Search results for "HIGGS"

showing 10 items of 1127 documents

Higgs mass predicted from the standard model with asymptotically safe gravity

2016

Tässä Pro Gradu -tutkielmassa tavoitteena on ennustaa Higgsin bosonin massa ottaen lähtökohdaksi hiukkasfysiikan standardimalli, johon on kytketty gravitaatio ns. asymptoottisesti turvallisena teoriana. Ennusteen laskemiseksi selvitetään Higgsin bosonin itseiskytkennän ja neljän muun standardimallin kytkinvakion juokseminen, eli kytkinvakioiden käyttäytyminen energiaskaalan funktiona, johtavassa kertaluvussa MS-skeemassa. Standardimallista saatuihin β-funktioihin lisätään asymptoottisesti turvallisen gravitaation antamat korjaukset suurilla energiaskaaloilla, jonka jälkeen β-funktioiden muodostama differentiaaliyhtälöryhmä ratkaistaan numeerisesti. Standardimallin osittainen äärellinen remo…

Higgs bosonrenormalisationHiggsin bosoniasymptoottihiukkasfysiikan standardimallirunning of couplingasymptotic safety
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"Table 44" of "Search for long-lived particles produced in $pp$ collisions at $\sqrt{s}=13$ TeV that decay into displaced hadronic jets in the ATLAS …

2018

Endcap MS vertex efficiencies (in %) for baryogenesis $\chi \rightarrow \tau\tau\nu$ benchmark samples ($m_{h}=125$ GeV). The vertex reconstruction efficiency is defined as the fraction of simulated LLP decays in the MS fiducial volume that match a reconstructed vertex ($\Delta R(\textrm{LLP,vertex}) = 0.4$) passing the baseline event selection and satisfying the vertex isolation criteria. A vertex is considered matched to a displaced decay if the vertex is within $\Delta R = 0.4$ of the simulated decay position. The MS vertex efficiency is parameterized as a function of the LLP decay position.

Higgs portal baryogenesis13000.0LLPComputer Science::Discrete Mathematics$pp \rightarrow h \rightarrow \chi\chi$displaced hadronic jetsSIG
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Modified majoron model for cosmological anomalies

2020

The vacuum expectation value $v_s$ of a Higgs triplet field $\Delta$ carrying two units of lepton number $L$ induces neutrino masses $\propto v_s$. The neutral component of $\Delta$ gives rise to two Higgs particles, a pseudoscalar $A$ and a scalar $S$. The most general renormalizable Higgs potential $V$ for $\Delta $ and the Standard-Model Higgs doublet $\Phi$ does not permit the possibility that the mass of either $A$ or $S$ is small, of order $v_s$, while the other mass is heavy enough to forbid the decay $Z\to A S$ to comply with LEP 1 data. We present a model with additional dimension-6 terms in $V$, in which this feature is absent and either $A$ or $S$ can be chosen light. Subsequentl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesOrder (ring theory)01 natural sciencesLepton numberPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs bosonddc:530High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsVacuum expectation valueMajoronBosonPhysical Review D
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Hidden sector dark matter and the Galactic Center gamma-ray excess: a closer look

2017

Stringent constraints from direct detection experiments and the Large Hadron Collider motivate us to consider models in which the dark matter does not directly couple to the Standard Model, but that instead annihilates into hidden sector particles which ultimately decay through small couplings to the Standard Model. We calculate the gamma-ray emission generated within the context of several such hidden sector models, including those in which the hidden sector couples to the Standard Model through the vector portal (kinetic mixing with Standard Model hypercharge), through the Higgs portal (mixing with the Standard Model Higgs boson), or both. In each case, we identify broad regions of parame…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsHyperchargeCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Hadron Collider010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)01 natural sciencesStandard ModelHidden sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Antiproton0103 physical sciencesHiggs bosonAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Measuring anomalous couplings in H -> WW* decays at the International Linear Collider

2010

The measurement of the Higgs coupling to W bosons is an important test of our understanding of the electroweak symmetry-breaking mechanism. We study the sensitivity of the International Linear Collider (ILC) to the presence of anomalous HW+W- couplings using ZH -> nu(nu) over bar WW* -> nu(nu) over bar 4j events. Using an effective Lagrangian approach, we calculate the differential decay rates of the Higgs boson including the effects of new dimension-five operators. We present a Monte Carlo simulation of events at the ILC, using a full detector simulation based on GEANT4 and a real event reconstruction chain. Expected constraints on the anomalous couplings are given.

High Energy Physics - PhenomenologyPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyHiggs-bosonFísicaHigh Energy Physics::ExperimentLHCHigh Energy Physics - Experiment
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The 1-loop effective potential for the Standard Model in curved spacetime

2018

The renormalisation group improved Standard Model effective potential in an arbitrary curved spacetime is computed to one loop order in perturbation theory. The loop corrections are computed in the ultraviolet limit, which makes them independent of the choice of the vacuum state and allows the derivation of the complete set of $\beta$-functions. The potential depends on the spacetime curvature through the direct non-minimal Higgs-curvature coupling, curvature contributions to the loop diagrams, and through the curvature dependence of the renormalisation scale. Together, these lead to significant curvature dependence, which needs to be taken into account in cosmological applications, which i…

