Search results for "Libraries"

showing 10 items of 255 documents

Minimal coupling in presence of non-metricity and torsion

2020

We deal with the question of what it means to define a minimal coupling prescription in presence of torsion and/or non-metricity, carefully explaining while the naive substitution $\partial\to\na$ introduces extra couplings between the matter fields and the connection that can be regarded as non-minimal in presence of torsion and/or non-metricity. We will also investigate whether minimal coupling prescriptions at the level of the action (MCPL) or at the level of field equations (MCPF) lead to different dynamics. To that end, we will first write the Euler-Lagrange equations for matter fields in terms of the covariant derivatives of a general non-Riemannian space, and derivate the form of the…

Physics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Space (mathematics)Computer Science::Digital Libraries01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakelcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityCovariant transformation010306 general physicsEngineering (miscellaneous)Mathematical PhysicsSpin-½Mathematical physicsMinimal couplingPhysics010308 nuclear & particles physicsCharge (physics)Mathematical Physics (math-ph)Action (physics)Connection (mathematics)Computer Science::Mathematical Softwaresymbolslcsh:QC770-798Noether's theorem
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JUNO sensitivity to low energy atmospheric neutrino spectra

2021

Atmospheric neutrinos are one of the most relevant natural neutrino sources that can be exploited to infer properties about cosmic rays and neutrino oscillations. The Jiangmen Underground Neutrino Observatory (JUNO) experiment, a 20 kton liquid scintillator detector with excellent energy resolution is currently under construction in China. JUNO will be able to detect several atmospheric neutrinos per day given the large volume. A study on the JUNO detection and reconstruction capabilities of atmospheric $\nu_e$ and $\nu_\mu$ fluxes is presented in this paper. In this study, a sample of atmospheric neutrino Monte Carlo events has been generated, starting from theoretical models, and then pro…

Physics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidenergy resolutionAtmospheric neutrinoQC770-798Astrophysics7. Clean energy01 natural sciencesneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)particle source [neutrino]neutrinoneutrino: atmosphere[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Cherenkovneutrino/e: particle identificationenergy: low [neutrino]Jiangmen Underground Neutrino ObservatoryPhysicsJUNOphotomultiplierliquid [scintillation counter]primary [neutrino]neutrino: energy spectrumDetectoroscillation [neutrino]neutrinosMonte Carlo [numerical calculations]atmosphere [neutrino]QB460-466observatorycosmic radiationComputer Science::Mathematical Softwareproposed experimentNeutrinonumerical calculations: Monte CarloComputer Science::Machine LearningParticle physicsdata analysis methodAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScintillatorComputer Science::Digital LibrariesNOStatistics::Machine LearningPE2_2neutrino: primaryneutrino: spectrumNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530structure010306 general physicsNeutrino oscillationEngineering (miscellaneous)Cherenkov radiationparticle identification [neutrino/mu]Scintillationneutrino/mu: particle identificationflavordetectorparticle identification [neutrino/e]010308 nuclear & particles physicsneutrino: energy: lowHigh Energy Physics::Phenomenologyspectrum [neutrino]resolutionenergy spectrum [neutrino]flux [neutrino]neutrino: particle source13. Climate actionHigh Energy Physics::Experimentneutrino: oscillationneutrino detector
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Dark matter stability and Dirac neutrinos using only Standard Model symmetries

2020

We provide a generic framework to obtain stable dark matter along with naturally small Dirac neutrino masses generated at the loop level. This is achieved through the spontaneous breaking of the global $U(1)_{B-L}$ symmetry already present in Standard Model. The $U(1)_{B-L}$ symmetry is broken down to a residual even $\mathcal{Z}_n$; $n \geq 4$ subgroup. The residual $\mathcal{Z}_n$ symmetry simultaneously guarantees dark matter stability and protects the Dirac nature of neutrinos. The $U(1)_{B-L}$ symmetry in our setup is anomaly free and can also be gauged in a straightforward way. Finally, we present an explicit example using our framework to show the idea in action.

Physics010308 nuclear & particles physicsDark matterDirac (software)FOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesAction (physics)Symmetry (physics)ddc:Standard Model (mathematical formulation)Theoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHomogeneous spaceAnomaly (physics)Neutrino010306 general physics
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SO(3) family symmetry and axions

2018

Motivated by the idea of comprehensive unification, we study a gauged SO(3) flavor extension of the extended Standard Model, including right-handed neutrinos and a Peccei-Quinn symmetry with simple charge assignments. The model accommodates the observed fermion masses and mixings and yields a characteristic, successful relation among them. The Peccei-Quinn symmetry is an essential ingredient.

