Search results for "GRAVITATION"

showing 10 items of 743 documents

Cluster size distributions in particle systems with asymmetric dynamics

2001

We present exact and asymptotic results for clusters in the one-dimensional totally asymmetric exclusion process (TASEP) with two different dynamics. The expected length of the largest cluster is shown to diverge logarithmically with increasing system size for ordinary TASEP dynamics and as a logarithm divided by a double logarithm for generalized dynamics, where the hopping probability of a particle depends on the size of the cluster it belongs to. The connection with the asymptotic theory of extreme order statistics is discussed in detail. We also consider a related model of interface growth, where the deposited particles are allowed to relax to the local gravitational minimum.

Particle systemAsymptotic analysisStatistical Mechanics (cond-mat.stat-mech)LogarithmStochastic processOrder statisticFOS: Physical sciencesGravitationCombinatoricsCluster (physics)ParticleStatistical physicsCondensed Matter - Statistical MechanicsMathematics
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Dynamical formation of Proca stars and quasistationary solitonic objects

2018

We perform fully non-linear numerical simulations within the spherically symmetric Einstein-(complex)Proca system. Starting with Proca field distributions that obey the Hamiltonian, momentum and Gaussian constraints, we show that the self-gravity of the system induces the formation of compact objects, which, for appropriate initial conditions, asymptotically approach stationary soliton-like solutions known as Proca stars. The excess energy of the system is dissipated by the mechanism of \textit{gravitational cooling} in analogy to what occurs in the dynamical formation of scalar boson stars. We investigate the dependence of this process on the phase difference between the real and imaginary…

Phase differencePhysics010308 nuclear & particles physicsGaussianFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Scalar boson01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationStarsNonlinear systemsymbols.namesakeClassical mechanicsAmplitude0103 physical sciencessymbols010306 general physicsHamiltonian (quantum mechanics)Physical Review D
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Critical and tricritical singularities of the three-dimensional random-bond Potts model for large $q$

2005

We study the effect of varying strength, $\delta$, of bond randomness on the phase transition of the three-dimensional Potts model for large $q$. The cooperative behavior of the system is determined by large correlated domains in which the spins points into the same direction. These domains have a finite extent in the disordered phase. In the ordered phase there is a percolating cluster of correlated spins. For a sufficiently large disorder $\delta>\delta_t$ this percolating cluster coexists with a percolating cluster of non-correlated spins. Such a co-existence is only possible in more than two dimensions. We argue and check numerically that $\delta_t$ is the tricritical disorder, which se…

Phase transitionCondensed matter physicsSpinsStatistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter::Disordered Systems and Neural NetworksPhase (matter)Cluster (physics)Gravitational singularityCritical exponentRandomnessCondensed Matter - Statistical MechanicsPotts modelMathematics
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Detecting gravitational waves from cosmological phase transitions with LISA: an update

2020

MC was funded by the Royal Society under the Newton International Fellowship program. GD would like to thank CNPq (Brazil) for financial support. MH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1), and the Academy of Finland (grant number 286769). SJH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1). The work of JK was supported by Department of Energy (DOE) grant DE-SC0019195 and NSF grant PHY-1719642. TK and GS are funded by the Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy - EXC 2121 \Quantum Universe" - 390833306. JMN is supported by Ramon y Cajal Fellowship contract RYC-2017-22986…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterstandard modelFOS: Physical sciencesContext (language use)gravitational radiation: direct detection01 natural sciencesdark matterbubble: nucleationGravitational wavesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciencesEffective field theoryenergy: densitynumerical calculationsCosmological phase transitionsperturbation theoryPhysics:Matematikk og Naturvitenskap: 400::Fysikk: 430 [VDP]wave: acousticLISACOSMIC cancer database010308 nuclear & particles physicsGravitational wavenew physicsGravitational theorygravitational radiationAstronomy and Astrophysicscritical phenomenagravitational radiation detectorHigh Energy Physics - PhenomenologyGravitational sourcesgravitational radiation: emission[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs modelPerturbation theory (quantum mechanics)gravitational radiation: power spectrum[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]dilatonAstrophysics - Cosmology and Nongalactic Astrophysics
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Neutron star collapse and gravitational waves with a non-convex equation of state

2018

The thermodynamical properties of the equation of state (EoS) of high-density matter (above nuclear saturation density) and the possible existence of exotic states such as phase transitions from nuclear/hadronic matter into quark-gluon plasma, or the appearance of hyperons, may critically influence the stability and dynamics of compact relativistic stars. From a theoretical point of view, establishing the existence of those states requires the analysis of the `convexity' of the EoS. We show indications of the existence of regions in the dense-matter EoS where the thermodynamics may be non-convex as a result of a non-monotonic dependence of the sound speed with the rest-mass density. When th…

Phase transitionEquation of stateAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physics0103 physical sciencesNuclear Experiment010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsBlack holeNeutron starStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceQuark–gluon plasmaAstrophysics - High Energy Astrophysical PhenomenaMonthly Notices of the Royal Astronomical Society
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Quantum sensor networks as exotic field telescopes for multi-messenger astronomy

2020

Multi-messenger astronomy, the coordinated observation of different classes of signals originating from the same astrophysical event, provides a wealth of information about astrophysical processes with far-reaching implications. So far, the focus of multi-messenger astronomy has been the search for conventional signals from known fundamental forces and standard model particles, like gravitational waves (GW). In addition to these known effects, quantum sensor networks could be used to search for astrophysical signals predicted by beyond-standard-model (BSM) theories. Exotic bosonic fields are ubiquitous features of BSM theories and appear while seeking to understand the nature of dark matter…

PhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesField (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesQuantum metrology010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesAstroparticle physicsPhysicsQuantum PhysicsGravitational waveQuantum sensorAstronomyAstronomy and AstrophysicsFundamental interactionQuantum Physics (quant-ph)Astrophysics - Instrumentation and Methods for AstrophysicsEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Observation of Gravitationally Induced Vertical Striation of Polarized Ultracold Neutrons by Spin-Echo Spectroscopy.

