Search results for "Standard Model"

showing 10 items of 1206 documents

Electroweak baryogenesis and dark matter from a singlet Higgs

2012

If the Higgs boson H couples to a singlet scalar S via lambda_m |H|^2 S^2, a strong electroweak phase transition can be induced through a large potential barrier that exists already at zero temperature. In this case properties of the phase transition can be computed analytically. We show that electroweak baryogenesis can be achieved using CP violation from a dimension-6 operator that couples S to the top-quark mass, suppressed by a new physics scale that can be well above 1 TeV. Moreover the singlet is a dark matter candidate whose relic density is < 3% of the total dark matter density, but which nevertheless interacts strongly enough with nuclei (through Higgs exchange) to be just below…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterElectroweak interactionHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesHiggs bosonCP violationInvariant massHigh Energy Physics::Experiment010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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All-inclusive interacting dark sector cosmologies

2020

In this paper we explore possible extensions of Interacting Dark Energy cosmologies, where Dark Energy and Dark Matter interact non-gravitationally with one another. In particular, we focus on the neutrino sector, analyzing the effect of both neutrino masses and the effective number of neutrino species. We consider the Planck 2018 legacy release data combined with several other cosmological probes, finding no evidence for new physics in the dark radiation sector. The current neutrino constraints from cosmology should be therefore regarded as robust, as they are not strongly dependent on the dark sector physics, once all the available observations are combined. Namely, we find a total neutri…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsLambda01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Dark radiation0103 physical sciencesDark energysymbolsHigh Energy Physics::ExperimentPlanckNeutrino010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Weakly interacting dark matter from the minimal walking technicolor

2009

We study a superweakly interacting dark matter particle motivated by minimal walking technicolor theories. Our WIMP is a mixture of a sterile state and a state with the charges of a standard model fourth family neutrino. We show that the model can give the right amount of dark matter over a range of the WIMP mass and mixing angle. We compute bounds on the model parameters from the current accelerator data including the oblique corrections to the precision electroweak parameters, as well as from cryogenic experiments, Super-Kamiokande and from the IceCube experiment. We show that consistent dark matter solutions exist which satisfy all current constraints. However, almost the entire paramete…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterElectroweak interactionFOS: Physical sciencesAstronomy and AstrophysicsTechnicolorWeinberg angleCosmologyStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)WIMPHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Observational properties of feebly coupled dark matter

2016

We show that decoupled hidden sectors can have observational consequences. As a representative model example, we study dark matter production in the Higgs portal model with one real singlet scalar $s$ coupled to the Standard Model Higgs via $\lambda_{\rm hs}\Phi^\dagger\Phi s^2$ and demonstrate how the combination of non-observation of cosmological isocurvature perturbations and astrophysical limits on dark matter self-interactions imply stringent bounds on the magnitude of the scalar self-coupling $\lambda_{\rm s}s^4$. For example, for dark matter mass $m_{\rm s}=10$ MeV and Hubble scale during cosmic inflation $H_*=10^{12}$ GeV, we find $10^{-4}\lesssim \lambda_{\rm s}\lesssim 0.2$.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterHigh Energy Physics::PhenomenologyScalar field dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsdark matterStandard ModelHidden sectorpimeä aineHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonProduction (computer science)Light dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Updated Z Parameters, and Standard Model Fits from Electroweak Precision Data

1999

Data taking around the Z resonance at LEP I ended in 1995, and determinations of the mass, width, hadronic pole cross section and leptonic couplings of the Z boson are approaching a final status. This is accompanied by an improved understanding of the beam energy during the high-statistics data taking approximately two GeV above and below the Z resonance in 1993 and 1995. Together with other precision measurements presented at this conference impressive tests of the consistency of the Standard Model can be made and an upper limit on the mass of the Higgs boson can be derived.

