Open Access

Table A.1.

Characteristic radii.

Kerr Dilaton Match
rISCO = 2M(B+B2+B3)

Notes. Kerr and dilaton balck hole event horizon (EH), equatorial photon sphere (PS), and innermost stable circular orbit (ISCO). The right column lists the dilaton parameter in relation to the Kerr spin a required to have the two black hole systems matched at the respective radius. Parameters B, C, Z1, Z2, and σ are reported in Appendix A. All expressions are taken from the supplemental material from Mizuno et al. (2018).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.