Search results for "Model theory"

showing 10 items of 681 documents

Optical and X-ray Observations of M31N 2007-12b: An Extragalactic Recurrent Nova with a Detected Progenitor?

2009

We report combined optical and X-ray observations of nova M31N 2007-12b. Optical spectroscopy obtained 5 days after the 2007 December outburst shows evidence of very high ejection velocities (FWHM H$\alpha \simeq 4500$ km s$^{-1}$). In addition, Swift X-ray data show that M31N 2007-12b is associated with a Super-Soft Source (SSS) which appeared between 21 and 35 days post-outburst and turned off between then and day 169. Our analysis implies that $M_{\rm WD} \ga 1.3 $M$_{\odot}$ in this system. The optical light curve, spectrum and X-ray behaviour are consistent with those of a recurrent nova. Hubble Space Telescope observations of the pre-outburst location of M31N 2007-12b reveal the prese…

Physics010504 meteorology & atmospheric sciencesRed giantLocal GroupFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsNova (laser)Type (model theory)Light curve01 natural sciencesSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Science0103 physical sciencesRS OphiuchiMagnitude (astronomy)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
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Numerical modeling and design of a disk-type rotating permanent magnet induction pump

2016

Abstract Electromagnetic induction pumps with rotating permanent magnets appear to be the most promising devices to transport liquid metals in high-temperature applications. Here we present a numerical methodology to simulate the operation of one particular modification of these types of pumps: a disk-type induction pump. The numerical model allows for the calculation and analysis of the flow parameters, including the pressure–flow rate characteristics of the pump. The simulations are based on an iterative fully coupled scheme for electromagnetic and hydrodynamic solvers. The developed model is verified by comparing with experimental data obtained using a Pb-Bi loop test facility, for press…

Physics020209 energyMechanical EngineeringFlow (psychology)Numerical modelingExperimental data02 engineering and technologyMechanicsType (model theory)01 natural sciences010305 fluids & plasmasElectromagnetic inductionVolumetric flow rateLoop (topology)Nuclear Energy and EngineeringMagnet0103 physical sciences0202 electrical engineering electronic engineering information engineeringGeneral Materials ScienceCivil and Structural EngineeringFusion Engineering and Design
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On Fučík type spectrum for problem with integral nonlocal boundary condition

2019

The Fučík equation x' '= -μ x+λ x- with two types of nonlocal boundary value conditions are considered. The Fučík type spectrum for both problems are constructed. The visualization of the spectrum for some values of parameter γ is provided.

PhysicsApplied MathematicsSpectrum (functional analysis)Mathematical analysisNonlocal boundaryFučik type problemlcsh:QA299.6-433lcsh:AnalysisType (model theory)integral nonlocal conditionValue (mathematics)AnalysisFučik spectrumNonlinear Analysis
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High energy neutrinos from novae in symbiotic binaries: The case of V407 Cygni

2010

Detection of high-energy (>= 100 MeV) gamma rays by the Fermi Large Area Telescope from a nova in the symbiotic binary system V407 Cygni has opened the possibility of high-energy neutrino detection from this type of source. A thermonuclear explosion on the white dwarf surface sets off a nova shell in motion that expands and slows down in a dense surrounding medium provided by the red giant companion. Particles are accelerated in the shocks of the shell and interact with the surrounding medium to produce observed gamma rays. We show that proton-proton interaction, which is most likely responsible for producing gamma rays via neutral pion decay, produces >= 0:1 GeV neutrinos that can be detec…

PhysicsAstrofísicaHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsRed giantAstrophysics::High Energy Astrophysical PhenomenaWhite dwarfFOS: Physical sciencesCosmic rayAstrophysicsType (model theory)High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)PionHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorAstrophysics::Solar and Stellar AstrophysicsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaNuclear ExperimentAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Small Angular Scale Simulations of the Microwave Sky

1996

We describe and compare two types of microwave sky simulations which are good for small angular scales. The first type uses expansions in spherical harmonics, and the second one is based on plane waves and the Fast Fourier Transform. The angular power spectrum is extracted from maps corresponding to both types of simulations, and the resulting spectra are appropriately compared. In this way, the features and usefulness of Fourier simulations are pointed out. For $\ell \geq 100$, all the simulations lead to similar accuracies; however, the CPU cost of Fourier simulations is $\sim 10$ times smaller than that for spherical harmonic simulations. For $\ell \leq 100$, the simulations based on sph…

PhysicsAstrophysics (astro-ph)Fast Fourier transformPlane waveFOS: Physical sciencesSpectral densitySpherical harmonicsAstronomy and AstrophysicsAstrophysicsType (model theory)AstrophysicsSpectral lineComputational physicssymbols.namesakeFourier transformSpace and Planetary SciencesymbolsMicrowaveThe Astrophysical Journal
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Radiative zone solar magnetic fields and g modes

2005

We consider a generalized model of seismic-wave propagation that takes into account the effect of a central magnetic field in the Sun. We determine the g-mode spectrum in the perturbative magnetic field limit using a one-dimensional Magneto-Hydrodynamics (MHD) picture. We show that central magnetic fields of about 600-800 kG can displace the pure g-mode frequencies by about 1%, as hinted by the helioseismic interpretation of GOLF observations.

