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Translationally invariant coupled cluster method in coordinate space for nuclei

2002

We study a formulation of the translationally invariant coupled cluster method in coordinate space for finite nuclei. The new formulation remedies convergence problems that plagued previous calculations in configuration space. The method is applied to light nuclei using semi-realistic central interactions.

PhysicsLight nucleusNuclear and High Energy Physics/dk/atira/pure/subjectarea/asjc/3100/3106Nuclear structureInvariant (physics)Physics and Astronomy(all)Coupled clusterClassical mechanics/dk/atira/pure/subjectarea/asjc/3100Quantum electrodynamicsNuclear binding energyConfiguration spaceCLOSED-SHELL NUCLEI; MODEL-CALCULATIONS; CBF THEORY; DEPENDENT CORRELATIONS; PAIR CORRELATIONS; FINITE SYSTEMS; GROUND-STATE; JASTROW; O-16; Nuclear binding energy; Nuclear model; Nuclear structure; Nucleon-nucleon potential (formulation of translationally invariant coupled cluster method in coordinate space for closed shell nuclei within 0p-shell with use of semi-realistic central nucleon-nucleon interactions)Coordinate spaceGround state
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London equation of state for a quantum-hard-sphere system

1994

The London analytical interpolation equation between zero and packing densities for the ground-state energy of a many-boson hard-sphere system is corrected for the reduced mass of a pair of particles in a ``sphere-of-influence'' picture. It is thus brought into good agreement with computer simulations and with experimental results extrapolated out to close packing.

PhysicsLondon equationsClassical mechanicsZero (complex analysis)Close-packing of equal spheresState (functional analysis)Reduced massGround stateQuantumInterpolationPhysical Review B
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Dynamic rigidity transition.

2003

An inflated closed loop (or membrane) is used to demonstrate a dynamic rigidity transition that occurs when impact energy is added to the loop in static equilibrium at zero temperature. The only relevant parameter in this transition is the ratio of the energy needed to collapse the loop and the impact energy. When this ratio is below a threshold value close to unity, the loop collapses into a high-entropy floppy state, and it does not return to the rigid state unless the impact energy can escape. The internal oscillations are in the floppy state dominated by 1/f(2) noise. When the ratio is above the threshold, the loop does not collapse, and the internal oscillations resulting from the impa…

PhysicsMechanical equilibriumClassical mechanicsRigidity (electromagnetism)lawImpact energyMechanicsZero temperatureClosed looplaw.inventionPhysical review. E, Statistical, nonlinear, and soft matter physics
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Translationally invariant treatment of pair correlations in nuclei - II. Tensor correlations

1998

We study the extension of our translationally invariant treatment of few-body nuclear systems to include tensor forces and correlations. It is shown that a direct application of our method is not as successful for realistic V6 interactions as our previous results for V4 potentials suggested. We investigate the cause in detail for the case of $^4$He, and show that a combination of our method with that of Jastrow-correlated wave functions seems to be a lot more powerful, thereby suggesting that for mildly to strongly repulsive forces such a hybrid procedure may be an appropriate description.

PhysicsNuclear and High Energy PhysicsCLOSED-SHELL NUCLEI; MONTE-CARLO CALCULATIONS; MODEL-CALCULATIONS; COORDINATE SPACE; CBF THEORY; POTENTIALS; CLUSTERS; SYSTEMS; STATE; HE-4Nuclear Theory/dk/atira/pure/subjectarea/asjc/3100/3106V6 forcesFOS: Physical sciencesFísicaInvariant (physics)A ≤ 16Translational invarianceNuclear Theory (nucl-th)Tensor correlationsJastrow correlationsWave functionMathematical physics
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Bloch analysis of finite periodic microring chains

2005

We apply Bloch analysis to the study of finite periodic cascading of microring resonators. Diagonalization of the standard transfer matrix approach not only allows to find an exact analytic expression for transmission and reflection, but also to derive a closed form solution for the field in every point of the structure. To give more physical insight we analyze the main features of the transmission resonances in a finite chain and we give some hints for their experimental verification

PhysicsPhysics and Astronomy (miscellaneous)Field (physics)Mathematical analysisGeneral EngineeringFOS: Physical sciencesGeneral Physics and AstronomyTransfer matrixResonatorReflection (mathematics)Chain (algebraic topology)Transmission (telecommunications)Point (geometry)Closed-form expressionOptics (physics.optics)Physics - OpticsApplied Physics B
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The Anti-de Sitter Gott Universe: A Rotating BTZ Wormhole

