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dc.contributor.authorMashhoon, Bahrameng
dc.date.issued2000eng
dc.descriptionhttp://arxiv.org/abs/gr-qc/0003014eng
dc.description.abstractThe theory of measurement is employed to elucidate the physical basis of general relativity. For measurements involving phenomena with intrinsic length or time scales, such scales must in general be negligible compared to the (translational and rotational) scales characteristic of the motion of the observer. Thus general relativity is a consistent theory of coincidences so long as these involve classical point particles and electromagnetic rays (geometric optics). Wave optics is discussed and the limitations of the standard theory in this regime are pointed out. A nonlocal theory of accelerated observers is briefly described that is consistent with observation and excludes the possibility of existence of a fundamental scalar field in nature.eng
dc.identifier.citationarXiv:gr-qc/0003014v1eng
dc.identifier.urihttp://hdl.handle.net/10355/8615eng
dc.languageEnglisheng
dc.publisherarXiveng
dc.relation.ispartofcollectionUniversity of Missouri--Columbia. College of Arts and Sciences. Department of Physics and Astronomy. Physics and Astronomy publicationseng
dc.subject.lcshBlack holes (Astronomy)eng
dc.subject.lcshRelativity (Physics)eng
dc.subject.lcshQuantum cosmologyeng
dc.titleMeasurement Theory and General Relativityeng
dc.typeArticleeng


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