Open strings and heterotic instantons

Motivated by closed string perturbation theory arguments by S. Shenker, we consider non-perturbative effects of characteristic strength O ( e − 1 / g s ) , with g s the closed string coupling constant, in supersymmetric critical heterotic string theories. We argue that in 10D such effects arise from heterotic “D-instantons,” i.e. heterotic disk diagrams, whose existence relies on a non-trivial interplay between worldsheet and spacetime degrees of freedom. In compactifications of the SemiSpin(32) heterotic string, we argue that similar effects can arise from wrapped Euclidean non-BPS “D-strings.” Two general principles arise: The first is that the consistency of those heterotic branes on which the fundamental string can end relies on an inflow mechanism for spacetime degrees of freedom. The second is that Shenker’s argument, taken to its logical conclusion, implies that all closed string theories must exhibit open strings as well.

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Publication Details

Journal
Physics Letters B
Published
2025-11-20
DOI
https://doi.org/10.1016/j.physletb.2025.140037
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Open strings and heterotic instantons

Rafael Álvarez‐García, Jacob M. Leedom, Christian Kneißl, Nicole Righi
Physics Letters B
Black Holes and Theoretical Physics
article

Open strings and heterotic instantons

Rafael Álvarez‐García, Jacob M. Leedom, Christian Kneißl, Nicole Righi
article en

Abstract

Motivated by closed string perturbation theory arguments by S. Shenker, we consider non-perturbative effects of characteristic strength O ( e − 1 / g s ) , with g s the closed string coupling constant, in supersymmetric critical heterotic string theories. We argue that in 10D such effects arise from heterotic “D-instantons,” i.e. heterotic disk diagrams, whose existence relies on a non-trivial interplay between worldsheet and spacetime degrees of freedom. In compactifications of the SemiSpin(32) heterotic string, we argue that similar effects can arise from wrapped Euclidean non-BPS “D-strings.” Two general principles arise: The first is that the consistency of those heterotic branes on which the fundamental string can end relies on an inflow mechanism for spacetime degrees of freedom. The second is that Shenker’s argument, taken to its logical conclusion, implies that all closed string theories must exhibit open strings as well.

Physics Letters BVol. 872
Universität Hamburg (DE), King's College London (GB), Deutsches Elektronen-Synchrotron DESY (DE), Max Planck Institute for Physics (DE)
Openalex Percentile: Top 84%
Black Holes and Theoretical Physics
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Open strings and heterotic instantons — Rafael Álvarez‐García, Jacob M. Leedom, et al. · Physics Letters B (2025) | TGRS Research Map | TGRS