Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4512
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dc.contributor.authorBalachandran, A.P.-
dc.contributor.authorDominici, D.-
dc.contributor.authorMarmo, G.-
dc.contributor.authorMukunda, N.-
dc.contributor.authorNilsson, J.-
dc.contributor.authorSamuel, J.-
dc.contributor.authorSudarshan, E.C.G.-
dc.contributor.authorZaccaria, F.-
dc.date.accessioned2012-05-23T03:47:26Z-
dc.date.available2012-05-23T03:47:26Z-
dc.date.issued1982-12-
dc.identifier.citationPhysical Review D, 1982, Vol.26, p3492en
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4512-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractThe problem of separability in recent models of classical relativistic interacting particles is examined. This physical requirement is shown to be more subtle than naive separability of all the constraints defining the system: it is adequate to be able to canonically transform the time-fixing constraints from an unseparated to a separated form when clusters emerge. Viewing separability in this way, and within a specific framework, we are led to a new no-interaction theorem which states the incompatibility of nontrivial interaction with relativistic invariance, separability, and invariant world lines for more than two particles.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1982PhRvD..26.3492Ben
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.26.3492en
dc.rights1982 The American Physical Societyen
dc.titleSeparability in relativistic Hamiltonian particle dynamicsen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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