0000000000153745

AUTHOR

Michael Williams

0000-0003-2198-2974

showing 10 related works from this author

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

2021

Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter under extreme conditions. A significant fraction of the known pulsar population belongs to binary systems. Searching for unknown neutron stars in binary systems requires specialized algorithms to address unknown orbital frequency modulations. We present a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, binaryskyhough pipeline. The search analyzes the most s…

binary: orbitneutron star: binaryPhysics and Astronomy (miscellaneous)Astronomybinary [neutron star]AstrophysicsGravitational Waves; LIGO (Observatory); Neutron Stars01 natural sciencesneutron starsGeneral Relativity and Quantum CosmologyMonte Carlo: Markov chainPhysics Particles & Fieldsbinary starsbinary systemsBinary SystemsLIGOgravitational waveQCQBpulsarastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studySettore FIS/03Physicsorbit [binary]General relativityPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenabinary stardata analysis methodsensitivity [detector]General relativitygr-qcfrequency [modulation]Populationneutron star: spinFOS: Physical sciencesalternative theories of gravityMarkov chain [Monte Carlo]General Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGravitational Waves Neutron Stars Binary Systems LIGO VirgoLIGO (Observatory)emission [gravitational radiation]Pulsarbinary: coalescence0103 physical sciencesBinary starddc:530spin [neutron star]background [gravitational radiation]010306 general physicseducationSTFCOrbital elementsGravitational WavesScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundmodulation: frequencyRCUKNeutron StarsLIGOgravitational radiation detectordetector: sensitivityNeutron starVIRGOgravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]binary stars; neutron stars
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First observation of the doubly charmed baryon decay Ξcc++→Ξc+π+

2018

The doubly charmed baryon decay Ξcc++→Ξc+π+ is observed for the first time, with a statistical significance of 5.9σ, confirming a recent observation of the baryon in the Λc+K−π+π+ final state. The data sample used corresponds to an integrated luminosity of 1.7 fb−1, collected by the LHCb experiment in pp collisions at a center-of-mass energy of 13 TeV. The Ξcc++ mass is measured to be 3620.6±1.5(stat)±0.4(syst)±0.3(Ξc+) MeV/c2 and is consistent with the previous result. The ratio of branching fractions between the decay modes is measured to be [B(Ξcc++→Ξc+π+)×B(Ξc+→pK−π+)]/[B(Ξcc++→Λc+K−π+π+)×B(Λc+→pK−π+)]=0.035±0.009(stat)±0.003(syst).

Particles and fieldGeneral Physics and Astronomy01 natural sciencesNONuclear physicsPhysics and Astronomy (all)Condensed Matter::Superconductivity0103 physical sciencesPhysicLHCb - Abteilung HintonSDG 7 - Affordable and Clean Energy010306 general physicsPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyParticle physicsHEPBaryonLHCbCharmed baryonHadron colliderHigh Energy Physics::ExperimentB physics Branching fraction CP violation Hadron-Hadron scattering (experiments)LHCFísica de partículesExperiments
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Model-Independent Evidence forJ/ψpContributions toΛb0→J/ψpK−Decays

2016

The data sample of Lambda(0)(b) -> J/psi pK(-) decays acquired with the LHCb detector from 7 and 8 TeV pp collisions, corresponding to an integrated luminosity of 3 fb(-1), is inspected for the presence of J/psi p or J/psi K- contributions with minimal assumptions about K(-)p contributions. It is demonstrated at more than nine standard deviations that Lambda(0)(b) -> J/psi pK(-) decays cannot be described with K- p contributions alone, and that J/psi K- contributions play a dominant role in this incompatibility. These model-independent results support the previously obtained model-dependent evidence for P-c(+)-> J/psi p charmonium-pentaquark states in the same data sample.

PhysicsLuminosity (scattering theory)010308 nuclear & particles physicsQuark modelGeneral Physics and AstronomyLambda01 natural sciencesPentaquarkNuclear physicsBaryon13. Climate action0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysical Review Letters
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Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

2021

We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. For the first time, we include Virgo data in our analysis and run our search with a new efficient pipeline called {\tt PyStoch} on data folded over one sidereal day. We use gravitational-wave radiometry (broadband and narrow band) to produce sky maps of stochastic gravitational-wave backgrounds and to search for gravitational waves from point sources. A spherical harmonic decomposition method is employed to look for gravitational-wave emission from spatially-extended sources. Neither technique found eviden…

gravitational radiation: anisotropyPhysics and Astronomy (miscellaneous)gravitational radiation: stochasticAstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsCosmology & Astrophysicsenergy: fluxenergy: densitygravitational radiation: energyLIGOQCQBPhysicsSettore FIS/01Spectral indexPhysicsGalactic CenterAmplitudeGeneral relativitySidereal timePhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]gravitational radiation: power spectrumGravitationdata analysis methodAnisotropic stochastic gravitational-wave backgroundExperimental studies of gravityFOS: Physical sciencesO3O2General Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsStochastic Background Gravitational Waves LIGO Virgo O1 O2 O3O1Gravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSstatistical analysis0103 physical sciencesadvanced LIGO and Virgoddc:530KAGRAKAGRACosmology & Astrophysics010306 general physicsSTFCgravitational waves; LIGO; VirgoGravitational WavesScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundRCUKGalaxyLIGOVIRGOgravitational radiation: emissionspectrum: densityRADIATIONCROSS-CORRELATION SEARCHStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikgalaxyExperimental studies of gravity; General relativity; Gravitational waves
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First experimental study of photon polarization in radiative B0s decays.

