0000000000723658

AUTHOR

Ho

showing 7 related works from this author

Measurement of the cross section for open b-quark production in two-photon interactions at LEP

2007

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Deuteron and anti-deuteron production in e+ e- collisions at the Z resonance

2006

Deuteron and anti-deuteron production in Z decays has been observed in the ALEPH experiment at LEP. The production rate of anti-deuterons is measured to be per hadronic Z decay in the anti-deuteron momentum range from 0.62 to 1.03 GeV/c. The coalescence parameter , which characterizes the likelihood of anti-deuteron production, is measured to be in Z decays. These measurements indicate that the production of anti-deuterons is suppressed in collisions compared to that in pp and photoproduction collisions

coalescence modelproduction
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Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo's third observing run

2021

We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper limits from the earlier O1 and O2 runs. Unlike in previous observing runs in the advanced detector era, we include Virgo in the search for the GWB. The results are consistent with uncorrelated noise, and therefore we place upper limits on the strength of the GWB. We find that the dimensionless energy density $\Omega_{\rm GW}\leq 5.8\times 10^{-9}$ at the 95% credible level for a flat (frequency-independent) GWB, using a prior which is uniform in the log of the strength of the GWB, with 99% of the sensitivity comi…

coalescencePhysics and Astronomy (miscellaneous)gravitation: modelAstronomypopulationAstrophysicspower spectrum01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wave backgroundbackground: magneticenergy: densitycorrelation functionLIGOQCPOPULATIONQBPhysicsSettore FIS/01education.field_of_studySpectral indexPhysicsstar-formation ratestatistical analysis: BayesianIsotropicSTAR-FORMATION RATE; BLACK-HOLE; MASS; COALESCENCE; POPULATION; EVOLUTION; RADIATION; PROSPECTSCOALESCENCEPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]LIGO; Virgo; isotropic gravitational-wave backgroundIsotropic gravitational wave backgrounds with LIGO and VirgoAstrophysics - Cosmology and Nongalactic Astrophysicsgravitational radiation: polarizationdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)black-holePopulationFOS: Physical sciencesGravitational Waves LIGO Virgo Stochastic Background IsotropicGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsMASSSTAR-FORMATION RATEBinary black holebinary: coalescence0103 physical sciencesevolutionddc:530SDG 7 - Affordable and Clean Energy2ND010306 general physicseducationGravitational Waves/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundSpectral densityprospectsbinary: compactnoise: magneticLIGOEVOLUTIONisotropic gravitational-wave backgroundBlack holeradiationdetector: sensitivityPROSPECTSVIRGOpolarization: scalarblack hole: binaryGravitation Cosmology AstrophysicsBLACK-HOLEpolarization: vectorRADIATIONmassStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Constraints on Cosmic Strings Using Data from the Third Advanced LIGO–Virgo Observing Run

2021

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 data set. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks and, for the first time, kink-kink collisions.cA template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension, $G\mu$, as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models.cAdditionally, we develop and test a third model which interpolat…

High Energy Physics - TheoryDewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftengravitational radiation: stochasticAstronomyCosmic stringsWAVESGeneral Physics and Astronomy01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyGravitation Cosmology & AstrophysicsGravitationLIMITSCosmic strings & domain wallCosmology & Astrophysicsddc:550Distribution modelsTransient signalenergy: densityLIGOQCstochastic modelLIGO Scientific CollaborationShort durationsCosmic strings & domain walls; Gravitational waves; Gravitation Cosmology & AstrophysicsQBPhysicsCosmic strings & domain wallskinkSettore FIS/03Stochastic systems[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thPhysicsGravitational effectsarticleGRAVITATIONAL-RADIATION; LIMITS; EVOLUTION; WAVEStensionGravitational-wave signalsCosmologyPhysical Sciencesastro-ph.COGrand unified theories[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational waveAstrophysics - Cosmology and Nongalactic AstrophysicsGravitational effects; Gravity waves; Stochastic models; Stochastic systems; Cosmic strings; Distribution models; Grand unified theories; Gravitational-wave signals; Orders of magnitude; Short durations; Template-based; Transient signalGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcPhysics MultidisciplinaryGRAVITATIONAL-RADIATIONO3FOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy(all)Gravity wavesGravitation and AstrophysicsGravitational wavesTheoretical physicsGeneral Relativity and Quantum Cosmologystatistical analysis0103 physical sciencesTemplate-basedCosmic Strings O3 LIGO Virgoddc:530010306 general physicscosmic stringSTFCInflation (cosmology)Science & Technology010308 nuclear & particles physicsGravitational wavestring tensionVirgogravitational radiation: backgroundRCUKLIGOEVOLUTIONCosmic stringStochastic modelsOrders of magnitudeVIRGOHigh Energy Physics - Theory (hep-th)Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Two-particle correlations in pp, (p)over-bar(p)over-bar and (KSKS0)-K-0 pairs from hadronic Z decays

2005

Two-particle correlations in pp, and pairs have been studied in hadronic Z decays recorded at LEP with the ALEPH detector. The correlations were measured as a function of the four-momentum difference Q of the pair. For pp, pairs a depletion of events is observed in the region , and for pairs an enhancement of events is observed in the region . These features are consistent with expectations from Fermi–Dirac and Bose–Einstein statistics, respectively.

INTERFERENCEINTERFEROMETRYZ(0) DECAYSBOSE-EINSTEIN CORRELATIONSLEPANNIHILATIONALEPHDETECTORMESONSMULTIPLE PRODUCTION
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Bose-Einstein correlations in W-pair decays with an event-mixing technique

2005

Bose-Einstein correlations in W-pair decays are studied using data collected by the ALEPH detector at LEP at e+e- centre-of-mass energies from 183 to 209 GeV. The analysis is based on the comparison of WW→qq̄qq̄ events to "mixed" events constructed with the hadronic part of WW→qq̄ℓν events. The data are in agreement with the hypothesis that Bose-Einstein correlations are present only for pions from the same W decay. The JETSET model with Bose-Einstein correlations between pions from different W bosons is disfavoured.

INTERFEROMETRYPHYSICSCOLLISIONSE+E-ANNIHILATIONSE(+)E(-)2-DIMENSIONAL ANALYSISHADRONSLEPZ(0)PEAK
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Improved measurement of the triple gauge-boson couplings gamma WW and ZWW in e(+)e(-) collisions

2005

Triple gauge-boson couplings ?WW and ZWW involving single-photon, single-W and W-pair production are determined using data samples collected at LEP with the ALEPH detector at centre-of-mass energies between 183 and 209 GeV. The integrated luminosity used is 700 pb-1 for the single-photon measurement and 683 pb-1 for the W channels. Restricting the measurement to C- and P-conserving terms and applying local SU(2) L×U(1)Y gauge invariance, the measured values of the parameters g1 Z, ?? and ?? are: g1 Z=1.001±0. 027(stat)±0.013(syst), ??=0.971±0.055(stat) ±0.030(syst), ??=-0.012±0.027(stat) ±0.011(syst) for single-parameter fits, where the two other parameters are fixed to their Standard Model…

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