PhysicsAstrophysics (astro-ph)Spectrum (functional analysis)FOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsAstrophysicsRadiation zoneInterpretation (model theory)Magnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Space and Planetary ScienceQuantum electrodynamicsAstrophysics::Solar and Stellar AstrophysicsLimit (mathematics)MagnetohydrodynamicsMonthly Notices of the Royal Astronomical Society
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Ultrasonic cavity solitons

2007

We report on a new type of localized structure, an ultrasonic cavity soliton, supported by large aspect-ratio acoustic resonators containing viscous media. These states of the acoustic and thermal fields are robust structures, existing whenever a spatially uniform solution and a periodic pattern coexist. Direct proof of their existence is given both through the numerical integration of the model and through the analysis and numerical integration of a generalized Swift-Hohenberg equation, derived from the microscopic equations under conditions close to nascent bistability. An analytical solution for the ultrasonic cavity soliton is given.

PhysicsBistabilityGeneral Physics and AstronomyFOS: Physical sciencesPattern Formation and Solitons (nlin.PS)Type (model theory)Nonlinear Sciences - Pattern Formation and SolitonsNumerical integrationResonatorClassical mechanicsThermalUltrasonic sensorDirect proofSoliton
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Topology of multiplex heterogeneous networks of Hodgkin-Huxley-type of models with bistability leading to stabilization stable equilibrium

2021

The dynamics of a multiplex heterogeneous networks of oscillators is studied. Two types of very similar models based on the Hodgkin-Huxley formalism are used as the basic elements of the network: the first one demonstrates bursting oscillations; the second one manifests bistability between bursting oscillations and stable equilibrium. Multiplex networks were developed and investigated, assuming more active communication between models with bistability. Different topologies of the networks are studied. It is shown that in this case it is enough to have one element with bistability in the subnetworks in order to stabilize the equilibrium state in the entire network.

PhysicsBistabilityThermodynamic equilibriumTopology (electrical circuits)MultiplexType (model theory)TopologyNetwork topologyHeterogeneous networkHodgkin–Huxley model2021 5th Scientific School Dynamics of Complex Networks and their Applications (DCNA)
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Lusternik-Schnirelmann Critical Values and Bifurcation Problems

1987

We present a method to calculate bifurcation branches for nonlinear two point boundary value problems of the following type $$ \{ _{u(a) = u(b) = 0,}^{ - u'' = \lambda G'(u)} $$ (1.1) where G : R → R is a smooth mapping. This problem can be formulated equivalently as $$ g' \left(u \right)= \mu u, $$ (1.2) where $$ g \left(u \right)= \overset{b} {\underset{a} {\int}} G \left(u \left(t \right) \right) dt $$ (1.3) and μ = 1/λ. Solutions of this problem can be found by locating the critical points of the functional g : H → R on the spheres \(S_r= \lbrace x \in H \mid \;\parallel x \parallel =r \rbrace, r >0.\) (The Lagrange multiplier theorem.)

PhysicsCombinatoricsPoint boundaryBogdanov–Takens bifurcationInfinite-period bifurcationType (model theory)Bifurcation
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The Zero-Check for Eliminating Non-Significant Elements

1970

During continued matrix operations like the simplex method a lot of small non-significant elements, the actual value of which is zero,usually augment the working coefficient matrix. These elements are caused by round-off errors. They arise in the following manner in a computation of the type: $${\rm{d}}\, = \,{\rm{a}}\,{\rm{ - }}\,{\rm{b}}{\rm{.c}}$$ with e.g. the data (in FORTRAN notation) $${\rm{a}}\, = \,{\rm{2}}\,{\rm{ = }}\,{\rm{.20000000}}\,{\rm{E}}\,{\rm{01}}$$ $${\rm{b}}\, = \,{\rm{6}}\,{\rm{ = }}\,{\rm{.60000000}}\,{\rm{E}}\,{\rm{01}}$$ $${\rm{c}}\, = \,{\rm{1/3}}\,{\rm{ = }}\,{\rm{.33333333}}\,{\rm{E}}\,{\rm{00}}$$

PhysicsCombinatoricsZero (complex analysis)Type (model theory)
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