Cosmological black holes are coloured too

Details Cosmological black holes are coloured too Cosmological black holes are coloured too

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phlb...79..340a&link_type=abstract

Physics Letters B, Volume 79, Issue 3, p. 340-342.

Physics

Scientific paper

A new solution of the Einstein-Yang-Mills system with axial symmetry and cosmological constant is given here. This new metric, which in the absence of matter becomes the de Sitter universe, is the natural generalization of both a recent result of Perry for stellar (asymptotically flat) black holes and a well-knwn family of solutions of the Einstein-Maxwell system with nonvanishing cosmological constant given some time ago by Carter. Calculations have been carried out making extensive use of the coordinates found by Plebanski.

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