We study the solutions to the N=2, d=4 Attractor Equations in a dyonic, extremal, static, spherically symmetric and asymptotically flat black hole background, in the simplest case of perturbative quantum corrected cubic Special Kahler geometry consistent with continuous axion-shift symmetry, namely in the 1-modulus Special Kahler geometry described (in a suitable special symplectic coordinate) by the holomorphic Kahler gauge-invariant prepotential F=t^3+i*lambda, with lambda real. By performing computations in the ``magnetic'' charge configuration, we find evidence for interesting phenomena (absent in the classical limit of vanishing lambda). Namely, for a certain range of the quantum parameter lambda we find a ``splitting'' of attractors, ...
We compute the effective black hole potential V of the most general N=2, d=4 (local) special Kaehler...
We review and extend results on higher-curvature corrections to different configurations describing ...
Non-extremal black holes in (Formula presented.) supergravity have two horizons, the geometric mean ...
We study the critical points of the black hole scalar potential $V_{BH}$ in N=2, d=4 supergravity co...
AbstractWe study N=2, d=4 attractor equations for the quantum corrected two-moduli prepotential F=st...
Motivated by the interpretation of the Ooguri-Strominger-Vafa conjecture as a holographic correspond...
We study N=2, d=4 attractor equations for the quantum corrected two-moduli prepotential $\mathcal{F}...
AbstractWe study the “flat” directions of non-BPS extremal black hole attractors for N=2, d=4 superg...
We consider extremal black hole attractors (both BPS and non-BPS) for N=3 and N=5 supergravity in d=...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with ...
We report on recent advances in the study of critical points of the ``black hole effective potential...
We consider attractor varieties arising in the construction of dyonic black holes in Calabi-Yau comp...
We construct finite mass, asymptotically flat black hole solutions in d = 5 Einstein– Yang-Mills–Che...
In this paper we study spherically symmetric single-centered attractors in N = 2 $$ \mathcal{N}=2 $$...
These lectures provide a pedagogical, introductory review of the so-called Attractor Mechanism (AM) ...
We compute the effective black hole potential V of the most general N=2, d=4 (local) special Kaehler...
We review and extend results on higher-curvature corrections to different configurations describing ...
Non-extremal black holes in (Formula presented.) supergravity have two horizons, the geometric mean ...
We study the critical points of the black hole scalar potential $V_{BH}$ in N=2, d=4 supergravity co...
AbstractWe study N=2, d=4 attractor equations for the quantum corrected two-moduli prepotential F=st...
Motivated by the interpretation of the Ooguri-Strominger-Vafa conjecture as a holographic correspond...
We study N=2, d=4 attractor equations for the quantum corrected two-moduli prepotential $\mathcal{F}...
AbstractWe study the “flat” directions of non-BPS extremal black hole attractors for N=2, d=4 superg...
We consider extremal black hole attractors (both BPS and non-BPS) for N=3 and N=5 supergravity in d=...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with ...
We report on recent advances in the study of critical points of the ``black hole effective potential...
We consider attractor varieties arising in the construction of dyonic black holes in Calabi-Yau comp...
We construct finite mass, asymptotically flat black hole solutions in d = 5 Einstein– Yang-Mills–Che...
In this paper we study spherically symmetric single-centered attractors in N = 2 $$ \mathcal{N}=2 $$...
These lectures provide a pedagogical, introductory review of the so-called Attractor Mechanism (AM) ...
We compute the effective black hole potential V of the most general N=2, d=4 (local) special Kaehler...
We review and extend results on higher-curvature corrections to different configurations describing ...
Non-extremal black holes in (Formula presented.) supergravity have two horizons, the geometric mean ...