Search results for "Ligo"

showing 10 items of 1427 documents

Search for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing Run

2019

We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO’s second observing run. In contrast to a previous search of Advanced LIGO data from the first observing run, this search includes the effects of component spin on the gravitational waveform. We identify no viable gravitational-wave candidates consistent with subsolar mass ultracompact binaries with at least one component between \ud0.2\ud \ud \udM\ud⊙\ud–\ud1.0\ud \ud \udM\ud⊙\ud. We use the null result to constrain the binary merger rate of (\ud0.2\ud \ud \udM\ud⊙\ud, \ud0.2\ud \ud \udM\ud⊙\ud) binaries to be less than \ud3.7\ud×\ud10\ud5\ud \ud \udGpc\ud−\ud3\ud \udyr\ud−\ud1\udand the binary …

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenbinary: massAstrofísicaGravitacióFormation modeldensity: fluctuationAstronomyGeneral Physics and Astronomydetector: networkspin01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSblack hole: formationddc:550black holeDark MatterAstrophysics::Solar and Stellar AstrophysicsLIGOQCQBnucleus: interactionSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational wave; physics; astronomyPhysicsarticleDensity fluctuationgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]astro-ph.COAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenablack hole: primordialGravitationAstrophysics - Cosmology and Nongalactic AstrophysicsMatter densitydensity: primordialCosmology and Nongalactic Astrophysics (astro-ph.CO)coolinggr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryCooling mechanismPrimordial black holesFOS: Physical sciencesdark matter: densityGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesNuclear interactionGravitation and AstrophysicsMergingGeneral Relativity and Quantum Cosmologynull resultSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technologymass: solarCosmologiaStellar evolutions010308 nuclear & particles physicsMatter fractionsgravitational radiationRCUKblack hole: massGalaxiesbinary: compactStarsgravitational radiation detectordetector: sensitivityVIRGOPhysics and Astronomygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Gravitational waves Black holes (astronomy) Gravitational self forcePhysical Review Letters
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Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run

2018

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 $M_\odot$ - 1.0 $M_\odot$ using data taken between September 12, 2015 and January 19, 2016. We find no viable gravitational wave candidates. Our null result constrains the coalescence rate of monochromatic (delta function) distributions of non-spinning (0.2 $M_\odot$, 0.2 $M_\odot$) ultracompact binaries to be less than $1.0 \times 10^6 \text{Gpc}^{-3} \text{yr}^{-1}$ and the coalescence rate of a similar distribution of (1.0 $M_\odot$, 1.0 $M_\odot$) ultracompact binaries to be less than $1.9 \times 10^4 \text{Gpc}^{-3} \text{yr}^{-1}$ (at 90 percent confidence). N…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftendensity: fluctuationMACHOAstronomyGeneral Physics and AstronomyPrimordial black holeAstrophysicsCoalescence01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationLIMITSddc:550Massive compact halo objectLIGOneutron starQCQBPhysicseducation.field_of_studyPhysicsDensity fluctuationBinary systemsgravitational wavesPhysical SciencesSearch enginesastro-ph.COblack hole: primordialAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcBinary formationAstrophysics::High Energy Astrophysical PhenomenaPopulationDark matterPhysics MultidisciplinaryEarly universeFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)dark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesCoalescence rateGravitation and AstrophysicsPhysics and Astronomy (all)General Relativity and Quantum Cosmologybinary: coalescence0103 physical sciencesddc:530Delta functions010306 general physicseducationSTFCAstrophysics::Galaxy AstrophysicsScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveStellar evolutionsbinary: formationgravitational radiationRCUKblack hole: massGalaxiesStarsGalaxyLIGOBlack holeVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikMicro-lensing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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GW170817: Measurements of Neutron Star Radii and Equation of State

