Search results for "RADIOACTIVITY"

showing 10 items of 334 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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2020 global reassessment of the neutrino oscillation picture

2021

We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, we give updated analyses of DeepCore and SNO data, respectively. We have also included the latest electron antineutrino data collected by the Daya Bay and RENO reactor experiments, and the long-baseline T2K and NO$\nu$A measurements. These new analyses result in more accurate measurements of $\theta_{13}$, $\theta_{12}$, $\Delta m_{21}^2$ and $|\Delta m_{31}^2|$. The best fit value for the atmospheric angle $\theta_{23}$ lies in the second octant, but first octan…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)CUOREDouble beta decay0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNeutrino oscillationNOνAPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsHigh Energy Physics - Phenomenology13. Climate actionBeyond Standard Modellcsh:QC770-798CP violationHigh Energy Physics::ExperimentNeutrinoElectron neutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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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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A QCD analysis of LHCb D-meson data in p plus Pb collisions

2020

We scrutinize the recent LHCb data for D$^0$-meson production in p+Pb collisions within a next-to-leading order QCD framework. Our calculations are performed in the SACOT-$m_{\rm T}$ variant of the general-mass variable-flavour-number scheme (GM-VFNS), which has previously been shown to provide a realistic description of the LHC p+p data. Using the EPPS16 and nCTEQ15 nuclear parton distribution functions (PDFs) we show that a very good agreement is obtained also in the p+Pb case both for cross sections and nuclear modification ratios in the wide rapidity range covered by the LHCb data. Encouraged by the good correspondence, we quantify the impact of these data on the nuclear PDFs by the Hes…

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciencesPartonhiukkasfysiikka01 natural sciences114 Physical sciencesHigh Energy Physics - Phenomenology (hep-ph)Factorization0103 physical sciencesD mesonRapiditylcsh:Nuclear and particle physics. Atomic energy. Radioactivityheavy ion phenomenology010306 general physicsParton showerNuclear ExperimentParticle Physics - PhenomenologyPhysicsQuantum chromodynamicsLarge Hadron Collider010308 nuclear & particles physicshep-phHeavy Ion PhenomenologyGluonHigh Energy Physics - Phenomenologylcsh:QC770-798High Energy Physics::Experiment
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Hidden-charm and bottom tetra- and pentaquarks with strangeness in the hadro-quarkonium and compact tetraquark models

2020

In two recent papers, we used the hadro-quarkonium model to study the properties of hidden-charm and bottom tetraquarks and pentaquarks. Here, we extend the previous results and calculate the masses of heavy-quarkonium-kaon/hyperon systems. We also compute the spectrum of hidden-charm and bottom tetraquarks with strangeness in the compact tetraquark (diquark-antidiquark) model. If heavy-light exotic systems with non-null strangeness content were to be observed experimentally, it might be possible to distinguish among the large variety of available theoretical pictures for tetra- and pentaquark states and, possibly, rule out those which are not compatible with the data. peerReviewed

Nuclear and High Energy PhysicsParticle physicsFOS: Physical scienceshiukkasfysiikkaStrangeness01 natural sciencesphenomenological modelsHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityCharm (quantum number)010306 general physicsPhenomenological ModelsPhysicsbiology010308 nuclear & particles physicsHyperonQCD PhenomenologyQCD phenomenologybiology.organism_classificationQuarkoniumPentaquarkHigh Energy Physics - Phenomenologylcsh:QC770-798TetraTetraquarkJournal of High Energy Physics
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Revisiting the D-meson hadroproduction in general-mass variable flavour number scheme

2018

We introduce a novel realization of the open heavy-flavour hadroproduction in general-mass variable flavour number scheme at next-to-leading order in perturbative QCD. The principal novelty with respect to the earlier works is in the treatment of small-transverse-momentum limit, which has been a particularly challenging kinematic region in the past. We show that by a suitable choice of scheme, it is possible to obtain a well-behaved description of the open heavy-flavour hadroproduction cross sections from zero up to asymptotically high transverse momentum. We contrast our calculation with the available D$^0$-meson data as measured by the LHCb and ALICE collaborations at the LHC, finding a v…

Nuclear and High Energy PhysicsParticle physicsFRAGMENTATION FUNCTIONSFlavourFOS: Physical sciences114 Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)HEAVY-QUARK PRODUCTION0103 physical sciencesD mesonSCATTERINGlcsh:Nuclear and particle physics. Atomic energy. RadioactivityNUCLEAR COLLISIONSLimit (mathematics)QCD ANALYSIS010306 general physicsVariable (mathematics)PhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyContrast (statistics)Perturbative QCDQCD phenomenologyHigh Energy Physics - PhenomenologyPARTON DISTRIBUTIONSlcsh:QC770-798High Energy Physics::ExperimentLHCHADRON-COLLISIONSMATTERRealization (systems)TO-LEADING ORDER
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Fingerprints of heavy scales in electroweak effective Lagrangians

2017

The couplings of the electroweak effective theory contain information on the heavy-mass scales which are no-longer present in the low-energy Lagrangian. We build a general effective Lagrangian, implementing the electroweak chiral symmetry breaking $SU(2)_L\otimes SU(2)_R\to SU(2)_{L+R}$, which couples the known particle fields to heavier states with bosonic quantum numbers $J^P=0^\pm$ and $1^\pm$. We consider colour-singlet heavy fields that are in singlet or triplet representations of the electroweak group. Integrating out these heavy scales, we analyze the pattern of low-energy couplings among the light fields which are generated by the massive states. We adopt a generic non-linear realiz…

Nuclear and High Energy PhysicsParticle physicsFísica-Modelos matemáticosHiggs PhysicsFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryFísica matemáticaPartículas (Física nuclear)lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectromagnetismoSymmetry breakingSinglet state010306 general physicsParticles (Nuclear physics)Huellas dactilares.PhysicsQuantum chromodynamics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionCromodinámica cuántica.Technicolor and Composite ModelsQuantum numberLagrangian functions.High Energy Physics - PhenomenologyFingerprints.Simetría (Física)Beyond Standard ModelChiral LagrangiansQuantum chromodynamics.Higgs bosonlcsh:QC770-798Chiral symmetry breakingSymmetry (Physics)Lagrange Funciones de.Journal of High Energy Physics
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