Search results for "Brane cosmology"

showing 10 items of 13 documents

Brane cosmology with an anisotropic bulk

2004

In the context of brane cosmology, a scenario where our universe is a 3+1-dimensional surface (the ``brane'') embedded in a five-dimensional spacetime (the ``bulk''), we study geometries for which the brane is anisotropic - more specifically Bianchi I - though still homogeneous. We first obtain explicit vacuum bulk solutions with anisotropic three-dimensional spatial slices. The bulk is assumed to be empty but endowed with a negative cosmological constant. We then embed Z_2-symmetric branes in the anisotropic spacetimes and discuss the constraints on the brane energy-momentum tensor due to the five-dimensional anisotropic geometry. We show that if the bulk is static, an anisotropic brane ca…

High Energy Physics - TheoryNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciencesContext (language use)Perfect fluidGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesBrane cosmologyTensor010306 general physicsmedia_commonPhysicsSpacetimeExtra Large Dimensions010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astrophysics (astro-ph)Cosmology of Theories beyond the SMUniverseHigh Energy Physics - Theory (hep-th)Brane
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Supersymmetry from boundary conditions

2004

We study breaking and restoration of supersymmetry in five-dimensional theories by determining the mass spectrum of fermions from their equations of motion. Boundary conditions can be obtained from either the action principle by extremizing an appropriate boundary action (interval approach) or by assigning parities to the fields (orbifold approach). In the former, fields extend continuously from the bulk to the boundaries, while in the latter the presence of brane mass-terms cause fields to jump when one moves across the branes. We compare the two approaches and in particular we carefully compute the non-trivial jump profiles of the wavefunctions in the orbifold picture for very general bra…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesEquations of motionFermionSupersymmetryHigh Energy Physics::TheoryTheoretical physicsHigh Energy Physics - Theory (hep-th)Differential geometryQuantum mechanicsBrane cosmologyBoundary value problemBraneOrbifoldNuclear Physics B
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The cosmological constant problem in codimension-two brane models

2005

We discuss the possibility of a dynamical solution to the cosmological constant problem in the contaxt of six-dimensional Einstein-Maxwell theory. A definite answer requires an understanding of the full bulk cosmology in the early universe, in which the bulk has time-dependent size and shape. We comment on the special properties of codimension two as compared to higher codimensions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesNon-standard cosmologyCosmological constantMetric expansion of spaceGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeFriedmann–Lemaître–Robertson–Walker metricBrane cosmologysymbolsBraneCosmological constant problemPhysics Letters B
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Aspects of D-brane Dynamics in Supergravity Backgrounds with Fluxes, Kappa-symmetry and Equations of Motion. Part IIB

2006

We derive and carry out a detailed analysis of the equations of motion of the type IIB D branes in generic supergravity backgrounds with fluxes making account of the worldvolume Born-Infeld gauge field and putting a special emphasis on the structure of the Dirac equation for Dp brane fermionic modes. We present an explicit form of the worldvolume field equations for each of the Dp branes (p=1,3,5,7,9) in the cases in which the Neveu-Schwarz flux and the Ramond-Ramond p-form flux along the Dp-brane worldvolume are zero and the supergravity backgrounds do not necessarily induce the worldvolume Born-Infeld flux. We then give several examples of D3, D5 and D7 brane configurations in which the w…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsInstantonCompactification (physics)SupergravityEquations of motionFOS: Physical sciencessymbols.namesakeHigh Energy Physics::TheoryClassical mechanicsHigh Energy Physics - Theory (hep-th)Mathematics::K-Theory and HomologyDirac equationsymbolsBrane cosmologyGauge theoryD-braneMathematical physics
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Q7-branes and their coupling to IIB supergravity

2007

We show how, by making use of a new basis of the IIB supergravity axion-dilaton coset, SL(2,R)/SO(2), 7-branes that belong to different conjugacy classes of the duality group SL(2,R) naturally couple to IIB supergravity with appropriate source terms characterized by an SL(2,R) charge matrix Q. The conjugacy classes are determined by the value of the determinant of Q. The (p,q) 7-branes are the branes in the conjugacy class detQ = 0. The 7-branes in the conjugacy class detQ > 0 are labelled by three numbers (p,q,r) which parameterize the matrix Q and will be called Q7-branes. We construct the full bosonic Wess--Zumino term for the Q7-branes. In order to realize a gauge invariant coupling …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsPure mathematicsSupergravityFOS: Physical sciencesMONOPOLESInvariant (physics)p-branesBRANESFIELDSINSTANTONSABELIAN BORN-INFELDConjugacy classDOMAIN-WALLSHigh Energy Physics - Theory (hep-th)DUALITYD-branesBrane cosmologyCoset6 DIMENSIONS
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The geometry of branes and extended superspaces

