
        <year>2026</year>
      </pub-date>
      <pub-date pub-type="epub">
        <day>23</day>
        <month>04</month>
        <year>2026</year>
      </pub-date>
      <volume>12</volume>
      <issue>1</issue>
      <fpage>35</fpage>
      <lpage>42</lpage>
      <uri content-type="arpha" xlink:href="http://openbiodiv.net/CA9866EB-EFB0-514B-A516-506B23B34866">CA9866EB-EFB0-514B-A516-506B23B34866</uri>
      <history>
        <date date-type="received">
          <day>15</day>
          <month>12</month>
          <year>2025</year>
        </date>
        <date date-type="accepted">
          <day>03</day>
          <month>03</month>
          <year>2026</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>Vladimir G. Kostishin, Albert A. Alekseev, Sergey V. Scherbakov, Aleksey G. Nalogin, Vitaliy A. Turchenko, Igor M. Isaev, Elena S. Savchenko, Alexander G. Savchenko, Boris M. Skibo, Ekaterina O. Matashneva</copyright-statement>
        <license license-type="creative-commons-attribution" xlink:href="http://creativecommons.org/licenses/by/4.0/" xlink:type="simple">
          <license-p>This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY 4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
        </license>
      </permissions>
      <abstract>
        <label>Abstract</label>
        <p>Hexagonal strontium ferrite has found wide application in the fabrication of permanent magnets and active media of UHF electronics and photonics. The performance of hexagonal strontium ferrites depends largely on their synthesis method. Hexagonal polycrystalline isotropic SrFe<sub>12</sub>O<sub>19</sub> ferrite specimens have been synthesized using fast electron beam radiation-thermal sintering (<abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>) in a PLU-6 electron accelerator of G.I. Budker Institute of Nuclear Physics of the Russian Academy of Sciences. The <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature has been varied from 1200 to 1400 °C, and the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time, from 10 to 90 min. The phase composition and lattice parameters of the specimens have been studied using X-ray diffraction on a DRON-8 diffractometer in Co<italic>K</italic><sub>α1</sub> radiation. The density of the specimens has been measured following Archimedean law on a UW620H electronic balance with a liquid density measurement attachment. The magnetic hysteresis loop parameters of the specimens have been studied with a VM-07 vibromagnetometer.</p>
        <p>The specimens has proven to be single-phase with a <italic>P</italic>63/<italic>mmc</italic> space group (No. 194), corresponding to a hexagonal ferrite structure. For the first time, changes in the magnetic hysteresis loop parameters of hexagonal SrFe<sub>12</sub>O<sub>19</sub> strontium ferrite specimens synthesized with fast electron beam <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> have been studied. We show that the width and intensity of the magnetic hysteresis loop decrease noticeably with an increase in the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature from 1200 to 1350–1400 °C. The magnetization coercive force <sub><italic>j</italic></sub><italic>H<sub>c</sub></italic> decline to the minimum values at <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperatures <italic>T</italic><sub>sint</sub> ≥1250 °C, probably due to recrystallization in the ferrite lattice: the combined impact of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and radiation-induced diffusion triggers intense grain growth, significantly reducing the number of domain boundaries and, hence, causing a drop in <sub><italic>j</italic></sub><italic>H</italic><sub>c</sub>. The high energy efficiency of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> in ferrite ceramics synthesis has been confirmed for the example of SrFe<sub>12</sub>O<sub>19</sub>.</p>
      </abstract>
      <kwd-group>
        <label>Keywords</label>
        <kwd>radiation-thermal sintering</kwd>
        <kwd>polycrystalline hexagonal isotropic ferrite SrFe<sub>12</sub>O<sub>19</sub></kwd>
        <kwd>X-ray diffraction</kwd>
        <kwd>fast electrons</kwd>
        <kwd>electron accelerator</kwd>
        <kwd>density</kwd>
        <kwd>lattice magnetic hysteresis loop parameters</kwd>
