Search results for "Orbital"

showing 10 items of 679 documents

On the timing properties of SAX J1808.4-3658 during its 2015 outburst

2017

We present a timing analysis of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, using non-simultaneous XMM-Newton and NuStar observations. We estimate the pulsar spin frequency and update the system orbital solution. Combining the average spin frequency from the previous observed, we confirm the long-term spin down at an average rate $\dot{\nu}_{\text{SD}}=1.5(2)\times 10^{-15}$ Hz s$^{-1}$. We also discuss possible corrections to the spin down rate accounting for mass accretion onto the compact object when the system is X-ray active. Finally, combining the updated ephemerides with those of the previous outbursts, we find a long-term orbital evolution compatibl…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsCompact star01 natural sciencespulsars: individual: SAX J1808.4-3658Gravitationstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsar0103 physical sciences010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsOrbital periodaccretion accretion discs; stars: neutron; pulsars: individual: SAX J1808.4-3658; X-rays: binaries13. Climate actionSpace and Planetary ScienceQuadrupole:accretion accretion discAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Quantum state engineering using one-dimensional discrete-time quantum walks

2017

Quantum state preparation in high-dimensional systems is an essential requirement for many quantum-technology applications. The engineering of an arbitrary quantum state is, however, typically strongly dependent on the experimental platform chosen for implementation, and a general framework is still missing. Here we show that coined quantum walks on a line, which represent a framework general enough to encompass a variety of different platforms, can be used for quantum state engineering of arbitrary superpositions of the walker's sites. We achieve this goal by identifying a set of conditions that fully characterize the reachable states in the space comprising walker and coin, and providing …

Angular momentumComputer scienceQuantum dynamicsQuantum technologiesFOS: Physical sciencesQuantum simulator02 engineering and technologyTopologySpace (mathematics)01 natural sciencesSettore FIS/03 - Fisica Della Materia010305 fluids & plasmasSet (abstract data type)Open quantum systemQuantum statequantum informationQuantum mechanics0103 physical sciencesExperimental platformquantum walksQuantum walk010306 general physicsPhysicsQuantum networkQuantum PhysicsHigh-dimensional systemsQuantum state preparationbusiness.industryOrbital angular momentumQuantum-state engineeringArbitrary superpositionOne-way quantum computer021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsArbitrary quantum stateQuantum technologyDiscrete time and continuous timeLine (geometry)PhotonicsQuantum Physics (quant-ph)0210 nano-technologybusiness
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Machine Learning-Based Classification of Vector Vortex Beams.

2020

Structured light is attracting significant attention for its diverse applications in both classical and quantum optics. The so-called vector vortex beams display peculiar properties in both contexts due to the non-trivial correlations between optical polarization and orbital angular momentum. Here we demonstrate a new, flexible experimental approach to the classification of vortex vector beams. We first describe a platform for generating arbitrary complex vector vortex beams inspired to photonic quantum walks. We then exploit recent machine learning methods -- namely convolutional neural networks and principal component analysis -- to recognize and classify specific polarization patterns. O…

Angular momentumComputer sciencequantum opticquanutm informationphotonicsPrincipal component analysisGeneral Physics and AstronomyFOS: Physical sciencesMachine learningcomputer.software_genre01 natural sciencesConvolutional neural networkSettore FIS/03 - Fisica Della Materiaquant-phPolarization0103 physical sciencesQuantum walk010306 general physicsQuantum opticsorbital angular momentum; machine learning; vector vortex beamsQuantum PhysicsQuantum opticsbusiness.industryVortex flowOptical polarizationVectorsVortexmachine learningConvolutional neural networksArtificial intelligencePhotonicsbusinessQuantum Physics (quant-ph)computerStructured lightPhysical review letters
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Gauge-origin independent calculation of magnetizabilities and rotational g tensors at the coupled-cluster level.

2007

An implementation of the gauge-origin independent calculation of magnetizabilities and rotational g tensors at the coupled-cluster (CC) level is presented. The properties of interest are obtained as second derivatives of the energy with respect to the external magnetic field (in the case of the magnetizability) or with respect to magnetic field and rotational angular momentum (in the case of the rotational g tensor), while gauge-origin independence and fast basis-set convergence are ensured by using gauge-including atomic orbitals (London atomic orbitals) as well as their extension to treat rotational perturbations (rotational London atomic orbitals). The implementation within our existing …

Angular momentumCoupled clusterMagnetic momentAtomic orbitalChemistryQuantum mechanicsGeneral Physics and AstronomyRotational transitionRotational temperatureTensorPhysical and Theoretical ChemistryAtomic physicsRotational partition functionThe Journal of chemical physics
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Evolutionary paths of binaries with a neutron star - I. The case of SAX J1808.4 - 3658

2018

The evolutionary status of the low mass X-ray binary SAX J1808.4-3658 is simulated by following the binary evolution of its possible progenitor system through mass transfer, starting at a period of $\sim$6.6 hr. The evolution includes angular momentum losses via magnetic braking and gravitational radiation. It also takes into account the effects of illumination of the donor by both the X-ray emission and the spin down luminosity of the pulsar. The system goes through stages of mass transfer and stages during which it is detached, where only the rotationally powered pulsar irradiates the donor. We show that the pulsar irradiation is a necessary ingredient to reach SAX J1808.4-3658 orbital pe…

