Rotating boson star as an effective mass torus in general relativity

Details Rotating boson star as an effective mass torus in general relativity Rotating boson star as an effective mass torus in general relativity

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phla..249..389s&link_type=abstract

Physics Letters A, Volume 249, Issue 5-6, p. 389-394.

Physics

20

Scientific paper

Scalar fields bounded by their own gravitational field can form absolutely stable boson stars, resembling neutron stars. Within general relativity, we construct for the first time the corresponding differentially rotating, localized configurations via numerical integration. The ratio of conserved angular momentum and particle number turns out to be an integer a. The resulting axisymmetric metric, the energy density and the Tolman mass are completely regular.

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