        <kwd>magnetization</kwd>
        <kwd>coercive force</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec sec-type="1. Introduction" id="sec1">
      <title>1. Introduction</title>
      <p><italic>M</italic>-type hexagonal SrFe<sub>12</sub>O<sub>19</sub> strontium ferrite has a crystalline structure that is isomorphic to that of magnetoplumbite (PbFe<sub>12</sub>O<sub>19</sub>) [<xref ref-type="bibr" rid="B1">1</xref>]. Due to the difference in the ionic radii of barium and strontium, a substitution of the former for the latter in the hexagonal ferrite lattice increases the magnetic crystallographic anisotropy constant <italic>K</italic> by 10 % [<xref ref-type="bibr" rid="B2">2</xref>]. Furthermore, SrМ hexaferrites have better processability as compared to BaFe<sub>12</sub>O<sub>19</sub> hexaferrites [<xref ref-type="bibr" rid="B2">2</xref>]. Due to its combination of magnetic properties and performance, SrМ ferrite has found wide application in the fabrication of permanent magnets [<xref ref-type="bibr" rid="B1">1</xref>, <xref ref-type="bibr" rid="B2">2</xref>], active media of millimeter-wavelength UHF electronics devices [<xref ref-type="bibr" rid="B3">3</xref>], and THz photonics devices [<xref ref-type="bibr" rid="B4">4</xref>]. In science and engineering, there is still great interest in the development of UHF electronics devices based on thick hexagonal ferrites films [<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B6">6</xref>]. Today, the main industrial synthesis process for the above materials is the ceramic technology [<xref ref-type="bibr" rid="B1">1</xref>, <xref ref-type="bibr" rid="B2">2</xref>, <xref ref-type="bibr" rid="B5">5</xref>]. Typical process diagram of polycrystalline hexagonal SrFe<sub>12</sub>O<sub>19</sub> ferrites is shown in Fig. <xref ref-type="fig" rid="F1">1</xref>. Along with the commonly known advantages, the ceramic technology has a number of drawbacks. One of the main drawbacks is the high energy consumption. Alternative SrFe<sub>12</sub>O<sub>19</sub> hexaferrite technology can be radiation-thermal sintering (<abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>) which has been well tested for a wide range of ferrites [<xref ref-type="bibr" rid="B7">7</xref>–<xref ref-type="bibr" rid="B9">9</xref>], including BaМ [<xref ref-type="bibr" rid="B7">7</xref>]. The difference of the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> process from the conventional ceramic one is that the thermal sintering of raw billets is replaced for fast electron beam sintering in an electron accelerator [<xref ref-type="bibr" rid="B7">7</xref>–<xref ref-type="bibr" rid="B9">9</xref>]. The aim of this work is to explore the possibility of synthesis of high-quality isotropic polycrystalline SrFe<sub>12</sub>O<sub>19</sub> hexaferrites using the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> technology and to study the magnetic properties of synthesized hexaferrite specimens.</p>
      <fig id="F1">
        <object-id content-type="arpha">47068F57-EFC4-5426-8341-28203668C572</object-id>
        <label>Figure 1.</label>
        <caption>
          <p>Typical synthesis process route of isotropic polycrystalline hexagonal ferrites using ceramic technology</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g001.jpg" id="oo_1646369.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646369</uri>
        </graphic>
      </fig>
    </sec>
    <sec sec-type="2. Experimental" id="sec2">
      <title>2. Experimental</title>
      <p>The iron-containing raw material for the preparation of the test specimens was MM-2 Grade Fe<sub>2</sub>O<sub>3</sub> iron oxide (TU6-09-4816–80, impurity contents (wt.