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dc.contributor.authorBHATKAR, SAYALI ATULen_US
dc.date.accessioned2021-07-23T10:25:20Z
dc.date.available2021-07-23T10:25:20Z
dc.date.issued2021-06en_US
dc.identifier.citationPhysical Review D, 103(12), 125026.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/6077
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.103.125026en_US
dc.description.abstractRecently it was shown that classical electromagnetism admits new asymptotic conservation laws [, New asymptotic conservation laws for electromagnetism, J. High Energy Phys. 02 (2021) 082.]. In this paper we derive the analog of the first of these asymptotic conservation laws upon the imposing Feynman boundary condition on the radiative field. We also show that the Feynman solution at O(e3) contains purely imaginary modes falling off as {loguunr,n≥0} which are absent in the retarded solution. The logu mode has also appeared [ and , Loop corrected soft photon theorem as a Ward identity, J. High Energy Phys. 10 (2019) 287; , Ward identity for loop level soft photon theorem for massless QED coupled to gravity, J. High Energy Phys. 10 (2020) 110.] and violates the Ashtekar-Struebel falloffs for the radiative field [ and , Symplectic geometry of radiative modes and conserved quantities at null infinity, Proc. R. Soc. A 376, 585 (1981).]. We expect that new (logu)mumr modes would appear in the Feynman solution at order O(e2m+1). Thus, all the other modes are expected to preserve the Ashtekar-Struebel falloffs.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectScatteringen_US
dc.subjectPhotonsen_US
dc.subject2021-JUL-WEEK3en_US
dc.subjectTOC-JUL-2021en_US
dc.subject2021en_US
dc.titleAsymptotic conservation law with Feynman boundary conditionen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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