High Energy Physics - TheoryDe Sitter spaceVacuum stateUNIVERSEfield theories in higher dimensionskosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)INFLATIONRADIATIVE-CORRECTIONSGauge theoryELECTROWEAK VACUUMMathematical physicsPhysics02 Physical SciencesPhysicshep-thhiukkasfysiikan standardimalliRENORMALIZATION-GROUP EQUATIONShep-phSPONTANEOUS SYMMETRY-BREAKINGNuclear & Particles PhysicsHigh Energy Physics - PhenomenologyHIGGS MASSPhysical SciencesGAUGE-THEORIESMathematics::Differential GeometryNuclear and High Energy Physicsgr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvatureclassical theories of gravityGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityfield theories in lower dimensions010306 general physics01 Mathematical SciencesInflation (cosmology)Science & TechnologySpacetimeSTABILITYta114010308 nuclear & particles physicsgravitaatioLoop (topology)High Energy Physics - Theory (hep-th)INTERACTING SCALAR FIELDlcsh:QC770-798Perturbation theory (quantum mechanics)Journal of High Energy Physics
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A non-perturbative study of massive gauge theories

2013

We consider a non-perturbative formulation of an SU(2) massive gauge theory on a space-time lattice, which is also a discretised gauged non-linear chiral model. The lattice model is shown to have an exactly conserved global SU(2) symmetry. If a scaling region for the lattice model exists and the lightest degrees of freedom are spin one vector particles with the same quantum numbers as the conserved current, we argue that the most general effective theory describing their low-energy dynamics must be a massive gauge theory. We present results of a exploratory numerical simulation of the model and find indications for the presence of a scaling region where both a triplet vector and a scalar re…

High Energy Physics - TheoryNuclear and High Energy PhysicsHiggs PhysicsHigh Energy Physics::Latticehep-latFOS: Physical sciences01 natural sciencesTheoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Lattice (order)0103 physical sciencesEffective field theoryGauge theory010306 general physicsConserved currentScalingLattice Gauge Field TheoriesPhysics010308 nuclear & particles physicshep-thHigh Energy Physics - Lattice (hep-lat)Físicahep-phQuantum numberHigh Energy Physics - PhenomenologyChiral modelHigh Energy Physics - Theory (hep-th)Gauge SymmetryNon-perturbativeSigma Models
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Gravitational footprints of massive neutrinos and lepton number breaking

2020

We investigate the production of primordial Gravitational Waves (GWs) arising from First Order Phase Transitions (FOPTs) associated to neutrino mass generation in the context of type-I and inverse seesaw schemes. We examine both "high-scale" as well as "low-scale" variants, with either explicit or spontaneously broken lepton number symmetry $U(1)_L$ in the neutrino sector. In the latter case, a pseudo-Goldstone majoron-like boson may provide a candidate for cosmological dark matter. We find that schemes with softly-broken $U(1)_L$ and with single Higgs-doublet scalar sector lead to either no FOPTs or too weak FOPTs, precluding the detectability of GWs in present or near future measurements.…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Spontaneous symmetry breakingDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Computer Science::Digital Libraries01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciences010306 general physicsPhysics010308 nuclear & particles physicsMass generationHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Higgs bosonNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The see-saw portal at future Higgs Factories

2020

We consider an extension of the Standard Model with two right-handed singlet fermions with mass at the electroweak scale that induce neutrino masses, plus a generic new physics sector at a higher scale $\Lambda$. We focus on the effective operators of lowest dimension $d=5$, which induce new production and decay modes for the singlet fermions. We assess the sensitivity of future Higgs Factories, such as FCC-ee, CLIC-380, ILC and CEPC, to the coefficients of these operators for various center of mass energies. We show that future lepton colliders can test the cut-off of the theory up to $\Lambda \simeq 500 - 1000\;$TeV, surpassing the reach of future indirect measurements of the Higgs and $Z…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHiggs PhysicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsBeyond Standard Model; Higgs Physics; Neutrino PhysicsPhysics010308 nuclear & particles physicsComputer Science::Information RetrievalHigh Energy Physics::PhenomenologyFermionHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Beyond Standard ModelHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentCenter of massElectroweak scaleNeutrinoLepton
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Elementary Goldstone Higgs boson and dark matter

2015

We investigate a perturbative extension of the Standard Model featuring elementary pseudo-Goldstone Higgs and dark matter particles. These are two of the five Goldstone bosons parametrising the SU(4)/Sp(4) coset space. They acquire masses, and therefore become pseudo-Goldstone bosons, due to the embedding of the Yukawa and the electroweak gauge interactions that do not preserve the full SU(4) symmetry. At the one-loop order the top corrections dominate and align the vacuum in the direction where the Higgs is mostly a pseudo-Goldstone boson. Because of the perturbative and elementary nature of the theory, the quantum corrections are precisely calculable. The remaining pseudo-Goldstone boson …

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHiggs bosonHigh Energy Physics::LatticeFOS: Physical sciencesElementary particleTechnicolor01 natural sciencesdark matterStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Goldstone bosons0103 physical sciences010306 general physicsCondensed Matter::Quantum GasesPhysicsGauge bosonta114relic densityelectroweak interaction010308 nuclear & particles physicshep-thHigh Energy Physics::Phenomenologyhep-phHigh Energy Physics - PhenomenologyHiggs fieldscalar particleHigh Energy Physics - Theory (hep-th)symbolsHiggs bosonLHCHiggs mechanismMinimal Supersymmetric Standard ModelPhysical Review D
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