Search results for " phenomenology"

showing 10 items of 3693 documents

胡塞尔现象学中人类社会的动物根源 (Version chinoise de « The Animal Roots of Human Society in Husserls Phenomenology)

2012

International audience

[SHS.PHIL] Humanities and Social Sciences/Philosophy[ SHS.PHIL ] Humanities and Social Sciences/PhilosophyHuman Society[ SHS ] Humanities and Social Sciences[SHS.PHIL]Humanities and Social Sciences/Philosophy[SHS] Humanities and Social SciencesAnimal RootsHusserls PhenomenologyComputingMilieux_MISCELLANEOUS[SHS]Humanities and Social Sciences
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The Pros and Cons of Beyond Standard Model Interpretations of ANITA Events

2019

The Antarctic Impulsive Transient Antenna (ANITA) experiment has observed two air shower events with energy $\sim 500~{\rm PeV}$ emerging from the Earth with exit angles $\sim 30^\circ$ above the horizon. As was immediately noted by the ANITA Collaboration, these events (in principle) could originate in the atmospheric decay of an upgoing $\tau$-lepton produced through a charged current interaction of a $\nu_\tau$ inside the Earth. However, the relatively steep arrival angles of these perplexing events create tension with the standard model (SM) neutrino-nucleon interaction cross section. Deepening the conundrum, the IceCube neutrino telescope and the Pierre Auger Observatory with substanti…

airAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesparticle: messengerAstrophysics01 natural scienceshorizonneutrino nucleon: interactioncharged currentIceCubeHigh Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciences010306 general physicsCharged currentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger Observatoryneutrino/tauCOSMIC cancer databaseshowers: atmosphere010308 nuclear & particles physicsHorizonANITAAstrophysics::Instrumentation and Methods for AstrophysicstensionsensitivityAugerfluxobservatoryHigh Energy Physics - Phenomenologyneutrino: detectorAir showerNeutrino detector[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
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Constraints on neutrino speed, weak equivalence principle violation, Lorentz invariance violation, and dual lensing from the first high-energy astrop…

2018

We derive stringent constraints on neutrino speed, weak equivalence principle violation, Lorentz invariance violation, and dual lensing from the first high-energy astrophysical neutrino source: TXS 0506+056. Observation of neutrino (IceCube-170922A) and photons in a similar time frame and from the same direction is used to derive these limits. We describe ways in which these constraints can be further improved by orders of magnitude.

astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)High Energy Physics - TheoryAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)hep-exhep-thAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-phHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)astro-ph.COHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaParticle Physics - TheoryParticle Physics - ExperimentParticle Physics - PhenomenologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for Axionlike Dark Matter through Nuclear Spin Precession in Electric and Magnetic Fields

2017

We report on a search for ultralow-mass axionlike dark matter by analyzing the ratio of the spinprecession frequencies of stored ultracold neutrons and 199Hg atoms for an axion-induced oscillating electric dipole moment of the neutron and an axion-wind spin-precession effect. No signal consistent with dark matter is observed for the axion mass range 10−24 ≤ ma ≤ 10−17 eV. Our null result sets the first laboratory constraints on the coupling of axion dark matter to gluons, which improve on astrophysical limits by up to 3 orders of magnitude, and also improves on previous laboratory constraints on the axion coupling to nucleons by up to a factor of 40. ispartof: Physical Review X vol:7 issue:…

axionsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryAtomic Physics (physics.atom-ph)Physics::Instrumentation and Detectors[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]QC1-999FOS: Physical sciencesmagnetic field[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterPhysics - Atomic PhysicsNuclear Theory (nucl-th)High Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph][ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]axion: couplingNuclear Experiment (nucl-ex)gluon: couplingNuclear Experiment[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]spin: precessionaxion: dark mattern: electric momentnucleus: spinatomPhysicsHigh Energy Physics::Phenomenologyspin precessionoscillation[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]neutron electric dipole momentelectric fieldHigh Energy Physics - PhenomenologyS029IAN[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axion: mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental resultsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review X
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Detecting the stimulated decay of axions at radio frequencies

2018

Assuming axion-like particles account for the entirety of the dark matter in the Universe, we study the possibility of detecting their decay into photons at radio frequencies. We discuss different astrophysical targets, such as dwarf spheroidal galaxies, the Galactic Center and halo, and galaxy clusters. The presence of an ambient radiation field leads to a stimulated enhancement of the decay rate; depending on the environment and the mass of the axion, the effect of stimulated emission may amplify the photon flux by serval orders of magnitude. For axion-photon couplings allowed by astrophysical and laboratory constraints(and possibly favored by stellar cooling), we find the signal to be wi…

axionsPhotonAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio telescopeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesStimulated emissionAxionGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsdark matter detectorsdark matter theory010308 nuclear & particles physicsGalactic CenterAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiesdwarfs galaxiesGalaxy3. Good healthHigh Energy Physics - Phenomenologyaxions; dark matter detectors; dark matter theory; dwarfs galaxiesAstrophysics of Galaxies (astro-ph.GA)Journal of Cosmology and Astroparticle Physics
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B-meson hadroproduction in the SACOT-mT scheme

