English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We derive a stationary and axisymmetric black hole solution inEinstein-Dilaton-Gauss-Bonnet gravity to quadratic order in the ratio of thespin angular momentum to the black hole mass squared. This solution introducesnew corrections to previously found nonspinning and linear-in-spin solutions.The location of the event horizon and the ergosphere are modified, as well asthe quadrupole moment. The new solution is of Petrov type I, although lowerorder in spin solutions are of Petrov type D. There are no closed timelikecurves or spacetime regions that violate causality outside of the event horizonin the new solution. We calculate the modifications to the binding energy,Kepler's third law, and properties of the innermost stable circular orbit.These modifications are important for determining how the electromagneticproperties of accretion disks around supermassive black holes are changed fromthose expected in general relativity.

Slowly-Rotating Black Holes in Einstein-Dilaton-Gauss-Bonnet Gravity: Quadratic Order in Spin Solutions