[
    {
        "id": "authors:y4ztg-hcf39",
        "collection": "authors",
        "collection_id": "y4ztg-hcf39",
        "cite_using_url": "https://authors.library.caltech.edu/records/y4ztg-hcf39",
        "type": "article",
        "title": "The CFT distance conjecture and tensionless string limits in N = 2 quiver gauge theories",
        "author": [
            {
                "family_name": "Calder\u00f3n-Infante",
                "given_name": "Jos\u00e9",
                "orcid": "0000-0002-9057-1012",
                "clpid": "Calderon-Infante-Jose"
            },
            {
                "family_name": "Mohseni",
                "given_name": "Amineh",
                "orcid": "0000-0002-3967-2854"
            }
        ],
        "abstract": "<p class=\"MsoNormal\">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&nbsp;N&nbsp;= 2&nbsp;<em>SU</em>&nbsp;quiver gauge theories with hypermultiplets in the bifundamental and fundamental representations. In the overall-free limit, we compute the large-<em>N</em>&nbsp;Hagedorn temperature&nbsp;<em>T<sub>H</sub></em>, 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&nbsp;<em>T<sub>H</sub></em>&nbsp;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&nbsp;<em>a</em>&nbsp;and&nbsp;<em>c</em>&nbsp;coincide in the large-<em>N</em>&nbsp;limit, we show that&nbsp;<em>T<sub>H</sub></em>&nbsp;coincides with that of&nbsp;N&nbsp;= 4 SYM, which befits the 10d Type IIB description of their gravitational duals. We also analyze the exponential rate&nbsp;<em>&alpha;</em>, 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-<em>N</em>&nbsp;regime, we derive sharp bounds on the minimal rate,&nbsp;1/<span class=\"st\"><span>&radic;2 </span></span>&le;&nbsp;<em>&alpha;</em><sub>min</sub>&nbsp;&le;, <span class=\"st\"><span>&radic;2/3 </span></span>attained in the overall-free limit. Moreover, we prove that the universal lower bound&nbsp;<em>&alpha;</em>&nbsp;&ge;&nbsp;1/<span class=\"st\"><span>&radic;2 </span></span>holds, including at finite&nbsp;<em>N</em>. Finally, we go beyond the overall-free ray by characterizing the convex hull of the&nbsp;&alpha;<span>&rarr;</span>-vectors that encode the exponential rate of the higher-spin towers along any (partial) weak-coupling limit.</p>",
        "doi": "10.1007/jhep04(2026)105",
        "issn": "1029-8479",
        "publisher": "Springer Science and Business Media LLC",
        "publication": "Journal of High Energy Physics",
        "publication_date": "2026-04",
        "series_number": "4",
        "volume": "2026",
        "issue": "4",
        "pages": "105"
    }
]