2018

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESGW170817BINARIESddc:550DENSELIGODENSE MATTEREquation of State010303 astronomy & astrophysicsQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsNeutron Star RadiusPhysicsGravitational effectsEquations of stateParametrizationsElectromagnetic observationsGravitational-wave signals3. Good healthQUADRUPOLE-MOMENTSMacroscopic propertiesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEquations of state of nuclear matterGravitational wavesaturation: densityBinary neutron starsNUCLEON MATTEREquations of state of nuclear matter; Gravitational wave sources; Gravitational waves; Nuclear matter in neutron starsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaGW170817 Neutron Star Radius Equation of StatePhysics Multidisciplinaryneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionGravitation and AstrophysicsNuclear matter in neutron starsGravitational waveselectromagnetic field: productionPhysics and Astronomy (all)Pulsargalaxy: binary0103 physical sciencesddc:530NeutronMASSESSTFCequation of state: parametrizationAstrophysics::Galaxy AstrophysicsNeutronsExtreme conditionsGravitational wave sourcesEquation of stateScience & TechnologyNeutron Star Interior Composition Explorer010308 nuclear & particles physicsGravitational wavegravitational radiationRCUKFlocculationSaturation densityUNIVERSAL RELATIONSStarsLIGOgravitational radiation detectorNeutron starStarsVIRGOPhysics and Astronomygravitational radiation: emissionneutron star: binary: coalescenceDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]MATTER
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Tests of General Relativity with GW170817

2019

The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This source, for the first time, permits tests of strong-field dynamics of compact binaries in presence of matter. In this paper, we place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime. Bounds on modified dispersion of gravitational waves are obtained; in combination with information from the observed electromagnetic counterpart we can also constrain effects due to large extra dimensions. Finally, the polari…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyTestingGravitational WaveGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologystrong fieldddc:550general relativityLIGOQCSettore FIS/01PhysicsPhysicsGravitational effectsarticlePolarization (waves)Gravitational-wave signalsExtra dimensionsgravitational wavesPhysical SciencesExtra dimensions[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Large extra dimensiondispersionBinary neutron starsgravitational radiation: polarizationGeneral RelativityGeneral relativitygr-qcPhysics MultidisciplinaryGRAVITATIONAL-WAVE OBSERVATIONSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)gravitational wavesblack holesGravity wavesMASSgravitational radiation: direct detectionGravitation and Astrophysicselectromagnetic field: productionRelativityGeneral Relativity and Quantum CosmologyDipole radiationsGRAVITYTests of general relativitygravitation: weak field0103 physical sciencesddc:530High Energy Physicscapture010306 general physicsGravitational Wave; General RelativitySTFCradiation: dipolepolarizationScience & TechnologyStrong fieldGravitational wavegravitational radiationRCUKbinary: compactgravitational radiation detectorLIGONeutron starVIRGODewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikNewtonianshigher-dimensional
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Mast cells promote homeostasis by limiting endothelin-1-induced toxicity

2004

Endothelin-1 (ET-1) is a 21-amino-acid peptide, derived from vascular endothelial cells, with potent vasoconstrictor activity. ET-1 has been implicated in diverse physiological or pathological processes, including the vascular changes associated with sepsis. However, the factors that regulate ET-1-associated toxicity during bacterial infections, or in other settings, are not fully understood. Both the pathology associated with certain allergic and autoimmune disorders, and optimal host defence against bacterial and parasitic infections are mediated by mast cells. In vitro, mast cells can produce ET-1 (ref. 11), undergo ET-1-dependent and endothelin-A receptor (ET(A))-dependent activation, a…

DiarrheaProteasesDrug-Related Side Effects and Adverse ReactionsCell SurvivalPeritonitisBiologyPeptides CyclicCell DegranulationBody TemperatureMiceChymasesIn vivomedicineAnimalsHomeostasisMast CellsReceptorEgtazic AcidMice KnockoutMultidisciplinaryEndothelin-1Stem CellsBody WeightSerine EndopeptidasesEndogenous mediatorMast cellEndothelin 1In vitroCell biologyMice Inbred C57BLSurvival RateProto-Oncogene Proteins c-kitmedicine.anatomical_structureMutationImmunologyFemaleOligopeptidesInjections IntraperitonealHomeostasisNature
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Propyl substituted 4-arylimino-1,2,3-trihydroacridylnickel complexes: Their synthesis, characterization and catalytic behavior toward ethylene

