Search results for "angular dependence"

showing 10 items of 614 documents

Angular dependence of the domain wall depinning field in the sensors with segmented corners

2017

Rotating domain wall based sensors that have recently been developed are based on a segmented looping geometry. In order to determine the crucial pinning of domain walls in this special geometry, we investigate the depinning under different angles of an applied magnetic field and obtain the angular dependence of the depinning field of the domain walls. Due to the geometry, the depinning field not only exhibits a 180$^\circ$-periodicity but a more complex dependence on the angle. The depinning field depends on two different angles associated with the initial state and the segmented geometry of the corner. We find that depending on the angle of the applied field two different switching proces…

010302 applied physics0301 basic medicineCondensed Matter - Materials ScienceHistoryMaterials scienceField (physics)Condensed matter physicsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciences01 natural sciencesComputer Science ApplicationsEducationMagnetic field03 medical and health sciences030104 developmental biologyDomain wall (magnetism)0103 physical sciencesAngular dependence
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"Table 12" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DPHI in the diphoton mass range 80 TO 350 GeV.

20477612047661InclusiveD2SIG/DM/DPHIPBAR P --> GAMMA GAMMA XAzimuthal Angular Dependence1960.0Double Differential Cross Section
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"Table 6" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DPHI in the diphoton mass range 30 TO 50 GeV.

20477612047661InclusiveD2SIG/DM/DPHIPBAR P --> GAMMA GAMMA XAzimuthal Angular Dependence1960.0Double Differential Cross Section
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"Table 9" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DPHI in the diphoton mass range 50 TO 80 GeV.

20477612047661InclusiveD2SIG/DM/DPHIPBAR P --> GAMMA GAMMA XAzimuthal Angular Dependence1960.0Double Differential Cross Section
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"Table 7" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DCOS(THETA) in the diphoton mass range 30 TO 50 GeV.

20477612047661InclusivePBAR P --> GAMMA GAMMA XD2SIG/DM/DCOS(THETA)1960.0Double Differential Cross SectionAngular Dependence
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"Table 10" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DCOS(THETA) in the diphoton mass range 50 TO 80 GeV.

20477612047661InclusivePBAR P --> GAMMA GAMMA XD2SIG/DM/DCOS(THETA)1960.0Double Differential Cross SectionAngular Dependence
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"Table 13" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Double differential cross section D2SIG/DM/DCOS(THETA) in the diphoton mass range 80 TO 350 GeV.

20477612047661InclusivePBAR P --> GAMMA GAMMA XD2SIG/DM/DCOS(THETA)1960.0Double Differential Cross SectionAngular Dependence
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"Table 3" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Single differential cross section DSIG/DPHI.

20477612047661InclusiveSingle Differential Cross SectionDSIG/DPHIPBAR P --> GAMMA GAMMA XAzimuthal Angular Dependence1960.0
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"Table 4" of "Measurement of direct photon pair production cross sections in ppbar collisions at sqrt(s)=1.96 TeV"

2010

Single differential cross section DSIG/DCOS(THETA).

20477612047661InclusiveSingle Differential Cross SectionPBAR P --> GAMMA GAMMA X1960.0DSIG/DCOS(THETA)Angular Dependence
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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

2007

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar…

Active galactic nucleus[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]Cosmic background radiationFOS: Physical sciencesFluxOsservatorio Pierre AugerCosmic rayanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmici0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsBackground radiationNuclei galattivi attiviPhysicsPierre Auger ObservatorySPECTRUMMultidisciplinary[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMedicine (all); MultidisciplinaryMedicine (all)Settore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)angular dependence [cosmic radiation]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaExperimental High Energy Physicsddc:500Energy (signal processing)experimental results
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