Search results for "WIMP"

showing 10 items of 76 documents

Weakly interacting dark matter from the minimal walking technicolor

2009

We study a superweakly interacting dark matter particle motivated by minimal walking technicolor theories. Our WIMP is a mixture of a sterile state and a state with the charges of a standard model fourth family neutrino. We show that the model can give the right amount of dark matter over a range of the WIMP mass and mixing angle. We compute bounds on the model parameters from the current accelerator data including the oblique corrections to the precision electroweak parameters, as well as from cryogenic experiments, Super-Kamiokande and from the IceCube experiment. We show that consistent dark matter solutions exist which satisfy all current constraints. However, almost the entire paramete…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterElectroweak interactionFOS: Physical sciencesAstronomy and AstrophysicsTechnicolorWeinberg angleCosmologyStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)WIMPHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Theories relating baryon asymmetry and dark matter

2014

The nature of dark matter and the origin of the baryon asymmetry are two of the deepest mysteries of modern particle physics. In the absence of hints regarding a possible solution to these mysteries, many approaches have been developed to tackle them simultaneously leading to very diverse and rich models. We give a short review where we describe the general features of some of these models and an overview on the general problem. We also propose a diagrammatic notation to label the different models.

PhysicsParticle physicsleptogenesisdark matterWIMP010308 nuclear & particles physicsMaterials Science (miscellaneous)General problemPhysicsDark matterBiophysicsGeneral Physics and AstronomyNotation01 natural sciencesDiagrammatic reasoningBaryon asymmetryLeptogenesisasymmetric dark matter0103 physical sciencesbaryon asymmetryddc:530electroweak phase transitionPhysical and Theoretical Chemistry010306 general physicsMathematical Physics
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Implications for relic neutralinos of the theoretical uncertainties in the neutralino-nucleon cross section

1999

We discuss the effect induced on the neutralino-nucleon cross-section by the present uncertainties in the values of the quark masses and of the quark scalar densities in the nucleon. We examine the implications of this aspect on the determination of the neutralino cosmological properties, as derived from measurements of WIMP direct detection. We show that, within current theoretical uncertainties, the DAMA annual modulation data are compatible with a neutralino as a major dark matter component, to an extent which is even larger than the one previously derived. We also comment on implications of the mentioned uncertainties for experiments of indirect dark matter detection.

PhysicsQuarkParticle physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyDark matterScalar (mathematics)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsHigh Energy Physics - PhenomenologyCross section (physics)High Energy Physics - Phenomenology (hep-ph)WIMPNeutralinoHigh Energy Physics::ExperimentNucleon
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Possibility of a dark matter interpretation for the excess in isotropic radio emission reported by ARCADE.

2011

The ARCADE 2 Collaboration has recently measured an isotropic radio emission which is significantly brighter than the expected contributions from known extra-galactic sources. The simplest explanation of such excess involves a ``new'' population of unresolved sources which become the most numerous at very low (observationally unreached) brightness. We investigate this scenario in terms of synchrotron radiation induced by weakly interacting massive particle (WIMP) annihilations or decays in extra-galactic halos. Intriguingly, for light-mass WIMPs with a thermal annihilation cross section, the level of expected radio emission matches the ARCADE observations.

Physicseducation.field_of_study010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaDark matterPopulationMassive particleGeneral Physics and AstronomyAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDark matter haloWIMPWeakly interacting massive particles0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHaloeducation010303 astronomy & astrophysicsLight dark matterAstrophysics::Galaxy AstrophysicsPhysical review letters
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IceCube: A multipurpose neutrino telescope

2008

IceCube is a new high-energy neutrino telescope which will be coming online in the near future. IceCube will be capable of measuring fluxes of all three flavors of neutrino, and its peak neutrino energy sensitivity will be in the TeV–PeV range. Here, after a brief description of the detector, we describe its anticipated performance with a selection of physics topics: supernovae, extraterrestrial diffuse and point sources of neutrinos, gamma-ray bursts, neutrinos from WIMP annihilation, and cosmic ray composition.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoGeneral Physics and AstronomyAstrophysics7. Clean energy01 natural sciencesWIMP0103 physical sciencesNeutrinos010306 general physicsCosmic rays; Neutrinos; WIMPsCosmic raysPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomySolar neutrino problemWIMPsCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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"Table 1" of "A low-mass dark matter search using ionization signals in XENON100"

2018

WIMP exclusion limit on the spin-independent WIMP-nucleon scattering cross section at 90% confidence level.

