Search results for "Rest frame"

showing 10 items of 29 documents

Observation of Photon Polarization in theb→sγTransition

2014

This Letter presents a study of the flavor-changing neutral current radiative $B^{\pm} \to K^{\pm}\pi^{\mp}\pi^{\pm}\gamma$ decays performed using data collected in proton-proton collisions with the LHCb detector at $7$ and $8\,$TeV center-of-mass energies. In this sample, corresponding to an integrated luminosity of $3\,\text{fb}^{-1}$, nearly $14\,000$ signal events are reconstructed and selected, containing all possible intermediate resonances with a $K^{\pm}\pi^{\mp}\pi^{\pm}$ final state in the $[1.1, 1.9]\,$GeV/$c^{2}$ mass range. The distribution of the angle of the photon direction with respect to the plane defined by the final-state hadrons in their rest frame is studied in interva…

Final statePhotonmedia_common.quotation_subject14.40.NdHadronGeneral Physics and AstronomyLHCb - Abteilung Hofmann12.15.MmAsymmetryHigh energy physics Polarization Tellurium compounds; Center-of-mass energies Direct observations Final state Flavor-changing neutral current Integrated luminosity Photon polarization Proton proton collisions; PhotonsNeutral currentNuclear physicsTellurium compoundsCenter-of-mass energiesPhysics and Astronomy (all)Flavor-changing neutral currentPolarizationPhoton polarizationLeptonic semileptonic and radiative decays of bottom mesonRadiative transferIntermediate stateSDG 7 - Affordable and Clean EnergyHigh energy physicsQCmedia_commonPhysicsIntegrated luminosityPhotons/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyProton proton collisionsNeutral currentDirect observationsParticle physicsRest framePhoton polarizationLHCb13.20.HeBottom mesons (|B|>0)High Energy Physics::ExperimentLHCFísica de partículesExperimentsPhysical Review Letters
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Determination of |Vub|/|Vcb| with DELPHI at LEP

2001

The ratio of the CKM quark-mixing matrix elements |Vub|/|Vcb| has been measured using B hadron semileptonic decays. The analysis uses the reconstructed mass M_X of the secondary hadronic system produced in association with an identified lepton. Since B -> X_u lepton anti-nu transitions are characterised by hadronic masses below those of the D mesons produced in B -> X_c lepton anti-nu transitions, events with a reconstructed value of M_X significantly below the D mass are selected. Further signal enrichments are obtained using the topology of reconstructed decays and hadron identification. A fit to the numbers of decays in the b -> u enriched and depleted samples with M_X above and…

Nuclear and High Energy PhysicsParticle physicsMesonHadronFOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesNuclear Experiment010306 general physicsDELPHIPhysicsEnergy distribution010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyRest frameLARGE ELECTRON POSITRON COLLIDERPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentParticle Physics - ExperimentLeptonPhysics Letters B
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W polarisation beyond helicity fractions in top quark decays

2010

30 páginas, 14 figuras, 1 tabla.-- arXiv:1005.5382v2

Nuclear and High Energy PhysicsTop quarkParticle physicsmedia_common.quotation_subjectDensityFOS: Physical sciences01 natural sciencesBottom quarkAsymmetryHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsSpin-½media_commonPhysics010308 nuclear & particles physicsFísicaRest frameTop quarkHelicityHigh Energy Physics - PhenomenologyElectric dipole momentPair production
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Evidence for two isospin zeroJ PC=2−+ mesons at 1645 and 1875 MeV

1996

Data on\(\bar pp \to \eta \pi ^0 \pi ^0 \pi ^0 \) taken at beam momenta of 1.2 and 1.94 GeV/c reveal evidence for twoI=0JPC=2−+ resonances inηππ. The first, at 1645±14(stat.)±15(syst.) MeV with width 180−21+40±25 MeV, decays toα2(1320)π withL=0. It may be interpreted as the\(q\bar q^1 \)D2 partner ofπ2(1670). A strong signal is also observed just above threshold inf2(1270)η withL=0. It is 11–22 times stronger than is expected for the high mass tail of the 1645 MeV resonance. It can be fitted as a second 2−+ resonance at 1875±20±35 MeV with width 200±25±45 MeV. A third resonance havingJPC=2++ is observed at 2135±20±45 MeV withΛ=250±25±45 MeV, decaying to botha2(1320)π andf2(1270)η withL=1. T…

Nuclear physicsPhysicsPhysics and Astronomy (miscellaneous)MesonIsospinZero (complex analysis)High massDalitz plotResonanceAtomic physicsRest frameBar (unit)Zeitschrift für Physik C: Particles and Fields
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Measurement of isolated-photon pair production in pp collisions at root s=7 TeV with the ATLAS detector

2013

The ATLAS experiment at the LHC has measured the production cross section of events with two isolated photons in the final state, in proton-proton collisions at √s = 7 TeV . The full data set collected in 2011, corresponding to an integrated luminosity of 4.9 fb[superscript −1], is used. The amount of background, from hadronic jets and isolated electrons, is estimated with data-driven techniques and subtracted. The total cross section, for two isolated photons with transverse energies above 25 GeV and 22 GeV respectively, in the acceptance of the electromagnetic calorimeter (|η|  0.4, is 44.0[+3.2 over −4.2] pb. The differential cross sections as a function of the di-photon invariant mass, …

