Positive Spin-induced Quadrupole Moment in String Theory
Iosif Bena, Angèle Lochet
TL;DR
The study addresses whether string-theory microstate geometries can realize a positive spin-induced quadrupole moment distinct from Kerr. It develops rotating Running-Kerr-Taub-Bolt solutions on an Euclidean-Kerr-Taub-Bolt base with self-dual fluxes, then reduces to four-dimensional asymptotically flat spacetimes and computes the multipole moments using ACMC coordinates; the results show $M_2>0$ for small running and possible sign flips as the rotation parameter grows, with $M_2$ diverging near $|oldsymbol{eta}| o 1$. The work provides an infinite family of regular, horizonless, rotating five-dimensional solutions parameterized by an integer $p$, along with explicit expressions for charges, angular momenta, and higher multipoles, and establishes the Taub-NUT/SUSY limits as cross-checks. This demonstrates a concrete string-theoretic mechanism for positive quadrupole moments in spinning objects, linked to the presence of nontrivial topology and fluxes, and lays groundwork for exploring duality-related families and multi-bubble configurations with potential connections to black-hole physics.
Abstract
We identify singularity-free Running-Kerr-Taub-Bolt solutions of eleven-dimensional supergravity that descend to four-dimensional rotating solutions with flat-space asymptotics. We compute their spin-induced quadrupole moment and find that for a certain range of charges this quadrupole moment is positive. This behavior differs from the Kerr black hole and from most other spinning objects constructed with ``normal'' four-dimensional matter, and we discuss the top-down physics of these solutions that could be responsible for this unusual behavior.
