Search results for "Planck"

showing 10 items of 159 documents

Search for extra dimensions in diphoton events from proton-proton collisions at root s=7 TeV in the ATLAS detector at the LHC

2013

The large difference between the Planck scale and the electroweak scale, known as the hierarchy problem, is addressed in certain models through the postulate of extra spatial dimensions. A search for evidence of extra spatial dimensions in the diphoton channel has been performed using the full set of proton–proton collisions at √s = 7 TeV recorded in 2011 with the ATLAS detector at the CERN Large Hadron Collider. This dataset corresponds to an integrated luminosity of 4.9fb[superscript −1]. The diphoton invariant mass spectrum is observed to be in good agreement with the Standard Model expectation. In the context of the model proposed by Arkani–Hamed, Dimopoulos and Dvali, 95% confidence le…

Particle physicsSignalsGravityGeneral Physics and Astronomyddc:500.201 natural sciencesNuclear physicsElectroweak scale; Planck scale; hierarchy problemContact InteractionsHierarchy0103 physical sciencesColliders[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]CutoffInvariant massddc:530EXTRA DIMENSIONSHierarchy problem010306 general physicsQCPhysicsddc:539Integrated luminosityLarge Hadron ColliderProton proton collisions010308 nuclear & particles physicsAtlas (topology)Parton DistributionsPhysicsSettore FIS/01 - Fisica SperimentaleHigh Energy Physics::PhenomenologyGravitonConfidence levelsFísicaHierarchy problemSpatial dimensionFermion-Pair ProductionCollaborationExtra dimensionsThe standard modelLarge Hadron ColliderInvariant-mass spectraHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentElectroweak scaleModel
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Higgs-portal assisted Higgs inflation with a sizeable tensor-to-scalar ratio

2014

We show that the Higgs portal interactions involving extra dark Higgs field can save generically the original Higgs inflation of the standard model (SM) from the problem of a deep non-SM vacuum in the SM Higgs potential. Specifically, we show that such interactions disconnect the top quark pole mass from inflationary observables and allow multi-dimensional parameter space to save the Higgs inflation, thanks to the additional parameters (the dark Higgs boson mass $m_{\phi}$, the mixing angle $\alpha$ between the SM Higgs $H$ and dark Higgs $\Phi$, and the mixed quartic coupling) affecting RG-running of the Higgs quartic coupling. The effect of Higgs portal interactions may lead to a larger t…

Particle physicsTop quarkCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelHigh Energy Physics::LatticeScalar (mathematics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010306 general physicsInflation (cosmology)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsHiggs fieldHigh Energy Physics - PhenomenologysymbolsHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Electron channeling experiments with bent silicon single crystals—a reanalysis based on a modified Fokker-Planck equation

2020

A surprising small dechanneling length was observed at (111) channeling of ultrarelativistic electrons in a 60 $\mu$m thick silicon single crystal with a bending radius of 0.15 m. The experiments were conducted at beam energies between 3.35 and 14 GeV at the Facility for Advanced Accelerator Experimental Tests (FACET at SLAC, USA). It is shown in this paper that the small dechanneling lengths can well be reproduced with a modified Fokker-Planck equation for plane crystals in which a crystal bending has been heuristically introduced. Encouraged by this result experiments have been reconsidered which were performed at the Mainz Microtron MAMI with (110) silicon undulator crystals. The results…

PhysicsAccelerator Physics (physics.acc-ph)Silicon010308 nuclear & particles physicsBent molecular geometrychemistry.chemical_elementFOS: Physical sciencesElectronUndulator01 natural sciencesCrystalchemistry0103 physical sciencesPhysics::Accelerator PhysicsFokker–Planck equationPhysics - Accelerator PhysicsAtomic physics010306 general physicsInstrumentationMicrotronMathematical PhysicsBeam (structure)Journal of Instrumentation
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Constraining dark matter late-time energy injection: decays and p-wave annihilations

2013

We use the latest cosmic microwave background (CMB) observations to provide updated constraints on the dark matter lifetime as well as on p-wave suppressed annihilation cross sections in the 1 MeV to 1 TeV mass range. In contrast to scenarios with an s-wave dominated annihilation cross section, which mainly affect the CMB close to the last scattering surface, signatures associated with these scenarios essentially appear at low redshifts ($z \lesssim 50$) when structure began to form, and thus manifest at lower multipoles in the CMB power spectrum. We use data from Planck, WMAP9, SPT and ACT, as well as Lyman-$\alpha$ measurements of the matter temperature at $z \sim 4$ to set a 95 % confide…

PhysicsAnnihilationStructure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterCosmic microwave backgroundCosmic background radiationFísicaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energyRedshiftdark matterHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)13. Climate actionsymbolsPlanckAstrophysics - Cosmology and Nongalactic Astrophysics
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Deconvolving the Beam in Small Angular Scale CMB Experiments