%) 0.01 SiO<sub>2</sub>, 0,01 Al<sub>2</sub>O<sub>3</sub>, 0,01 Cr<sub>2</sub>O<sub>3</sub>, 0,01 Na<sub>2</sub>O). The strontium containing raw material was Ch Grade (99.0% purity) crystalline strontium carbonate from Isfara Chemical Factory (Tajikistan). The raw billets were prepared in accordance with the diagram presented in Fig. <xref ref-type="fig" rid="F1">1</xref>. The preparation route included all conventional operations except thermal sintering. The final operation was replaced for <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>. The replacement of conventional sintering for fast electron beam <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> was chosen due to the far lower energy consumption and higher sintering quality delivered by fast electron beam <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> [<xref ref-type="bibr" rid="B7">7</xref>–<xref ref-type="bibr" rid="B9">9</xref>]. For <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>, along with the high-temperature treatment, radiation-enhanced diffusion contributes significantly to the process. The combination of the above factors delivers sintering at lower temperatures and in a shifter time [<xref ref-type="bibr" rid="B7">7</xref>–<xref ref-type="bibr" rid="B9">9</xref>]. Radiation-thermal sintering of the specimens was carried out in a fast electron beam of an ILU-6 electron accelerator used for radiation technologies (maximum fast electron energy 2.5 MeV) at the G.I. Budker Institute of Nuclear Physics, Siberian Branch of the Russian Academy of Sciences [<xref ref-type="bibr" rid="B10">10</xref>]. Fast electron beam sintering of hexagonal ferrites was carried out in a cell for ferrite ceramic sintering designed at the Chair of Electronics Materials of the MISIS Research and Technology University Table <xref ref-type="table" rid="T1">1</xref> summarizes data on the SrМ specimens.</p>
      <table-wrap id="T1" position="float" orientation="portrait">
        <label>Table 1.</label>
        <caption>
          <p>Radiation-thermal sintering parameters for SrFe<sub>12</sub>O<sub>19</sub> specimens</p>
        </caption>
        <table>
          <tbody>
            <tr>
              <td rowspan="1" colspan="1">#</td>
              <td rowspan="1" colspan="1">Raw billet No.</td>
              <td rowspan="1" colspan="1">Specimen</td>
              <td rowspan="1" colspan="1"><abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature (°C)</td>
              <td rowspan="1" colspan="1"><abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time (min)</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">1</td>
              <td rowspan="1" colspan="1">8-p6</td>
              <td rowspan="1" colspan="1">GSI_# 8</td>
              <td rowspan="1" colspan="1">1200</td>
              <td rowspan="1" colspan="1">60</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">2</td>
              <td rowspan="1" colspan="1">9-p6</td>
              <td rowspan="1" colspan="1">GSI_# 9</td>
              <td rowspan="1" colspan="1">1250</td>
              <td rowspan="1" colspan="1">60</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">3</td>
              <td rowspan="1" colspan="1">11-p6</td>
              <td rowspan="1" colspan="1">GSI_# 11</td>
              <td rowspan="1" colspan="1">1300</td>
              <td rowspan="1" colspan="1">10</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">4</td>
              <td rowspan="1" colspan="1">12-p6</td>
              <td rowspan="1" colspan="1">GSI_# 12</td>
              <td rowspan="1" colspan="1">1300</td>
              <td rowspan="1" colspan="1">30</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">5</td>
              <td rowspan="1" colspan="1">10-p6</td>
              <td rowspan="1" colspan="1">GSI_# 10</td>
              <td rowspan="1" colspan="1">1300</td>
              <td rowspan="1" colspan="1">60</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">6</td>
              <td rowspan="1" colspan="1">13-p6</td>
              <td rowspan="1" colspan="1">GSI_# 13</td>
              <td rowspan="1" colspan="1">1300</td>
              <td rowspan="1" colspan="1">90</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">7</td>
              <td rowspan="1" colspan="1">14-p6</td>
              <td rowspan="1" colspan="1">GSI_# 14</td>
              <td rowspan="1" colspan="1">1350</td>
              <td rowspan="1" colspan="1">40; 60</td>
            </tr>
            <tr>
              <td rowspan="1" colspan="1">8</td>
              <td rowspan="1" colspan="1">30-p6</td>
              <td rowspan="1" colspan="1">GSI_# 30</td>
              <td rowspan="1" colspan="1">1400</td>
              <td rowspan="1" colspan="1">30; 60</td>
            </tr>
          </tbody>
        </table>
      </table-wrap>
