0000000000153562

AUTHOR

Aristide Lemaître

showing 3 related works from this author

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

2021

Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter under extreme conditions. A significant fraction of the known pulsar population belongs to binary systems. Searching for unknown neutron stars in binary systems requires specialized algorithms to address unknown orbital frequency modulations. We present a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, binaryskyhough pipeline. The search analyzes the most s…

binary: orbitneutron star: binaryPhysics and Astronomy (miscellaneous)Astronomybinary [neutron star]AstrophysicsGravitational Waves; LIGO (Observatory); Neutron Stars01 natural sciencesneutron starsGeneral Relativity and Quantum CosmologyMonte Carlo: Markov chainPhysics Particles & Fieldsbinary starsbinary systemsBinary SystemsLIGOgravitational waveQCQBpulsarastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studySettore FIS/03Physicsorbit [binary]General relativityPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenabinary stardata analysis methodsensitivity [detector]General relativitygr-qcfrequency [modulation]Populationneutron star: spinFOS: Physical sciencesalternative theories of gravityMarkov chain [Monte Carlo]General Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGravitational Waves Neutron Stars Binary Systems LIGO VirgoLIGO (Observatory)emission [gravitational radiation]Pulsarbinary: coalescence0103 physical sciencesBinary starddc:530spin [neutron star]background [gravitational radiation]010306 general physicseducationSTFCOrbital elementsGravitational WavesScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundmodulation: frequencyRCUKNeutron StarsLIGOgravitational radiation detectordetector: sensitivityNeutron starVIRGOgravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]binary stars; neutron stars
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Unusual domain-wall motion in ferromagnetic semiconductor films with tetragonal anisotropy

2009

International audience; Magnetic field-driven domain-wall propagation in the flow regime is investigated in (Ga, Mn) As ferromagnetic semiconductor layers. Square-shape magnetic domains with an unexpected orientation of their edges, at pi/8 with respect to the anisotropy axes, are found. This is shown to arise from the effect of tetragonal magnetic anisotropy on domain-wall dynamics. Using a one-dimensional model for domain-wall motion and modeling domain growth by contour dynamics the shape and orientation of domains and their field range for existence are well reproduced. These results point to the key role of the vectorial nature of the order parameter in the dynamics of ferromagnetic do…

010302 applied physicsPhysicsCondensed matter physicsMagnetic domainDemagnetizing fieldCondensed Matter PhysicsMagnetocrystalline anisotropy01 natural sciencesMagnetic susceptibilityElectronic Optical and Magnetic MaterialsMagnetic anisotropyDomain wall (magnetism)Magnetic shape-memory alloy0103 physical sciences[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]Single domain010306 general physicsPhysical Review B
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Current-induced fingering instability in magnetic domain walls

2015

The shape instability of magnetic domain walls under current is investigated in a ferromagnetic (Ga,Mn)(As,P) film with perpendicular anisotropy. Domain wall motion is driven by the spin transfer torque mechanism. A current density gradient is found either to stabilize domains with walls perpendicular to current lines or to produce finger-like patterns, depending on the domain wall motion direction. The instability mechanism is shown to result from the non-adiabatic contribution of the spin transfer torque mechanism.

Materials scienceMagnetic domainCiencias FísicasINSTABILITYFOS: Physical sciencesINGENIERÍAS Y TECNOLOGÍAS02 engineering and technologySPINTRONIC01 natural sciencesInstabilityPhysics::Fluid Dynamics//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/2.10 [https]0103 physical sciencesPerpendicular[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]010306 general physicsNanotecnologíaCondensed Matter - Materials ScienceCondensed matter physicsSpin-transfer torqueMaterials Science (cond-mat.mtrl-sci)//purl.org/becyt/ford/1.3 [https]Nano-materiales021001 nanoscience & nanotechnologyCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsAstronomíaDomain wall (magnetism)Ferromagnetism//purl.org/becyt/ford/2 [https]Current (fluid)0210 nano-technologyCurrent densityCIENCIAS NATURALES Y EXACTAS
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