Interacting non-BPS black holes
arXiv:1106.5806 · doi:10.1007/s10714-011-1256-9
Abstract
We explain how to exploit systematically the structure of nilpotent orbits to obtain a solvable system of equations describing extremal solutions of (super-)gravity theories, i.e. systems that can be solved in a linear way. We present the procedure in the case of the STU model, where we show that all extremal solutions with a flat three-dimensional base are fully described with the help of three different nilpotent orbits: the BPS, the almost-BPS and the composite non-BPS. The latter describes a new class of solutions for which the orientation of half of the constituent branes have been inverted with respect to the BPS one, such that all the centres are intrinsically non-BPS, and interact with each others. We finally recover explicitly the ensemble of the almost-BPS solutions in our formalism and present an explicit two-centre solution of the new class.
49 pages
References in corpus (18)
- Black Hole Microstates and Attractor Without Supersymmetry
- Microstates of a Neutral Black Hole in M Theory
- Non-Supersymmetric Attractor Flow in Symmetric Spaces
- Universal BPS structure of stationary supergravity solutions
- First Order Description of Black Holes in Moduli Space
- Almost BPS black holes
- U-duality and non-BPS solutions
- First-order flow equations for extremal and non-extremal black holes
- Multi-Center non-BPS Black Holes - the Solution
- Non-extremal black holes of N=2, d=4 supergravity
- First order flows for N=2 extremal black holes and duality invariants
- Constituent Model of Extremal non-BPS Black Holes
- Extremal solutions of the S3 model and nilpotent orbits of G2(2)
- First-order flows and stabilisation equations for non-BPS extremal black holes
- Moduli and (un)attractor black hole thermodynamics
- Exact Solutions and the Attractor Mechanism in Non-BPS Black Holes
- A Black Ring with two Angular Momenta in Taub-NUT
- On the symmetry orbits of black holes in non-linear sigma models
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- Spherically Symmetric Solutions in Higher-Derivative Gravity
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- Non-extremal Black Hole Microstates: Fuzzballs of Fire or Fuzzballs of Fuzz ?
- The black-hole/qubit correspondence: an up-to-date review
- Subtracted Geometry From Harrison Transformations
- Black Holes Lessons from Multipole Ratios
- Gravitational Footprints of Black Holes and Their Microstate Geometries
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- Metastable Supertubes and non-extremal Black Hole Microstates
- Bolting Multicenter Solutions
- Ungauging black holes and hidden supercharges
- Hair in the Back of a Throat: Non-Supersymmetric Multi-Center Solutions from Kähler Manifolds
- Duality covariant non-BPS first order systems
- Non-supersymmetric Microstates of the MSW System
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- Freudenthal Dual Lagrangians
- On Extremal Limits and Duality Orbits of Stationary Black Holes
- New Supersymmetric Bubbles on AdS_3xS^3
- Extremal Limits of Rotating Black Holes
- Black hole solutions to the -model and their orbits (I)
- New instability of non-extremal black holes: spitting out supertubes
- Extremal Multicenter Black Holes: Nilpotent Orbits and Tits Satake Universality Classes
- Geroch Group Description of Black Holes
- Duality covariant multi-centre black hole systems
- Phases of non-extremal multi-centered bound states
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- Black holes and equivariant charge vectors in N=2,d=4 supergravity
- Corrugated Multi-Supersheets
- Nilpotent orbits in real symmetric pairs and stationary black holes
- Linearizing the BPS Equations with Vector and Tensor Multiplets
- Black holes and general Freudenthal transformations
- Black hole solutions of N=2, d=4 supergravity with a quantum correction, in the H-FGK formalism
- Black Holes and Fourfolds
- Stationary Black Holes in Supergravity: The Issue of Real Nilpotent Orbits
- non-BPS walls of marginal stability
- Multi-Centered Black Hole Flows
- Non-perturbative black holes in Type-IIA String Theory vs. the No-Hair conjecture
- Geroch Group Description of Bubbling Geometries
- Non-extremal and non-BPS extremal five-dimensional black strings from generalized special real geometry
- Multi-Centered First Order Formalism
- Multi-Centered Invariants, Plethysm and Grassmannians
- On Symmetries of Extremal Black Holes with One and Two Centers