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               <dc:title>The imaginary part of the high-harmonic cutoff</dc:title>
               <dc:creator>Pisanty, Emilio</dc:creator>
               <dc:creator>Ciappina, Marcelo F.</dc:creator>
               <dc:creator>Lewenstein, Maciej</dc:creator>
               <dc:subject>Àrees temàtiques de la UPC::Física</dc:subject>
               <dc:subject>Radiation</dc:subject>
               <dc:subject>high-harmonic generation</dc:subject>
               <dc:subject>Radiació</dc:subject>
               <dc:description>High-harmonic generation   the emission of high-frequency radiation by the ionization and&#xd;
subsequent recombination of an atomic electron driven by a strong laser  eld   is widely understood&#xd;
using a quasiclassical trajectory formalism, derived from a saddle-point approximation, where&#xd;
each saddle corresponds to a complex-valued trajectory whose recombination contributes to the&#xd;
harmonic emission. However, the classi cation of these saddle points into individual quantum&#xd;
orbits remains a high-friction part of the formalism. Here we present a scheme to classify these&#xd;
trajectories, based on a natural identi cation of the (complex) time that corresponds to the&#xd;
harmonic cuto . This identi cation also provides a natural complex value for the cuto  energy,&#xd;
whose imaginary part controls the strength of quantum-path interference between the quantum&#xd;
orbits that meet at the cuto . Our construction gives an e cient method to evaluate the location&#xd;
and brightness of the cuto  for a wide class of driver waveforms by solving a single saddle-point&#xd;
equation. It also allows us to explore the intricate topologies of the Riemann surfaces formed by&#xd;
the quantum orbits induced by nontrivial waveforms.</dc:description>
               <dc:description>Peer Reviewed</dc:description>
               <dc:description>Postprint (published version)</dc:description>
               <dc:date>2020-07-22</dc:date>
               <dc:type>Article</dc:type>
               <dc:relation>https://iopscience.iop.org/article/10.1088/2515-7647/ab8f1e</dc:relation>
               <dc:relation>FIS2016-79508-P</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/MINECO//SEV-2015-0522/ES/AGR-INSTITUTO DE CIENCIAS FOTONICAS/</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/EC/H2020/833801/EU/NOvel Quantum simulators – connectIng Areas/NOQIA</dc:relation>
               <dc:relation>IU16-011424</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PCI2019-111828-2/ES/SIMULADOR CUANTICO DE ATOMO MAGNETICO/</dc:relation>
               <dc:relation>10.13039</dc:relation>
               <dc:relation>501100011033</dc:relation>
               <dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/es/</dc:rights>
               <dc:rights>Open Access</dc:rights>
               <dc:rights>Attribution-NonCommercial-NoDerivs 3.0 Spain</dc:rights>
               <dc:publisher>IOP</dc:publisher>
            </oai_dc:dc>
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