Search results for "Observable"

showing 10 items of 634 documents

Discerning the Origins of the Amplitude Fluctuations in Dynamic Raman Nanospectroscopy

2012

International audience; We introduce a novel experimental and analytical method for discerning rare surface-enhanced Raman scattering (SERS) events observable at the nanoscale. We show that the kinetics of the Raman activity recorded on an isolated nanostructure is punctuated by intense and rare events of large amplitude and spectral variations. The fluctuations of thousands of SERS spectra were analyzed statistically in terms of power density functions, and the occurrence of the rare events was quantified by a wavenumber statistics. Our analysis enables one to extract valuable and unique spectroscopic signature of Raman variations usually hidden in time-average or space-average measurement…

NanostructureSURFACEELECTRODESBENZENETHIOL02 engineering and technology010402 general chemistry01 natural sciencesMolecular physicsSpectral lineRESONANCE FLUORESCENCEsymbols.namesakeOpticsRare eventsBLINKINGWavenumberSCATTERINGPhysical and Theoretical ChemistrySPECTROSCOPYChemistrybusiness.industrySERSObservable021001 nanoscience & nanotechnologySTATISTICS0104 chemical sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsGeneral EnergyAmplitudesymbolsADATOMS0210 nano-technologyRaman spectroscopybusinessRaman scattering
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Chiral theory of nucleons and pions in the presence of an external gravitational field

2020

We extend the standard second order effective chiral Lagrangian of pions and nucleons by considering the coupling to an external gravitational field. As an application we calculate one-loop corrections to the one-nucleon matrix element of the energy-momentum tensor to fourth order in chiral counting, and next-to-leading order tree-level amplitude of the pion-production in an external gravitational field. We discuss the relation of the obtained results to experimentally measurable observables. Our expressions for the chiral corrections to the nucleon gravitational form factors differ from those in the literature. That might require to revisit the chiral extrapolation of the lattice data on t…

Nuclear TheoryHigh Energy Physics::LatticeNuclear TheoryExtrapolationFOS: Physical sciences01 natural sciences530Nuclear Theory (nucl-th)GravitationHigh Energy Physics - Phenomenology (hep-ph)PionHigh Energy Physics - LatticeGravitational fieldLattice (order)0103 physical sciencesddc:530010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)ObservableHigh Energy Physics - PhenomenologyAmplitudeQuantum electrodynamicsNucleon
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Structure of transactinide nuclei with relativistic energy density functionals

2013

A microscopic theoretical framework based on relativistic energy density functionals (REDFs) is applied to studies of shape evolution, excitation spectra, and decay properties of transactinide nuclei. Axially symmetric and triaxial relativistic Hartree-Bogoliubov (RHB) calculations, based on the functional DD-PC1 and with a separable pairing interaction, are performed for the even-even isotopic chains between Fm and Fl. The occurrence of a deformed shell gap at neutron number $N=162$ and its role on the stability of nuclei in the region around $Z=108$ is investigated. A quadrupole collective Hamiltonian, with parameters determined by self-consistent constrained triaxial RHB calculations, is…

Nuclear and High Energy PhysicsNuclear TheoryTransactinide element01 natural sciencesenergy density functionalsSeparable spacesymbols.namesake0103 physical sciences010306 general physicsPhysicsta114010308 nuclear & particles physicsObservablecollective modelstransactinide nuclei ; energy density functionals ; collective modelsNATURAL SCIENCES. Physics.PRIRODNE ZNANOSTI. Fizika.transactinide nucleiTheoretical nuclear physicsPairingNeutron numberQuadrupolesymbolsAtomic physicsHamiltonian (quantum mechanics)Axial symmetry
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Weak kaon production off the nucleon and Watson's theorem

2021

We have improved the tree-level model of Ref arXiv:1004.5484 [hep-ph] for weak production of kaons off nucleons by partially restoring unitarity. This is achieved by imposing Watson's theorem to the dominant vector and axial-vector contributions in appropriate angular momentum and isospin quantum number sectors. The observable consequences of this procedure are investigated.

Nuclear and High Energy PhysicsParticle physicsAngular momentumNuclear TheoryQC1-999Nuclear TheoryFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsUnitarity010308 nuclear & particles physicsWatsonPhysicsHigh Energy Physics::PhenomenologyObservableQuantum numberHigh Energy Physics - PhenomenologyIsospinProduction (computer science)NucleonPhysics Letters B
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Phenomenology of maximal and near-maximal lepton mixing

2000

We study the phenomenological consequences of maximal and near-maximal mixing of the electron neutrino with other ($x$=tau and/or muon) neutrinos. We describe the deviations from maximal mixing in terms of a parameter $\epsilon\equiv1-2\sin^2\theta_{ex}$ and quantify the present experimental status for $|\epsilon|<0.3$. We find that the global analysis of solar neutrino data allows maximal mixing with confidence level better than 99% for $10^{-8}$ eV$^2\lsim\Delta m^2\lsim2\times10^{-7}$ eV$^2$. In the mass ranges $\Delta m^2\gsim 1.5\times10^{-5}$ eV$^2$ and $4\times10^{-10}$ eV$^2\lsim\Delta m^2\lsim2\times10^{-7}$ eV$^2$ the full interval $|\epsilon|<0.3$ is allowed within 4$\sigma$(99.9…

