Search results for "98"

showing 10 items of 1447 documents

The importance of kinematic twists and genuine saturation effects in dijet production at the Electron-Ion Collider

2021

We compute the differential yield for quark anti-quark dijet production in high-energy electron-proton and electron-nucleus collisions at small $x$ as a function of the relative momentum $\boldsymbol{P}_\perp$ and momentum imbalance $\boldsymbol{k}_\perp$ of the dijet system for different photon virtualities $Q^2$, and study the elliptic and quadrangular anisotropies in the relative angle between $\boldsymbol{P}_\perp$ and $\boldsymbol{k}_\perp$. We review and extend the analysis in [1], which compared the results of the Color Glass Condensate (CGC) with those obtained using the transverse momentum dependent (TMD) framework. In particular, we include in our comparison the improved TMD (ITMD…

Nuclear Theoryquark antiquarkQC770-798hiukkasfysiikkaPROTONtransverse momentum dependence01 natural scienceslaw.inventionColor-glass condensateGLUON DISTRIBUTION-FUNCTIONSHigh Energy Physics - Phenomenology (hep-ph)lawEQUATIONSaturation (graph theory)Wave functionPhysicselectron nucleon: colliding beamsQUARK PAIR PRODUCTIONFLUCTUATIONSQCD PhenomenologyQCD phenomenologyHigh Energy Physics - PhenomenologykinematicstwistPhysics::Space PhysicsProduction (computer science)Quarkdijet: productionCOLLISIONSNuclear and High Energy PhysicsParticle physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesanisotropy114 Physical sciencesdihadron: angular correlationdeep inelastic scattering (phenomenology)AZIMUTHAL CORRELATIONSMomentumelectron p: scatteringNuclear Theory (nucl-th)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesWAVE-FUNCTIONS010306 general physicsColliderDeep Inelastic Scattering (Phenomenology)010308 nuclear & particles physicselectron nucleus: scatteringHigh Energy Physics::PhenomenologyEVOLUTIONGluon[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]gluon: saturationcolor glass condensateHigh Energy Physics::ExperimentkvanttiväridynamiikkaJournal of High Energy Physics
researchProduct

Consistent Searches for SMEFT Effects in Non-Resonant Dilepton Events

2019

Employing the framework of the Standard Model Effective Field Theory, we perform a detailed reinterpretation of measurements of the Weinberg angle in dilepton production as a search for new-physics effects. We truncate our signal prediction at order $1/\Lambda^2$, where $\Lambda$ denotes the new-physics mass scale, and introduce a theory error to account for unknown contributions of order $1/\Lambda^4$. Two linear combinations of four-fermion operators with distinct angular behavior contribute to dilepton production with growing impact at high energies. We define suitable angular observables and derive bounds on those two linear combinations using data from the Tevatron and the LHC. We find…

Nuclear and High Energy Physics530 PhysicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesEffective Field Theories10192 Physics InstituteHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Beyond Standard Modellcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity3106 Nuclear and High Energy Physics
researchProduct

Searching for Physics Beyond the Standard Model in an Off-Axis DUNE Near Detector

2021

Next generation neutrino oscillation experiments like DUNE and T2HK are multi-purpose observatories, with a rich physics program beyond oscillation measurements. A special role is played by their near detector facilities, which are particularly well-suited to search for weakly coupled dark sector particles produced in the primary target. In this paper, we demonstrate this by estimating the sensitivity of the DUNE near detectors to the scattering of sub-GeV DM particles and to the decay of sub-GeV sterile neutrinos ("heavy neutral leptons"). We discuss in particular the importance of the DUNE-PRISM design, which allows some of the near detectors to be moved away from the beam axis. At such o…

Nuclear and High Energy Physics530 Physicshep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-ph10192 Physics InstituteQC770-79801 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. RadioactivityBeyond Standard Model0103 physical sciencesNeutrino PhysicsHigh Energy Physics::Experiment3106 Nuclear and High Energy Physics010306 general physicsParticle Physics - ExperimentParticle Physics - Phenomenology
researchProduct

Cuckoo's Eggs in Neutron Stars: Can LIGO Hear Chirps from the Dark Sector?

2018

We explore in detail the possibility that gravitational wave signals from binary inspirals are affected by a new force that couples only to dark matter particles. We discuss the impact of both the new force acting between the binary partners as well as radiation of the force carrier. We identify numerous constraints on any such scenario, ultimately concluding that observable effects on the dynamics of binary inspirals due to such a force are not possible if the dark matter is accrued during ordinary stellar evolution. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dark matter particles, from the requ…

Nuclear and High Energy PhysicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectgr-qcDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsStellar evolutionmedia_commonParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsStar formationGravitational wavehep-exGeneral Relativity and CosmologyFifth forcehep-phCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyNeutron starBeyond Standard Modelastro-ph.COlcsh:QC770-798Particle Physics - ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Detailed characterization of laboratory magnetized super-critical collisionless shock and of the associated proton energization

2021

Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of nonthermal particles and high-energy radiation. In the absence of particle collisions in the system, theory shows that the interaction of an expanding plasma with a pre-existing electromagnetic structure (as in our case) is able to induce energy dissipation and allow shock formation. Shock formation can alternatively take place when two plasmas interact, through microscopic instabilities inducing electromagnetic fields that are able in turn to mediate energy dissipation and shock formation. Using our platform in which we couple a rapidly expanding plasma induced by high-power lasers (JLF/Titan…

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldQC770-798shock waves01 natural sciencesAtomic and Molecular Physics and OpticsPhysics - Plasma Physics010305 fluids & plasmasPlasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaNuclear Energy and Engineering[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesPhysics::Space PhysicsElectrical and Electronic Engineering010306 general physics
researchProduct

