Search results for "graviton"

showing 10 items of 31 documents

Search for high-mass resonances decaying to dimuons at CDF.

2009

We present a search for high-mass neutral resonances using dimuon data corresponding to an integrated luminosity of 2.3 fb(-1) collected in pp collisions at s=1.96 TeV by the CDF II detector at the Fermilab Tevatron. No significant excess above the standard model expectation is observed in the dimuon invariant-mass spectrum. We set 95% confidence level upper limits on sigma BR(pp -> X ->mu mu), where X is a boson with spin-0, 1, or 2. Using these cross section limits, we determine lower mass limits on sneutrinos in R-parity-violating supersymmetric models, Z(') bosons, and Kaluza-Klein gravitons in the Randall-Sundrum model.

HIGH MASS RESONANCEParticle physicsFermilab TevatronTevatronGeneral Physics and AstronomyFOS: Physical sciencesddc:500.2114 Physical sciencesResonance7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsHigh Energy Physics - Experiment (hep-ex)Integrated luminosities0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsBosonsBosonPhysicsMuonMass spectrometryhep-ex010308 nuclear & particles physicsPhysicsInvariant-mass spectrum13.85.Rm 13.85.Qk 12.60.Cn 14.70.Pw 04.50.-hHigh Energy Physics::PhenomenologyConfidence levelsGravitonSupersymmetryUpper limitsSupersymmetric modelsCross sectionsRandall–Sundrum modelThe standard modelsMass spectrumCDFHigh Energy Physics::ExperimentPhysical review letters
researchProduct

Massless positivity in graviton exchange

2021

We formulate Positivity Bounds for scattering amplitudes including exchange of massless particles. We generalize the standard construction through dispersion relations to include the presence of a branch cut along the real axis in the complex plane for the Maldestam variable $s$. In general, validity of these bounds require the cancellation of divergences in the forward limit of the amplitude, proportional to $t^{-1}$ and $\log(t)$. We show that this is possible in the case of gravitons if one assumes a Regge behavior of the amplitude at high energies below the Planck scale, as previously suggested in the literature, and that the concrete UV behaviour of the amplitude is uniquely determined…

High Energy Physics - TheoryField (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)hiukkasfysiikkakosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationeffective field theorycanonical quantum gravityDispersion relation0103 physical sciencessironta010306 general physicsquantum field theoryperturbation theoryMathematical physicsPhysics010308 nuclear & particles physicsGravitonFísicagravitaatioDark Energyalternative gravity theoriesBimetric Theoriesscattering amplitudesMassless particleScattering amplitudeAmplitudeHigh Energy Physics - Theory (hep-th)Complex planeGravitation
researchProduct

Relations for Einstein–Yang–Mills amplitudes from the CHY representation

2017

We show that a recently discovered relation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with one graviton and $(n-1)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons, can be derived from the CHY representation. In addition we show that there is a generalisation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with $r$ gravitons and $(n-r)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons. We present a general formula for this case.

High Energy Physics - TheoryNuclear and High Energy PhysicsTrace (linear algebra)High Energy Physics::LatticeFOS: Physical sciencesYang–Mills existence and mass gap01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryQuantum mechanics0103 physical sciencesEinstein010306 general physicsLinear combinationMathematical physicsPhysicsCondensed Matter::Quantum GasesIntroduction to gauge theoryGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonlcsh:QC1-999High Energy Physics - Theory (hep-th)Supersymmetric gauge theorysymbolslcsh:PhysicsPhysics Letters B
researchProduct

Instability of black holes in massive gravity

2013

We show that linear perturbations around the simplest black hole solution of massive bi-gravity theories, the bi-Schwarzschild solution, exhibit an unstable mode featuring the Gregory-Laflamme instability of higher dimensional black strings. The result is obtained for the massive gravity theory which is free from the Boulware-Deser ghost, as well as for its extension with two dynamical metrics. These results may indicate that static black holes in massive gravity do not exist. For the graviton mass of the order of the Hubble scale, however, the instability timescale is of order of the Hubble time.

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)Field (physics)Scale (ratio)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesBlack stringStrings010306 general physicsPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]GravitonP-BranesBlack holeMassive gravityHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
researchProduct

Kaluza-Klein FIMP dark matter in warped extra-dimensions

2020

We study for the first time the case in which Dark Matter (DM) is made of Feebly Interacting Massive Particles (FIMP) interacting just gravitationally with the standard model particles in an extra-dimensional Randall-Sundrum scenario. We assume that both the dark matter and the standard model are localized in the IR-brane and only interact via gravitational mediators, namely the graviton, the Kaluza-Klein gravitons and the radion. We found that in the early Universe DM could be generated via two main processes: the direct freeze-in and the sequential freeze-in. The regions where the observed DM relic abundance is produced are largely compatible with cosmological and collider bounds.

