Search results for "Weak"

showing 10 items of 1417 documents

Determining the dark matter mass with DeepCore

2013

Cosmological and astrophysical observations provide increasing evidence of the existence of dark matter in our Universe. Dark matter particles with a mass above a few GeV can be captured by the Sun, accumulate in the core, annihilate, and produce high energy neutrinos either directly or by subsequent decays of Standard Model particles. We investigate the prospects for indirect dark matter detection in the IceCube/DeepCore neutrino telescope and its capabilities to determine the dark matter mass.

AstrofísicaNuclear and High Energy PhysicsLarge Underground Xenon experimentAstrophysics::High Energy Astrophysical PhenomenaDark matterScalar field dark matterFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesWarm dark matter010306 general physicsLight dark matterPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmologia010308 nuclear & particles physicsHot dark matterAstronomyDetectorsHigh Energy Physics - Phenomenology13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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(Standard model) universe dominated by the right matter

2009

14 pages, 3 figures. References on late time enthropy release included, several points clarified. PACS numbers: 14.60.Pq, 98.80.Cq. ArXiv pre-print available at http://arxiv.org/abs/0806.4389

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsGrand-Unified-TheoryDark-MatterHigh Energy Physics::PhenomenologyElectroweak interactionDark matterBaryogenesisFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsTime Entropy ProductionBaryogenesisBaryon asymmetryDecaying ParticlesConstraintsHigh Energy Physics::ExperimentGravitinoNeutrinoNeutrino MassNeutrino oscillationPhenomenology (particle physics)Inflationary UniversePhysical Review D
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Electroweak baryogenesis from a dark sector

2017

Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ lepto…

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)standard model of particle physicsPhysics beyond the Standard ModelSTANDARD MODELFOS: Physical sciences01 natural sciences7. Clean energy114 Physical sciencesdark matterHiggs sectorStandard Modelpimeä aineHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesSINGLET010306 general physicsParticle Physics - PhenomenologyPhysicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalliRADIATIVE NEUTRINO MASShep-phSphaleronBaryogenesisHigh Energy Physics - Phenomenologyastro-ph.COHiggs bosonPHASE-TRANSITIONHigh Energy Physics::ExperimentMATTERAstrophysics - Cosmology and Nongalactic Astrophysics
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An original way to evaluate daily rainfall variability simulated by a regional climate model: the case of South African austral summer rainfall

2014

We discuss the value of a clustering approach as a tool for evaluating daily rainfall output from climate models. Ascendant hierarchical clustering is used to evaluate how well South African recurrent daily rainfall patterns are simulated during the austral summer (December to February 1970–1971 to 1998–1999). A set of 35-km regional climate simulations, run with the WRF model and driven by the ERA40 reanalysis, is chosen as a case study. Six recurrent patterns are identified and compared to the observed clusters obtained by applying the same methodology to 5352 daily rain gauge records. Two of the WRF clusters describe either a persistent and widespread dryness (65% of the days) or pattern…

Atmospheric Science010504 meteorology & atmospheric sciencesFrequency of occurrenceRain gauge0207 environmental engineering02 engineering and technologySpatial Projection01 natural sciencesHierarchical clustering13. Climate actionWeather Research and Forecasting ModelClimatologyWeak modelmedicineDrynessEnvironmental scienceClimate modelmedicine.symptom020701 environmental engineering0105 earth and related environmental sciencesInternational Journal of Climatology
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Observationally Weak TGFs in the RHESSI Data

2019

Abstract Terrestrial gamma ray flashes (TGFs) are sub‐millisecond bursts of high energetic gamma radiation associated with intracloud flashes in thunderstorms. In this paper we use the simultaneity of lightning detections by World Wide Lightning Location Network to find TGFs in the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) data that are too faint to be identified by standard search algorithms. A similar approach has been used in an earlier paper, but here we expand the data set to include all years of RHESSI + World Wide Lightning Location Network data and show that there is a population of observationally weak TGFs all the way down to 0.22 of the RHESSI detection thresh…