1999

We argue that a description of supersymmetric extended objects from a unified geometric point of view requires an enlargement of superspace. To this aim we study in a systematic way how superspace groups and algebras arise from Grassmann spinors when these are assumed to be the only primary entities. In the process, we recover generalized spacetime superalgebras and extensions of supersymmetry found earlier. The enlargement of ordinary superspace with new parameters gives rise to extended superspace groups, on which manifestly supersymmetric actions may be constructed for various types of p-branes, including D-branes (given by Chevalley-Eilenberg cocycles) with their Born-Infeld fields. Thi…

High Energy Physics - TheoryPhysicsQuantum PhysicsNuclear and High Energy PhysicsSpinorSpacetimeFOS: Physical sciencesField (mathematics)Mathematical Physics (math-ph)SupersymmetrySuperspaceGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryTheoretical physicsHigh Energy Physics - Theory (hep-th)Brane cosmologylcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityPoint (geometry)BraneQuantum Physics (quant-ph)Mathematical PhysicsNuclear Physics B
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Oh, wait, O8 de Sitter may be unstable!

2021

We analyze the stability of four-dimensional de Sitter vacua constructed by compactifying massive Type IIA supergravity in the presence of two O8 sources [1]. When embedded in String Theory the first source has a clear interpretation as an O8$_-$ plane, but the second one could correspond to either an O8$_+$ plane or to an O8$_-$ plane with 16 D8-branes on top. We find that this latter solution has a tachyonic instability, corresponding to the D8-branes moving away from the O8$_-$ plane. We comment on the possible ways of distinguishing between these sources.

High Energy Physics - Theoryvacuum state: de SitterNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi Matematicidimension: 4compactificationSuperstring VacuaFOS: Physical sciencesD-braneString theory01 natural sciencessupergravity: Type IIADe Sitter universeFlux compactifications0103 physical sciencesC++ string handlingBrane cosmologylcsh:Nuclear and particle physics. Atomic energy. RadioactivityD-brane010306 general physicsMathematical physicsPhysicsCompactification (physics)010308 nuclear & particles physicsPlane (geometry)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Supergravitytachyon: stabilitySuperstring Vacua D-branes Flux compactificationsHigh Energy Physics - Theory (hep-th)D-branesstringlcsh:QC770-798
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M-theory, graphene-branes and superconducting wormholes

2017

Exploiting an M-brane system whose structure and symmetries are inspired by those of graphene (what we call a graphene-brane), we propose here a similitude between two layers of graphene joined by a nanotube and wormholes scenarios in the brane world. By using the symmetries and mathematical properties of the M-brane system, we show here how to possibly increase its conductivity, to the point of making it as a superconductor. The questions of whether and under which condition this might point to the corresponding real graphene structures becoming superconducting are briefly outlined.

M-theoryPhysicsSuperconductivityQuantum field theory in curved spacetimePhysics and Astronomy (miscellaneous)Condensed matter physics010308 nuclear & particles physicsGraphene01 natural sciencesSimilitudelaw.inventionTheoretical physicslaw0103 physical sciencesHomogeneous spaceBrane cosmologyWormhole010306 general physicsInternational Journal of Geometric Methods in Modern Physics
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Micro-orbits in a many-brane model and deviations from Newton’s $$1/r^2$$ 1 / r 2 law

2016

We consider a 5-dimensional model with geometry ${\cal M} = {\cal M}_4 \times {\cal S}_1$, with compactification radius $R$. The Standard Model particles are localized onto a brane located at y=0, with identical branes localized at different points in the extra dimension. Objects located on our brane can orbit around objects located on a brane at a distance $d=y/R$, with an orbit and a period significantly different from the standard Newtonian ones. We study the kinematical properties of the orbits, finding that it is possible to distinguish one motion from the other in a large region of the initial conditions parameter space. This is a warm-up to study if a SM-like mass distribution on one…

PhysicsCompactification (physics)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsDark matterMotion (geometry)Parameter space01 natural sciencesStandard ModelLaw0103 physical sciencesOrbit (dynamics)Brane cosmologyBrane010306 general physicsEngineering (miscellaneous)The European Physical Journal C
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Neutrinos confronting large extra dimensions

2001

We study neutrino physics in a model with one large extra dimension. We assume the existence of two four-dimensional branes in the five-dimensional space-time, one for the ordinary particles and the other one for mirror particles, and we investigate neutrino masses and mixings in this scheme. Comparison of experimental neutrino data with the predictions of the model leads to various restrictions on the parameters of the model. For instance, the size of the extra dimension, R, turns out to be bounded from below. Cosmological considerations seem to favor a large R. The usual mixing schemes proposed as solutions to the solar and atmospheric neutrino anomalies are compatible with our model.

PhysicsHigh Energy Physics - PhenomenologyNuclear and High Energy PhysicsParticle physicsHigh Energy Physics - Phenomenology (hep-ph)Dimension (vector space)Bounded functionBrane cosmologyFOS: Physical sciencesLarge extra dimensionNeutrinoAtmospheric neutrinoMixing (physics)Physics Letters B
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