Search results for "light"

showing 10 items of 3575 documents

Nonlinear dynamics of a semilinear photorefractive oscillator

2001

The experimental study of the dynamics of an empty coherent semilinear photorefractive oscillator is reported. It is shown that starting from a certain coupling strength the oscillation occurs with two frequencies shifted symmetrically with respect to the frequency of the pump wave. The threshold of bifurcation in oscillation spectrum depends on pump intensity ratio.

PhysicsOscillationbusiness.industrySpectrum (functional analysis)Physics::OpticsPhotorefractive effectNonlinear systemFour-wave mixingLight intensityOpticsQuantum electrodynamicsFresnel numberbusinessBifurcationPhotorefractive Effects, Materials, and Devices
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Echolocation signals of the plecotine bat, Plecotus macrobullaris Kuzyakin, 1965

2006

Plecotus macrobullaris was recorded in an alpine region in Switzerland. Like other species of the genus Plecotus, P. macrobullaris emitted multiharmonic, downward frequency-modulated signals consisting mostly of the 1st and the lower part of the 2nd harmonic. Signal structure depended on the distance to the background. The shortest signals (0.8 ms) were recorded close to the background. The first harmonic began at about 46 kHz and ended around 23 kHz. Signals were emitted in groups. The longest signals (up to 7.3 ms) were recorded above a meadow, far from background targets. These signals, which were more shallowly modulated, started at about 42 kHz and ended around 15 kHz. They occasionall…

PhysicsPaleontologybiologyEcologyGenus PlecotusWing beatPlecotus macrobullarisHarmonicAnimal Science and ZoologyHuman echolocationFlight behaviourbiology.organism_classificationSignalActa Chiropterologica
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Λc± production in pp collisions with a new fragmentation function

2020

We study inclusive ${\mathrm{\ensuremath{\Lambda}}}_{c}^{\ifmmode\pm\else\textpm\fi{}}$-baryon production in $pp$ collisions in the general-mass variable-flavor-number scheme and compare with data from the LHCb, ALICE, and CMS collaborations. We perform a new fit of the $c\ensuremath{\rightarrow}{\mathrm{\ensuremath{\Lambda}}}_{c}^{+}$ fragmentation function combining ${e}^{+}{e}^{\ensuremath{-}}$ data from OPAL and Belle. The agreement with LHC data is slightly worse compared with a calculation using an older fragmentation function, and the tension between different determinations of ${\mathrm{\ensuremath{\Lambda}}}_{c}^{\ifmmode\pm\else\textpm\fi{}}$ production cross sections from the LHC…

PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::Phenomenology0103 physical sciencesFragmentation functionHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLambda01 natural sciencesSlightly worsePhysical Review D
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Search for Pair Production of Scalar Bottom Quarks inpp¯Collisions ats=1.96  TeV

2006

A search for direct production of scalar bottom quarks ((b) over bar) is performed with 310 pb(-1) of data collected by the D0 experiment in p (p) over bar collisions at root s = 1.96 TeV at the Fermilab Tevatron Collider. The topology analyzed consists of two b jets and an imbalance in transverse momentum due to undetected neutralinos (chi(0)(1)), with chi(0)(1) assumed to be the lightest supersymmetric particle. We find the data consistent with standard model expectations, and set a 95% C.L. exclusion domain in the (m(b), m(chi 1)(0)) mass plane, improving significantly upon the results from run I of the Tevatron.

PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronTevatronGeneral Physics and AstronomyD0 experiment01 natural sciencesLightest Supersymmetric ParticleStandard ModelNuclear physicsPair production0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsMinimal Supersymmetric Standard ModelPhysical Review Letters
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X-Ray Lines from Dark Matter Annihilation at the keV Scale.

2018

In 2014, several groups reported hints for a yet unidentified line in astrophysical x-ray signals from galaxies and galaxy clusters at an energy of 3.5 keV. While it is not unlikely that this line is simply a reflection of imperfectly modeled atomic transitions, it has renewed the community’s interest in models of keV-scale dark matter, whose decay would lead to such a line. The alternative possibility of dark matter annihilation into monochromatic photons is far less explored, a lapse that we strive to amend in this Letter. More precisely, we introduce a novel model of fermionic dark matter χ with O(keV) mass, annihilating to a scalar state ϕ which in turn decays to photons, for instance v…

PhysicsParticle physics010308 nuclear & particles physicsHot dark matterDark matterScalar field dark matterGeneral Physics and Astronomy01 natural sciencesBaryonic dark matterWeakly interacting massive particles0103 physical sciencesWarm dark matter010303 astronomy & astrophysicsLight dark matterDark fluidPhysical review letters
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Dark Matter Decay between Phase Transitions at the Weak Scale