Atmospheric Science010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Atmospheric ElectricityPopulationHard radiationAstrophysics01 natural sciencesLightningterrestrial gamma‐ray flahesAerosol and CloudsLatitude0103 physical sciencesEarth and Planetary Sciences (miscellaneous)RHESSIobservationally weakeducation010303 astronomy & astrophysicsResearch Articles0105 earth and related environmental sciencesPhysicseducation.field_of_studyGamma rayNetwork datathunderstormsLightningWorld widehard radiationGeophysicsSpace and Planetary ScienceAtmospheric ProcessesThunderstormResearch ArticleJournal of Geophysical Research: Atmospheres
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Quantum localization and bound state formation in Bose-Einstein condensates

2010

We discuss the possibility of exponential quantum localization in systems of ultracold bosonic atoms with repulsive interactions in open optical lattices without disorder. We show that exponential localization occurs in the maximally excited state of the lowest energy band. We establish the conditions under which the presence of the upper energy bands can be neglected, determine the successive stages and the quantum phase boundaries at which localization occurs, and discuss schemes to detect it experimentally by visibility measurements. The discussed mechanism is a particular type of quantum localization that is intuitively understood in terms of the interplay between nonlinearity and a bou…

Atomic Physics (physics.atom-ph)FOS: Physical sciences01 natural sciencesSpectral linelocalization010305 fluids & plasmaslaw.inventionPhysics - Atomic PhysicslawQuantum mechanics0103 physical sciencesBound state010306 general physicsElectronic band structureQuantumPhysicsQuantum PhysicsAtomic and Molecular Physics and Optics3. Good healthExponential functionWeak localizationQuantum Gases (cond-mat.quant-gas)Excited stateQuantum electrodynamicsQuantum Physics (quant-ph)Condensed Matter - Quantum GasesBose–Einstein condensate
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The Belle II Physics Book

2019

cd. autorów: L. Cao48,‡, G. Caria145,‡, G. Casarosa57,‡, C. Cecchi56,‡,D. Cˇ ervenkov10,‡,M.-C. Chang22,‡, P. Chang92,‡, R. Cheaib146,‡, V. Chekelian83,‡, Y. Chen154,‡, B. G. Cheon28,‡, K. Chilikin77,‡, K. Cho70,‡, J. Choi14,‡, S.-K. Choi27,‡, S. Choudhury35,‡, D. Cinabro170,‡, L. M. Cremaldi146,‡, D. Cuesta47,‡, S. Cunliffe16,‡, N. Dash33,‡, E. de la Cruz Burelo9,‡, E. de Lucia52,‡, G. De Nardo54,‡, †Editor. ‡Belle II Collaborator. §Theory or external contributing author. M. De Nuccio16,‡, G. De Pietro59,‡, A. De Yta Hernandez9,‡, B. Deschamps129,‡, M. Destefanis60,‡, S. Dey116,‡, F.Di Capua54,‡, S.Di Carlo75,‡, J. Dingfelder129,‡, Z. Doležal10,‡, I. Domínguez Jiménez125,‡, T.V. Dong30,26,…

