Search results for "muon"

showing 10 items of 1376 documents

On the flavor composition of the high-energy neutrinos in IceCube

2016

The IceCube experiment has recently released 3 years of data of the first ever detected high-energy (>30 TeV) neutrinos, which are consistent with an extraterrestrial origin. In this talk, we compute the compatibility of the observed track-to-shower ratio with possible combinations of neutrino flavors with relative proportion (alpha_e:alpha_mu:alpha_tau). Although this observation is naively favored for the canonical (1:1:1) at Earth, once we consider the IceCube expectations for the atmospheric muon and neutrino backgrounds, this flavor combination presents some tension with data. We find that, for an astrophysical neutrino E_nu^{-2} energy spectrum, (1:1:1) at Earth is currently disfav…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsHigh energyParticle physicsMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical scienceshigh-energy neutrinos01 natural sciencesIceCubeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)flavor ratios0103 physical sciencesEnergy spectrumHigh Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaFlavorNuclear and Particle Physics Proceedings
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Sterile neutrinos and flavor ratios in IceCube

2017

The flavor composition of astrophysical neutrinos observed in neutrino telescopes is a powerful discriminator between different astrophysical neutrino production mechanisms and can also teach us about the particle physics properties of neutrinos. In this paper, we investigate how the possible existence of light sterile neutrinos can affect these flavor ratios. We consider two scenarios: (i) neutrino production in conventional astrophysical sources, followed by partial oscillation into sterile states; (ii) neutrinos from dark matter decay with a primary flavor composition enhanced in tau neutrinos or sterile neutrinos. Throughout the paper, we constrain the sterile neutrino mixing parameters…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrinoHigh energyParticle physicsMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesFluxAstronomy and AstrophysicsBaseline data01 natural sciences3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsFlavorJournal of Cosmology and Astroparticle Physics
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Probing decaying heavy dark matter with the 4-year IceCube HESE data

2017

After the first four years of data taking, the IceCube neutrino telescope has observed 54 high-energy starting events (HESE) with deposited energies between 20 TeV and 2 PeV. The background from atmospheric muons and neutrinos is expected to be of about 20 events, all below 100 TeV, thus pointing towards the astrophysical origin of about 8 events per year in that data set. However, their precise origin remains unknown. Here, we perform a detailed analysis of this event sample (considering simultaneously the energy, hemisphere and topology of the events) by assuming two contributions for the signal events: an isotropic power-law flux and a flux from decaying heavy dark matter. We fit the mas…

High Energy Astrophysical Phenomena (astro-ph.HE)QuarkPhysicsSpectral indexMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesFluxAstronomy and AstrophysicsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrino detector13. Climate action0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena010306 general physicsJournal of Cosmology and Astroparticle Physics
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Hadronic light-by-light scattering contribution to the muon $g-2$ from lattice QCD: semi-analytical calculation of the QED kernel

2023

Hadronic light-by-light scattering is one of the virtual processes that causes the gyromagnetic factor $g$ of the muon to deviate from the value of two predicted by Dirac's theory. This process makes one of the largest contributions to the uncertainty of the Standard Model prediction for the muon $(g-2)$. Lattice QCD allows for a first-principles approach to computing this non-perturbative effect. In order to avoid power-law finite-size artifacts generated by virtual photons in lattice simulations, we follow a coordinate-space approach involving a weighted integral over the vertices of the QCD four-point function of the electromagnetic current carried by the quarks. Here we present in detai…

High Energy Physics - TheoryNuclear and High Energy Physicsmagnetic momentn-point function530 Physicsspace Euclidean4FOS: Physical sciences[PHYS.HLAT] Physics [physics]/High Energy Physics - Lattice [hep-lat]nonperturbativeEuclideandimension 4quarkHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)dimensionmuonquantum chromodynamicsquantum electrodynamicsphoton photoncomputerlatticeperturbation theoryphoton photon scatteringeffect nonperturbative[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat][PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]effectHigh Energy Physics - Lattice (hep-lat)scatteringphotonlattice field theoryspace530 Physikcurrent[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics - PhenomenologyelectromagneticHigh Energy Physics - Theory (hep-th)photon virtualn-point function 4finite size[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]virtual[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]current electromagnetic
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Measurement of CP asymmetry in D 0 → K - K + and D 0 → π - πdecays

2014

Time-integrated $CP$ asymmetries in $D^0$ decays to the final states $K^- K^+$ and $\pi^- \pi^+$ are measured using proton-proton collisions corresponding to $3\mathrm{\,fb}^{-1}$ of integrated luminosity collected at centre-of-mass energies of $7\mathrm{\,Te\kern -0.1em V}$ and $8\mathrm{\,Te\kern -0.1em V}$. The $D^0$ mesons are produced in semileptonic $b$-hadron decays, where the charge of the accompanying muon is used to determine the initial flavour of the charm meson. The difference in $CP$ asymmetries between the two final states is measured to be \begin{align} \Delta A_{CP} = A_{CP}(K^-K^+)-A_{CP}(\pi^-\pi^+) = (+0.14 \pm 0.16\mathrm{\,(stat)} \pm 0.08\mathrm{\,(syst)})\% \ . \nonu…

