Search results for "SCALAR"

showing 10 items of 1002 documents

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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Search for New Physics with a Dijet Plus MissingETSignature inpp¯Collisions ats=1.96  TeV

2010

We present results of a signature-based search for new physics using a dijet plus missing transverse energy (E{sub T}) data sample collected in 2 fb{sup -1} of p{bar p} collisions at {radical}s = 1.96 TeV with the CDF II detector at the Fermilab Tevatron. We observe no significant event excess with respect to the standard model prediction and extract a 95% C.L. upper limit on the cross section times acceptance for a potential contribution from a non-standard model process. Based on this limit the mass of a potential first or second generation scalar leptoquark is constrained to be above 187 GeV/c{sup 2}.

PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyScalar (mathematics)TevatronGeneral Physics and Astronomy01 natural sciencesStandard ModelNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentLeptoquarkLimit (mathematics)Fermilab010306 general physicsEnergy (signal processing)Physical Review Letters
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Search for Scalar Neutrino Superpartners ine+μFinal States inpp¯Collisions ats=1.96  TeV

2008

We report a search for R-parity-violating production and decay of sneutrino particles in the e mu final state with 1.04 +/- 0.06 fb(-1) of data collected with the D-0 detector at the Fermilab Tevatron Collider in 2002-2006. Good agreement between the data and the standard model prediction is observed. With no evidence for new physics, we set limits on the R-parity-violating couplings lambda'(311) and lambda(312) as a function of the sneutrino mass.

PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyTevatronScalar (physics)General Physics and AstronomySupersymmetryLambda01 natural sciencesNuclear physicsParticle decay0103 physical sciencesHigh Energy Physics::ExperimentFermilabNeutrino010306 general physicsPhysical Review Letters
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Antiproton-proton annihilation in-flight

1994

This is an overview of the preliminary results of\(\bar pp\) annihilation at incident\(\bar p\) momenta of 600, 1200 and 1940 MeV/c(*). The data was taken at LEAR with the Crystal Barrel Detector (E. Akeret al.:Nucl. Instrum. Methods A,321, 108 (1992)). In the two pseudoscalar final states seven different channels are observable and their angular distributions are measured. They are compared to older data, if existent, and are found to be equal within the experimental errors. In the three-meson final states, an overview of the already examined final states is given. Striking signals in the Dalitz plots and invariant-mass projections for a set of final states are observed. In the final state…

PhysicsParticle physicsAnnihilationProton010308 nuclear & particles physics[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear TheoryDalitz plotObservable[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesPseudoscalarNuclear physicsAntiproton0103 physical sciencesInvariant massNuclear Experiment010306 general physicsBar (unit)
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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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Chiral unitary theory: Application to nuclear problems

2001

In this talk we briefly describe some basic elements of chiral perturbation theory, $\chi PT$, and how the implementation of unitarity and other novel elements lead to a better expansion of the $T$ matrix for meson meson and meson baryon interactions. Applications are then done to the $ \pi \pi $ interaction in nuclear matter in the scalar and vector channels, antikaons in nuclei and $K^-$ atoms, and how the $\phi$ meson properties are changed in a nuclear medium.

PhysicsParticle physicsChiral perturbation theoryNuclear TheoryMesonUnitarityHigh Energy Physics::LatticeScalar (mathematics)High Energy Physics::PhenomenologyNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesFísicaNuclear matterUnitary stateBaryonNuclear Theory (nucl-th)Matrix (mathematics)High Energy Physics::ExperimentNuclear Experiment
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WEAK DECAY OF Λ–HYPERNUCLEI

2005

The nonmesonic weak decay of L hypernuclei is studied in a shell model framework. A complete strangeness-changing weak LN!NN transition potential, based on one boson exchange, is constructed by including the exchange of the pseudoscalar mesons p, K, h as well as the vector mesons r,v, and K*, whose weak-coupling constants are obtained from soft meson theorems and SU~6! w . General expressions for nucleons in arbitrary shells are obtained. The transition matrix elements include realistic LN short-range correlations and NN final state interactions based on the Nijmegen baryon-baryon potential. The decay rates are found to be especially sensitive to the inclusion of the strange mesons K and K*…

PhysicsParticle physicsChiral perturbation theoryProtonMesonmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyNuclear TheoryStochastic matrixAsymmetryPseudoscalarHigh Energy Physics::ExperimentNuclear ExperimentNucleonmedia_commonBosonTheoretical Nuclear Physics in Italy
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Baryonic resonances from baryon decuplet-meson octet interaction

2004

We study $S$-wave interactions of the baryon decuplet with the octet of pseudoscalar mesons using the lowest order chiral Lagrangian. In the S=1 sector, we find an attractive interaction in the $\Delta K$ channel with I=1 while it is repulsive for I=2. The attractive interaction leads to a pole in the second Riemann sheet of the complex plane and is manifested as a large strength in the scattering amplitude close to the $\Delta K$ threshold, which is not the case for I=2. We use the unitarized coupled channel approach to also investigate all the other possible values of strangeness and isospin. We find two bound states in the SU(3) limit corresponding to the octet and decuplet representatio…

PhysicsParticle physicsChiral symmetryNuclear and High Energy PhysicsMesonOctetUnitarityNuclear TheoryHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaAstronomy and AstrophysicsAtomic and Molecular Physics and OpticsBaryonNuclear physicsPseudoscalarNuclear Theory (nucl-th)Nuclear theory
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Cosmological searches for a non-cold dark matter component

2017

We explore an extended cosmological scenario where the dark matter is an admixture of cold and additional non-cold species. The mass and temperature of the non-cold dark matter particles are extracted from a number of cosmological measurements. Among others, we consider tomographic weak lensing data and Milky Way dwarf satellite galaxy counts. We also study the potential of these scenarios in alleviating the existing tensions between local measurements and Cosmic Microwave Background (CMB) estimates of the $S_8$ parameter, with $S_8=\sigma_8\sqrt{\Omega_m}$, and of the Hubble constant $H_0$. In principle, a sub-dominant, non-cold dark matter particle with a mass $m_X\sim$~keV, could achieve…

PhysicsParticle physicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsHot dark matterDark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesMixed dark matterWarm dark matter010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics - Cosmology and Nongalactic Astrophysics
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