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Please use this identifier to cite or link to this item: http://hdl.handle.net/11375/11523
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dc.contributor.advisorBurgess, Cliffen_US
dc.contributor.advisorChen, Alanen_US
dc.contributor.advisorPospelov, Maximen_US
dc.contributor.authorvan, Nierop Leoen_US
dc.date.accessioned2014-06-18T16:54:55Z-
dc.date.available2014-06-18T16:54:55Z-
dc.date.created2011-11-04en_US
dc.date.issued2012-04en_US
dc.identifier.otheropendissertations/6487en_US
dc.identifier.other7510en_US
dc.identifier.other2331733en_US
dc.identifier.urihttp://hdl.handle.net/11375/11523-
dc.description<p>Defended on November 3rd, 2011</p>en_US
dc.description.abstract<p>In this thesis, we describe the properties of brane worlds embedded in a spacetime with two extra dimensions. We derive and describe the boundary conditions that branes impose on the bulk fields in the theory, and show that they reproduce known results for D7 branes in F-theory compactifications of type IIB supergravity. We show how brane-bulk couplings can stabilize moduli of a flux stabilized compactification of extra dimensions. An important new ingredient is that the branes can have a magnetic coupling to the flux that stabilizes the bulk. This coupling allows the system to relax the stringent constraints of flux quantization, which allows the bulk spacetime to respond to perturbations of the branes. We derive the dynamics of the lower-dimensional effective theory below the Kaluza-Klein scale, and show that the contributions of the magnetic coupling can be competitive with the tension of the brane. We first describe the simplest flux compactification: an Einstein-scalar- Maxwell theory in 6 dimensions. We find that the effective potential in 4 dimensions gets minimized at the position one would naively expect - at the stationary point of the sum of all the brane Lagrangians - but its value at the minimum gets changed by the magnetic coupling to the brane. Next we find that if the bulk is described by 6 dimensional gauged chiral supergravity, the effect of the magnetic coupling allows the curvature on the brane to be suppressed relative to the generic scale of the tension on the branes. We use this observation to construct an explicit brane-bulk system that has a technically natural cosmological constant of the correct size. The classical on-brane curvature vanishes in our construction, and the first order quantum corrections give a value to the cosmological constant of the right order of magnitude. We estimate higher loop corrections, and they are greatly suppressed.</p>en_US
dc.subjectParticle physicsen_US
dc.subjectCosmologyen_US
dc.subjectExtra dimensionsen_US
dc.subjectElementary Particles and Fields and String Theoryen_US
dc.subjectElementary Particles and Fields and String Theoryen_US
dc.titlePhenomenology of codimension-2 brane worlds: the importance of back-reactionen_US
dc.typethesisen_US
dc.contributor.departmentPhysics and Astronomyen_US
dc.description.degreeDoctor of Philosophy (PhD)en_US
Appears in Collections:Open Access Dissertations and Theses

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