      <p>X-ray structural analysis of the test specimens was carried out on a DRON-8 X-ray diffractometer (NPP Burevestnik JSC, St. Petersburg, Russia) in Co<italic>K</italic><sub>α1</sub> radiation (λ = 0.178897 nm) with Bragg-Brentano focusing by two Soller slots at room temperature.</p>
      <p>The density of the specimens was measured using Archimedean law on a UW620H electronic balance with a liquid density measurement attachment and calculated using the following formula:</p>
      <p><mml:math id="M1"><mml:mi>ρ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>ρ</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:msub><mml:mi>W</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>−</mml:mo><mml:msub><mml:mi>W</mml:mi><mml:mi>l</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow><mml:mo>,</mml:mo></mml:math>	(1)</p>
      <p>where ρ is the specimen density (g/cm<sup>3</sup>) ρ<sub>0</sub> is the known liquid density (g/cm<sup>3</sup>), <italic>W<sub>a</sub></italic> is the specimen weight in air (g), and <italic>W<sub>l</sub></italic> is the liquid sample weight (g).</p>
      <p>The X-ray density of the ferrites was calculated based on X-ray analysis data using the following formula:</p>
      <p><mml:math id="M2"><mml:msub><mml:mi>ρ</mml:mi><mml:mrow><mml:mrow><mml:mi>X</mml:mi></mml:mrow><mml:mo>−</mml:mo><mml:mrow><mml:mi>ray</mml:mi></mml:mrow></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mn>2</mml:mn><mml:msub><mml:mi>M</mml:mi><mml:mi>A</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi>V</mml:mi><mml:msub><mml:mi>N</mml:mi><mml:mi>A</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mn>2</mml:mn><mml:msub><mml:mi>M</mml:mi><mml:mi>A</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:msup><mml:mi>a</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mn>3</mml:mn><mml:msqrt><mml:mn>3</mml:mn></mml:msqrt><mml:msub><mml:mi>N</mml:mi><mml:mi>A</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>,</mml:mo></mml:math>	(2)</p>
      <p>where <italic>M<sub>A</sub></italic> is the molecular weight of hexaferrite, <italic>c</italic> and <italic>a</italic> are the lattice parameters of hexaferrite, <italic>N</italic><sub>A</sub> is the Avogadro number, and <italic>V</italic> is the unit cell volume. The average density proved to be 5.1 g/cm<sup>3</sup>.</p>
      <p>The hysteresis loops of the 1.0−3.0 mm diam. spherical sintered hexaferrite specimens were recorded using a VM-07 vibromagnetometer.</p>
    </sec>
    <sec sec-type="3. Results and discussion" id="sec3">
      <title>3. Results and discussion</title>
      <p>Analysis of the X-ray diffraction spectra showed that the synthesized specimens were single-phase (space group <italic>P</italic>6<sub>3</sub>/<italic>mmc</italic> (No. 194), i.e., hexagonal ferrites. Figure <xref ref-type="fig" rid="F2">2</xref> shows <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>-synthesized SrFe<sub>12</sub>O<sub>19</sub> hexagonal ferrite specimen density as a function of (<italic>a</italic>) sintering time at <italic>T</italic> = 1300 °C and (<italic>b</italic>) of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature for sintering time 30 and 60 min.</p>
      <fig id="F2">
        <object-id content-type="arpha">72C9CBC7-5921-53A5-B7E8-C74CCA67170A</object-id>
        <label>Figure 2.</label>
        <caption>
          <p>SrFe<sub>12</sub>O<sub>19</sub> hexaferrite specimen density as a function of (<italic>a</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time at 1300 °C and (<italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g002.jpg" id="oo_1646370.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646370</uri>
        </graphic>
      </fig>
      <p>The density of SrFe<sub>12</sub>O<sub>19</sub> decreases with an increase in the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time at 1300 °C (Fig. <xref ref-type="fig" rid="F2">2</xref><italic>a</italic>) and increases with the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature (Fig. <xref ref-type="fig" rid="F2">2</xref><italic>b</italic>). It can be seen from Fig. <xref ref-type="fig" rid="F2">2</xref> that the optimum <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> mode for SrFe<sub>12</sub>O<sub>19</sub> is 1250–1300 °C for 30–60 min.</p>