2015

Propyl substituted 4-arylimino-1,2,3-trihydroacridylnickel dihalide complexes were designed and prepared by metal-induced template reaction with NiCl2 center dot 6H(2)O or (DME)NiBr2. They were characterized by infrared spectroscopy and elemental analysis. Single crystal X-ray crystallography of representative complex Ni3 revealed a distorted trigonal bipyramidal geometry around nickel. The catalytic activities of the title nickel complexes were negatively affected by propyl substituent on their backbone when comparing with the results by unsubstituted ones. With the activation of diethylaluminium chloride, all nickel complexes exhibited moderate activity (up to 5.10 x 10(5) g mol(-1)(Ni) h…

Diethylaluminium chlorideEthyleneStereochemistryOrganic ChemistrySubstituentchemistry.chemical_elementInfrared spectroscopyBiochemistryMedicinal chemistryCatalysis2-propyl-4-arylimino-1Inorganic ChemistryNickelchemistry.chemical_compoundTemplate reactionTrigonal bipyramidal molecular geometrychemistryMaterials Chemistry3-dihydroacridine; Nickel complex; Ethylene oligomerizationPhysical and Theoretical ChemistryJournal of Organometallic Chemistry
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Dip Pen Lithography of oligonucleotides on flexible substrates for point-of-care malaria disease testing

2015

The first step for prevention and treatment of diseases is the accurate diagnosis. However, proper diagnostic technologies are not available in developing countries due to the lack of reliable electrical power, refrigeration and trained personnel. For this reason, there is an urgent need of low cost, rapid assays not requiring any external support. By coupling such technologies to communication infrastructures, healthcare in areas without access to medical personnel would be possible. “Paper” like substrates are ideal for fabricating such devices since they are cheap, easy to degradate after use and compatible with most of existing printing technologies [1]. We had previously shown the poss…

Dip Pen Lithography oligonucleotides flexible substrates malaria
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Vibrio cholerae cytolysin: assembly and membrane insertion of the oligomeric pore are tightly linked and are not detectably restricted by membrane fl…

2000

AbstractHemolytic strains of Vibrio cholerae secrete a cytolysin that, upon binding as a monomer, forms pentameric pores in animal cell membranes. Pore formation is inhibited at low temperature and in the absence of cholesterol. We here posed the following questions: firstly, can oligomerization be observed in the absence of pore formation? Secondly, is membrane fluidity responsible for the effect of temperature or of cholesterol upon pore formation? The first issue was approached by chemical cross-linking, by electrophoretic heteromer analysis, and by electron microscopy. None of these methods yielded any evidence of a non-lytic pre-pore oligomer. The second question was addressed by the u…

DiphenylhexatrieneCell Membrane PermeabilityMembrane permeabilityMembrane FluidityBacterial ToxinsBiophysicsPorinsFluorescence PolarizationBiologymedicine.disease_causePore forming toxinBiochemistrychemistry.chemical_compoundProtein oligomerizationBacterial ProteinsBacteriocinsmedicineMembrane fluidityProtein oligomerizationVibrio choleraePhospholipidsFluorescent DyesLiposomeCytotoxinsCell MembraneCell BiologyFluoresceinsCholesterolMembranechemistryBiochemistryVibrio choleraeLiposomesPhosphatidylcholinesCytolysinDiphenylhexatrieneBiochimica et Biophysica Acta (BBA) - Biomembranes
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Rupture Force of Single Small Drug Molecule Binding a Split Aptamer

2012

Aptamers are specific oligonucleotides (DNA or RNA) which bind small inorganic or organic molecules, large proteins or cells. In particular, the high affinity of aptamers is expected to lead to a new class of therapeutic reagents. Thus the detection and characterization of binding strength of small molecules is important for drug and medical research. Atomic force spectroscopy (AFS) with a force resolution in the piconewton range is a valuable tool for studying interactions on a single molecular level. The detection of very small target molecules less than 500 Dalton is characterized by only a few hydrogen interactions between the aptamer and the target molecules. Thus tiny rupture forces w…

Dissociation constantAnalyteOligonucleotideChemistryStereochemistryAptamerForce spectroscopyBiophysicsBiophysicsMoleculeBinding siteSmall moleculeBiophysical Journal
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1984

Dissociation constantchemistry.chemical_compoundChemistryPhotochemistryOligomerDie Makromolekulare Chemie, Rapid Communications
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