<p>In this work, we studied the role of Ba and Sr substitutions on the structural, morphological, magnetic, and magnetocaloric properties of the La<InlineEquation ID="IEq17"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq1.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.7} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.7</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>Ca<InlineEquation ID="IEq18"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq18.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.3} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.3</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>MnO<InlineEquation ID="IEq19"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq19.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="8" /> </InlineMediaObject> <EquationSource Format="TEX">\( _3 \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> manganite. The La<InlineEquation ID="IEq20"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq1.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.7} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.7</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>Ca<InlineEquation ID="IEq21"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq2.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.2} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.2</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>Ba<InlineEquation ID="IEq22"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq3.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.1} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.1</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>MnO<InlineEquation ID="IEq23"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq4.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="8" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{3} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> and La<InlineEquation ID="IEq24"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq1.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.7} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.7</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>Ca<InlineEquation ID="IEq25"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq2.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.2} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.2</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>Sr<InlineEquation ID="IEq26"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq3.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{0.1} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow> <mn>0.1</mn> </mrow> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>MnO<InlineEquation ID="IEq27"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10948_2025_7008_Article_IEq4.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="8" /> </InlineMediaObject> <EquationSource Format="TEX">\( _{3} \)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> manganites were synthetized using the combustion method. FT-IR, X-ray diffraction, and magnetization measurements were performed to investigate the crystallographic structure and the magnetocaloric properties. The samples exhibit a ferromagnetic behavior, and the ferromagnetic-paramagnetic transition occurs around the room temperature. The critical temperatures are 298.5 K and 308.7 K for the LCBM and LCSM samples, respectively. The maxima values of magnetic entropy at a field of 3T are 1.64 J/Kg K and 2.08 J/Kg K for the LCBM and LCSM samples. The LCSM manganite shows a better magnetocaloric performance, which could be related to an enhancement of the double exchange interaction due to the shorter average bond length between Mn and O ions for this sample. These results are in agreement with those reported in the literature, highlighting that the solution combustion synthesis route presents potential advantages, such as a faster and simpler route for obtaining manganites.</p>

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Structural and Magnetocaloric Properties of La\( _{0.7} \)Ca\( _{0.2} \)Ba\( _{0.1} \)MnO\( _{3} \) and La\( _{0.7} \)Ca\( _{0.2} \)Sr\( _{0.1} \)MnO\( _{3} \) Manganites Obtained by the Solution Combustion Method

  • Valeria Nástar,
  • Sonia Gaona,
  • Alejandra I. Guerrero

摘要

In this work, we studied the role of Ba and Sr substitutions on the structural, morphological, magnetic, and magnetocaloric properties of the La \( _{0.7} \) 0.7 Ca \( _{0.3} \) 0.3 MnO \( _3 \) 3 manganite. The La \( _{0.7} \) 0.7 Ca \( _{0.2} \) 0.2 Ba \( _{0.1} \) 0.1 MnO \( _{3} \) 3 and La \( _{0.7} \) 0.7 Ca \( _{0.2} \) 0.2 Sr \( _{0.1} \) 0.1 MnO \( _{3} \) 3 manganites were synthetized using the combustion method. FT-IR, X-ray diffraction, and magnetization measurements were performed to investigate the crystallographic structure and the magnetocaloric properties. The samples exhibit a ferromagnetic behavior, and the ferromagnetic-paramagnetic transition occurs around the room temperature. The critical temperatures are 298.5 K and 308.7 K for the LCBM and LCSM samples, respectively. The maxima values of magnetic entropy at a field of 3T are 1.64 J/Kg K and 2.08 J/Kg K for the LCBM and LCSM samples. The LCSM manganite shows a better magnetocaloric performance, which could be related to an enhancement of the double exchange interaction due to the shorter average bond length between Mn and O ions for this sample. These results are in agreement with those reported in the literature, highlighting that the solution combustion synthesis route presents potential advantages, such as a faster and simpler route for obtaining manganites.