<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-14T13:40:52Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/36734" metadataPrefix="ese">https://uvadoc.uva.es/oai/request</request><GetRecord><record><header><identifier>oai:uvadoc.uva.es:10324/36734</identifier><datestamp>2025-03-26T19:10:03Z</datestamp><setSpec>com_10324_36327</setSpec><setSpec>com_10324_954</setSpec><setSpec>com_10324_894</setSpec><setSpec>com_10324_1159</setSpec><setSpec>com_10324_931</setSpec><setSpec>col_10324_36329</setSpec><setSpec>col_10324_1310</setSpec></header><metadata><europeana:record xmlns:europeana="http://www.europeana.eu/schemas/ese/" xmlns:confman="org.dspace.core.ConfigurationManager" xmlns:doc="http://www.lyncode.com/xoai" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.europeana.eu/schemas/ese/ http://www.europeana.eu/schemas/ese/ESE-V3.4.xsd">
<dc:title>Magnetostatic Dipolar Energy of Large Periodic Ni fcc Nanowires, Slabs and Spheres</dc:title>
<dc:creator>Cabria Álvaro, Iván</dc:creator>
<dc:subject>Nanomagnetism</dc:subject>
<dc:subject>Nanomagnetismo</dc:subject>
<dc:subject>Magnetostatic dipolar energy</dc:subject>
<dc:subject>Energía dipolar magnetostática</dc:subject>
<dc:subject>Ewald method</dc:subject>
<dc:subject>Método de Ewald</dc:subject>
<dc:description>Producción Científica</dc:description>
<dc:description>The computational effort to calculate the magnetostatic dipolar energy, MDE, of a periodic cell of N magnetic moments&#xd;
is an O(N2) task. Compared with the calculation of the Exchange and Zeeman energy terms, this is the most&#xd;
computationally expensive part of the atomistic simulations of the magnetic properties of large periodic magnetic&#xd;
systems. Two strategies to reduce the computational effort have been studied: An analysis of the traditional Ewald&#xd;
method to calculate the MDE of periodic systems and parallel calculations. The detailed analysis reveals that, for certain&#xd;
types of periodic systems, there are many matrix elements of the Ewald method identical to another elements, due&#xd;
to some symmetry properties of the periodic systems. Computation timing experiments of the MDE of large periodic&#xd;
Ni fcc nanowires, slabs and spheres, up to 32000 magnetic moments in the periodic cell, have been carried out and&#xd;
they show that the number of matrix elements that should be calculated is approximately equal to N, instead of N2/2,&#xd;
if these symmetries are used, and that the computation time decreases in an important amount. The time complexity&#xd;
of the analysis of the symmetries is O(N3), increasing the time complexity of the traditional Ewald method. MDE is&#xd;
a very small energy and therefore, the usual required precision of the calculation of the MDE is so high, about 10−6&#xd;
eV/cell, that the calculations of large periodic magnetic systems are very expensive and the use of the symmetries&#xd;
reduces, in practical terms, the computation time of the MDE in a significant amount, in spite of the increase of the&#xd;
time complexity. The second strategy consists on parallel calculations of the MDE without using the symmetries of&#xd;
the periodic systems. The parallel calculations have been compared with serial calculations that use the symmetries.</dc:description>
<dc:description>Ministerio de Economía, Industria y Competitividad ( grant MAT2014-54378-R)</dc:description>
<dc:description>Junta de Castilla y León (grants VA050U14 and VA124G18)</dc:description>
<dc:date>2019-07-08T12:01:16Z</dc:date>
<dc:date>2019-07-08T12:01:16Z</dc:date>
<dc:date>2019</dc:date>
<dc:type>info:eu-repo/semantics/article</dc:type>
<dc:type>info:eu-repo/semantics/submittedVersion</dc:type>
<dc:identifier>Applied Surface Science, 2019, vol. 490. p. 352-364</dc:identifier>
<dc:identifier>0169-4332</dc:identifier>
<dc:identifier>http://uvadoc.uva.es/handle/10324/36734</dc:identifier>
<dc:identifier>10.1016/j.apsusc.2019.05.307</dc:identifier>
<dc:language>eng</dc:language>
<dc:relation>https://www.sciencedirect.com/science/article/pii/S0169433219316150?via%3Dihub</dc:relation>
<dc:rights>Attribution-NonCommercial-NoDerivatives 4.0 Internacional</dc:rights>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:rights>http://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights>
<dc:rights>© 2019 Elsevier</dc:rights>
<dc:format>application/pdf</dc:format>
<dc:publisher>Elsevier</dc:publisher>
<europeana:object>https://uvadoc.uva.es/bitstream/10324/36734/4/Magnetostatic-dipolar-energy.pdf.jpg</europeana:object>
<europeana:provider>Hispana</europeana:provider>
<europeana:type>TEXT</europeana:type>
<europeana:rights>http://creativecommons.org/licenses/by-nc-nd/4.0/</europeana:rights>
<europeana:dataProvider>UVaDOC. Repositorio Documental de la Universidad de Valladolid</europeana:dataProvider>
<europeana:isShownAt>http://uvadoc.uva.es/handle/10324/36734</europeana:isShownAt>
</europeana:record></metadata></record></GetRecord></OAI-PMH>