Broad excitations in a 2+1D overoccupied gluon plasma

2021

Motivated by the initial stages of high-energy heavy-ion collisions, we study excitations of far-from-equilibrium 2+1 dimensional gauge theories using classical-statistical lattice simulations. We evolve field perturbations over a strongly overoccupied background undergoing self-similar evolution. While in 3+1D the excitations are described by hard-thermal loop theory, their structure in 2+1D is nontrivial and nonperturbative. These nonperturbative interactions lead to broad excitation peaks in spectral and statistical correlation functions. Their width is comparable to the frequency of soft excitations, demonstrating the absence of soft quasiparticles in these theories. Our results also su…

Nuclear and High Energy PhysicsCOLLISIONSNuclear TheoryField (physics)FOS: Physical sciencesLattice QCDQC770-798hiukkasfysiikka01 natural sciences114 Physical sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesPerturbative QCDfysikkField theory (psychology)Gauge theory010306 general physicsKINETIC-THEORYUNIVERSAL DYNAMICSPhysics:Matematikk og Naturvitenskap: 400::Fysikk: 430 [VDP]MASS SCALENUCLEI010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)kvarkki-gluoniplasmaPerturbative QCDLattice QCDFIELD-THEORY3. Good healthGluonHigh Energy Physics - PhenomenologyQuantum electrodynamicsQuark–gluon plasmaQuasiparticleQuark-Gluon PlasmaGAUGE-THEORIESJournal of High Energy Physics
researchProduct

Unitarized Chiral Perturbation Theory in a finite volume: scalar meson sector

2011

We develop a scheme for the extraction of the properties of the scalar mesons f0(600), f0(980), and a0(980) from lattice QCD data. This scheme is based on a two-channel chiral unitary approach with fully relativistic propagators in a finite volume. In order to discuss the feasibility of finding the mass and width of the scalar resonances, we analyze synthetic lattice data with a fixed error assigned, and show that the framework can be indeed used for an accurate determination of resonance pole positions in the multi-channel scattering.

Nuclear and High Energy PhysicsChiral perturbation theoryeffect [threshold]MesonNuclear TheoryHigh Energy Physics::LatticeFOS: Physical scienceschiral [perturbation theory]f0(980)a0(980)Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLattice (order)relativistic [propagator]unitarityddc:530energy levelsScalar mesonnumerical calculationsMathematical physicsPhysicsFinite volume methodScatteringscalar [resonance]High Energy Physics - Lattice (hep-lat)PropagatorFísicascalar mesonLattice QCDf0(600)boundary conditionpole [resonance]High Energy Physics - Phenomenologyfinite size
researchProduct

Searching for Earth/Solar axion halos

2020

We discuss the sensitivity of the present and near-future axion dark matter experiments to a halo of axions or axion-like particles gravitationally bound to the Earth or the Sun. The existence of such halos, assuming they are formed, renders a significant gain in the sensitivity of axion searches while satisfying all the present experimental bounds. The structure and coherence properties of these halos also imply novel signals, which can depend on the latitude or orientation of the detector. We demonstrate this by analysing the sensitivity of several distinct types of axion dark matter experiments.

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesPhysics - Atomic PhysicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsAxionAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyCP violationBeyond Standard Modellcsh:QC770-798CP violationHaloEarth (classical element)Astrophysics - Cosmology and Nongalactic AstrophysicsCoherence (physics)Journal of High Energy Physics
researchProduct

Critical point Higgs inflation in the Palatini formulation

2021

We study Higgs inflation in the Palatini formulation with the renormalisation group improved potential in the case when loop corrections generate a feature similar to an inflection point. Assuming that there is a threshold correction for the Higgs quartic coupling $\lambda$ and the top Yukawa coupling $y_t$, we scan the three-dimensional parameter space formed by the two jumps and the non-minimal coupling $\xi$. The spectral index $n_s$ can take any value in the observationally allowed range. The lower limit for the running is $\alpha_s>-3.5\times10^{-3}$, and $\alpha_s$ can be as large as the observational upper limit. Running of the running is small. The tensor-to-scalar ratio is $2.2\tim…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesRIEMANNGeneral Relativity and Quantum Cosmology (gr-qc)Parameter spaceINITIAL CONDITIONSkosmologia01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyEINSTEINCritical point (thermodynamics)0103 physical sciencesRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. Radioactivityteoreettinen fysiikkaGENERAL-RELATIVITY010306 general physicscosmology of theories beyond the SMDISSIPATIONBosonMathematical physicsInflation (cosmology)Physics010308 nuclear & particles physicsYukawa potentialCONSTRAINTSBOSONGRAVITATIONRenormalization groupAFFINE VARIATIONAL-PRINCIPLESCosmology of Theories beyond the SMInflection pointHiggs bosonSCALARONlcsh:QC770-798renormalization groupAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
researchProduct

Production of dark-matter bound states in the early universe by three-body recombination

2018

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energy. A particularly predictive model for the self-interactions is resonant short-range interactions with an S-wave scattering length that is much larger than the range. The velocity dependence of the cross section in such a model provides an excellent fit to self-interaction cross sections inferred from dark-matter halos of galaxies and clusters of galaxies if the dark-matter mass is about 19 GeV and the scattering length is about 17 fm. Such a model makes definite predictions for the few-body physics of weakly bound clusters of the dark-matter particl…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear Theorymedia_common.quotation_subjectPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateEffective field theoryCluster (physics)lcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsNuclear Experimentmedia_commonPhysics010308 nuclear & particles physicsScattering lengthCosmology of Theories beyond the SMUniverseGalaxyHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct