Search results for "RADIOACTIVITY"

showing 10 items of 334 documents

Dispersion relation formalism for the two-photon exchange correction to elastic muon-proton scattering: elastic intermediate state

2018

We evaluate the two-photon exchange correction to the unpolarized cross section in the elastic muon-proton scattering within dispersion relations. One of the six independent invariant amplitudes requires a subtraction. We fix the subtraction function to the model estimate of the full two-photon exchange at one of three MUSE beam energies and make a prediction for the two other energies. Additionally, we present single and double polarization observables accounting for the lepton mass.

Physics and Astronomy (miscellaneous)Nuclear TheoryFOS: Physical scienceslcsh:Astrophysics01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Two-photon excitation microscopyDispersion relation0103 physical scienceslcsh:QB460-466Intermediate statelcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)Nuclear ExperimentPhysicsMuon010308 nuclear & particles physicsScatteringSubtractionHigh Energy Physics - PhenomenologyAmplitudeQuantum electrodynamicslcsh:QC770-798Lepton
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$\texttt{HEPfit}$: a Code for the Combination of Indirect and Direct Constraints on High Energy Physics Models

2020

The European physical journal / C Particles and fields C80(5), 456 (2020). doi:10.1140/epjc/s10052-020-7904-z

Physics and Astronomy (miscellaneous)Physics beyond the Standard ModelMonte Carlo methoddoublet: 2 [Higgs particle]Parameter space01 natural sciencesMonte Carlo: Markov chainHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)effective field theoryHigh Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Statistical physicsStandard model (cryptography)Physicsnew physicsHiggs particle: doublet: 2statistical analysis: BayesianObservablehep-phHigh Energy Physics - PhenomenologysymbolsParticle Physics - Experimentcorrection: obliqueBayesian probabilityFOS: Physical scienceslcsh:AstrophysicsMarkov chain [Monte Carlo]Bayesian [statistical analysis]530programmingSet (abstract data type)oblique [correction]symbols.namesake0103 physical scienceslcsh:QB460-466operator: dimension: 6ddc:530lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsnumerical calculationsEngineering (miscellaneous)Particle Physics - Phenomenology010308 nuclear & particles physicshep-exMarkov chain Monte Carlomanual[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798dimension: 6 [operator]
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Cutoff dependence of the thrust peak position in the dipole shower

2020

We analyse the dependence of the peak position of the thrust distribution on the cutoff value in the Nagy-Soper dipole shower. We compare the outcome of the parton shower simulations to a relation of the dependence from an analytic computation, derived within soft-collinear effective theory. We show that the result of the parton shower simulations and the analytic computation are in good agreement.

Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsComputationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical scienceslcsh:AstrophysicsThrust01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Position (vector)lcsh:QB460-4660103 physical sciencesEffective field theoryCutofflcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsParton showerEngineering (miscellaneous)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsComputational physicsDipoleHigh Energy Physics - PhenomenologyDistribution (mathematics)lcsh:QC770-798High Energy Physics::Experiment
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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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Erratum to: Monopole production via photon fusion and Drell–Yan processes: MadGraph implementation and perturbativity via velocity-dependent coupling…

2019

It has been found that the central and right-hand-side graphs in Fig. 27 were produced with an incorrect run configuration in MadGraph; the correct graphs are presented here

Physics and Astronomy (miscellaneous)lcsh:QB460-466lcsh:QC770-798lcsh:Astrophysicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityEngineering (miscellaneous)MathematicsofComputing_DISCRETEMATHEMATICSEuropean Physical Journal
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The observation of vibrating pear-shapes in radon nuclei

2019

6 pags., 4 fig.s, 1 tab. -- Open Access funded by Creative Commons Atribution Licence 4.0

Physics beyond the Standard ModelScienceNuclear TheoryGeneral Physics and Astronomychemistry.chemical_elementRadon[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular BiologyRadiumQuantum state0103 physical sciencesCP: violationground stateNuclear Physics - ExperimentPhysics::Atomic PhysicsExperimental nuclear physicslcsh:Science010306 general physicsnumerical calculationsNuclear ExperimentPhysicsMultidisciplinaryIsotope010308 nuclear & particles physicsnew physicsnucleusQradonGeneral ChemistryPublisher Correctionradiumexotic nucleielectric momentchemistryradioactivityMoment (physics)Atomic nucleusCP violationlcsh:QExotic atoms and moleculesAtomic physicsydinfysiikka
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Massless Spectra and Gauge Couplings at One-Loop on Non-Factorisable Toroidal Orientifolds