      <p>The decrease in the polycrystal density for <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> beginning from a certain time seems to be accounted for by the fact that, upon reaching the optimum density of the material, the energy of fast electrons starts to exert the contrary impact, i.e., lattice degradation, making the polycrystal structure looser [<xref ref-type="bibr" rid="B11">11</xref>–<xref ref-type="bibr" rid="B14">14</xref>].</p>
      <p>Figure <xref ref-type="fig" rid="F3">3</xref> shows magnetic hysteresis loops for the specimens synthesized with 60 min <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>.</p>
      <fig id="F3">
        <object-id content-type="arpha">5F5ABAE5-4355-519A-9EC5-172BE96D41E1</object-id>
        <label>Figure 3.</label>
        <caption>
          <p>Magnetic hysteresis loops for polycrystalline SrFe<sub>12</sub>O<sub>19</sub> hexagonal isotropic ferrite specimens synthesized using <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> at different temperatures: (<italic>a</italic>) 1200 °C, (<italic>b</italic>) 1250 °C, (<italic>c</italic>) 1300 °C, and (<italic>d</italic>) 1400 °C. Sintering time 60 min.</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g003.jpg" id="oo_1646371.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646371</uri>
        </graphic>
      </fig>
      <p>Figure <xref ref-type="fig" rid="F4">4</xref> shows magnetic hysteresis loops for the specimens synthesized with <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> at 1300 °C for different time.</p>
      <fig id="F4">
        <object-id content-type="arpha">B9CC0FAD-E018-56E0-96FA-261CB4F164E2</object-id>
        <label>Figure 4.</label>
        <caption>
          <p>Magnetic hysteresis loops for polycrystalline SrFe<sub>12</sub>O<sub>19</sub> hexagonal isotropic ferrite specimens synthesized using <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> at different time: (<italic>a</italic>) 10 min, (<italic>b</italic>) 30 min, (<italic>c</italic>) 60 min, and (<italic>d</italic>) 90 min. Sintering temperature 1300 °C</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g004.jpg" id="oo_1646372.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646372</uri>
        </graphic>
      </fig>
      <p>It can be seen from Figs <xref ref-type="fig" rid="F3">3</xref> and <xref ref-type="fig" rid="F4">4</xref> that the intensity and width of the magnetic hysteresis loops decrease with an increase in the sintering temperature and time.</p>
      <p>Figure <xref ref-type="fig" rid="F5">5</xref> shows specific saturation magnetization σ<sub><italic>s</italic></sub> and specific remanent magnetization of the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic> and <italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature for 60 min sintering time and (<italic>c</italic> and <italic>d</italic>) sintering time for 1300 °C <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature. Figures <xref ref-type="fig" rid="F6">6</xref>, <xref ref-type="fig" rid="F7">7</xref>, <xref ref-type="fig" rid="F8">8</xref>, <xref ref-type="fig" rid="F9">9</xref> show coercive force <sub><italic>j</italic></sub><italic>H<sub>c</sub></italic>, magnetic anisotropy field <italic>H<sub>k</sub></italic>, magnetic hysteresis loop area <italic>S</italic><sub>loop</sub>, and magnetic hysteresis loop rectangularity, respectively, as a function of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and time.</p>
      <fig id="F5">
        <object-id content-type="arpha">E86AB5B7-4C9F-543A-8511-4C693C37C8FE</object-id>
        <label>Figure 5.</label>
        <caption>
          <p>(<italic>a</italic> and <italic>c</italic>) Specific saturation magnetization σ<italic><sub>s</sub></italic> and (<italic>b</italic> and <italic>d</italic>) specific remanent magnetization of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic> and <italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and (<italic>c</italic> and <italic>d</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g005.jpg" id="oo_1646373.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646373</uri>
        </graphic>
      </fig>
      <fig id="F6">
        <object-id content-type="arpha">394E83D3-0D23-5384-BCE5-FE0283DCB015</object-id>
        <label>Figure 6.</label>
        <caption>