2023

We apply the SACOT-mT general-mass variable flavour number scheme (GM-VFNS) to the inclusive B-meson production in hadronic collisions at next-to-leading order in perturbative Quantum Chromodynamics. In the GM-VFNS approach one matches the fixed-order heavy-quark production cross sections, accurate at low transverse momentum (pT), with the zero-mass cross sections, accurate at high pT. The physics idea of the SACOT-mT scheme is to do this by accounting for the finite momentum transfer required to create a heavy quark-antiquark pair throughout the calculation. We compare our results with the latest LHC data from proton-proton and proton-lead collisions finding a very good agreement within th…

bottom quarksParton distributionsspecific QCD phenomenology
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Motivational Analysis in Husserl’s Genetic Phenomenology

2018

The paper discusses motivation as the inner lawfulness of consciousness and a central methodological principle of genetic phenomenology, highlighting the problem of its ambiguous status oscillating between a historical-empirical and a transcendental account of consciousness. The focus on motivation allows for the practical character of intentionality to emerge, thus presenting genetic phenomenology as a more comprehensive approach to subjective life which takes into account its constitutive indeterminacy.

constitution motivation association practical intentionality genetic phenomenologySettore M-FIL/03 - Filosofia Morale
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The effective cross section for double parton scattering within a holographic AdS/QCD approach

2017

A first attempt to apply the AdS/QCD framework for a bottom-up approach to the evaluation of the effective cross section for double parton scattering in proton-proton collisions is presented. The main goal is the analytic evaluation of the dependence of the effective cross section on the longitudinal momenta of the involved partons, obtained within the holographic Soft-Wall model. If measured in high-energy processes at hadron colliders, this momentum dependence could open a new window on 2-parton correlations in a proton.

correlation: two-particleNuclear and High Energy PhysicsParticle physicsp p: scatteringNuclear TheoryProton[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryHadronFOS: Physical sciencesParton01 natural sciences[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]quantum chromodynamics: holographyNuclear Theory (nucl-th)Nuclear physicsMomentumCross section (physics)12.38.AwHigh Energy Physics - Phenomenology (hep-ph)parton: multiple scattering0103 physical sciencesparton: correlation010306 general physicsNuclear Experimentparton: interaction[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Quantum chromodynamicsPhysicsAdS/CFT correspondence010308 nuclear & particles physicsScattering[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics::Phenomenology12.39.Kilcsh:QC1-999High Energy Physics - PhenomenologyAdS/CFT correspondence[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]14.20.DhPhysics::Accelerator Physics[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentlcsh:Physics
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A strong electroweak phase transition from the inflaton field

2016

We study a singlet scalar extension of the Standard Model. The singlet scalar is coupled non-minimally to gravity and assumed to drive inflation, and also couple sufficiently strongly with the SM Higgs field in order to provide for a strong first order electroweak phase transition. Requiring the model to describe inflation successfully, be compatible with the LHC data, and yield a strong first order electroweak phase transition, we identify the regions of the parameter space where the model is viable. We also include a singlet fermion with scalar coupling to the singlet scalar to probe the sensitivity of the constraints on additional degrees of freedom and their couplings in the singlet sec…

cosmological inflationParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelScalar (mathematics)Degrees of freedom (physics and chemistry)FOS: Physical sciences01 natural sciences7. Clean energyStandard ModelGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsInflatonextensions of the Standard ModelHiggs fieldHigh Energy Physics - Phenomenologyelectroweak phase transitionAstrophysics - Cosmology and Nongalactic Astrophysics
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Estimating QCD uncertainties in Monte Carlo event generators for gamma-ray dark matter searches

2018

Motivated by the recent galactic center gamma-ray excess identified in the Fermi-LAT data, we perform a detailed study of QCD fragmentation uncertainties in the modeling of the energy spectra of gamma-rays from Dark-Matter (DM) annihilation. When Dark-Matter particles annihilate to coloured final states, either directly or via decays such as $W^{(*)}\to q\bar{q}'$, photons are produced from a complex sequence of shower, hadronisation and hadron decays. In phenomenological studies, their energy spectra are typically computed using Monte Carlo event generators. These results have however intrinsic uncertainties due to the specific model used and the choice of model parameters, which are diffi…

dark matter simulationsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonAstrophysics::High Energy Astrophysical Phenomenamodel [hadronization]SLDgamma ray theoryDark matterMonte Carlo methodHadronFOS: Physical sciencesmass [dark matter]01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)fragmentationquantum chromodynamics0103 physical sciencesconservation lawddc:530High Energy PhysicsMonte Carloenergy spectrum [gamma ray]Quantum chromodynamicsPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsphotonGamma rayCERN LEP StorAstronomy and AstrophysicsshowersGalaxyHigh Energy Physics - PhenomenologyannihilationExperimental High Energy PhysicsHigh Energy Physics::Experimentgalaxydecay [hadron]GLAST [interpretation of experiments]Astrophysics - Cosmology and Nongalactic Astrophysics
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