2015

We describe a spin-echo method for ultracold neutrons (UCNs) confined in a precession chamber and exposed to a $|B_0|=1~\text{\mu T}$ magnetic field. We have demonstrated that the analysis of UCN spin-echo resonance signals in combination with knowledge of the ambient magnetic field provides an excellent method by which to reconstruct the energy spectrum of a confined ensemble of neutrons. The method takes advantage of the relative dephasing of spins arising from a gravitationally induced striation of stored UCN of different energies, and also permits an improved determination of the vertical magnetic-field gradient with an exceptional accuracy of $1.1~\text{pT/cm}$. This novel combination …

Physics - Instrumentation and DetectorsDephasingGeneral Physics and AstronomyFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesResonance (particle physics)Nuclear physics0103 physical sciencesNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentQCPhysicsNeutrons010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Models TheoreticalNeutron spectroscopyMagnetic fieldCold TemperatureElectric dipole momentKineticsSpin echoUltracold neutronsAtomic physicsGravitationPhysical review letters
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Lorentzian-geometry-based analysis of airplane boarding policies highlights "slow passengers first" as better.

2019

We study airplane boarding in the limit of large number of passengers using geometric optics in a Lorentzian metric. The airplane boarding problem is naturally embedded in a 1+1 dimensional space-time with a flat Lorentzian metric. The duration of the boarding process can be calculated based on a representation of the one-dimensional queue of passengers attempting to reach their seats, into a two-dimensional space-time diagram. The ability of a passenger to delay other passengers depends on their queue positions and row designations. This is equivalent to the causal relationship between two events in space-time, whereas two passengers are time-like separated if one is blocking the other, an…

Physics - Physics and Societygravitation cosmology & astrophysicsbusiness.product_categoryGeodesicComputer scienceinterdisciplinary physicsProcess (computing)FOS: Physical sciencesstatistical physicsGeometryPhysics and Society (physics.soc-ph)Aisleatomic molecular & optical01 natural sciences010305 fluids & plasmasAirplane0103 physical sciencesMetric (mathematics)general physicsLimit (mathematics)010306 general physicsRepresentation (mathematics)businessQueuePhysical review. E
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GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

Physics and Astronomy (miscellaneous)AstronomyGravitational wave detection Gravitational wave sources Gravitational waves Astronomical black holesagn discsAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldsstar-clustersgravitational waves black holesgravitational waves; black holesAGN DISCSgravitational waves; black holes; LIGO; Virgoblack holegeneral relativityLIGOgravitational waveQCQBPhysicsSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)GRAVITATIONAL WAVE-FORMSPROGENITORSCOMPACT BINARIESblack hole: spinPhysicsPERTURBATIONSgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical PhenomenaMETALLICITYmass: asymmetrymetallicitydata analysis methodGeneral relativityMERGERSgr-qcAstrophysics::High Energy Astrophysical PhenomenamultipolePREDICTIONSFOS: Physical sciencesgravitational wavesblack holesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGravitational wavesGeneral Relativity and Quantum CosmologyTheory of relativityBinary black holeSettore FIS/05 - Astronomia e AstrofisicaAstronomical black holesbinary: coalescence0103 physical sciencesnumerical methodsddc:530STAR-CLUSTERS010306 general physicsnumerical calculationsSTFCAstrophysiqueGravitational wave sourcesScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKblack hole: massMass ratioblack holesLIGOEVOLUTIONgravitational radiation detectorBlack holedetector: sensitivityPhysics and Astronomyblack hole: binaryrelativity theorygravitational radiation: emissionmass ratioMultipole expansion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physics
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All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

2018

Made available in DSpace on 2018-11-26T17:45:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-03-22 Australian Research Council Council of Scientific and Industrial Research of India Department of Science and Technology, India Science AMP; Engineering Research Board (SERB), India Ministry of Human Resource Development, India Spanish Agencia Estatal de Investigacion Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme Conselleria d'Educacio i Universitat del Govern de les Illes Balears Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana National Science Centre of Poland Swiss National Science Foundation (SNSF) Russian Foundation for Basic Rese…

Physics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLIGO-VirgoMagnetar01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational waves long transients LIGOGravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSSearch algorithmSIGNALS0103 physical sciencesWaveformlong transientsHigh Energy PhysicsLIGO010306 general physicsgravitational wave010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsLIGO-Virgo; gravitational waves; long duration transient[PHYS]Physics [physics]Gravitational wavelong duration transientLIGOgravitational waves; LIGO-Virgo; long duration transient; Physics and Astronomy (miscellaneous)Black holeMODELNeutron starAmplitudegravitational wavesBLACK-HOLEComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONNEUTRINOAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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