Search results for "Standard Model"

showing 10 items of 1206 documents

Precision mass measurements for nuclear astro- and neutrino physics

2012

Nuclear masses are indispensable ingredients in numerous physics applications ranging from nuclear structure physics, where, e.g., the shell closures and nucleon correlation energies can be studied by accurate mass measurements, via the nuclear astrophysics, where the masses of nuclei far from the valley of β-stability determine the pathways of, e.g., rp-and r-processes of nucleosynthesis in stars, to tests of the standard model and fundamental interactions, where, e.g., the very-accurate masses of parent and superallowed β-decay daughter nuclei serve as one of inputs for the checking of the unitarity of the CKM quark-mixing matrix. In this review we focus on recent direct mass measurements…

PhysicsHistoryParticle physicsUnitarityNuclear TheoryNuclear structurePenning trapComputer Science ApplicationsEducationStandard ModelNuclear physicsNucleosynthesisNuclear astrophysicsNeutrinoNuclear ExperimentNucleonJournal of Physics: Conference Series
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Theg-factor of highly charged ions

2015

Highly charged ions provide a unique opportunity to test our understanding of atomic properties under extreme conditions: The electric field strength seen by an electron bound to a nucleus at the distance of the Bohr radius ranges from 1010 V/cm in hydrogen to1016 V/cm in hydrogenlike uranium. The theory of quantum electrodynamics (QED) allows for calculation e.g. of binding energies, transition probabilities or magnetic moments. While at low fields QED is tested to very high precision, new, hypothetical nonlinear effects like photon- photon interaction or a violation of Lorentz symmetry may occur in strong fields which then would lead to an extension of the Standard Model. The ultra-high p…

PhysicsHistoryPhotonMagnetic momentHighly charged ionElectronComputer Science ApplicationsEducationIonStandard ModelElectric fieldPräzisionsexperimente - Abteilung BlaumAtomic physicsBohr radiusJournal of Physics: Conference Series
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Neutrino masses: evidences and implications

2014

I give an overview of the evidences for neutrino masses and mixing, the associated neutrino mass generation schemes, as well as the resulting implications in particle physics experiments and cosmology.

PhysicsHistorySterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaPhysics beyond the Standard ModelSolar neutrinoHigh Energy Physics::PhenomenologyMass generationSolar neutrino problemComputer Science ApplicationsEducationNuclear physicsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationJournal of Physics: Conference Series
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Testing the Standard Model and beyond with the LENA proposal

2014

We discuss the possibility of a precision measurement of the electroweak mixing angle and a probe for new physics in the leptonic process of neutrino electron scattering. In the new physics schemes we explore the case of non standard neutrino interactions (NSI). The LENA proposal, currently under discussion, considers a large detector and the use of an articial, 51 Cr, radioactive neutrino source with of 5 MCi intensity. We also discuss the possible use of the solar neutrino

PhysicsHistorySterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsEducationNuclear physicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationJournal of Physics: Conference Series
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Search for sterile neutrinos with SOX: Monte Carlo studies of the experiment sensitivity and systematic effects

2020

Abstract Some neutrino experiments reveal anomalous results which can make room for new physics beyond the three-flavor neutrino oscillation model. These hints suggest the existence of sterile neutrinos with mass m <eV. SOX will be a short-baseline disappearance experiment aiming to test this hypotesis, performed with the liquid scintillator detector Borexino at Gran Sasso National Laboratory in Italy [1]. Due to the good energy and position resolution, a light sterile neutrino can create an oscillatory pattern in the signal. The SOX sensitivity, the related analysis and systematics will be briefly discussed.

PhysicsHistorySterile neutrinoPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyDetectorScintillatorComputer Science ApplicationsEducationNuclear physicsHigh Energy Physics::ExperimentSensitivity (control systems)NeutrinoNeutrino oscillationBorexinoJournal of Physics: Conference Series
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Collider signals of the Mirror Twin Higgs boson through the hypercharge portal

2019

We consider the collider signals arising from kinetic mixing between the hypercharge gauge boson of the Standard Model and its twin counterpart in the Mirror Twin Higgs model, in the framework in which the twin photon is massive. Through the mixing, the Standard Model fermions acquire charges under the mirror photon and the mirror Z boson. We determine the current experimental bounds on this scenario, and show that the mixing can be large enough to discover both the twin photon and the twin Z at the LHC, or at a future 100 TeV hadron collider, with dilepton resonances being a particularly conspicuous signal. We show that, in simple models, measuring the masses of both the mirror photon and …

