The CFT distance conjecture and tensionless string limits in $$ \mathcal{N} $$ = 2 quiver gauge theories

A bstract We initiate the study of infinite-distance limits on (complex) multi-dimensional conformal manifolds of 4d SCFTs and their bulk interpretation as tensionless-string limits in AdS/CFT. In particular, we focus on 4d $$ \mathcal{N} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>N</mml:mi> </mml:math> = 2 SU quiver gauge theories with hypermultiplets in the bifundamental and fundamental representations. In the overall-free limit, we compute the large- N Hagedorn temperature T H , which governs the stringy exponential growth of the density of states at high energies. We argue that this quantity determines the type of stringy ultraviolet completion in the bulk: it captures the type of string theory in which the bulk physics is embedded while remaining insensitive to detailed geometric data. For linear quivers, we find that T H depends only on the quiver length, which is tied to the number of NS5-branes in the underlying brane construction and, in turn, to the string theory in which the bulk is embedded. For holographic quivers, where we impose that the two central charges a and c coincide in the large- N limit, we show that T H coincides with that of $$ \mathcal{N} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>N</mml:mi> </mml:math> = 4 SYM, which befits the 10d Type IIB description of their gravitational duals. We also analyze the exponential rate α , which controls how the leading tower of higher-spin currents becomes conserved in these limits, as suggested by the CFT Distance Conjecture. In the large- N regime, we derive sharp bounds on the minimal rate, $$ 1/\sqrt{2} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:msqrt> <mml:mn>2</mml:mn> </mml:msqrt> </mml:math> ≤ α min ≤ $$ \sqrt{2/3} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msqrt> <mml:mrow> <mml:mn>2</mml:mn> <mml:mo>/</mml:mo> <mml:mn>3</mml:mn> </mml:mrow> </mml:msqrt> </mml:math> , attained in the overall-free limit. Moreover, we prove that the universal lower bound α ≥ $$ 1/\sqrt{2} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:msqrt> <mml:mn>2</mml:mn> </mml:msqrt> </mml:math> holds, including at finite N . Finally, we go beyond the overall-free ray by characterizing the convex hull of the $$ \overrightarrow{\alpha} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mover> <mml:mi>α</mml:mi> <mml:mo>→</mml:mo> </mml:mover> </mml:math> -vectors that encode the exponential rate of the higher-spin towers along any (partial) weak-coupling limit.

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Journal
Journal of High Energy Physics
Published
2026-04-14
DOI
https://doi.org/10.1007/jhep04(2026)105
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

The CFT distance conjecture and tensionless string limits in $$ \mathcal{N} $$ = 2 quiver gauge theories

Amineh Mohseni, José Calderón-Infante
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

The CFT distance conjecture and tensionless string limits in $$ \mathcal{N} $$ = 2 quiver gauge theories

Amineh Mohseni, José Calderón-Infante
article en

Abstract

A bstract We initiate the study of infinite-distance limits on (complex) multi-dimensional conformal manifolds of 4d SCFTs and their bulk interpretation as tensionless-string limits in AdS/CFT. In particular, we focus on 4d $$ \mathcal{N} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>N</mml:mi> </mml:math> = 2 SU quiver gauge theories with hypermultiplets in the bifundamental and fundamental representations. In the overall-free limit, we compute the large- N Hagedorn temperature T H , which governs the stringy exponential growth of the density of states at high energies. We argue that this quantity determines the type of stringy ultraviolet completion in the bulk: it captures the type of string theory in which the bulk physics is embedded while remaining insensitive to detailed geometric data. For linear quivers, we find that T H depends only on the quiver length, which is tied to the number of NS5-branes in the underlying brane construction and, in turn, to the string theory in which the bulk is embedded. For holographic quivers, where we impose that the two central charges a and c coincide in the large- N limit, we show that T H coincides with that of $$ \mathcal{N} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>N</mml:mi> </mml:math> = 4 SYM, which befits the 10d Type IIB description of their gravitational duals. We also analyze the exponential rate α , which controls how the leading tower of higher-spin currents becomes conserved in these limits, as suggested by the CFT Distance Conjecture. In the large- N regime, we derive sharp bounds on the minimal rate, $$ 1/\sqrt{2} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:msqrt> <mml:mn>2</mml:mn> </mml:msqrt> </mml:math> ≤ α min ≤ $$ \sqrt{2/3} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msqrt> <mml:mrow> <mml:mn>2</mml:mn> <mml:mo>/</mml:mo> <mml:mn>3</mml:mn> </mml:mrow> </mml:msqrt> </mml:math> , attained in the overall-free limit. Moreover, we prove that the universal lower bound α ≥ $$ 1/\sqrt{2} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:msqrt> <mml:mn>2</mml:mn> </mml:msqrt> </mml:math> holds, including at finite N . Finally, we go beyond the overall-free ray by characterizing the convex hull of the $$ \overrightarrow{\alpha} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mover> <mml:mi>α</mml:mi> <mml:mo>→</mml:mo> </mml:mover> </mml:math> -vectors that encode the exponential rate of the higher-spin towers along any (partial) weak-coupling limit.

Journal of High Energy PhysicsVol. 2026(4)
California Institute of Technology (US), Harvard University Press (US)
National Science Foundation, U.S. Department of Energy, Simons Foundation, California Institute of Technology, Aspen Center for Physics, Office of Science, Walter Burke Institute for Theoretical Physics, High Energy Physics
Openalex Percentile: Top 26%
Black Holes and Theoretical Physics
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