arXiv subjects

Sébastien Reymond

Publications and source records attributed to Sébastien Reymond.

3 recordsLinked to original sources

arXiv2026

The IKKT renormalization group flow is IIB: toward zero-d holography

Supergravity solutions describing stacks of D$p$-branes with $p\neq 3$ feature a non-constant dilaton profile, which is holographically mapped to the running of the SYM coupling in $(p+1)$ dimensions. For D-instantons ($p=-1$), the lack of space and time in the IKKT matrix model makes such an interpretation difficult at first. In this letter, we propose a method to achieve this based on two closely related concepts: the IKKT method of integrating out heavy strings in a Coulomb branch vacuum and the matrix RG flow of Brézin and Zinn-Justin (BZJ). The notable difference between the two is that the BZJ RG flow also integrates over the Coulomb branch position. We first apply the Coulomb branch method and by relating the coefficient of the leading correction to the IKKT action with the string coupling, we can compute its dependence on the Coulomb branch position, finding a match between matrix theory and supergravity. Next, we apply the BZJ-flow to the IKKT partition function, which leads to a running of the coupling constant $g$ with the rank $N$ of the matrix model, reproducing the $N$-dependence of the axio-dilaton field in supergravity.

hep-th↗

arXiv2025

Black Holes, Moduli Stabilisation and the Swampland

In theories with moduli, extremal black holes behave such that for generic initial conditions, the distance traveled by the scalars from infinity to the horizon can grow with the size of the black hole. This, in turn, implies that larger black holes can probe more of the UV ingredients of the theory, in contrast with (naive) EFT expectations. We relate this discrepancy to the lack of cosmological moduli stabilisation. Indeed, for would-be scale-separated string vacua with parametrically heavy stabilised scalars -- dubbed \emph{rigid} compactifications -- one recovers the EFT intuition where only small black holes probe the UV. We make this explicit in a toy model and then turn to top-down models and construct near-horizon solutions in IIA scale-separated compactifications with stabilised moduli. In these top-down models we still observe large field variations for large black holes which can be traced back to the absence of parametrically heavy moduli. We are led to speculate that needing UV physics to allow for non-local effects near the horizon of large black holes is at odds with having a rigid compactification, hinting to the possibility that such compactifications are in the Swampland.

hep-th↗

arXiv2025

Supergravity solutions for D$p$-D$(6-p)$ bound states: from $p=7$ to $p=-1$

Near horizon geometries of D$p$-branes with $p\neq 3$ are singular with a running dilaton. Bound states of D$p$ branes with their magnetic cousins, D$(6-p)$ branes, can stabilise the dilaton such that an AdS factor might appear in the near horizon region, potentially leading to a chain of AdS vacua of the form $AdS_{p+2}\times S^{p+2} \times \mathbb{T}^{6-2p}$. The solutions with $p=-1, 1, 3$ are supersymmetric with the cases $p=1, 3$ being well-known examples already. We construct the explicit (partially smeared) brane bound state solutions for all such configurations where the cases $p=-1,2$ are entirely novel and we find no AdS geometry for these. The two novel classes of solutions feature ghost branes (negative tension branes), and we suggest they are physical for the D$(-1)-$D$7$ solutions but unphysical for the D$2-$D$4$ solutions. The bound state of a D$(-1)$ and a D7 brane in supergravity was only hinted upon recently in \cite{Aguilar-Gutierrez:2022kvk} and here we correct the solution in order to preserve supersymmetry and find that the dilaton can indeed be stabilised which indicates there could be a holographic dual matrix theory which generalises the IKKT matrix model to allow for conformal invariance.

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