2017

The polarization of photons produced in radiative $B^{0}_{s}$ decays is studied for the first time. The data are recorded by the LHCb experiment in $pp$ collisions corresponding to an integrated luminosity of 3fb$^{-1}$ at center-of-mass energies of $7$ and $8$TeV. A time-dependent analysis of the $B^{0}_{s} \to \phi \gamma$ decay rate is conducted to determine the parameter ${\mathcal{A}}^\Delta$, which is related to the ratio of right- over left-handed photon polarization amplitudes in $b \to s \gamma$ transitions. A value of ${\mathcal{A}}^\Delta=-0.98^{\,+0.46\,+0.23}_{\,-0.52\,-0.20}$ is measured. This result is consistent with the Standard Model prediction within two standard deviatio…

General PhysicsPhotonModels beyond the standard modeldistributions asymmetries toolPhysics MultidisciplinaryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareNONuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ASYMMETRIES0103 physical sciencesPhoton polarizationLeptonic semileptonic and radiative decays of bottom mesonDISTRIBUTIONS; ASYMMETRIES; TOOLRadiative transfer[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]DISTRIBUTIONSTOOLSDG 7 - Affordable and Clean Energy010306 general physicsPhysicsScience & Technology02 Physical Sciences/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyhep-ex010308 nuclear & particles physicsPhysicsParticle physicsPolarization (waves)HEPB physics photon polarization.3. Good healthLHCbAmplitudePhysical SciencesBottom mesons (|B|>0)High Energy Physics::ExperimentLHCFísica de partículesExperimentsPolarization in interactions and scatteringParticle Physics - Experiment
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Measurement of the c0 Baryon Lifetime

2018

We report a measurement of the lifetime of the $��_c^0$ baryon using proton-proton collision data at center-of-mass energies of 7 and 8~TeV, corresponding to an integrated luminosity of 3.0 fb$^{-1}$ collected by the LHCb experiment. The sample consists of about 1000 $��_b^-\to��_c^0��^-\bar��_�� X$ signal decays, where the $��_c^0$ baryon is detected in the $pK^-K^-��^+$ final state and $X$ represents possible additional undetected particles in the decay. The $��_c^0$ lifetime is measured to be $��_{��_c^0} = 268\pm24\pm10\pm2$ fs, where the uncertainties are statistical, systematic, and from the uncertainty in the $D^+$ lifetime, respectively. This value is nearly four times larger than, …

Particles and fieldGeneral PhysicsMesonGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyOmega09 EngineeringNOLuminosityHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciencesPhysicHeavy baryonTOOLSDG 7 - Affordable and Clean EnergyLHCb - Abteilung Hinton010306 general physicsINCLUSIVE WEAK DECAYS; DISCARDING 1/N(C); RULE; TOOL01 Mathematical SciencesQuantum chromodynamicsPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy02 Physical Sciences010308 nuclear & particles physicsQuark modelParticle physicsState (functional analysis)HEPDISCARDING 1/N(C)BaryonLHCbHadron colliderHigh Energy Physics::ExperimentINCLUSIVE WEAK DECAYSLHCAtomic physicsFísica de partículesExperimentsRULECharm physics Oscillation Flavor physics Hadron-Hadron scattering
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Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

2020

We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perfor…

Gravitational waves; Neutron stars; Pulsars; Gravitational wave sources010504 meteorology & atmospheric sciencesAstronomyAstrophysicsVela01 natural sciencesGeneral Relativity and Quantum Cosmology[SPI]Engineering Sciences [physics]neutronMillisecond pulsaremission010303 astronomy & astrophysicsQCQBSettore FIS/01Physicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]PhysicsAstrophysics::Instrumentation and Methods for Astrophysics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational-Waves Pulsars Neutron StarsGravitational wavePROPER MOTIONProper motiongr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNeutron starGeneral Relativity and Quantum Cosmology (gr-qc)Gravitational-WavesGravitational wavesNeutron starsSEARCHESSettore FIS/05 - Astronomia e AstrofisicaPulsar0103 physical sciencesPulsar[CHIM]Chemical SciencesAstrophysiqueSTFCPulsarsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesGravitational wave sourcescrab pulsarGravitational waveCrab PulsarRCUKAstronomy and AstrophysicsNeutron StarsGravitational waves Neutron stars Pulsars Gravitational wave sourcesLIGONeutron starSpace and Planetary Science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Amplitude analysis ofB+→J/ψϕK+decays