B: semileptonic decayPhysics beyond the Standard ModelHadronelectroproduction [charmonium]General Physics and AstronomyComputingMilieux_LEGALASPECTSOFCOMPUTINGB: radiative decayannihilation [electron positron]7. Clean energy01 natural sciencescharmonium: electroproductionB physicsHigh Energy Physics - Experimentlaw.inventionHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Z'law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Charm (quantum number)dark sector searchesPhysicslifetimeradiative decay [B]doublet [Higgs particle]new physicsPhysicsHigh Energy Physics - Lattice (hep-lat)ddc:530Electroweak interactionlepton: flavor: violationhep-phParticle Physics - LatticeMonte Carlo [numerical calculations]electron positron: colliding beamsQuarkoniumasymmetry: CPquarkonium physicselectroweak interaction: penguinHigh Energy Physics - PhenomenologyImproved performancecolliding beams [electron positron]CP violationinterfaceelectroproduction [quarkonium]electroweak precision measurementsnumerical calculations: Monte CarlophysicsParticle Physics - ExperimentperformanceParticle physicsflavor: violation [lepton]reviewhep-latFOS: Physical sciencesBELLEHigh Energy Physics - Experiment; High Energy Physics - Experiment; High Energy Physics - Lattice; High Energy Physics - Phenomenologyelectron positron: annihilationquarkonium: electroproductionCP [asymmetry]E(6)Higgs particle: doubletmixing [D0 anti-D0]Theoretical physicsCP: violation: time dependenceHigh Energy Physics - LatticeKEK-B0103 physical sciencesquantum chromodynamicshidden sector [photon]ddc:530composite010306 general physicsColliderParticle Physics - PhenomenologyHigh Energy Physics - Experiment; High Energy Physics - Lattice; High Energy Physics - Phenomenologyphoton: hidden sectorhep-ex010308 nuclear & particles physics[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]C50 Other topics in experimental particle physicsviolation: time dependence [CP]D0 anti-D0: mixingB2TiP530 PhysikExperimental physicsB: leptonic decayCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]penguin [electroweak interaction]leptonic decay [B]semileptonic decay [B]charmparticle identificationexperimental results
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CMB Anisotropy Computations Using Hydra Gas Code

2014

From FFP6 to FFP11, we presented the advances in our Cosmic Microwave Background (CMB) anisotropy computations using N-body Hydra Codes. For such computations, codes without baryons were used: First sequential versions and afterwards parallel ones. With both of them we computed the weak lensing and the Rees-Sciama contributions to the CMB angular power spectrum. Using our numerical techniques, we reported a lensing effect higher than that estimated in previous papers (for very small angular scales). Our CMB computations require less interpolations and approximations than other approaches. This could explain part of our excess of power in lensing computations. Our higher time and angular res…

BaryonPhysicsComputationCosmic microwave backgroundDark matterAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAnisotropySpectral lineWeak gravitational lensingComputational physics
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A New Numerical Approach to Estimate the Sunyaev–Zel’dovich Effect

2013

Several years ago, we designed a particular ray tracing method. Combined with a Hydra parallel code (without baryons), it may compute some CMB anisotropies: weak lensing (WL) and Rees–Sciama (RS) effects. Only dark matter is fully necessary to estimate these effects. For very small angular scales, we made an exhaustive study leading to a lensing contribution slightly—but significantly—greater than previous ones. Afterwards, the same ray tracing procedure was included in a parallel Hydra code with baryons. The resulting code was then tested. This code is being currently applied to the study of the thermal and kinetic Sunyaev–Zel’dovich (SZ) contributions to the CMB anisotropies. We present h…

BaryonPhysicsRay tracing (physics)Cosmic microwave backgroundDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsTest particleKinetic energySunyaev–Zel'dovich effectWeak gravitational lensing
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Influence of a thin horizontal weak layer on the mechanical behaviour of shallow foundations resting on sand

2021

The presence of minor details of the ground, including soil or rock masses, occurs more frequently than what is normally believed. Thin weak layers, shear bands, and slickensided surfaces can substantially affect the behaviour of foundations, as well as that of other geostructures. In fact, they can affect the failure mechanisms, the ultimate bearing capacity of footings, and the safety factor of the geotechnical system. In this research, numerically conducted through Finite Element Code Plaxis 2D, the influence of a horizontal thin weak layer on the mechanical behaviour of shallow footings was evaluated. The obtained results prove that the weak layer strongly influences both the failure me…

Bearing capacityQE1-996.5FEMSafety factorSettore ICAR/07 - GeotecnicaFoundation (engineering)GeologyWeak layerFinite element methodShear (sheet metal)Shallow foundationFailure mechanismsGeneral Earth and Planetary SciencesGeotechnical engineeringBearing capacityLayer (electronics)Shear strength (discontinuity)GeologyStrip footing
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