High Energy Physics::Lattice14.40.Lb01 natural sciencesLuminositySettore FIS/04 - Fisica Nucleare e SubnucleareFlavor physicsABSORPTIONPhysics::Chemical PhysicsNuclear ExperimentQCmedia_commonCharm physicsPhysicsHadronic decays of charmed mesonCharm physics; CP violation; Flavor physics; Hadron-Hadron ScatteringParticle physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronCharge conjugation parity time reversal and other discrete symmetrieFIS/01 - FISICA SPERIMENTALECP violation13.25.FtSCATTERING-AMPLITUDEFísica nuclearLHCParticle physicsCharm physicNuclear and High Energy PhysicsMesonmedia_common.quotation_subjectLHCb - Abteilung HofmannHadronsAsymmetryREGENERATIONTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYSEARCH0103 physical sciencesPiSCATTERINGSCATTERING-AMPLITUDE; REGENERATION; ABSORPTION; SEARCHSDG 7 - Affordable and Clean Energy010306 general physicsLarge Hadron Collider (France and Switzerland)/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyMuonHadron-Hadron Scattering010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGran Col·lisionador d'HadronsCharge (physics)LHCbFlavor physic11.30.ErHigh Energy Physics::ExperimentFísica de partículesExperiments13.85.NiCharmed mesons (|C|>0 B=0)FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
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Multi-boson block factorization of fermions

2017

The numerical computations of many quantities of theoretical and phenomenological interest are plagued by statistical errors which increase exponentially with the distance of the sources in the relevant correlators. Notable examples are baryon masses and matrix elements, the hadronic vacuum polarization and the light-by-light scattering contributions to the muon g-2, and the form factors of semileptonic B decays. Reliable and precise determinations of these quantities are very difficult if not impractical with state-of-the-art standard Monte Carlo integration schemes. I will review a recent proposal for factorizing the fermion determinant in lattice QCD that leads to a local action in the g…

High Energy Physics::Latticeaction: local01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Vacuum polarizationcorrelation functionQuantum Chromodynamics Lattice gauge theory Computational PhysicsMonte CarloBosonPhysicsform factorPhysicsHigh Energy Physics - Lattice (hep-lat)lattice field theoryPropagatorpropagator [quark]hep-phParticle Physics - Latticestatistical [error]Lattice QCDFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - Phenomenologyerror: statisticalquark: factorizationquark: propagatorMonte Carlo integrationQuarkParticle physicsQC1-999fermion: determinantdeterminant [fermion]FOS: Physical scienceshep-latbaryon: massHigh Energy Physics - LatticeFactorization0103 physical sciencesmagnetic moment [muon]hadronic [vacuum polarization]010306 general physicsnumerical calculationsParticle Physics - Phenomenologymuon: magnetic moment010308 nuclear & particles physicsvacuum polarization: hadronicHigh Energy Physics::Phenomenologyphoton photon: scatteringB: decaylocal [action]Fermiondecay [B]mass [baryon]scattering [photon photon]gauge field theoryHigh Energy Physics::Experimentfactorization [quark]
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"Table 4" of "Inclusive heavy-flavour production at central and forward rapidity in Xe-Xe collisions at $\sqrt {s_{NN}}$=5.44$ TeV"

2021

Transverse momentum differential production of muons from heavy-flavour hadron decays at forward rapidity in Xe-Xe collisions at 5.44 TeV.

High Energy Physics::PhenomenologyPhysics::Accelerator PhysicsHigh Energy Physics::Experiment$frac{1}{2#pi #it{p}_{T}} #frac{1}{#it{N}_{ev}} #frac{d^{2}#it{N}}{d#it{p}_{T} d#it{y}} (GeV/#it{c})^{-2}$Nuclear ExperimentXe Xe --> MUON X5440
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"Table 2" of "Inclusive heavy-flavour production at central and forward rapidity in Xe-Xe collisions at $\sqrt {s_{NN}}$=5.44$ TeV"

2021

Transverse momentum differential production of muons from heavy-flavour hadron decays at forward rapidity in Xe-Xe collisions at 5.44 TeV.

High Energy Physics::PhenomenologyPhysics::Accelerator PhysicsHigh Energy Physics::Experiment$frac{1}{2#pi #it{p}_{T}} #frac{1}{#it{N}_{ev}} #frac{d^{2}#it{N}}{d#it{p}_{T} d#it{y}} (GeV/#it{c})^{-2}$Nuclear ExperimentXe Xe --> MUON X5440
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"Table 1" of "Inclusive heavy-flavour production at central and forward rapidity in Xe-Xe collisions at $\sqrt {s_{NN}}$=5.44$ TeV"

2021

Transverse momentum differential production of muons from heavy-flavour hadron decays at forward rapidity in Xe-Xe collisions at 5.44 TeV.

High Energy Physics::PhenomenologyPhysics::Accelerator PhysicsHigh Energy Physics::Experiment$frac{1}{2#pi #it{p}_{T}} #frac{1}{#it{N}_{ev}} #frac{d^{2}#it{N}}{d#it{p}_{T} d#it{y}} (GeV/#it{c})^{-2}$Nuclear ExperimentXe Xe --> MUON X5440
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"Table 3" of "Inclusive heavy-flavour production at central and forward rapidity in Xe-Xe collisions at $\sqrt {s_{NN}}$=5.44$ TeV"

2021

Transverse momentum differential production of muons from heavy-flavour hadron decays at forward rapidity in Xe-Xe collisions at 5.44 TeV.

High Energy Physics::PhenomenologyPhysics::Accelerator PhysicsHigh Energy Physics::Experiment$frac{1}{2#pi #it{p}_{T}} #frac{1}{#it{N}_{ev}} #frac{d^{2}#it{N}}{d#it{p}_{T} d#it{y}} (GeV/#it{c})^{-2}$Nuclear ExperimentXe Xe --> MUON X5440
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