Physics::Instrumentation and DetectorsNuclear TheoryAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsSIGWIMP NUCLEON --> X
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Higgs in space!

2010

We consider the possibility that the Higgs can be produced in dark matter annihilations, appearing as a line in the spectrum of gamma rays at an energy determined by the masses of the WIMP and the Higgs itself. We argue that this phenomenon occurs generally in models in which the the dark sector has large couplings to the most massive states of the SM and provide a simple example inspired by the Randall-Sundrum vision of dark matter, whose 4d dual corresponds to electroweak symmetry-breaking by strong dynamics which respect global symmetries that guarantee a stable WIMP. The dark matter is a Dirac fermion that couples to a Z' acting as a portal to the Standard Model through its strong coupl…

QuarkParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaDark matter theoryDark matterGamma ray experimentsFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsParticle Physics - PhenomenologyPhysicsAnnihilation010308 nuclear & particles physicsElectroweak interactionAstronomy and AstrophysicsCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyDark matter experimentsDirac fermionsymbolsHiggs bosonAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeJournal of Cosmology and Astroparticle Physics
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XENON100 dark matter results from a combination of 477 live days

2016

We report on WIMP search results of the XENON100 experiment, combining three runs summing up to 477 live days from January 2010 to January 2014. Data from the first two runs were already published. A blind analysis was applied to the last run recorded between April 2013 and January 2014 prior to combining the results. The ultra-low electromagnetic background of the experiment, ~$5 \times 10^{-3}$ events/(keV$_{\mathrm{ee}}\times$kg$\times$day) before electronic recoil rejection, together with the increased exposure of 48 kg $\times$ yr improves the sensitivity. A profile likelihood analysis using an energy range of (6.6 - 43.3) keV$_{\mathrm{nr}}$ sets a limit on the elastic, spin-independe…

Scattering cross-sectionPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsProton010308 nuclear & particles physicsDark matterFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciences7. Clean energyXENON DARK MATTER WIMP TPCNuclear physicsRecoilWIMPLikelihood analysis0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Sensitivity (control systems)010306 general physicsEnergy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Novel Human-to-Human Interactions from the Evolution of HCI

2011

The interaction ways made available by the evolution of the human-computer interfaces, led to novel Human-to-Human Interaction (HHI) modes, enabling people to cooperate for almost any task any time and any where. HHI nowadays is largely indirect and mediated by a wide variety of technologies and devices. This new and exciting field of design originates from the convergence of a few well-established research fields within the HCI area, such as traditional Graphical User Interfaces (GUI), Tangible User Interfaces (TUI), Touchless Gesture User Interface (TGUI), Voice User Interfaces (VUI), and Brain Computer Interfaces (BCI). We analyze and describe the evolution of the HCI in those fields, an…

Settore ING-INF/05 - Sistemi Di Elaborazione Delle Informazionihuman-to-human interactionMultimediaComputer sciencebusiness.industryPost-WIMPmediated social interactionscomputer.software_genreField (computer science)Variety (cybernetics)novel interfacehuman-computer interactionHuman–computer interactionHuman interactionUser interfacebusinesscomputerBrain–computer interfaceGraphical user interfaceGesture2011 International Conference on Complex, Intelligent, and Software Intensive Systems
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Human-to-human interfaces: emerging trends and challenges

2011

We present a new research domain, human-to-human interaction (HHI) that describes how today's human interaction is largely indirect and mediated by a wide variety of technologies and devices. We show how this new and exciting field of design originates from the convergence of a few well-established research areas, such as traditional graphical user interfaces (GUIs), tangible user interfaces (TUIs), touchless gesture user interfaces (TGUIs), voice user interfaces (VUIs), and brain computer interfaces (BCIs). We analyse and describe current research in those areas and offer a first-hand view and presentation of its salient aspects for the human-to human interaction domain.

Settore ING-INF/05 - Sistemi Di Elaborazione Delle Informazionihuman-to-human interactionMultimediabusiness.industryComputer scienceHHIhuman-to-human interfacePost-WIMPcomputer.software_genreField (computer science)Variety (cybernetics)Domain (software engineering)Human–computer interactionUser interfacebusinesscomputerhuman-to-computer interfacesGraphical user interfaceBrain–computer interfaceGesture
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