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<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Flavor symmetries and automatic enhancement in the 6D supergravity swampland</dc:title><dc:creator>Cvetič,	Mirjam	(Avtor)
	</dc:creator><dc:creator>Lin,	Ling	(Avtor)
	</dc:creator><dc:creator>Turner,	Andrew P.	(Avtor)
	</dc:creator><dc:subject>supergravity theories</dc:subject><dc:subject>supersymmetric strings</dc:subject><dc:subject>quantum gravity constraints</dc:subject><dc:subject>Gauge theories</dc:subject><dc:subject>Higher-dimensional field theories</dc:subject><dc:subject>strings &amp; branes</dc:subject><dc:subject>supergravity</dc:subject><dc:subject>symmetries</dc:subject><dc:description>We argue for the quantum-gravitational inconsistency of certain 6D N ¼ ð1; 0Þ supergravity theories, whose anomaly-free gauge algebra g and hypermultiplet spectrum M were observed by Raghuram et al. [J. High Energy Phys. 07 (2021) 048] to be realizable only as part of a larger gauge sector ðg0 ⊃ g; M0 ⊃ MÞ in F-theory. To detach any reference to a string theoretic method of construction, we utilize flavor symmetries to provide compelling reasons why the vast majority of such ðg; MÞ theories are not compatible with quantum gravity constraints, and how the “automatic enhancement” to ðg0 ; M0 Þ remedies this. In the first class of models, with g0 ¼ g ⊕ h, we show that there exists an unbroken flavor symmetry h acting on the matter M, which, if ungauged, would violate the no-global-symmetries hypothesis. This argument also applies to 1-form center symmetries, which govern the gauge group topology and massive states in representations different from those of massless states. In a second class, we find that g is incompatible with the flavor symmetry of certain supersymmetric strings that must exist by the completeness hypothesis.</dc:description><dc:publisher>APS</dc:publisher><dc:date>2022</dc:date><dc:date>2023-09-25 09:54:39</dc:date><dc:type>Znanstveno delo</dc:type><dc:identifier>85991</dc:identifier><dc:identifier>UDK: 530.145</dc:identifier><dc:identifier>COBISS_ID: 136975875</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevD.105.046005</dc:identifier><dc:identifier>ISSN pri članku: 2470-0029</dc:identifier><dc:language>sl</dc:language></metadata>
