Search results for "STANDARD"

showing 10 items of 3299 documents

On axionic dark matter in Type IIA string theory

2013

We investigate viable scenarios with various axions in the context of supersymmetric field theory and in globally consistent D-brane models. The Peccei-Quinn symmetry is associated with an anomalous U(1) symmetry, which acquires mass at the string scale but remains as a perturbative global symmetry at low energies. The origin of the scalar Higgs-axion potential from F-, D- and soft breaking terms is derived, and two Standard Model examples of global intersecting D6-brane models in Type II orientifolds are presented, which differ in the realisation of the Higgs sector and in the hidden sector, the latter of which is of particluar importance for the soft supersymmetry breaking terms.

High Energy Physics - TheoryPhysicsHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesGlobal symmetryString theorySupersymmetry breakingString (physics)Symmetry (physics)Higgs sectorStandard ModelHidden sectorHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)
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Gravitino dark matter in the constrained next-to-minimal supersymmetric standard model with neutralino next-to-lightest superpartner

2010

The viability of a possible cosmological scenario is investigated. The theoretical framework is the constrained next-to-minimal supersymmetric standard model (cNMSSM), with a gravitino playing the role of the lightest supersymmetric particle (LSP) and a neutralino acting as the next-to-lightest supersymmetric particle (NLSP). All the necessary constraints from colliders and cosmology have been taken into account. For gravitino we have considered the two usual production mechanisms, namely out-of equillibrium decay from the NLSP, and scattering processes from the thermal bath. The maximum allowed reheating temperature after inflation, as well as the maximum allowed gravitino mass are determi…

High Energy Physics - TheoryPhysicsInflation (cosmology)Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesSuperpartnerFísicaGeneral Relativity and Quantum Cosmology (gr-qc)Lightest Supersymmetric ParticleGeneral Relativity and Quantum CosmologyNext-to-Minimal Supersymmetric Standard ModelHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)NeutralinoGravitinoHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsMinimal Supersymmetric Standard Model
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Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
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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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Gauge and Yukawa unification with broken R-parity

1998

We study gauge and Yukawa coupling unification in the simplest extension of the Minimal Supersymmetric Standard Model (MSSM) which incorporates R-Parity violation through a bilinear superpotential term. Contrary to what happens in the MSSM, we show that bottom-tau unification at the scale M_GUT where the gauge couplings unify can be achieved for any value of tan(beta) by choosing appropriately the sneutrino vacuum expectation value. In addition, we show that bottom-tau-top unification occurs in a slightly wider tan(beta) range than in the MSSM.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsUnificationHigh Energy Physics::PhenomenologySuperpotentialYukawa potentialFOS: Physical sciencesFísicaGauge (firearms)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)R-parityHigh Energy Physics::ExperimentBeta (velocity)Vacuum expectation valueMinimal Supersymmetric Standard ModelPhysics Letters B
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Modular invariant dynamics and fermion mass hierarchies around τ = i

2021

We discuss fermion mass hierarchies within modular invariant flavour models. We analyse the neighbourhood of the self-dual point $\tau=i$, where modular invariant theories possess a residual $Z_4$ invariance. In this region the breaking of $Z_4$ can be fully described by the spurion $\epsilon \approx \tau - i$, that flips its sign under $Z_4$. Degeneracies or vanishing eigenvalues of fermion mass matrices, forced by the $Z_4$ symmetry at $\tau=i$, are removed by slightly deviating from the self-dual point. Relevant mass ratios are controlled by powers of $|\epsilon|$. We present examples where this mechanism is a key ingredient to successfully implement an hierarchical spectrum in the lepto…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSupersymmetric Standard Model010308 nuclear & particles physicsSpectrum (functional analysis)Compactification and String ModelsFermionQC770-798Invariant (physics)01 natural sciencesSymmetry (physics)High Energy Physics - PhenomenologyNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesBeyond Standard ModelNeutrino Physics010306 general physicsEigenvalues and eigenvectorsLeptonMinimal Supersymmetric Standard ModelMathematical physicsSign (mathematics)Journal of High Energy Physics
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Structure Formation Limits on Axion-Like Dark Matter

