Search results for " connection"

showing 10 items of 138 documents

First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

PHOTINOAstrophysicsMASSIVE PARTICLES01 natural sciencesLIMITSDirect searchCANDIDATESPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilationdark matter detectors[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsAstrophysics::Instrumentation and Methods for AstrophysicsCAPTURELIGHTparticle physics - cosmology connectionWeakly interacting massive particlesneutrino experiments; particle physics - cosmology connection; dark matter detectors; supersymmetry and cosmologyFísica nuclearNeutrinosupersymmetry andAstrophysics - High Energy Astrophysical PhenomenaCosmology connectionsupersymmetry and cosmologyFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Supersymmetry and cosmologydark matter detectorAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeDark matterFOS: Physical sciencesddc:500.2neutrino experimentsSEARCH0103 physical sciencesDETECTORS010306 general physicsSelection (genetic algorithm)Dark matter detectors010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsNeutrino experimentsFISICA APLICADAParticle physics - cosmology connectionneutrino experimentHigh Energy Physics::ExperimentcosmologySYSTEM
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On thermo-mechanical issues induced by irradiation swelling inside the back-plate of the IFMIF target assembly

2011

Abstract Within the framework of the IFMIF R&D program and in close cooperation with ENEA-Brasimone, at the Department of Nuclear Engineering of the University of Palermo a research campaign has been launched to investigate the thermo-mechanical issues potentially induced by irradiation swelling in the threaded connections between frame and back-plate of IFMIF target assembly. The main aim of the research campaign has relied in the assessment of the maximum swelling-induced volumetric strain that may be accepted in order to allow screws to withstand thermo-mechanical stresses and work in safe conditions or to avoid unduly high unscrewing torques during back-plate remotely handled maintenanc…

Parametric analysisComputer sciencebusiness.industryMechanical EngineeringFrame (networking)Structural engineeringFinite element methodNuclear Energy and EngineeringmedicineTorqueGeneral Materials ScienceBoundary value problemIrradiationSwellingmedicine.symptomIFMIF Irradiation swelling Threaded connection FEM analysisbusinessSettore ING-IND/19 - Impianti NucleariThermo mechanicalCivil and Structural EngineeringFusion Engineering and Design
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The full Boltzmann hierarchy for dark matter-massive neutrino interactions

2020

The impact of dark matter-neutrino interactions on the measurement of the cosmological parameters has been investigated in the past in the context of massless neutrinos exclusively. Here we revisit the role of a neutrino-dark matter coupling in light of ongoing cosmological tensions by implementing the full Boltzmann hierarchy for three massive neutrinos. Our tightest 95% CL upper limit on the strength of the interactions, parameterized via $u_\chi =\frac{\sigma_0}{\sigma_{Th}}\left(\frac{m_\chi}{100 \text{GeV}}\right)^{-1}$, is $u_\chi\leq3.34 \cdot 10^{-4}$, arising from a combination of Planck TTTEEE data, Planck lensing data and SDSS BAO data. This upper bound is, as expected, slightly …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesContext (language use)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckWeak gravitational lensingneutrino propertiesPhysicsdark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Massless particleHigh Energy Physics - Phenomenologyparticle physics-cosmology connectioncosmological perturbation theorysymbolsNeutrinoHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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A model for dark matter, naturalness and a complete gauge unification

2015

We consider dark matter in a minimal extension of the Standard Model (SM) which breaks electroweak symmetry dynamically and leads to a complete unification of the SM and technicolor coupling constants. The unification scale is determined to be $M_{\rm U} \approx 2.2 \times 10^{15}$ GeV and the unified coupling $\alpha_{\rm U} \approx 0.0304$. Moreover, unification strongly suggest that the technicolor sector of the model must become strong at the scale of ${\cal O}$(TeV). The model also contains a tightly constrained sector of mixing neutral fields stabilized by a discrete symmetry. We find the lightest of these states can be DM with a mass in the range $m_{\rm DM} \approx 30-800$ GeV. We f…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesTechnicolorParameter space01 natural sciences7. Clean energyStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCoupling constantPhysicsdark matter theory010308 nuclear & particles physicsdark matter experimentsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsCoupling (probability)High Energy Physics - Phenomenologyparticle physics - cosmology connectionHigh Energy Physics::ExperimentDiscrete symmetryAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings

2017

Apparent metastability of the electroweak vacuum poses a number of cosmological questions. These concern evolution of the Higgs field to the current vacuum, and its stability during and after inflation. Higgs-inflaton and non-minimal Higgs-gravity interactions can make a crucial impact on these considerations potentially solving the problems. In this work, we allow for these couplings to be present simultaneously and study their interplay. We find that different combinations of the Higgs-inflaton and non-minimal Higgs-gravity couplings induce effective Higgs mass during and after inflation. This crucially affects the Higgs stability considerations during preheating. In particular, a wide ra…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Metastability0103 physical sciencesphysics of the early universeinflationparticle physicscosmology connectionELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMmedia_commonInflation (cosmology)PhysicsSTABILITY010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsBOSONInflaton115 Astronomy Space scienceUniverseHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Observational signatures of Higgs inflation