2000

This paper is concerned with experiments which measure CMB anisotropies on small angular scales. A certain coverage, a beam structure and a level of uncorrelated noise define each experiment. We focus our atention on the reversion of the beam average. In each experiment, we look for the best pixelization for reversion, namely, for the pixelization that -after reversion- leads to good maps containing right spectra for the most wide range of angular scales. Squared pixels having different sizes "smaller" than the beam radius are considered. For a given size, the following question arises: How well can we assign a temperature to each pixel? Various mathematical methods are used to show that, i…

PhysicsAstrophysics (astro-ph)Cosmic microwave backgroundFOS: Physical sciencesSpectral densityAstronomy and AstrophysicsAstrophysicsRadiusAstrophysicsNoise (electronics)Computational physicssymbols.namesakeSpace and Planetary SciencesymbolsDeconvolutionPlanckPixelizationInstrumentationBeam (structure)
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Semiadiabatic High-Field Polarization Response in Ferroelectrics I: Hysteresis and Nonlinear Susceptibility

2004

Ginzburg-Landau theory for ferroelectric phase instability is combined with Langevin, Fokker-Planck and imaginary time Schrodinger equation techniques to model impact of thermal noise in the kinetics of ferroelectric polarization. The proposed real space/real time numerical method allows to efficiently simulating relaxation, dynamic hysteresis and general dielectric response.

PhysicsCondensed matter physicsCondensed Matter PhysicsPolarization (waves)FerroelectricityImaginary timeElectronic Optical and Magnetic MaterialsSchrödinger equationLangevin equationCondensed Matter::Materials ScienceNonlinear systemsymbols.namesakesymbolsGinzburg–Landau theoryFokker–Planck equationFerroelectrics
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A fake Interacting Dark Energy detection?

2020

Models involving an interaction between the Dark Matter and the Dark Energy sectors have been proposed to alleviate the long standing Hubble constant tension. In this paper we analyze whether the constraints and potential hints obtained for these interacting models remain unchanged when using simulated Planck data. Interestingly, our simulations indicate that a dangerous fake detection for a non-zero interaction among the Dark Matter and the Dark Energy fluids could arise when dealing with current CMB Planck measurements alone. The very same hypothesis is tested against future CMB observations, finding that only cosmic variance limited polarization experiments, such as PICO or PRISM, could …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundDark matterCosmic background radiationFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Cosmic varianceAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Space and Planetary Science0103 physical sciencesDark energysymbolsPlanck010303 astronomy & astrophysicsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Running of featureful primordial power spectra

2017

Current measurements of the temperature and polarization anisotropy power spectra of the Cosmic Microwave Background (CMB) seem to indicate that the naive expectation for the slow-roll hierarchy within the most simple inflationary paradigm may not be respected in nature. We show that a primordial power spectra with localized features could in principle give rise to the observed slow-roll anarchy when fitted to a featureless power spectrum. Future CMB missions have the key to disentangle among the two possible paradigms and firmly establish the slow-roll mechanism as the responsible one for the inflationary period in the early universe. From a model comparison perspective, and assuming that …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundSpectral densityFOS: Physical sciencesCosmological modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPolarization (waves)01 natural sciencesSpectral linesymbols.namesake0103 physical sciencessymbolsStatistical analysisPlanck010306 general physicsAnisotropyAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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More about a successful vector-tensor theory of gravitation

2016

The vector-tensor (VT) theory of gravitation revisited in this article was studied in previous papers, where it was proved that VT works and deserves attention. New observational data and numerical codes have motivated further development which is presented here. New research has been planed with the essential aim of proving that current cosmological observations, including Planck data, baryon acoustic oscillations (BAO), and so on, may be explained with VT, a theory which accounts for a kind of dark energy which has the same equation of state as vacuum. New versions of the codes CAMB and COSMOMC have been designed for applications to VT, and the resulting versions have been used to get the…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Current (mathematics)010308 nuclear & particles physicsGeneral relativityEquation of state (cosmology)FOS: Physical sciencesValue (computer science)Astronomy and Astrophysics01 natural sciencesGravitationsymbols.namesakeTheoretical physics0103 physical sciencesDark energysymbolsBaryon acoustic oscillationsPlanck010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Exploring dark matter microphysics with galaxy surveys

2015

We use present cosmological observations and forecasts of future experiments to illustrate the power of large-scale structure (LSS) surveys in probing dark matter (DM) microphysics and unveiling potential deviations from the standard $\Lambda$CDM scenario. To quantify this statement, we focus on an extension of $\Lambda$CDM with DM-neutrino scattering, which leaves a distinctive imprint on the angular and matter power spectra. After finding that future CMB experiments (such as COrE+) will not significantly improve the constraints set by the Planck satellite, we show that the next generation of galaxy clustering surveys (such as DESI) could play a leading role in constraining alternative cos…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)MicrophysicsMatter power spectrumDark matterCosmic microwave backgroundFísicaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologyGalaxy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)symbolsPlanckAstrophysics - Cosmology and Nongalactic Astrophysics
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