Particle physicsNuclear and High Energy PhysicsPhoton530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesFotonesddc:500.27. Clean energy01 natural sciences530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)0103 physical sciencesmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Invariant massddc:530High Energy Physics010306 general physicsNuclear ExperimentCiencias Exactashadron-hadron scatteringPhysicsLuminosity (scattering theory)Large Hadron ColliderScience & TechnologyHadron-Hadron ScatteringATLAS detector010308 nuclear & particles physicsATLAS experimentSettore FIS/01 - Fisica Sperimentale:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]FísicaRest frameATLAS:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]medicine.anatomical_structurePair productionHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGproton-proton collisionsHigh Energy Physics::ExperimentLHCParticle Physics - Experiment
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Lattice QCD study of the $H$ dibaryon using hexaquark and two-baryon interpolators

2019

Physical review / D 99(7), 074505 (2019). doi:10.1103/PhysRevD.99.074505

Particle physicsnucl-thNuclear TheoryHigh Energy Physics::LatticeNuclear TheoryLattice field theoryFOS: Physical scienceshep-latCorrelation function (quantum field theory)530Computer Science::Digital Libraries01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Lattice0103 physical sciencesBound stateddc:530010306 general physicsParticle Physics - PhenomenologyQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)hep-phParticle Physics - LatticeLattice QCDRest frameBaryonHigh Energy Physics - PhenomenologyNuclear Physics - TheoryIsospin
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Reply to "Comment on 'Insensitivity of Hawking radiation to an invariant Planck-scale cutoff' "

2010

We clarify the relationship between the conclusions of the previous Comment of A. Helfer and that of our Brief Report.

PhysicsAstrofísicaNuclear and High Energy PhysicsWorld lineQuantum field theory in curved spacetimeSpacetimeeducationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Rest framehumanitiesRadiacióGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyQuantum mechanicsProper timeCamps Teoria quàntica deScalar fieldHawking radiationMathematical physics
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GRB 061121: Broadband Spectral Evolution through the Prompt and Afterglow Phases of a Bright Burst

2007

Swift triggered on a precursor to the main burst of GRB 061121 (z=1.314), allowing observations to be made from the optical to gamma-ray bands. Many other telescopes, including Konus-Wind, XMM-Newton, ROTSE and the Faulkes Telescope North, also observed the burst. The gamma-ray, X-ray and UV/optical emission all showed a peak ~75s after the trigger, although the optical and X-ray afterglow components also appear early on - before, or during, the main peak. Spectral evolution was seen throughout the burst, with the prompt emission showing a clear positive correlation between brightness and hardness. The Spectral Energy Distribution (SED) of the prompt emission, stretching from 1eV up to 1MeV…

PhysicsBrightnessX-rays: individual (GRB 061121)Astrophysics::High Energy Astrophysical PhenomenaMolecular cloudAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRest frameAstrophysicsSpectral lineAfterglowlaw.inventionGamma Rays: BurstsTelescopeGamma Rays: Bursts; X-rays: individual (GRB 061121)Space and Planetary SciencelawSpectral energy distributionGamma-ray burstThe Astrophysical Journal
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Phantom Dirac-Born-Infeld dark energy

2017

Motivated by the apparent discrepancy between Cosmic Microwave Background measurements of the Hubble constant and measurements from Type-Ia supernovae, we construct a model for Dark Energy with equation of state $w = p / ��< -1$, violating the Null Energy Condition. Naive canonical models of so-called "Phantom" Dark Energy require a negative scalar kinetic term, resulting in a Hamiltonian unbounded from below and associated vacuum instability. We construct a scalar field model for Dark Energy with $w < -1$, which nonetheless has a Hamiltonian bounded from below in the comoving reference frame, {\it i.e.} in the rest frame of the fluid. We demonstrate that the solution is a cosmologica…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsKinetic termRest frame01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciencesAttractorsymbolsEnergy conditionDark energyHamiltonian (quantum mechanics)010303 astronomy & astrophysicsScalar fieldAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physicsHubble's lawPhysical Review D
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A Robust Determination of the size of quasar accretion disks using gravitational microlensing

2012

Using microlensing measurements from a sample of 27 image-pairs of 19 lensed quasars we determine a maximum likelihood estimate for the accretion disk size of an {{\em}average} quasar of $r_s=4.0^{+2.4}_{-3.1} $ light days at rest frame $=1736$\AA\ for microlenses with a mean mass of $=0.3M_\odot$. This value, in good agreement with previous results from smaller samples, is roughly a factor of 5 greater than the predictions of the standard thin disk model. The individual size estimates for the 19 quasars in our sample are also in excellent agreement with the results of the joint maximum likelihood analysis.

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsMaximum likelihoodFOS: Physical sciencesAstronomy and AstrophysicsQuasarMaximum likelihood analysisAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRest frameGravitational microlensing01 natural sciencesAccretion discThin diskSpace and Planetary Science0103 physical sciencesAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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