Non-supersymmetric AdS6 and the swampland

被引:19
作者
Apruzzi, Fabio [1 ,2 ]
De Luca, G. Bruno [3 ]
Lo Monaco, Gabriele [4 ,5 ]
Uhlemann, Christoph F. [6 ]
机构
[1] Univ Oxford, Math Inst, Andrew Wiles Bldg,Woodstock Rd, Oxford OX2 6GG, England
[2] Univ Bern, Albert Einstein Ctr Fundamental Phys, Inst Theoret Phys, Sidlerstr 5, CH-3012 Bern, Switzerland
[3] Stanford Univ, Stanford Inst Theoret Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[4] Univ Paris Saclay, Inst Phys Theor, CEA, CNRS, F-91191 Gif Sur Yvette, France
[5] Stockholm Univ, Dept Phys, AlbaNova, S-10691 Stockholm, Sweden
[6] Univ Michigan, Leinweber Ctr Theoret Phys, Dept Phys, Ann Arbor, MI 48109 USA
基金
瑞典研究理事会; 瑞士国家科学基金会; 欧盟地平线“2020”; 美国国家科学基金会;
关键词
AdS-CFT Correspondence; Gauge-gravity correspondence; Superstring Vacua; Supersymmetry Breaking;
D O I
10.1007/JHEP12(2021)187
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We discuss infinite families of non-supersymmetric AdS(6) solutions in Type IIB string theory. They are siblings of supersymmetric solutions which are associated with (p, q) 5-brane webs and holographically dual to 5d SCFTs engineered by those brane webs. The non-supersymmetric backgrounds carry identical 5-brane charges and are connected to the supersymmetric ones by RG flows. We study the stability of the non-supersymmetric solutions, identifying perturbative and non-perturbative decay channels for all the backgrounds explicitly available. We also identify likely decay mechanisms for solutions that have not been constructed explicitly but may be expected to exist based on brane web considerations. Finally, we exclude scale separation by constructing universal spin 2 modes with masses comparable to the mass-scale of the cosmological constant.
引用
收藏
页数:47
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