          <p>Magnetization coercive force of SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and (<italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g006.jpg" id="oo_1646374.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646374</uri>
        </graphic>
      </fig>
      <fig id="F7">
        <object-id content-type="arpha">717FDD9B-78B0-5BBA-983B-D722E5DEBC73</object-id>
        <label>Figure 7.</label>
        <caption>
          <p>Magnetic anisotropy of SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and (<italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g007.jpg" id="oo_1646375.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646375</uri>
        </graphic>
      </fig>
      <fig id="F8">
        <object-id content-type="arpha">92550FE4-762C-5404-9EC6-7C67EDB62411</object-id>
        <label>Figure 8.</label>
        <caption>
          <p>Magnetic energy (magnetic hysteresis loop area) of SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and (<italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g008.jpg" id="oo_1646376.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646376</uri>
        </graphic>
      </fig>
      <fig id="F9">
        <object-id content-type="arpha">77262816-9C54-5298-B444-47A6C734023C</object-id>
        <label>Figure 9.</label>
        <caption>
          <p>Magnetic hysteresis loop rectangularity coefficient of SrFe<sub>12</sub>O<sub>19</sub> specimens as a function of (<italic>a</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and (<italic>b</italic>) <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time</p>
        </caption>
        <graphic xlink:href="moem-12-e182531-g009.jpg" id="oo_1646377.jpg">
          <uri content-type="original_file">https://binary.pensoft.net/fig/1646377</uri>
        </graphic>
      </fig>
      <p>As can be seen from Figs <xref ref-type="fig" rid="F5">5</xref>, <xref ref-type="fig" rid="F6">6</xref>, <xref ref-type="fig" rid="F7">7</xref>, <xref ref-type="fig" rid="F8">8</xref>, <xref ref-type="fig" rid="F9">9</xref>, the magnetic hysteresis parameters of the SrFe<sub>12</sub>O<sub>19</sub> specimens change in a similar manner during <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> with an increase in the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and time. <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature determines the shape and parameters of the hysteresis loop. With an increase in the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and time, all magnetic hysteresis loop parameters of the test specimens decline in comparison with their parameters for the lowest <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature and shortest time.</p>
      <p>The <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature growing from 1200 to 1350–1400 °C (sintering time 60 min), the specific saturation magnetization σ<italic><sub>s</sub></italic> declines by 32 %; the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> time increasing from 10 to 90 min (sintering temperature 1300 °C), σ<italic><sub>s</sub></italic> drops by 29.5 %. The specific remanent magnetization σ<italic><sub>r</sub></italic> for the same <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> modes drops by 93 and 91 %, respectively; the magnetization coercive force <italic><sub>j</sub>H<sub>c</sub></italic> declines by 96 % in both cases; the magnetic field anisotropy <italic>H<sub>k</sub></italic> decreases by 81 and 82 %, respectively; the magnetic energy (magnetic hysteresis loop area) drops by 79 and 80 %, respectively; the magnetic hysteresis loop rectangularity coefficient drops by 88 and 90 %, respectively. Similar changes, though less intense, were observed [<xref ref-type="bibr" rid="B15">15</xref>] for <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev>-synthesized hexagonal BaFe<sub>12</sub>O<sub>19</sub> ferrites.</p>
