Search results for "Physics::General Physics"

showing 10 items of 63 documents

On the bicrossproduct structures for the family of algebras

1998

It is shown that the family of deformed algebras has a different bicrossproduct structure for each in analogy to the undeformed case.

Physics::Fluid DynamicsPhysicsPhysics::General PhysicsHigh Energy Physics::TheoryTheoretical physicsMathematics::Quantum AlgebraStructure (category theory)General Physics and AstronomyAnalogyStatistical and Nonlinear PhysicsMathematical PhysicsJournal of Physics A: Mathematical and General
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Search for dilepton resonances in pp collisions at √s = 7 TeV with the ATLAS detector

2011

This Letter reports on a search for narrow high-mass resonances decaying into dilepton final states. The data were recorded by the ATLAS experiment in pp collisions at sqrt(s) = 7 TeV at the Large Hadron Collider and correspond to a total integrated luminosity of 1.08 (1.21) fb(-1) in the e(+)e(-) (mu(+)mu(-)) channel. No statistically significant excess above the standard model expectation is observed and upper limits are set at the 95% C. L. on the cross section times branching fraction of Z' resonances and Randall-Sundrum gravitons decaying into dileptons as a function of the resonance mass. A lower mass limit of 1.83 TeV on the sequential standard model Z' boson is set. A Randall-Sundru…

Physics::General PhysicsAcceleradors de partículesHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentDetectors de radiació
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The richest superclusters. II. Galaxy populations

2007

We study the morphology of galaxy populations of the richest superclusters from the catalogue of superclusters of galaxies in the 2dF Galaxy Redshift Survey using the luminosity density distribution and Minkowski functional V3. We compare the properties of grouped and isolated galaxies in regions of different density in superclusters. We find that in high-density cores of rich superclusters there is an excess of early type, passive galaxies, among galaxies in groups and clusters, as well as among those which do not belong to groups, while in lower density outer regions there are more blue, star-forming galaxies both in groups and among those galaxies which do not belong to groups. This also…

Physics::General PhysicsAstrophysics (astro-ph)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics::Galaxy Astrophysics
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Some Special Applications

2010

We have learned from the preceding chapters that the chemical and physical state of a Mossbauer atom in any kind of solid material can be characterized by way of the hyperfine interactions which manifest themselves in the Mossbauer spectrum by the isomer shift and, where relevant, electric quadrupole and/or magnetic dipole splitting of the resonance lines. On the basis of all the parameters obtainable from a Mossbauer spectrum, it is, in most cases, possible to identify unambiguously one or more chemical species of a given Mossbauer atom occurring in the same material.

Physics::General PhysicsCondensed Matter::Materials ScienceChemical speciesMaterials scienceMössbauer spectroscopyAtomQuadrupolePhysics::Atomic PhysicsQuadrupole splittingAtomic physicsHyperfine structureResonance (particle physics)Magnetic dipole
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The environmental effects in the origin of angular momenta of galaxies

2011

We study the galaxy alignment in the sample of very rich Abell clusters located in and outside superclusters. The statistically significant difference among investigated samples exists. We found that in contrast to whole sample of cluster, where alignment increase with the cluster richness, the cluster belonging to the superclusters does not show this effect. Moreover, the alignment decreased with the supercluster richness. One should note however that orientations of galaxies in analyzed clusters are not random, both in the case when we analyzed whole sample of the clusters and only clusters belonging to the superclusters. The observed trend, dependence of galaxy alignment on both cluster …

Physics::General PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics of Galaxies (astro-ph.GA)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of GalaxiesPhysics::History of PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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"Table 5" 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

Observed and predicted W+W- transverse mass distribution in the E-MU channel. Also tabulated are the predictions for a RS graviton of mass 1000 GeV and a bulk RS graviton with mass 600 GeV.

Physics::General PhysicsElectron productionP P --> W+ W-7000.0Single Differential DistributionMuon productionGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryProton-Proton ScatteringDN/DMExclusiveHigh Energy Physics::ExperimentNuclear ExperimentW Production
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How to interpret black hole entropy?

1998

We consider a possibility that the entropy of a Schwarzschild black hole has two different interpretations: The black hole entropy can be understood either as an outcome of a huge degeneracy in the mass eigenstates of the hole, or as a consequence of the fact that the interior region of black hole spacetime is separated from the exterior region by a horizon. In the latter case, no degeneracy in the mass eigenstates needs to be assumed. Our investigation is based on calculations performed with Lorentzian partition functions obtained for a whole maximally extended Schwarzschild spacetime, and for its right-hand-side exterior region. To check the correctness of our analysis we reproduce, in th…

Physics::General PhysicsGeneral Relativity and Quantum CosmologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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Search for resonant diboson production in the WW/WZ -> lvjj decay channels with the ATLAS detector at root s=7 TeV

2013

A search for resonant diboson production using a data sample corresponding to 4.7 fb(-1) of integrated luminosity collected by the ATLAS experiment at the Large Hadron Collider in pp collisions at root s = 7 TeV is presented. The search for a narrow resonance in the WW or WZ mass distribution is conducted in a final state with an electron or a muon, missing transverse momentum, and at least two jets. No significant excess is observed and limits are set using three benchmark models: WW resonance masses below 940 and 710 GeV are excluded at 95% confidence level for spin-2 Randall-Sundrum and bulk Randall-Sundrum gravitons, respectively; WZ resonance masses below 950 GeV are excluded at 95% co…

Physics::General PhysicsHigh Energy Physics::ExperimentFísica nuclear
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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

2013

This Letter reports a search for a heavy particle that decays to WW using events produced in pp collisions at sqrt(s) = 7 TeV. The data were recorded in 2011 by the ATLAS detector and correspond to an integrated luminosity of 4.7 fb-1. WW to l nu l' nu'(l, l' = e or mu) final states are considered and the distribution of the transverse mass of the WW candidates is found to be consistent with Standard Model expectations. Upper limits on the production cross section times branching ratio into W boson pairs are set for Randall-Sundrum and bulk Randall-Sundrum gravitons, which result in observed 95% CL lower limits on the masses of the two particles of 1.23 TeV and 0.84 TeV, respectively.

Physics::General PhysicsHigh Energy Physics::ExperimentFísica nuclear
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"Table 41" of "Multiplicity dependence of K*(892)$^{0}$ and $\phi$(1020) production in pp collisions at $\sqrt{s}$ = 13 TeV"

2020

K$^{*0}$ transverse momentum integrated yield vs multiplicity - V0M multiplicity classes, average of particle and antiparticle

Physics::General PhysicsP P --> Kstar+XKstar13000.0Proton-Proton CollisionsSIGyieldResonanceV0M Multiplicity
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