Physics010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesCharge (physics)FermionComputer Science::Digital Libraries01 natural sciencesSymmetry (physics)High Energy Physics - PhenomenologyTheoretical physicsStandard Model (mathematical formulation)High Energy Physics - Phenomenology (hep-ph)Simple (abstract algebra)0103 physical sciencesNeutrino010306 general physicsAxionRotation group SOPhysical Review D
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Dynamical symmetry breaking and fermion mass hierarchy in the scale-invariant 3-3-1 model

2020

We propose an extension of the Standard Model (SM) based on the $SU(3)_C\otimes SU(3)_L\otimes U(1)_X$ (3-3-1) gauge symmetry and scale invariance. Maintaining the main features of the so-called 3-3-1 models, such as the cancellation of gauge anomalies related to the number of chiral fermion generations, this model exhibits a very compact scalar sector. Only two scalar triplets and one singlet are necessary and sufficient to break the symmetries dynamically via the Coleman-Weinberg mechanism. With the introduction of an Abelian discrete symmetry and assuming a natural hierarchy among the vacuum expectation values of the neutral scalar fields, we show that all particles in the model can get …

Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyScalar (mathematics)FOS: Physical sciencesFermionComputer Science::Digital Libraries01 natural sciencesSymmetry (physics)Standard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanism0103 physical sciences010306 general physicsMathematical physicsBosonGauge symmetryDiscrete symmetryPhysical Review D
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Next-to-leading order Balitsky-Kovchegov equation beyond large Nc

2020

We calculate finite-Nc corrections to the next-to-leading order (NLO) Balitsky-Kovchegov (BK) equation. We find analytical expressions for the necessary correlators of six Wilson lines in terms of the two-point function using the Gaussian approximation. In a suitable basis, the problem reduces from the diagonalization of a six-by-six matrix to the diagonalization of a three-by-three matrix, which can easily be done analytically. We study numerically the effects of these finite-Nc corrections on the NLO BK equation. In general, we find that the finite-Nc corrections are smaller than the expected 1/Nc2∼10%. The corrections may be large for individual correlators, but have less of an influence…

PhysicsBasis (linear algebra)010308 nuclear & particles physicsFunction (mathematics)114 Physical sciences01 natural sciencesComputer Science::Digital LibrariesGaussian approximationMatrix (mathematics)DipoleAmplitude0103 physical sciencesOrder (group theory)Rapidity010306 general physicsMathematical physicsPhysical Review
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Testing WWγ vertex in radiative muon decay

2019

Large numbers of muons will be produced at facilities developed to probe the lepton-flavor-violating process μ→eγ. We show that by constructing a suitable asymmetry, radiative muon decay μ→eγνμν̄e can also be used to test the WWγ vertex at such facilities. The process has two missing neutrinos in the final state, and upon integrating their momenta the partial differential decay rate shows no radiation-amplitude zero. However, we establish that an easily separable part of the normalized differential decay rate that is odd under the exchange of photon and electron energies does have a zero in the case of the standard model (SM). This new type of zero has hitherto not been studied in the liter…

PhysicsConservation lawParticle physicsPhotonMuon010308 nuclear & particles physicsmedia_common.quotation_subjectElectronComputer Science::Digital Libraries01 natural sciencesAsymmetryVertex (geometry)Separable space0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsmedia_commonPhysical Review D
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Flavor of cosmic neutrinos preserved by ultralight dark matter

2019

Within the standard propagation scenario, the flavor ratios of high-energy cosmic neutrinos at neutrino telescopes are expected to be around the democratic benchmark resulting from hadronic sources, $\left( 1 : 1 : 1 \right)_\oplus$. We show how the coupling of neutrinos to an ultralight dark matter complex scalar field would induce an effective neutrino mass that could lead to adiabatic neutrino propagation. This would result in the preservation at the detector of the production flavor composition of neutrinos at sources. This effect could lead to flavor ratios at detectors well outside the range predicted by the standard scenario of averaged oscillations. We also present an electroweak-in…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Particle physicsRange (particle radiation)COSMIC cancer database010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterHadronHigh Energy Physics::PhenomenologyFOS: Physical sciencesCoupling (probability)Computer Science::Digital Libraries7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsAdiabatic processAstrophysics - High Energy Astrophysical PhenomenaScalar field
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Enumerating higher-dimensional operators with on-shell amplitudes

2020

We establish a simple formula for the minimal dimension of operators leading to any helicity amplitude. It eases the systematic enumeration of independent operators from the construction of massless non-factorizable on-shell amplitudes. Little-group constraints can then be solved algorithmically for each helicity configuration to extract a complete set of spinor structures with lowest dimension. Occasionally, further reduction using momentum conservation, on-shell conditions and Schouten identities is required. A systematic procedure to account for the latter is presented. Dressing spinor structures with dot products of momenta finally yields the independent Lorentz structures for each heli…

PhysicsHigh Energy Physics - TheorySpinor010308 nuclear & particles physicsLorentz transformationGravitonFOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesHelicitysymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Dimension (vector space)0103 physical sciencessymbolsEffective field theory010306 general physicsMathematical physicsGauge symmetrySpin-½
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Jet transition values for the anti-$$k_{\bot }$$ k⊥ algorithm

2019

We define jet transition values for the anti-$k_{\bot}$ algorithm for both hadron and $e^+e^-$ colliders. We show how these transition values can be computed and how they can be used to improve the performance of clusterization when jet resolution parameters are varied over a larger set of values. Finally we present a simple performance test to illustrate the behavior of the new method compared to the original one.

PhysicsJet (fluid)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsHadronFOS: Physical scienceslcsh:Astrophysics01 natural sciencesComputer Science::Digital LibrariesHigh Energy Physics - ExperimentSet (abstract data type)High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::Experiment010306 general physicsEngineering (miscellaneous)AlgorithmComputer Science::DatabasesEuropean Physical Journal
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