Search results for "Theories"

showing 10 items of 302 documents

Relaxing cosmological neutrino mass bounds with unstable neutrinos

2020

At present, cosmological observations set the most stringent bound on the neutrino mass scale. Within the standard cosmological model ($\Lambda$CDM), the Planck collaboration reports $\sum m_\nu < 0.12\,\text{eV}$ at 95% CL. This bound, taken at face value, excludes many neutrino mass models. However, unstable neutrinos, with lifetimes shorter than the age of the universe $\tau_\nu \lesssim t_U$, represent a particle physics avenue to relax this constraint. Motivated by this fact, we present a taxonomy of neutrino decay modes, categorizing them in terms of particle content and final decay products. Taking into account the relevant phenomenological bounds, our analysis shows that 2-body deca…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Age of the universeFOS: Physical sciencesLambda-CDM model7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityPlanck010306 general physicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMass generationElectroweak interactionCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard ModelGoldstone bosonsymbolslcsh:QC770-798High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Shining Light on the Scotogenic Model: Interplay of Colliders and Cosmology

2019

In the framework of the scotogenic model, which features radiative generation of neutrino masses, we explore light dark matter scenario. Throughout the paper we chiefly focus on keV-scale dark matter which can be produced either via freeze-in through the decays of the new scalars, or from the decays of next-to-lightest fermionic particle in the spectrum, which is produced through freeze-out. The latter mechanism is required to be suppressed as it typically produces a hot dark matter component. Constraints from BBN are also considered and in combination with the former production mechanism they impose the dark matter to be light. For this scenario we consider signatures at High Luminosity LH…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsLight dark matterPhysicsLarge Hadron ColliderMissing energy010308 nuclear & particles physicsHot dark matterCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentNeutrinoLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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The Dispirited Case of Gauged $U(1)_{B-L}$ Dark Matter

2018

We explore the constraints and phenomenology of possibly the simplest scenario that could account at the same time for the active neutrino masses and the dark matter in the Universe within a gauged $U(1)_{B-L}$ symmetry, namely right-handed neutrino dark matter. We find that null searches from lepton and hadron colliders require dark matter with a mass below 900 GeV to annihilate through a resonance. Additionally, the very strong constraints from high-energy dilepton searches fully exclude the model for $ 150 \, \text{GeV} &lt; m_{Z'} &lt; 3 \, \text{TeV}$. We further explore the phenomenology in the high mass region (i.e. masses $\gtrsim \mathcal{O}(1) \, \text{TeV}$) and highlight theoret…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelHadronDark matterFOS: Physical sciencesParameter space01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesLandau polelcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)LeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Kaluza-Klein FIMP dark matter in warped extra-dimensions

2020

We study for the first time the case in which Dark Matter (DM) is made of Feebly Interacting Massive Particles (FIMP) interacting just gravitationally with the standard model particles in an extra-dimensional Randall-Sundrum scenario. We assume that both the dark matter and the standard model are localized in the IR-brane and only interact via gravitational mediators, namely the graviton, the Kaluza-Klein gravitons and the radion. We found that in the early Universe DM could be generated via two main processes: the direct freeze-in and the sequential freeze-in. The regions where the observed DM relic abundance is produced are largely compatible with cosmological and collider bounds.

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectKaluza–Klein theoryDark matterFOS: Physical sciences01 natural scienceslaw.inventionStandard ModelGravitationHigh Energy Physics - Phenomenology (hep-ph)law0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsCollidermedia_commonPhysics010308 nuclear & particles physicsGravitonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyExtra dimensionsBeyond Standard Modellcsh:QC770-798Astrophysics - Cosmology and Nongalactic Astrophysics
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Gravity-mediated dark matter in clockwork/linear dilaton extra-dimensions

2020

We study for the first time the possibility that Dark Matter (represented by particles with spin $0,1/2$ or $1$) interacts gravitationally with Standard Model particles in an extra-dimensional Clockwork/Linear Dilaton model. We assume that both, the Dark Matter and the Standard Model, are localized in the IR-brane and only interact via gravitational mediators, namely the Kaluza-Klein (KK) graviton and the radion/KK-dilaton modes. We analyse in detail the Dark Matter annihilation channel into Standard Model particles and into two on-shell Kaluza-Klein towers (either two KK-gravitons, or two radion/KK-dilatons, or one of each), finding that it is possible to obtain the observed relic abundanc…

Nuclear and High Energy PhysicsParticle physicsDark matterFOS: Physical sciencesStrings and branes phenomenology01 natural sciencesStandard ModelGravitationHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Phenomenology of Field Theories in Higher Dimensions0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsSpin (physics)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsGravitonHigh Energy Physics - PhenomenologyExtra dimensionslcsh:QC770-798DilatonAstrophysics - High Energy Astrophysical PhenomenaJournal of High Energy Physics
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Three-body hadron systems with strangeness