      <p>It was shown that the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> technology allows ferrite sintering in several decades of minutes. The predominant factor was the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature, differing for each type of ceramics. The physical mechanism of ceramic sintering process acceleration by fast electrons is not yet clear [<xref ref-type="bibr" rid="B16">16</xref>–<xref ref-type="bibr" rid="B23">23</xref>]. Most researchers believe that the predominant mechanism of radiation acceleration of mass transport in ferrite ceramics is surface recombination. Irradiation of ceramics billets induces electron excitation in grains and powder compacts. Excited electrons tend to localize at grain boundaries and recombine, releasing energy. This results in the formation of temperature gradients, causing thermal diffusion flows which significantly accelerate solid state reactions of ferrite synthesis.</p>
      <p>The results reported herein show that, for the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> modes used, the highest SrFe<sub>12</sub>O<sub>19</sub> hexaferrite density was obtained for sintering temperature <italic>T</italic><sub>sint</sub> = 1200÷1300 °C and sintering time <italic>t</italic><sub>sint</sub> = 60 min, and at sintering temperature <italic>T</italic><sub>sint</sub> = 1300÷1400 °C and sintering time <italic>t</italic><sub>sint</sub> = 30 min. However, at <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature ≥1350 °C, even for a sintering time of 30 min, the magnetization drops by 30 % and the coercive force, by 96 %. Thus, strontium hexaferrite, in fact, becomes low-magnetization and low-coercive force hexaferrite, i.e., a magnetically soft material. This material cannot be used for the fabrication of high-quality permanent magnets. The problem of its applications in other conventional application domains of hexagonal ferrites requires further study. The experiments carried out in this work showed that the existing <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> process modes for polycrystalline SrFe<sub>12</sub>O<sub>19</sub> require improvement. Yet it is obvious that the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperature should be within 1250–1300 °C.</p>
      <p>The abrupt decline of <italic><sub>j</sub>H<sub>c</sub></italic> at <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperatures of above ≥1250 °C can be accounted for by recrystallization in the material. Elevated <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> temperatures cause intense grain growth. The overall quantity of domain boundaries decreases abruptly, also leading to a significant decrease in the coercive force [<xref ref-type="bibr" rid="B24">24</xref>].</p>
    </sec>
    <sec sec-type="Conclusion" id="sec4">
      <title>Conclusion</title>
      <p>Changes in the parameters of magnetic hysteresis loop parameters in hexagonal SrFe<sub>12</sub>O<sub>19</sub>, strontium ferrite synthesized using fast electron beam <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> were studied for the first time.</p>
      <p>The high energy efficiency of <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> technology of ferrite ceramics was confirmed for the example of <italic>M</italic>-type hexagonal strontium ferrite.</p>
      <p>We showed that the <abbrev xlink:title="radiation-thermal sintering">RTS</abbrev> modes tested are not suitable for the synthesis of high-quality polycrystalline SrFe<sub>12</sub>O<sub>19</sub> hexaferrites and require improvement.</p>
      <p>The significant decline of <sub><italic>j</italic></sub><italic>H<sub>c</sub></italic> of the SrFe<sub>12</sub>O<sub>19</sub> specimens at <italic>T</italic><sub>sint</sub> ≥1250 °C is accounted for by recrystallization and intense grain growth due to high temperatures and radiation-enhanced diffusion.</p>
    </sec>
    <sec sec-type="Acknowledgements" id="sec5">
      <title>Acknowledgements</title>
      <p>The authors are grateful to M.V. Korobeinikov and M.A. Mikhailenko for carrying out radiation-thermal sintering of the specimens.</p>
    </sec>
    <sec sec-type="Conflict of interests" id="sec6">
      <title>Conflict of interests</title>
      <p>The authors claim no conflict of interests.</p>
    </sec>
    <sec sec-type="Funding" id="sec7">
      <title>Funding</title>
      <p>This work was funded at the expense of project Russian Science Foundation No. 24-13-00268.</p>
    </sec>
    <sec sec-type="Additional information" id="sec8">
      <title>Additional information</title>
      <p>No AI tools were used in the work on the article.</p>
    </sec>
  </body>
  <back>
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