2020

We derive structure formation limits on dark matter (DM) composed of keV-scale axion-like particles (ALPs), produced via freeze-in through the interactions with photons and Standard Model (SM) fermions. We employ Lyman-alpha (Ly-{\alpha}) forest data sets as well as the observed number of Milky Way (MW) subhalos. We compare results obtained using Maxwell-Boltzmann and quantum statistics for describing the SM bath. It should be emphasized that the presence of logarithmic divergences complicates the calculation of the production rate, which can not be parameterized with a simple power law behaviour. The obtained results, in combination with X-ray bounds, exclude the possibility for a photophi…

High Energy Physics - TheoryPhysicsParticle physicsStructure formationPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterFOS: Physical sciencesAstronomy and AstrophysicsFermion01 natural sciencesStandard ModelMomentumHigh Energy Physics - PhenomenologyDistribution functionHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Higgs production in a warped extra dimension

2012

Measurements of the Higgs-boson production cross section at the LHC are an important tool for studying electroweak symmetry breaking at the quantum level, since the main production mechanism gg → h is loop-suppressed in the Standard Model (SM). Higgs production in extra-dimensional extensions of the SM is sensitive to the Kaluza-Klein (KK) excitations of the quarks, which can be exchanged as virtual particles in the loop. In the context of the minimal Randall-Sundrum (RS) model with bulk fields and a brane-localized Higgs sector, we derive closed analytical expressions for the gluon-gluon fusion process, finding that the effect of the infinite tower of virtual KK states can be described in …

High Energy Physics - TheoryPhysicsQuarkParticle physicsNuclear and High Energy PhysicsLarge Hadron ColliderHiggs Physics010308 nuclear & particles physicsBrane Dynamics in Gauge TheoriesElectroweak interactionHigh Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesField Theories in Higher Dimensions01 natural sciencesStandard ModelHiggs sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesHiggs bosonSymmetry breaking010306 general physicsHiggs Physics; Field Theories in Higher Dimensions; Brane Dynamics in Gauge Theories
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Fitting formulae for photon spectra from WIMP annihilation

2011

Annihilation of different dark matter (DM) candidates into Standard Model (SM) particles could be detected through their contribution to the gamma ray fluxes that are measured on the Earth. The magnitude of such contributions depends on the particular DM candidate, but certain imprints of produced photon spectra may be analyzed in a model-independent fashion. In this work we provide the fitting formulae for the photon spectra generated by WIMP annihilation into quarks, leptons and gauge bosons channels in a wide range of WIMP masses.

High Energy Physics - TheoryQuarkHistoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciences01 natural sciencesEducationStandard ModelNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsPhysicsGauge bosonAnnihilation010308 nuclear & particles physicsFísicaComputer Science ApplicationsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Weakly interacting massive particlesAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonJournal of Physics: Conference Series
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Consistent QFT description of non-standard neutrino interactions

2019

Neutrino oscillations are precision probes of new physics beyond the Standard Model. Apart from neutrino masses and mixings, they are also sensitive to possible deviations of low-energy interactions between quarks and leptons from the Standard Model predictions. In this paper we develop a systematic description of such non-standard interactions (NSI) in oscillation experiments within the quantum field theory framework. We calculate the event rate and oscillation probability in the presence of general NSI, starting from the effective field theory (EFT) in which new physics modifies the flavor or Lorentz structure of charged-current interactions between leptons and quarks. We also provide the…

High Energy Physics - TheoryQuarkNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard Modelfield theory01 natural sciencesStandard Modeleffective field theory0103 physical sciencesEffective field theorylcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physicsneutrino: massQuantum field theory010306 general physicsNeutrino oscillationnumerical calculationsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsHigh Energy Physics::Phenomenologyquantum mechanicsEffective Field Theories3. Good healthHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798neutrino: oscillationNeutrinoneutrino: mixingLepton
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