2017

The first full amplitude analysis of B+→J/ψϕK+ with J/ψ→μ+μ−, ϕ→K+K− decays is performed with a data sample of 3 fb−1 of pp collision data collected at s√=7 and 8 TeV with the LHCb detector. The data cannot be described by a model that contains only excited kaon states decaying into ϕK+, and four J/ψϕ structures are observed, each with significance over 5 standard deviations. The quantum numbers of these structures are determined with significance of at least 4 standard deviations. The lightest is best described as a D±sD∗∓s cusp, but a resonant interpretation is also possible with mass consistent with, but width much larger than, previous measurements of the claimed X(4140) state. The mode…

Cusp (singularity)PhysicsParticle physics010308 nuclear & particles physicsState (functional analysis)Quantum number01 natural sciencesStandard deviationNuclear physicsAmplitudeExcited state0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsSpin-½Physical Review D
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Observation of Bc+→J/ψD(*)K(*) decays

2017

A search for the decays B + c → J / ψ D ( * ) 0 K + and B + c → J / ψ D ( * ) + K * 0 is performed with data collected at the LHCb experiment corresponding to an integrated luminosity of 3     fb − 1 . The decays B + c → J / ψ D 0 K + and B + c → J / ψ D * 0 K + are observed for the first time, while first evidence is reported for the B + c → J / ψ D * + K * 0 and B + c → J / ψ D + K * 0 decays. The branching fractions of these decays are determined relative to the B + c → J / ψ π + decay. The B + c mass is measured, using the J / ψ D 0 K + final state, to be 6274.28 ± 1.40 ( stat ) ± 0.32 ( syst )     MeV / c 2 . This is the most precise single measurement of the B + c mass to date.

PhysicsNuclear magnetic resonanceMeson010308 nuclear & particles physicsBranching fractionGenerator (category theory)0103 physical sciencesSingle measurementAnalytical chemistry010306 general physics01 natural sciencesLuminosityPhysical Review D
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Study of J/ψ Production in Jets

2017

The production of $J/\psi$ mesons in jets is studied in the forward region of proton-proton collisions using data collected with the LHCb detector at a center-of-mass energy of 13 TeV. The fraction of the jet transverse momentum carried by the $J/\psi$ meson, $z \equiv p_{\rm T}(J/\psi)/p_{\rm T}({\rm jet})$, is measured using jets with $p_{\rm T}({\rm jet}) > 20$ GeV in the pseudorapidity range $2.5 < \eta({\rm jet}) < 4.0$. The observed $z$ distribution for $J/\psi$ mesons produced in $b$-hadron decays is consistent with expectations. However, the results for prompt $J/\psi$ production do not agree with predictions based on fixed-order non-relativistic QCD. This is the first measurement o…

13000 GeV-cmsQuantum chromodynamics: Experimental testNuclear TheoryGeneral Physics and Astronomy01 natural sciences7. Clean energytransverse momentum [jet]Settore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentParticle production Quantum chromodynamicsddc:550scattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]LHCb - Abteilung HintonParticle productionNuclear ExperimentQuantum chromodynamicsPhysicsJet (fluid)Large Hadron Collider02 Physical SciencesHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronParticle physicsQuarkoniumPROMPTJ/psi mesonLeptonic semileptonic and radiative decays of J/ψ Υ and other quarkoniaCERN LHC Collhadroproduction [J/psi(3100)]Pseudorapidityrapidity [jet]root S=7 TEVPhysical SciencesLHCcolliding beams [p p]Particle Physics - ExperimentParticle physicsGeneral PhysicsMesonPSI(2S)Astrophysics::High Energy Astrophysical PhenomenaPhysics Multidisciplinarynonrelativistic [quantum chromodynamics]OCTET QUARKONIA PRODUCTIONNOJets in large-Q2 scatteringNuclear physicsOctet quarkonia production PP collision root S=7 TEV PSI(2S) physics prompt decayPHYSICSPhysics and Astronomy (all)OCTET QUARKONIA PRODUCTION; PP COLLISIONS; ROOT-S=7 TEV; PSI(2S); PHYSICS; PROMPT; DECAY0103 physical sciencesRapiditySDG 7 - Affordable and Clean Energy010306 general physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & TechnologyPP COLLISIONSROOT-S=7 TEV010308 nuclear & particles physicsPP collisionhep-exHigh Energy Physics::PhenomenologyLHC-BHEPLHCbHigh Energy Physics::ExperimentHeavy quarkoniaFísica de partículesExperimentsDECAYQuantum chromodynamicsexperimental results
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