2013

Recently, many efforts are being put in studying three-hadron systems made of mesons and baryons and interesting results are being found. In this talk, we summarize the main features of the formalism used to study such three hadron systems with strangeness S = -1, 0 within a framework built on the basis of unitary chiral theories and solution of the Faddeev equations. In particular, we present the results obtained for the pi(K) over barN, K (K) over barN and KK (K) over bar systems and their respective coupled channels. In the first case, we find four Sigma's and two A's with spin-parity J(P) = 1/2(+), in the 1500-1800 MeV region, as two meson-one baryon s-wave resonances. In the second cas…

Nuclear and High Energy PhysicsParticle physicsFaddeev equationsMesonNuclear TheoryHadronNuclear TheoryFOS: Physical sciencesStrangenessFew-body systems01 natural sciencesNuclear physicsNuclear Theory (nucl-th)Few-body systemsHadron spectroscopy0103 physical sciences010306 general physicsNuclear ExperimentPhysicsUnitarity010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaUnitary chiral theoriesBaryonHigh Energy Physics::Experiment
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Pinch technique for Schwinger-Dyson equations

2007

40 pages, 11 figures.-- ISI Article Identifier: 000245922000041.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ph/0611354

Nuclear and High Energy PhysicsParticle physicsGeneralizationStructure (category theory)FOS: Physical sciencesContext (language use)Skeleton (category theory)Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Self-energiesBackground-field MethodAbelian Gauge TheoriesPhysicsBackground field methodScalar (physics)FísicaPerturbation-theoryEffective ChargeFundamental interaction3-point VertexHigh Energy Physics - PhenomenologyNonperturbative EffectsQuantum Chromodynamics (QCD)Gauge SymmetryPinchBRST SymmetryJournal of High Energy Physics
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A tale of two portals: testing light, hidden new physics at future e + e − colliders

2017

We investigate the prospects for producing new, light, hidden states at a future $e^+ e^-$ collider in a Higgsed dark $U(1)_D$ model, which we call the Double Dark Portal model. The simultaneous presence of both vector and scalar portal couplings immediately modifies the Standard Model Higgsstrahlung channel, $e^+ e^- \to Zh$, at leading order in each coupling. In addition, each portal leads to complementary signals which can be probed at direct and indirect detection dark matter experiments. After accounting for current constraints from LEP and LHC, we demonstrate that a future $e^+ e^-$ Higgs factory will have unique and leading sensitivity to the two portal couplings by studying a host o…

Nuclear and High Energy PhysicsParticle physicsHiggs PhysicsPhysics beyond the Standard ModelDark matterScalar (mathematics)FOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Experimentlaw.inventionStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)law0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsColliderCouplingPhysicsLarge Hadron Collider010308 nuclear & particles physicsCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard ModelHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentJournal of High Energy Physics
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Novel mechanism for primordial perturbations in minimal extensions of the Standard Model

2020

Abstract We demonstrate that light spectator fields in their equilibrium can source sizeable CMB anisotropies through modulated reheating even in the absence of direct couplings to the inflaton. The effect arises when the phase space of the inflaton decay is modulated by the spectator which generates masses for the decay products. We call the mechanism indirect modulation and using the stochastic eigenvalue expansion show that it can source perturbations even four orders of magnitude larger than the observed amplitude. Importantly, the indirect mechanism is present in the Standard Model extended with right- handed neutrinos. For a minimally coupled Higgs boson this leads to a novel lower bo…

Nuclear and High Energy PhysicsParticle physicsHiggs Physicshiukkasfysiikka114 Physical sciences01 natural sciencesUpper and lower boundsPhysics Particles & FieldsStandard Model0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicscosmology of theories beyond the SM0206 Quantum PhysicsPhysicsScience & Technology0105 Mathematical Physics010308 nuclear & particles physicsHiggsin bosoniPhysicshep-thHigh Energy Physics::PhenomenologyHiggs physicshep-phInflatonCosmology of Theories beyond the SMNuclear & Particles PhysicsAmplitudeOrders of magnitude (time)Phase spacePhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma Physicsastro-ph.COHiggs bosonlcsh:QC770-798NeutrinoJournal of High Energy Physics
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Supersymmetric type-III seesaw mechanism: Lepton flavor violation and LHC phenomenology

2013

We study a supersymmetric version of the type-III seesaw mechanism considering two variants of the model: a minimal version for explaining neutrino data with only two copies of 24 superfields and a model with three generations of 24-plets. The latter predicts, in general, rates for mu -> e gamma inconsistent with experimental data. However, this bound can be evaded if certain special conditions within the neutrino sector are fulfilled. In the case of two 24-plets, lepton flavor violation constraints can be satisfied much more easily. After specifying the corresponding regions in the minimal supergravity parameter space, we show that under favorable conditions one can test the corresponding …

Nuclear and High Energy PhysicsParticle physicsMassesPhysics beyond the Standard Model01 natural sciences0103 physical sciencesRoot-S=7 tev010306 general physicsRight-handed neutrinosPhysicsLarge Hadron ColliderElectroweak010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionFísicaNon-conservationSupersymmetrySeesaw mechanismUnificationGrand unified theoriesHigh Energy Physics::ExperimentNeutrinoModel higgs-bosonDecaysPhenomenology (particle physics)LeptonStandard model
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