Search results for "loop"

showing 10 items of 608 documents

Gluon spectrum in the glasma from JIMWLK evolution

2011

The JIMWLK equation with a "daughter dipole" running coupling is solved numerically starting from an initial condition given by the McLerran-Venugopalan model. The resulting Wilson line configurations are then used to compute the spectrum of gluons comprising the glasma inital state of a high energy heavy ion collision. The development of a geometrical scaling region makes the spectrum of produced gluons harder. Thus the ratio of the mean gluon transverse momentum to the saturation scale grows with energy. Also the total gluon multiplicity increases with energy slightly faster than the saturation scale squared.

PhysicsNuclear and High Energy PhysicsParticle physicsWilson loopta114Nuclear Theory010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesYang–Mills existence and mass gapRenormalization group01 natural sciencesGluonNuclear Theory (nucl-th)High Energy Physics - PhenomenologyDipoleHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamics0103 physical sciencesInitial value problemBoundary value problem010306 general physicsNuclear ExperimentScaling
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Irradiation study of a fully monolithic HV-CMOS pixel sensor design in AMS 180 nm

2018

Abstract High-Voltage Monolithic Active Pixel Sensors (HV-MAPS) based on a 180 nm HV-CMOS process have been proposed to realize thin, fast and highly integrated pixel sensors. The MuPix7 prototype, fabricated in the commercial AMS H18 process, features a fully integrated on-chip readout, i.e. hit-digitization, zero suppression and data serialization. MuPix7 is the first fully monolithic HV-CMOS pixel sensor that has been tested for the use in high irradiation environments like HL-LHC. We present results from laboratory and test beam measurements of MuPix7 prototypes irradiated with neutrons (up to 5.0 × 1015 neq/cm2) and 24 GeV protons (up to 7.8 × 1015 protons/cm2) and compare the performa…

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPixelPhysics::Instrumentation and Detectors010308 nuclear & particles physicsbusiness.industryFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciencesNoise (electronics)030218 nuclear medicine & medical imagingPhase-locked loop03 medical and health sciences0302 clinical medicineCMOS0103 physical sciencesOptoelectronicsNeutronIrradiationbusinessInstrumentationZero suppressionData transmission
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QUANTUM YANG-MILLS THEORY ON ARBITRARY SURFACES

1992

We study quantum Maxwell and Yang-Mills theory on orientable two-dimensional surfaces with an arbitrary number of handles and boundaries. Using path integral methods we derive general and explicit expressions for the partition function and expectation values of contractible and noncontractible Wilson loops on closed surfaces of any genus, as well as for the kernels on manifolds with handles and boundaries. In the Abelian case we also compute correlation functions of intersecting and self-intersecting loops on closed surfaces, and discuss the role of large gauge transformations and topologically nontrivial bundles.

PhysicsNuclear and High Energy PhysicsPure mathematicsWilson loopAstronomy and AstrophysicsYang–Mills theoryPartition function (mathematics)Contractible spaceAtomic and Molecular Physics and OpticsGenus (mathematics)Quantum mechanicsPath integral formulationGauge theoryQuantum field theoryInternational Journal of Modern Physics A
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Quantum bubble dynamics in the presence of gravity

1991

Abstract The dynamics of spherical quantum bubbles in 3+1 dimensions is governed by a Klein-Gordon-type equation which simulates the quantum mechanical motion of a relativistic point particle in 1+1 dimensions. This dimensional reduction is especially clear in the minisuperspace formulation first used in quantum cosmology and adapted here to quantum bubble dynamics. The payoff of this formulation is the discovery of the gravitational analogue of the Klein effect, namely the crossing of positive and negative energy levels of the particle spectrum induced by an external gravitational field. This phenomenon gives rise to a finite probability that a vacuum bubble might tunnel from an initial bo…

PhysicsNuclear and High Energy PhysicsQuantization (physics)Classical mechanicsString and brane phenomenologyQuantum cosmologyQuantum processQuantum dynamicsQuantum mechanicsQuantum gravityNegative energyQuantum dissipationLoop quantum cosmology
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Infrared and extended on-mass-shell renormalization of two-loop diagrams

2003

Using a toy model Lagrangian we demonstrate the application of both infrared and extended on-mass-shell renormalization schemes to multiloop diagrams by considering as an example a two-loop self-energy diagram. We show that in both cases the renormalized diagrams satisfy a straightforward power counting.