1999

Recently it has been shown that a 2+1 dimensional black hole can be created by a collapse of two colliding massless particles in otherwise empty anti-de Sitter space. Here we generalize this construction to the case of a non-zero impact parameter. The resulting spacetime, which may be regarded as a Gott universe in anti-de Sitter background, contains closed timelike curves. By treating these as singular we are able to interpret our solution as a rotating black hole, hence providing a link between the Gott universe and the BTZ black hole. When analyzing the spacetime we see how the full causal structure of the interior can be almost completely inferred just from considerations of the conform…

PhysicsPhysics and Astronomy (miscellaneous)Spacetimemedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyUniverseBlack holeGeneral Relativity and Quantum CosmologyRotating black holeAnti-de Sitter spaceWormholeBTZ black holemedia_commonMathematical physicsClosed timelike curve
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New insights into black bodies

2012

Planck's law describes the radiation of black bodies. The study of its properties is of special interest, as black bodies are a good description for the behavior of many phenomena. In this work a new mathematical study of Planck's law is performed and new properties of this old acquaintance are obtained. As a result, the exact form for the locus in a color-color diagrams has been deduced, and an analytical formula to determine with precision the black body temperature of an object from any pair of measurements has been developed. Thus, using two images of the same field obtained with different filters, one can compute a fast estimation of black body temperatures for every pixel in the image…

PhysicsPixelGeneral Physics and AstronomyClassical Physics (physics.class-ph)FOS: Physical sciencesPhysics - Classical PhysicsRadiationClosed and exact differential formssymbols.namesakeBlack bodysymbolsStatistical physicsPlanckLocus (mathematics)Astrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Binary evolution of PSR J1713+0747

2007

PSR J1713+0747 is a binary millisecond radio pulsar with a long orbital period (Porb ∼ 68 d) and a very low neutron star mass (M NS = 1.3 ± 0.2 M⊙). We simulate the evolution of this binary system with an accurate numerical code, which keeps into account both the evolution of the primary and of the whole binary system. We show that strong ejection of matter from the system is fundamental to obtain a mass at the end of the evolution that is within 1 - σ from the observed one, but propeller effects are almost negligible in such a system, where the accretion rate is always near to the Eddington limit. We show that there are indeed two mechanisms can account for the amount of mass loss from the…

PhysicsPulsars: individual: PSR J1713+0747close; Pulsars: individual: PSR J1713+0747; Relativity; Stars: neutron; X-rays: binaries [Accretion accretion discs; Binaries]X-ray binaryAstrophysicsBinary pulsarStars: neutronRelativityNeutron starsymbols.namesakeX-rays: binariesPulsarMillisecond pulsarBinaries: closeStellar mass lossEddington luminositysymbolsBinary systemAccretion accretion disc
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The different fates of a low-mass X-ray binary - I. Conservative mass transfer

2003

We study the evolution of a low mass x-ray binary coupling a binary stellar evolution code with a general relativistic code that describes the behavior of the neutron star. We assume the neutron star to be low--magnetized (B~10^8 G). In the systems investigated in this paper, our computations show that during the binary evolution the companion transfers as much as 1 solar mass to the neutron star, with an accretion rate of 10^-9 solar masses/yr. This is sufficient to keep the inner rim of the accretion disc in contact with the neutron star surface, thus preventing the onset of a propeller phase capable of ejecting a significant fraction of the matter transferred by the companion. We find th…

PhysicsSolar massGravitational waveAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)X-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysicsAccretion (astrophysics)Black holeNeutron starrelativity binaries: close stars: neutron pulsars: general X-rays: binariesPulsarSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsStellar evolutionAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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El “Aula del Cel”: astronomy approaching high school

2005

The “Aula del Cel” is a project carried out by the Astronomical Obsevatory of the University of Valencia, Spain. It offers high-school teachers a tool for teaching Astronomy to 10 to 17 year-old students. Different programs, experiments, and audiovisual presentations have been prepared by a team formed both by professional astronomers and teachers, and are offered in a format chosen to suit each particular age and curriculum group. Special sessions have been designed for students with special needs (for example blind or autistic children) in close contact with the pedagogical teams responsible for their education. Nearly three thousand students have already visited the “Aula del Cel” over t…

PhysicsSpace and Planetary ScienceGeneral EngineeringAstronomyAstronomy and AstrophysicsSpecial needsSchool communityClose contactCurriculumEAS Publications Series
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