<?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>2026-07-29T09:33:04Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/137005" metadataPrefix="marc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/137005</identifier><datestamp>2026-05-29T00:19:11Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><record xmlns="http://www.loc.gov/MARC21/slim" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/MARC21/slim http://www.loc.gov/standards/marcxml/schema/MARC21slim.xsd">
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      <subfield code="a">Fernández Álvarez-Estrada, Ramón</subfield>
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      <subfield code="a">Pastor, I.</subfield>
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      <subfield code="a">Roso, L.</subfield>
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      <subfield code="a">Castejon, F.</subfield>
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      <subfield code="c">2023-12-13</subfield>
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      <subfield code="a">Motivated by the renewed interest due to the presently available extreme light sources, the dynamics of a single classical relativistic (spinless) extended electron interacting with a classical electromagnetic field (an incoming radiation and the field radiated by the electron) is revisited. The field is treated in Lorentz gauge, with the Lorentz condition. By assumption, there is a crucial finite cut-off kmax on the magnitude of any wavevector contributing to the field (preventing a point electron) and, for a simple formulation, the initial conditions for particle and fields are given in the infinitely remote past. In an infinite three-dimensional vacuum and in an inertial system, Hamilton’s dynamical equations for the particle and the complex field amplitudes acting as canonical variables (a's) yield an exact Lorentz force equation for the former, that includes the incoming radiation and an exact radiation reaction force FRR due to the field radiated by the electron. Uniform motion is obtained as a test of consistency. Based upon numerical computations, some approximations on FRR are given. A covariant formulation is also presented.</subfield>
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      <subfield code="a">R F Álvarez-Estrada et al 2023 J. Phys. Commun. 7 125001</subfield>
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      <subfield code="a">2399-6528</subfield>
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      <subfield code="a">10.1088/2399-6528/ad1049</subfield>
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      <subfield code="a">https://hdl.handle.net/20.500.14352/137005</subfield>
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      <subfield code="a">https//doi.org/10.1088/2399-6528/ad1049</subfield>
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      <subfield code="a">https://iopscience.iop.org/article/10.1088/2399-6528/ad1049</subfield>
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      <subfield code="a">Classical relativistic electron-field dynamics: Hamiltonian approach to radiation reaction</subfield>
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