PhysicsNuclear and High Energy PhysicsToy modelNuclear TheoryInfraredDiagramShell (structure)FOS: Physical sciencesPower (physics)Nuclear Theory (nucl-th)Loop (topology)RenormalizationTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicsFunctional renormalization group
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Structure of chromomagnetic fields in the glasma

2014

The initial stage of a heavy ion collision is dominated by nonperturbatively strong chromoelectric and -magnetic fields. The spatial Wilson loop provides a gauge invariant observable to probe the dynamics of the longitudinal chromomagnetic field. We discuss recent results from a real time lattice calculation of the area-dependence of the expectation value of the spatial Wilson loop. We show that at relatively early times after the collision, a universal scaling as a function of the area emerges at large distances for very different initial conditions, with a nontrivial critical exponent. A similar behavior has earlier been seen in calculations of the gluon transverse momentum spectrum, whic…

PhysicsNuclear and High Energy PhysicsWilson loopNuclear Theoryta114High Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesObservableExpectation valueInvariant (physics)GluonColor-glass condensateNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicsCritical exponentScalingNuclear Physics A
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Bouncing Cosmologies in Palatini $f(R)$ Gravity

2009

7 pages, 4 figures.-- PACS nrs.: 04.50.Kd; 98.80.-k; 98.80.Qc.-- ArXiv pre-print available at: http://arxiv.org/abs/0907.0318

PhysicsNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)UniverseCosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsQuantum cosmologyGravitational collapsef(R) gravityGravitational singularityBig Bouncemedia_commonLoop quantum cosmology
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Inclination of Large Coronal Loops Observed by TRACE

2000

A TRACE field of view well inside the solar disk shows very well defined large loops, likely to be very inclined to the solar surface. On the other hand there is little evidence of large loops perpendicular to the solar surface. We show that this does not mean that most large loops have such large inclination but that perpendicular loops are much less visible to TRACE, because of density stratification. We quantitatively evaluate this effect by modeling in detail loops with different inclinations.

PhysicsOpticsbusiness.industryPhysics::Space PhysicsPerpendicularAstrophysics::Solar and Stellar AstrophysicsField of viewSolar surfaceAstrophysics::Earth and Planetary AstrophysicsCoronal loopbusinessSolar diskComputational physics
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Determination of the ηHe3 threshold structure from the low energy pd→ηHe3 reaction

2017

We analyze the data on cross sections and asymmetries for the $pd\ensuremath{\rightarrow}\ensuremath{\eta}\phantom{\rule{0.16em}{0ex}}^{3}\mathrm{He}$ reaction close to threshold and look for bound states of the $\ensuremath{\eta}\phantom{\rule{0.16em}{0ex}}^{3}\mathrm{He}$ system. Rather than parameterizing the scattering matrix, as is usually done, we develop a framework in which the $\ensuremath{\eta}{\phantom{\rule{0.16em}{0ex}}}^{3}\mathrm{He}$ optical potential is the key ingredient, and its strength, together with some production parameters, are fitted to the available experimental data. The relationship of the scattering matrix to the optical potential is established using the Bethe…

PhysicsParticle physicsBethe–Salpeter equation010308 nuclear & particles physicsScatteringScattering length01 natural sciencesLoop (topology)Matrix (mathematics)0103 physical sciencesBound stateProduction (computer science)Atomic physics010306 general physicsS-matrixPhysical Review C
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NLO corrections to Z production in association with several jets

2014

In this talk we report on first results from the NLO computation of Z production in association with five jets in hadron-hadron collisions. The results are obtained with the help of the numerical method, where apart from the phase space integration also the integration over the loop momentum is performed numerically. In addition we discuss several methods and techniques for the improvement of the Monte Carlo integration.

PhysicsParticle physicsComputationNumerical analysisMonte Carlo methodFOS: Physical sciencesMomentumLoop (topology)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Phase spaceProduction (computer science)Monte Carlo integrationHigh Energy Physics::ExperimentNuclear Experiment
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