Attractor Mechanism and Charge-Only Entropy
For a regular extremal black hole, scalar fields can flow from arbitrary asymptotic moduli to charge-determined horizon values. The entropy is then independent of continuous asymptotic moduli within the same basin of attraction. Existence of a critical point, regularity, and the distinction between single- and multicenter solutions remain essential hypotheses.
Required background. BPS Indices, Absolute Degeneracies, and Wall Crossing supplies chamber dependence; BPS Particles and Central Charges supplies the central charge.
Helpful background. Charge Lattices, Duality Frames, and Local Systems fixes symplectic charge conventions; Black-Hole Thermodynamics at the QFT Interface supplies the entropy interpretation.
Radial flow and the black-hole potential
Section titled “Radial flow and the black-hole potential”For a static extremal solution reduced to one radial dimension, scalar dynamics can be written schematically as
The charge vector enters the black-hole potential. In four-dimensional supergravity,
A BPS attractor obeys , so the horizon values extremize and
in units . Ferrara, Kallosh, and Strominger established this fixed-point behavior for supersymmetric black holes Ferrara, Kallosh, and Strominger 1995.
First application: a two-charge dilaton attractor
Section titled “First application: a two-charge dilaton attractor”Consider a normalization in which one scalar has effective potential
The attractor equation gives
and hence
The asymptotic value has disappeared. Both charges must be nonzero: if or , the putative extremum runs to infinite distance and the two-derivative horizon is singular. The example therefore displays both charge-only entropy and its regularity condition.
Basins, multicenters, and corrections
Section titled “Basins, multicenters, and corrections”Several critical points may exist for the same charge, with distinct basins and entropies. A total charge can also support multicenter configurations whose existence depends on asymptotic moduli through integrability conditions. The single-center attractor entropy may remain charge-only while the total indexed spectrum jumps across walls.
Higher-derivative interactions replace the area formula by an entropy-function or Noether-charge extremization. Sen’s entropy function makes the charge-fixed variational problem explicit and remains applicable beyond supersymmetry when a regular extremal near-horizon solution exists Sen 2005.
Adversarial control: charges without an attractor
Section titled “Adversarial control: charges without an attractor”Choose charges for which has no finite positive critical point, as in the one-charge limit above. There is then no regular single-center two-derivative horizon, so inserting the charges into a formal entropy expression is invalid. Alternatively, cross a wall where a multicenter bound state disappears; the single-center attractor can persist while the total microscopic index changes.
Thus “charge-only” means independence from continuous asymptotic moduli inside a specified regular attractor basin. It does not mean that every charge vector has a black hole, that multicenter sectors are irrelevant, or that quantum corrections are absent.
The chapter overview contains the structure diagram and validity and failure diagram. They are embedded there once so that their shared chapter-level context is not repeated on every article.
For the chapter-wide comparison of assumptions, counterevidence, falsifiers, and claim ceilings, see the claim-domain table.
References
Section titled “References”- Ferrara, Sergio, Renata Kallosh, and Andrew Strominger. “ Extremal Black Holes.” Physical Review D 52, R5412–R5416 (1995). DOI. Open PDF.
- Sen, Ashoke. “Black Hole Entropy Function and the Attractor Mechanism in Higher Derivative Gravity.” Journal of High Energy Physics 2005, 9 (2005): 038. DOI. Open PDF.