2018

So-called `non-factorisable' toroidal orbifolds can be rewritten in a factorised form as a product of three two-tori by imposing an additional shift symmetry. This finding of Blaszczyk et al., arXiv:1111.5852, provides a new avenue to Conformal Field Theory methods, by which the vector-like massless matter spectrum - and thereby the type of gauge group enhancement on orientifold invariant fractional D6-branes - and the one-loop corrections to the gauge couplings in Type IIA orientifold theories can be computed in addition to the well-established chiral matter spectrum derived from topological intersection numbers among three-cycles. We demonstrate this framework for the $\mathbb{Z}_4 \times…

PhysicsCouplingHigh Energy Physics - TheoryNuclear and High Energy PhysicsToroid010308 nuclear & particles physicsConformal field theoryFOS: Physical sciencesTorus01 natural sciencesMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Gauge groupOrientifoldQuantum electrodynamics0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityInvariant (mathematics)010306 general physicsMathematical physics
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Gravity-mediated Scalar Dark Matter in Warped Extra-Dimensions

2020

We revisit the case of scalar dark matter interacting just gravitationally with the Standard Model (SM) particles in an extra-dimensional Randall-Sundrum scenario. We assume that both, the dark matter and the Standard Model, are localized in the TeV brane and only interact via gravitational mediators, namely the graviton Kaluza-Klein modes and the radion. We analyze in detail the dark matter annihilation channel into two on-shell KK-gravitons, and contrary to previous studies which overlooked this process, we find that it is possible to obtain the correct relic abundance for dark matter masses in the range [1, 10] TeV even after taking into account the strong bounds from LHC Run II. We also…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsParticle physicsPhysics::General PhysicsLarge Hadron Collider010308 nuclear & particles physicsDark matterScalar (mathematics)GravitonFOS: Physical sciences01 natural sciencesStandard ModelGravitationExtra dimensionsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPhenomenology of Field Theories in Higher Dimensionslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityBrane010306 general physicsAstrophysics - High Energy Astrophysical Phenomena
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Generalized Ashtekar variables for Palatini f(R) models

2021

We consider special classes of Palatini f(R) theories, featured by additional Loop Quantum Gravity inspired terms, with the aim of identifying a set of modified Ashtekar canonical variables, which still preserve the SU(2) gauge structure of the standard theory. In particular, we allow for affine connection to be endowed with torsion, which turns out to depend on the additional scalar degree affecting Palatini f(R) gravity, and in this respect we successfully construct a novel Gauss constraint. We analyze the role of the additional scalar field, outlining as it acquires a dynamical character by virtue of a non vanishing Immirzi parameter, and we describe some possible effects on the area ope…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsImmirzi parameterGaussScalar (mathematics)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)Affine connection01 natural sciencesGeneral Relativity and Quantum CosmologyAshtekar variablessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityEinstein010306 general physicsScalar fieldMathematical physics
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Finite Entanglement Entropy in Asymptotically Safe Quantum Gravity

2018

Entanglement entropies calculated in the framework of quantum field theory on classical, flat or curved, spacetimes are known to show an intriguing area law in four dimensions, but they are also notorious for their quadratic ultraviolet divergences. In this paper we demonstrate that the analogous entanglement entropies when computed within the Asymptotic Safety approach to background independent quantum gravity are perfectly free from such divergences. We argue that the divergences are an artifact due to the over-idealization of a rigid, classical spacetime geometry which is insensitive to the quantum dynamics.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsQuantum dynamicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Quantum entanglementRenormalization group01 natural sciencesGeneral Relativity and Quantum CosmologySpacetime geometryTheoretical physicsQuadratic equationHigh Energy Physics - Theory (hep-th)0103 physical sciencesModels of Quantum Gravitylcsh:QC770-798Quantum gravityRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. RadioactivityQuantum field theory010306 general physics
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