Bicycling black rings

By Henriette Elvang, Maria J Rodriguez. 2007

147 citations recorded by the source corpus.

We present detailed physics analyses of two different 4+1-dimensional asymptotically flat vacuum black hole solutions with spin in two independent planes: the doubly spinning black ring and the bicycling black ring system (``bi-rings''). The latter is a new solution describing two concentric orthogonal rotating black rings which we construct using the inverse scattering technique. We focus particularly on extremal zero-temperature limits of the solutions. We construct the phase diagram of currently known zero-temperature vacuum black hole solutions with a single event horizon, and discuss the non-uniqueness introduced by more exotic black hole configurations such as bi-rings and multi-ring saturns.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/81306c2527fd454ddb9c61b46559e89bc17971b7

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

In Statistical and Nonlinear Physics

Citations in the corpus

CFT Duals for Extreme Black Holes (2008, background): “There are also many five-dimensional black holes with non-trivial horizon topology, including the Myers-Perry black hole, black rings, and black saturns [30–36], that have Rt ×U(1)2 spacetime symmetry.”
Black Holes in Higher Dimensions (2008, methodology): “An analysis of the physical properties of the solution, and in particular the phase space has been presented in [60].”
The Phase Structure of Higher-Dimensional Black Rings and Black Holes (2007, background): “[4, 5, 6]. The latter have been constructed using inverse-scattering techniques [7, 8, 9, 10], which have also yielded a black ring solution and multi-black rings with two independent angular momenta [11, 12]. There exist furthermore algebraic classiﬁcations of spacetimes [13, 14, 15, 16], and theor”