2017

We propose a new alternative to the weakly interacting massive particle paradigm for dark matter. Rather than being determined by thermal freeze-out, the dark matter abundance in this scenario is set by dark matter decay, which is allowed for a limited amount of time just before the electroweak phase transition. More specifically, we consider fermionic singlet dark matter particles coupled weakly to a scalar mediator S_{3} and to auxiliary dark sector fields, charged under the standard model gauge groups. Dark matter freezes out while still relativistic, so its abundance is initially very large. As the Universe cools down, the scalar mediator develops a vacuum expectation value (VEV), which…

PhysicsParticle physics010308 nuclear & particles physicsHot dark matterHigh Energy Physics::PhenomenologyDark matterScalar field dark matterGeneral Physics and AstronomyAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesBaryonic dark matter0103 physical sciencesMixed dark matterWarm dark matter010306 general physicsLight dark matterDark fluidPhysical Review Letters
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Shell-model study on event rates of lightest supersymmetric particles scattering offKr83andTe125

2016

We investigate the elastic and inelastic scattering of lightest supersymmetric particle (LSP) dark matter off two possible target nuclei, $^{83}\mathrm{Kr}$ and $^{125}\mathrm{Te}$. For the nuclear-structure calculations, we employ the nuclear shell model using recently generated realistic interactions. We have condensed the nuclear-physics contribution to a set of nuclear-structure factors that are independent of the adopted supersymmetric (SUSY) model. Total event rates are then easily calculated by combining the nuclear-structure factors with SUSY parameters of choice. In particular, $^{125}\mathrm{Te}$ shows promise as a detector material with both the elastic and inelastic channels yie…

PhysicsParticle physics010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyNuclear TheoryNuclear shell modelSupersymmetryInelastic scattering7. Clean energy01 natural sciencesLightest Supersymmetric ParticleNuclear physicsWeakly interacting massive particles0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLight dark matterPhysical Review D
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Light-by-light scattering sum rule for radiative transitions of bottomonia

2020

We generalize a forward light-by-light scattering sum rule to the case of heavy quarkonium radiative transitions. We apply such sum rule to the bottomonium states, and use available data on radiative transitions in its evaluation. For the transitions that are not known experimentally, we provide theoretical estimates within a potential model, and consider the spread between similar approaches in the literature as an estimate for the model error. For the $\Upsilon(1S)$, $\Upsilon(2S)$, and $\Upsilon(3S)$ states we observe that, due to a cancellation between transitions involving $\chi_{b0}, \chi_{b1}$, and $\chi_{b2}$ states, the sum rule is satisfied within experimental and theoretical erro…

PhysicsParticle physics010308 nuclear & particles physicsScatteringSpectrum (functional analysis)High Energy Physics::PhenomenologyFOS: Physical sciencesQuarkonium01 natural sciencesLight scatteringHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRadiative transferHigh Energy Physics::ExperimentSum rule in quantum mechanics010306 general physicsPhysical Review
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Review of dark photon searches

2016

Dark Photons are hypothetical extra-U(1) gauge bosons, which are motivated by a number of astrophysical anomalies as well as the presently seen deviation between the Standard Model prediction and the direct measurement of the anomalous magnetic moment of the muon, (g − 2)μ . The Dark Photon does not serve as the Dark Matter particle itself, but acts as a messenger particle of a hypothetical Dark Sector with residual interaction to the Standard Model. We review recent Dark Photon searches, which were carried out in a global effort at various hadron and particle physics facilities. We also comment on the perspectives for future invisble searches, which directly probe the existence of Light Da…

PhysicsParticle physicsAnomalous magnetic dipole moment010308 nuclear & particles physicsAxion Dark Matter ExperimentHot dark matterPhysicsQC1-999Dark matterScalar field dark matterAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesDark photonNuclear physicsWeakly interacting massive particles0103 physical sciences010306 general physicsLight dark matterEPJ Web of Conferences
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Observational properties of feebly coupled dark matter

2016

We show that decoupled hidden sectors can have observational consequences. As a representative model example, we study dark matter production in the Higgs portal model with one real singlet scalar $s$ coupled to the Standard Model Higgs via $\lambda_{\rm hs}\Phi^\dagger\Phi s^2$ and demonstrate how the combination of non-observation of cosmological isocurvature perturbations and astrophysical limits on dark matter self-interactions imply stringent bounds on the magnitude of the scalar self-coupling $\lambda_{\rm s}s^4$. For example, for dark matter mass $m_{\rm s}=10$ MeV and Hubble scale during cosmic inflation $H_*=10^{12}$ GeV, we find $10^{-4}\lesssim \lambda_{\rm s}\lesssim 0.2$.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterHigh Energy Physics::PhenomenologyScalar field dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsdark matterStandard ModelHidden sectorpimeä aineHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonProduction (computer science)Light dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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