Maze Topiary in Supergravity

TL;DR

This paper introduces a unified 'maze' function framework to characterize 1/4-BPS intersecting M2 and M5 brane solutions in supergravity, revealing connections to AdS geometries and black hole entropy without horizons.

Contribution

It presents a novel 'maze' equation for supergravity solutions and explores their relations to AdS spaces, brane probes, and dualities, advancing understanding of black-hole microstates.

Findings

Supergravity solutions are characterized by a single maze function.

Near-brane limits relate to warped AdS3 x S3 x S3 geometries.

Adding momentum charges leads to blackening and BTZ geometries.

Abstract

We show that the supergravity solutions for 1/4-BPS intersecting systems of M2 and M5 branes are completely characterized by a single ``maze'' function that satisfies a non-linear ``maze'' equation similar to the Monge-Amp\`ere equation. We also show that the near-brane limit of certain intersections are $AdS_3 \times S^3 \times S^3$ solutions warped over a Riemann surface, $\Sigma$. There is an extensive literature on these subjects and we construct mappings between various approaches and use brane probes to elucidate the relationships between the M2-M5 and AdS systems. We also use dualities to map our results onto other systems of intersecting branes. This work is motivated by the recent realization that adding momentum to M2-M5 intersections gives a supermaze that can reproduce the black-hole entropy without ever developing an event horizon. We take a step in this direction by adding a certain type of momentum charges that blackens the M2-M5 intersecting branes. The near-brane limit of these solutions is a BTZ$^{extremal} \times S^3 \times S^3 \times \Sigma$ geometry in which the BTZ momentum is a function of the Riemann surface coordinates.