Observable consequences of dynamical compactification in Kaluza-Klein cosmology

Details Observable consequences of dynamical compactification in Kaluza-Klein cosmology Observable consequences of dynamical compactification in Kaluza-Klein cosmology

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phlb..150..107k&link_type=abstract

Physics Letters B, Volume 150, Issue 1-3, p. 107-112.

Physics

20

Scientific paper

Time variation of the compactified size of the extra small space is inevitable in Kaluza-Klein type of theories. This can generate observable remmants of ultrahigh energy cosmic rays that have an enhanced spectrum around 1019-1025 eV. This and other consequences of the time variation are closely examined in a model that realizes compactification via the gravitational Casimir energy.

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