Search results for "spin: 2"

showing 2 items of 2 documents

Non-supersymmetric AdS6 and the swampland

2021

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 cons…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesQC770-798domain wallAdS-CFT Correspondencestring model: Type IIB01 natural sciencesGauge-gravity correspondenceHigh Energy Physics::TheoryNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciences010306 general physicsAdS-CFT Correspondence Gauge-gravity correspondence Superstring Vacua Supersymmetry BreakingSupersymmetry Breaking[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsbubbleComputer Science::Information RetrievalAdS-CFT Correspondence; Gauge-gravity correspondence; Superstring Vacua; Supersymmetry Breakingduality: holographystabilitydecay: nonperturbativeHigh Energy Physics - Theory (hep-th)renormalization group: flowD-brane: 5spin: 2Journal of High Energy Physics
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Zero rest-mass fields and the Newman-Penrose constants on flat space

2020

Zero rest-mass fields of spin 1 (the electromagnetic field) and spin 2 propagating on flat space and their corresponding Newman-Penrose (NP) constants are studied near spatial infinity. The aim of this analysis is to clarify the correspondence between data for these fields on a spacelike hypersurface and the value of their corresponding NP constants at future and past null infinity. To do so, Friedrich's framework of the cylinder at spatial infinity is employed to show that, expanding the initial data in terms spherical harmonics and powers of the geodesic spatial distance $\rho$ to spatial infinity, the NP constants correspond to the data for the second highest possible spherical harmonic …

High Energy Physics - TheorycylinderGeodesicField (physics)media_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Space (mathematics)01 natural sciencesGeneral Relativity and Quantum Cosmologyelectromagnetic field0103 physical sciencesBoundary value problem0101 mathematics[MATH]Mathematics [math]Mathematical PhysicsMathematical physicsmedia_commonPhysics010102 general mathematicsNull (mathematics)Spherical harmonicsStatistical and Nonlinear PhysicsInfinityboundary conditionHypersurfaceHigh Energy Physics - Theory (hep-th)spin: 1spin: 2010307 mathematical physicsgeodesic
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