PhysicsHyperchargeGauge bosonParticle physicsPhotonLarge Hadron ColliderHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-phlaw.inventionStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)lawHiggs bosonHigh Energy Physics::ExperimentColliderBoson
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Inflationary Imprints on Dark Matter

2015

We show that dark matter abundance and the inflationary scale $H$ could be intimately related. Standard Model extensions with Higgs mediated couplings to new physics typically contain extra scalars displaced from vacuum during inflation. If their coupling to Standard Model is weak, they will not thermalize and may easily constitute too much dark matter reminiscent to the moduli problem. As an example we consider Standard Model extended by a $Z_2$ symmetric singlet $s$ coupled to the Standard Model Higgs $\Phi$ via $\lambda \Phi^{\dag}\Phi s^2$. Dark matter relic density is generated non-thermally for $\lambda \lesssim 10^{-7}$. We show that the dark matter yield crucially depends on the inf…

PhysicsInflation (cosmology)Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelScalar (mathematics)Dark matterFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyModuliStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs boson010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Peccei–Quinn field for inflation, baryogenesis, dark matter, and much more

2016

We propose a scenario of brane cosmology in which the Peccei-Quinn field plays the role of the inflaton and solves simultaneously many cosmological and phenomenological issues such as the generation of a heavy Majorana mass for the right-handed neutrinos needed for seesaw mechanism, MSSM $\mu$-parameter, the right amount of baryon number asymmetry and dark matter relic density at the present universe, together with an axion solution to the strong CP problem without the domain wall obstacle. Interestingly, the scales of the soft SUSY-breaking mass parameter and that of the breaking of $U(1)_{\rm PQ}$ symmetry are lower bounded at $\mathcal{O}(10) {\mathrm TeV}$ and $\mathcal{O}(10^{11}) {\ma…

PhysicsInflation (cosmology)Particle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsInflaton01 natural scienceslcsh:QC1-999BaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBrane cosmologyStrong CP problemHigh Energy Physics::Experiment010306 general physicsAxionlcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters B
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Coulomb excitation of pear-shaped nuclei

2019

There is a large body of evidence that atomic nuclei can undergo octupole distortion and assume the shape of a pear. This phenomenon is important for measurements of electric-dipole moments of atoms, which would indicate CP violation and hence probe physics beyond the Standard Model of particle physics. Isotopes of both radon and radium have been identified as candidates for such measurements. Here, we have observed the low-lying quantum states in 224Rn and 226Rn by accelerating beams of these radioactive nuclei. We show that radon isotopes undergo octupole vibrations but do not possess static pear-shapes in their ground states. We conclude that radon atoms provide less favourable condition…

PhysicsIsotope010308 nuclear & particles physicsPhysicsQC1-999Physics beyond the Standard Modelchemistry.chemical_elementRadonCoulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural scienceschemistryQuantum state0103 physical sciencesMoment (physics)Atomic nucleusCP violationNuclear Physics - ExperimentPhysics::Atomic PhysicsAtomic physics010306 general physicsydinfysiikka
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Dependence of atomic parity-violation effects on neutron skins and new physics

2019

We estimate the relative contribution of nuclear structure and new physics couplings to the parity non-conserving spin-independent effects in atomic systems, for both single isotopes and isotopic ratios. General expressions are presented to assess the sensitivity of isotopic ratios to neutron skins and to couplings beyond standard model at tree level. The specific coefficients for these contributions are calculated assuming Fermi distribution for proton and neutron nuclear densities for isotopes of Cs, Ba, Sm, Dy, Yb, Pb, Fr, and Ra. The present work aims to provide a guide to the choice of the best isotopes and pairs of isotopes for conducting atomic PNC measurements.

PhysicsIsotopeAtomic Physics (physics.atom-ph)010308 nuclear & particles physicsPhysics beyond the Standard ModelNuclear TheoryNuclear structureFOS: Physical sciencesParity (physics)7. Clean energy01 natural sciencesPhysics - Atomic PhysicsNuclear physicssymbols.namesake0103 physical sciencessymbolsFermi–Dirac statisticsNeutronPhysics::Atomic Physics010306 general physicsNuclear Experiment
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