Angular momentumastro-ph.SRAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityPulsars: individual: SAX J1808.4Settore FIS/05 - Astronomia E AstrofisicaPulsarBinaries: closeMass transfer0103 physical sciencesBinaries: generalStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)3658 -X-rays: binarieHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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Island Homoaromaticity in the W-Shaped 2,4-Diphospha-3-arsapentadienide Anion and Related Compounds - Theoretical and Experimental Investigations

2012

A series of anions with general formula (R2C=P)2Pn– (Pn = N, P, As, Sb; R = H, Me, CF3, SiH3, SiMe3, SiF3) was investigated theoretically at the DFT (RI-BP86/TZVP) and RI-MP2/TZVP levels of approximation. Significantly sharpened central PPnP bond angles were predicted for the species with π-acceptor R substituents. The corresponding bond angle values decrease in the order Pn = N >> P > As > Sb. This finding is in agreement with the previously published structural data for [(Me3Si)2C=P]2P–. An island homoaromaticity was proposed as a suitable explanation for the observed effect. In more detail, it consists of shifting negative charge to the electron-withdrawing terminal groups with formation…

AnionsHomoaromaticity010405 organic chemistryChemistryCharge (physics)010402 general chemistry01 natural sciencesHomoaromaticity0104 chemical sciencesIonInorganic ChemistryCrystallographyDensity functional calculationsMolecular geometryComputational chemistryAb initio quantum chemistry methodsMolecular orbitalsMoleculeMoietyMolecular orbitalAb initio calculations
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The cryogenic anticoincidence detector for ATHENA-XMS: preliminary results from the new prototype

2012

ATHENA has been the re-scoped IXO mission, and one of the foreseen focal plane instrument was the X-ray Microcalorimeter Spectrometer (XMS) working in the energy range 0.3-10 keV, which was a kilo-pixel array based on TES (Transition Edge Sensor) detectors. The need of an anticoincidence (AC) detector is legitimated by the results performed with GEANT4 simulations about the impact of the non x-ray background onto XMS at L2 orbit (REQ. < 0.02 cts/cm2/s/keV). Our consortium has both developed and tested several samples, with increasing area, in order to match the large area of the XMS (64 mm2). Here we show the preliminary results from the last prototype. The results achieved in this work off…

Anticoincidence detectorLow temperature DetectorAnticoincidence detectorsAstrophysicsOrbital mechanicslaw.inventionOpticslawElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringAnticoincidence detectors; High Energy Astrophysics; Low temperature Detectors; TES; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringPhysicsLow temperature DetectorsSpectrometerbusiness.industryApplied MathematicsElectronic Optical and Magnetic MaterialBolometerDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsApplied MathematicCardinal pointMillimeterSatelliteTransition edge sensorHigh Energy AstrophysicbusinessTESHigh Energy AstrophysicsSPIE Proceedings
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Inverted responses of the carbon cycle to orbital forcing in Mesozoic peri‐platform marginal basins: implications for astrochronology

2020

International audience; Astrochronology depends on the faithful record of insolation forcing in climatic proxies, including the carbon isotope composition measured on bulk carbonates (δ13Ccarb). In marginal basins close to carbonate platforms, the source of carbonate is varied, which can impact the record of the astronomical cycles in the δ13Ccarb signal. We compare here the δ13Ccarb values together with detrital and weathering proxies before and during a crisis in the platform carbonate production (Weissert event, Valanginian, ~135 Ma) to document how a change in the carbonate source can affect the record of the orbital forcing by the carbon isotope system. The level of burial diagenesis w…

Astrochronology010506 paleontologyAtmospheric ScienceOrbital forcingGeochemistryPaleontologyWeatheringStructural basin010502 geochemistry & geophysicsOceanography01 natural sciencesDiagenesisCarbon cyclechemistry.chemical_compoundchemistry13. Climate action[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryMarlCarbonateGeology0105 earth and related environmental sciences
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Milankovitch forcing of Early Jurassic wildfires

2019

The Early Jurassic was characterized by major climatic and environmental perturbations which can be seen preserved at high resolution on orbital timescales. The Early Jurassic is a period of overall global warmth, and therefore serves as a suitable modern-day analogue to understand changes in the Earth System. Presently, Earth’s climate is warming and the frequency of large wildfires appears to be increasing. Recent research has indicated that Quaternary deposits reveal that wildfires respond to orbital forcings; however, to date no study has been able to test whether wildfire activity corresponds to changes over Milankovitch timescales in the deep past. A high-resolution astrochronology ex…

AstrochronologyMilankovitch cyclesOrbital forcingSedimentary rockPhysical geographyVegetationForcing (mathematics)QuaternaryMonsoonGeology
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XMM-Newton detection of the 2.1 ms coherent pulsations from IGR J17379-3747

2018

We report on the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from which we estimate an orbital period of ~1.9 hours and a projected semi-major axis of ~8 lt-ms. Taking into account the lack of eclipses (inclination angle of &lt; 75 deg) and assuming a neutron star mass of 1.4 Msun, we estimated a minimum companion star of ~0.06 Msun. Considerations on the probability distribution of the binary inclination angle make less likely the hypothesis of a main-sequence companion star. On the other hand, the close correspondence with the orbital parameters of the accreting millisecond puls…

Astrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesgeneral; stars: neutron; X-rays: binaries; accretion accretion disks [binaries]AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesstars: neutronSettore FIS/05 - Astronomia E AstrofisicaMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsOrbital elementsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion accretion disksAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsOrbital periodX-rays: binarieNeutron starbinaries: generalSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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