Nuclear and High Energy PhysicsParticle physicsAstrofísica nuclearRadiació solarSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsAsymmetryPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsDouble beta decayPhenomenological theory (Physics)Solar radiationmedia_commonParticles (Nuclear physics)PhysicsHigh Energy Physics::PhenomenologyFísicaObservableLeptonsSupernovaHigh Energy Physics - PhenomenologyLeptons (Nuclear physics)Fenomenologia (Física)High Energy Physics::ExperimentNuclear astrophysicsNeutrinoPhenomenology (particle physics)Lepton
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Neutrinos, DUNE and the world best bound on CPT invariance

2017

CPT symmetry, the combination of Charge Conjugation, Parity and Time reversal, is a cornerstone of our model building strategy and therefore the repercussions of its potential violation will severely threaten the most extended tool we currently use to describe physics, i.e. local relativistic quantum fields. However, limits on its conservation from the Kaon system look indeed imposing. In this work we will show that neutrino oscillation experiments can improve this limit by several orders of magnitude and therefore are an ideal tool to explore the foundations of our approach to Nature. Strictly speaking testing CPT violation would require an explicit model for how CPT is broken and its effe…

Nuclear and High Energy PhysicsParticle physicsCPT symmetryFOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationQuantumPhysics010308 nuclear & particles physicsOscillationHigh Energy Physics::PhenomenologyParity (physics)Observablelcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoModel buildinglcsh:Physics
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Neutrino Mass from Cosmology

2012

Neutrinos can play an important role in the evolution of the Universe, modifying some of the cosmological observables. In this contribution we summarize the main aspects of cosmological relic neutrinos and we describe how the precision of present cosmological data can be used to learn about neutrino properties, in particular their mass, providing complementary information to beta decay and neutrinoless double-beta decay experiments. We show how the analysis of current cosmological observations, such as the anisotropies of the cosmic microwave background or the distribution of large-scale structure, provides an upper bound on the sum of neutrino masses of order 1 eV or less, with very good p…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyUpper and lower boundsPartícules (Física nuclear)CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyObservableBeta decaylcsh:QC1-999High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Power Corrections to Event Shapes with Mass-Dependent Operators

2013

We introduce an operator depending on the "transverse velocity'' r that describes the effect of hadron masses on the leading 1/Q power correction to event-shape observables. Here, Q is the scale of the hard collision. This work builds on earlier studies of mass effects by Salam and Wicke [J. High Energy Phys. 05 (2001) 061] and of operators by Lee and Sterman [Phys. Rev. D 75, 014022 (2007)]. Despite the fact that different event shapes have different hadron mass dependence, we provide a simple method to identify universality classes of event shapes whose power corrections depend on a common nonperturbative parameter. We also develop an operator basis to show that at a fixed value of Q, the…

Nuclear and High Energy PhysicsParticle physicsExponentiationFOS: Physical sciences01 natural sciencesOperator (computer programming)High Energy Physics - Phenomenology (hep-ph)Factorization0103 physical sciencesRenormalonsResummationFactorization010306 general physicsMathematical physicsPhysicsQuantum chromodynamics010308 nuclear & particles physicsMultiplicative functionObservableUniversality (dynamical systems)HadronizationHigh Energy Physics - PhenomenologyQCD correctionsE&E-annihilationDistributionsResummationJet cross-sectionsQuantum chromodynamics
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Evaluating the double parton scattering contribution to Mueller-Navelet jets production at the LHC

2015

We propose a model to study the importance of double parton scattering (DPS) in Mueller-Navelet jets production at the LHC which is consistent with the BFKL framework used to compute the single parton scattering contribution to this process. We study this model in kinematics corresponding to existing and possible future measurements at the LHC and estimate the importance of this DPS contribution on relevant observables for this process, namely the cross section and the azimuthal correlation of the jets.

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciencesParton01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRapidity010306 general physicsNuclear ExperimentQuantum chromodynamicsPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyObservableHigh Energy Physics - Phenomenologydouble parton scatteringHigh Energy Physics::ExperimentLHCPhoton scattering
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A model of neutrino mass and dark matter with large neutrinoless double beta decay

2017

We propose a model where neutrino masses are generated at three loop order but neutrinoless double beta decay occurs at one loop. Thus we can have large neutrinoless double beta decay observable in the future experiments even when the neutrino masses are very small. The model receives strong constraints from the neutrino data and lepton flavor violating decays, which substantially reduces the number of free parameters. Our model also opens up the possibility of having several new scalars below the TeV regime, which can be explored at the collider experiments. Additionally, our model also has an unbroken $Z_2$ symmetry which allows us to identify a viable Dark Matter candidate.

Nuclear and High Energy PhysicsParticle physicsHiggs PhysicsDark matterFOS: Physical sciences01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)lawDouble beta decay0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsColliderPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaObservableSymmetry (physics)High Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentNeutrinoLeptonFree parameterJournal of High Energy Physics
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