PhysicsParticle physicsCross section (physics)Consistency (statistics)High Energy Physics::PhenomenologyElectroweak interactionHadronHiggs bosonHigh Energy Physics::ExperimentLimit (mathematics)Resonance (particle physics)Standard Model
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Radiative Seesaw Dark Matter

2021

The singlet majoron model of seesaw neutrino mass is appended by one dark Majorana fermion singlet $\chi$ with $L=2$ and one dark complex scalar singlet $\zeta$ with $L=1$. This simple setup allows $\chi$ to obtain a small radiative mass anchored by the same heavy right-handed neutrinos, whereas the one-loop decay of the standard-model Higgs boson to $\chi \chi + \bar{\chi} \bar{\chi}$ provides the freeze-in mechanism for $\chi$ to be the light dark matter of the Universe.

PhysicsParticle physicsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHiggs bosonHigh Energy Physics::ExperimentNeutrinoLight dark matterMajorana fermionMajoron
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Fascinating puzzle called double beta decay

2019

The question of whether neutrinos are Majorana or Dirac particles and what are their average masses remains one of the most fundamental problems in physics today. Observation of neutrinoless double beta decay (0νββ) would verify the Majorana nature of the neutrino and constrain the absolute scale of the neutrino mass spectrum. The inverse half-life for 0νββ-decay is given by the product of a phase space factor (PSF), a nuclear matrix element (NME), which both rely on theoretical description, and a function f containing the physics beyond the standard model. Recent calculations of PSF and NME will be reviewed together with comparison to other available results. These calculations serve the p…

PhysicsParticle physicsDirac (video compression format)Physics beyond the Standard ModelHigh Energy Physics::Phenomenologyneutriinotdouble beta decaynuclear matrix elementshiukkasfysiikkaMAJORANADouble beta decayPhase spaceMass spectrumHigh Energy Physics::ExperimentNeutrinoydinfysiikkaAbsolute scale
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A Monochromatic Neutrino Beam to Obtain U(e3) and the CP Phase

2007

The goal for future neutrino facilities is the determination of the [Ue3] mixing and CP violation in neutrino oscillations. This will require precision experiments with a very intense neutrino source. The future experiments such as T2K, NOVA and Double CHOOZ will measure the [Ue3] mixing. In order to explore CP violation, we present a novel method to create a monochromatic neutrino beam based on the recent discovery of nuclei that decay fast through electron capture in a superallowed Gamow-Teller transition. The boost of such radioactive ions will generate an intense monochromatic directional neutrino beam when decaying at high energy in a storage ring with long straight sections. We show t…

PhysicsParticle physicsElectron capturePhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFísicaCHOOZSolar neutrino problemNuclear physicsCP violationMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationAIP Conference Proceedings
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Perturbative unitarity constraints on gauge portals

2017

Abstract Dark matter that was once in thermal equilibrium with the Standard Model is generally prohibited from obtaining all of its mass from the electroweak phase transition. This implies a new scale of physics and mediator particles to facilitate dark matter annihilation. In this work, we focus on dark matter that annihilates through a generic gauge boson portal. We show how partial wave unitarity places upper bounds on the dark gauge boson, dark Higgs and dark matter masses. Outside of well-defined fine-tuned regions, we find an upper bound of 9 TeV for the dark matter mass when the dark Higgs and dark gauge bosons both facilitate the dark matter annihilations. In this scenario, the uppe…

PhysicsParticle physicsGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionDark matterAstronomy and AstrophysicsElementary particleAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesStandard ModelSpace and Planetary Science0103 physical sciencesHiggs bosonGrand Unified Theory010306 general physicsBosonPhysics of the Dark Universe
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Testing triplet fermions at the electron-positron and electron-proton colliders using fat jet signatures

2020

The addition of $SU(2)_L$ triplet fermions of zero hypercharge with the Standard Model (SM) helps to explain the origin of the neutrino mass by the so-called seesaw mechanism. Such a scenario is commonly know as the type-III seesaw model. After the electroweak symmetry breaking the mixings between the light and heavy mass eigenstates of the neutral leptons are developed which play important roles in the study of the charged and neutral multiplets of the triplet fermions at the colliders. In this article we study such interactions to produce these multiplets of the triplet fermion at the electron-positron and electron-proton colliders at different center of mass energies. We focus on the hea…

PhysicsParticle physicsGauge bosonHypercharge010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermion01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Seesaw mechanism0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsLepton
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