2016

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the scenario robustly predicts the spectral index $n_s \simeq 0.97$ and the tensor-to-scalar ratio $r\simeq 0.003$. The matching is however non-trivial, even the best-fit values $m_h=125.09$ GeV and $m_t=173.21$ GeV require a jump $\delta \lambda \sim 0.01$ in the Higgs coupling below the inflationary scale. For $m_t\lesssim 171.8$ GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of $n_s$ and $r$ vary but…

Particle physicsMatching (statistics)Cosmology and Nongalactic Astrophysics (astro-ph.CO)STANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesphysics of the early universeinflationELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMBosonInflation (cosmology)PhysicsSpectral index010308 nuclear & particles physicsINDUCED GRAVITY INFLATIONHigh Energy Physics::PhenomenologySpectral densityBOSONAstronomy and Astrophysics115 Astronomy Space scienceHigh Energy Physics - Phenomenologyparticle physics - cosmology connectionJumpHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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A new control system prototype for the energy production maximization of a unequally irradiated PV system

2011

This paper deals with the mismatch effect due to a unequally irradiation on a PV (PhotoVoltaic) system. The mismatch effect due to the partial shading of a PV module can be limited thanks to the installation of both bypass and block diodes. Unfortunately, this solution cannot fully solve the disvantages related to the mismatch effect. The Authors, in previous papers [1, 2], have theoretically demonstrated that the mismatch effect can be solved by changing the parallel/series connections of the modules of a PV system, taking into account each module radiating condition. This paper represents a first step of the experimental development of the above mentioned theoretical result. Specifically,…

PhotoVoltaic mismatch series/parallel connections FPGA controllerSettore ING-IND/32 - Convertitori Macchine E Azionamenti Elettrici
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Metric-affine f(R,T) theories of gravity and their applications

2018

We study $f(R,T)$ theories of gravity, where $T$ is the trace of the energy-momentum tensor ${T}_{\ensuremath{\mu}\ensuremath{\nu}}$, with independent metric and affine connection (metric-affine theories). We find that the resulting field equations share a close resemblance with their metric-affine $f(R)$ relatives once an effective energy-momentum tensor is introduced. As a result, the metric field equations are second-order and no new propagating degrees of freedom arise as compared to GR, which contrasts with the metric formulation of these theories, where a dynamical scalar degree of freedom is present. Analogously to its metric counterpart, the field equations impose the nonconservatio…

Physics010308 nuclear & particles physics0103 physical sciencesScalar (mathematics)Degrees of freedom (statistics)Weak fieldAffine transformationAffine connectionPoisson's equation010306 general physicsField equation01 natural sciencesMathematical physicsPhysical Review D
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Berry-curvatures and anomalous Hall effect in Heusler compounds

2011

Berry curvatures are computed for a set of Heusler compounds using density functional calculations and the wave functions that they provide. The anomalous Hall conductivity is obtained from the Berry curvatures. It is compared with experimental values in the case of Co${}_{2}$CrAl and Co${}_{2}$MnAl. A notable trend cannot be seen but the range of values is quite enormous. The results for the anomalous Hall conductivities and their large variations as well as the degree of the spin polarization of the Hall current can be qualitatively understood by means of the band structure and the Fermi-surface topology.

PhysicsCondensed Matter - Materials ScienceCurrent (mathematics)Degree (graph theory)Spin polarizationCondensed matter physicsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesComputational Physics (physics.comp-ph)Condensed Matter PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall EffectElectronic Optical and Magnetic MaterialsHall conductivityHall effectQuantum mechanicsBerry connection and curvatureElectronic band structurePhysics - Computational PhysicsTopology (chemistry)
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Dzyaloshinskii-Moriya Interaction and Hall Effects in the Skyrmion Phase ofMn1−xFexGe

2015

We carry out density functional theory calculations which demonstrate that the electron dynamics in the Skyrmion phase of Fe-rich Mn_{1-x}Fe_{x}Ge alloys is governed by Berry phase physics. We observe that the magnitude of the Dzyaloshinskii-Moriya interaction directly related to the mixed space-momentum Berry phases, changes sign and magnitude with concentration x in direct correlation with the data of Shibata et al. [Nat. Nanotechnol. 8, 723 (2013)]. The computed anomalous and topological Hall effects in FeGe are also in good agreement with available experiments. We further develop a simple tight-binding model able to explain these findings. Finally, we show that the adiabatic Berry phase…

PhysicsCondensed matter physicsSkyrmionSPIN-DENSITY WAVEGeneral Physics and Astronomy02 engineering and technologyCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnology01 natural sciencesCRYSTALSLATTICEGeometric phaseAb initio quantum chemistry methodsLattice (order)MAGNETIC SKYRMIONSMNSI0103 physical sciencesSpin density waveDensity functional theoryMETALSBerry connection and curvature010306 general physics0210 nano-technologyAdiabatic processAPPROXIMATIONPhysical Review Letters
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