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectKaluza–Klein theoryDark matterFOS: Physical sciences01 natural scienceslaw.inventionStandard ModelGravitationHigh Energy Physics - Phenomenology (hep-ph)law0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsCollidermedia_commonPhysics010308 nuclear & particles physicsGravitonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyExtra dimensionsBeyond Standard Modellcsh:QC770-798Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Gravity-mediated dark matter in clockwork/linear dilaton extra-dimensions

2020

We study for the first time the possibility that Dark Matter (represented by particles with spin $0,1/2$ or $1$) interacts gravitationally with Standard Model particles in an extra-dimensional Clockwork/Linear Dilaton model. We assume that both, the Dark Matter and the Standard Model, are localized in the IR-brane and only interact via gravitational mediators, namely the Kaluza-Klein (KK) graviton and the radion/KK-dilaton modes. We analyse in detail the Dark Matter annihilation channel into Standard Model particles and into two on-shell Kaluza-Klein towers (either two KK-gravitons, or two radion/KK-dilatons, or one of each), finding that it is possible to obtain the observed relic abundanc…

Nuclear and High Energy PhysicsParticle physicsDark matterFOS: Physical sciencesStrings and branes phenomenology01 natural sciencesStandard ModelGravitationHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Phenomenology of Field Theories in Higher Dimensions0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsSpin (physics)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsGravitonHigh Energy Physics - PhenomenologyExtra dimensionslcsh:QC770-798DilatonAstrophysics - High Energy Astrophysical PhenomenaJournal of High Energy Physics
researchProduct

Scalar spectrum in a graviton soft wall model

2020

In this study we present a unified phenomenological analysis of the scalar glueball and scalar meson spectra within an AdS/QCD framework in the bottom up approach. For this purpose we generalize the recently developed graviton soft-wall (GSW) model, which has shown an excellent agreement with the lattice QCD glueball spectrum, to a description of glueballs and mesons with a unique energy scale. In this scheme, dilatonic effects, are incorporated in the metric as a deformation of the AdS space. We apply the model also to the heavy meson spectra with success. We obtain quadratic mass equations for all scalar mesons while the glueballs satisfy an almost linear mass equation. Besides their spec…

Nuclear and High Energy PhysicsParticle physicsMesonNuclear TheoryHigh Energy Physics::LatticeScalar (mathematics)FOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Spectrum0103 physical sciencesAdS/CFT010306 general physicsScalar mesonQuantum chromodynamicsPhysics010308 nuclear & particles physicsGlueballHigh Energy Physics::PhenomenologyGravitonLattice QCDMesonMass formulaHigh Energy Physics - PhenomenologyGlueballHigh Energy Physics::Experiment
researchProduct

"Table 2" of "Search for new phenomena in the WW to l nu l' nu' final state in pp collisions at sqrt(s) = 7 TeV with the ATLAS detector"

2012

Expected and observed 95% upper limits on cross section time branching ration for pp --> Graviton*(bulk) < W+ W- >.

P P --> GRAVITON XInclusiveProton-Proton ScatteringIntegrated Cross SectionW pair Production7000.0Cross SectionSIGW Production
researchProduct

Search for high-mass resonances decaying to dilepton final states in pp collisions at √s = 7 TeV with the ATLAS detector

2012

The ATLAS detector at the Large Hadron Collider is used to search for high-mass resonances decaying to an electron-positron pair or a muon-antimuon pair. The search is sensitive to heavy neutral Z′ gauge bosons, Randall-Sundrum gravitons, Z [superscript *] bosons, techni-mesons, Kaluza-Klein Z/γ bosons, and bosons predicted by Torsion models. Results are presented based on an analysis of pp collisions at a center-of-mass energy of 7 TeV corresponding to an integrated luminosity of 4.9 fb[superscript −1] in the e [superscript +] e [superscript −] channel and 5.0 fb[superscript −1] in the μ [superscript +] μ [superscript −] channel. A Z [superscript ′] boson with Standard Model-like couplings…

Particle physicsNuclear and High Energy PhysicsPhysics::General PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]Kaluza–Klein theoryTechnicolorddc:500.27. Clean energy01 natural sciences530Nuclear physics0103 physical sciencesddc:530EXTRA DIMENSIONSHigh Energy Physics010306 general physicsCiencias Exactashadron-hadron scatteringBosonPhysicsddc:539Gauge bosonLarge Hadron ColliderHadron-Hadron scattering; Nuclear and High Energy PhysicsScience & TechnologyHadron-Hadron ScatteringATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleHigh Energy Physics::PhenomenologyGravitonFísicaATLASExtra dimensionsRandall–Sundrum modelHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearproton-proton collisionsHigh Energy Physics::ExperimentLHC
researchProduct

Spin-dependence of gravity-mediated dark matter in warped extra-dimensions

2021

We study the spin-dependence of Dark Matter (DM) particles which interact gravitationally with the Standard Model (SM) in an extra-dimensional Randall-Sundrum scenario. We assume that both the Dark Matter and the Standard Model are confined to the TeV (Infra-red) brane and only interact via gravitational mediators, namely Kaluza-Klein gravitons and the radion. We analyze the different DM annihilation channels and find that it is possible to achieve the presently observed relic abundance of Dark Matter, $\Omega_{\rm DM}$, within the freeze-out mechanism for DM particles of spin 0, 1/2 and 1. We study the region of the model parameter space for which $\Omega_{\rm DM}$ is achieved and compare …

Particle physicsPhysics and Astronomy (miscellaneous)Dark matterScalar (mathematics)FOS: Physical scienceslcsh:Astrophysics01 natural sciences7. Clean energyStandard ModelVector bosonHigh Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Spin-½High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonHigh Energy Physics - PhenomenologyExtra dimensionslcsh:QC770-798DilatonAstrophysics - High Energy Astrophysical PhenomenaThe European Physical Journal C
researchProduct