N2 HOMO-1 orbital cross section revealed through high-order-harmonic generation

dc.citation.doi10.1103/PhysRevA.95.033419
dc.citation.issn2469-9926
dc.citation.issue3
dc.citation.jtitlePhysical Review A
dc.citation.volume95
dc.contributor.authorTroß, Jan
dc.contributor.authorRen, Xiaoming
dc.contributor.authorMakhija, Varun
dc.contributor.authorMondal, Sudipta
dc.contributor.authorKumarappan, Vinod
dc.contributor.authorTrallero-Herrero, Carlos A.
dc.date.accessioned2023-12-07T22:35:31Z
dc.date.available2023-12-07T22:35:31Z
dc.date.issued2017-03-20
dc.date.published2017-03-20
dc.description.abstractWe measure multi-orbital contributions to high harmonic generation from aligned nitrogen. We show that the change in revival structure in the cutoff harmonics has a counterpart in the angular distribution when a lower-lying orbital contributes to the harmonic yield. This angular distribution is directly observed in the laboratory without any further deconvolution. Because of the high degree of alignment we are able to distinguish angular contributions of the highest occupied molecular orbital 1 (HOMO-1) orbital from angle-dependent spectroscopic features of the HOMO. In particular, we are able to make a direct comparison with the cross section of the HOMO-1 orbital in the extreme ultraviolet region.
dc.identifier.urihttps://hdl.handle.net/2097/44005
dc.relation.urihttps://link.aps.org/doi/10.1103/PhysRevA.95.033419
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dc.titleN2 HOMO-1 orbital cross section revealed through high-order-harmonic generation
dc.typeText

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