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Results for “TRIPLETS”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Singlet-Triplet Excitations and Long-Range Entanglement in the Spin-Orbital Liquid Candidate FeSc 2 S 4
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Energy deposition studies for the high-luminosity Large Hadron Collider inner triplet magnets
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Design of Coil-Dominated Quadrupole Triplet for High Rigidity Isotope Beams
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Singlet, Triplet, Electron and Hole Transport Along Single Polymer Chains
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Direct observation of triplet energy transfer from semiconductor nanocrystals
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Triplet p-wave superconductivity in the low-density extended hubbard model with Coulomb repulsion
We analyze superconducting instabilities in 3D and 2D extended Hubbard model with Coulomb repulsion between electrons on neighboring sites in the limit of low electron density on simple cubic (square) lattice.
Triplet Network with Attention for Speaker Diarization
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A 3D FPGA Track Segment Seeding Engine Based on the Tiny Triplet Finder
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APS March Meeting 2024: "Error attribution for singlet-triplet qubits through randomized benchmarking in the presence of temporally correlated noise"
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Dephasing and error dynamics affecting a singlet-triplet qubit during coherent spin shuttling
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Increasing the Radiative Rates of Triplet Emitters to Achieve Long-Lived and Efficient White-Emitting Organic Light Emitting Devices (OLEDs)
The objective of the project is to develop and validate white organic light emitting device WOLEDs with internal efficiencies of 100% and lifetimes exceeding a time at which the luminance drops by 30% (T 70 ) of 50,000 hr at an initial luminance of L 0 = 3000 cd/m 2 .
Magnetic field study of spin-orbit and nuclear spin dynamics on singlet-triplet qubit coherence in Si/SiGe quantum dots
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Time-sequence Spectroscopy of Epsilon CrA: The 518 nm Mg i Triplet Region Analyzed with Broadening Functions
High-resolution spectroscopic observations of the W UMa-type binary ϵ CrA obtained as a time-monitoring sequence on four full and four partial nights within two weeks have been used to derive orbital elements of the system and discuss the validity of the Lucy model for description of the radial-velocity data. The observations had more extensive temporal coverage and better quality than similar time-sequence observations of the contact binary AW UMa. The two binaries share several physical properties and show very similar deviations from the Lucy model: the primary component is a rapidly rotating star almost unaffected by the presence of the secondary component, while the latter is embedded in a complex gas flow and appears to have its own rotation-velocity field, in contradiction to the model. The spectroscopic mass ratio is found to be larger than the one derived from the light-curve analysis, as in many other W UMa-type binaries, but the discrepancy for ϵ CrA is relatively minor, much smaller than for AW UMa. The presence of the complex velocity flows contradicting the assumption of solid-body rotation suggests a necessity of modification to the Lucy model, possibly along the lines outlined by Stȩpień in his concept of energy transfer between the binary components.
POLARIZATION AND THE TRIPLET ELECTRON-HYDROGEN SCATTERING LENGTH
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Oscillator strengths for singlet and triplet series in neutral helium
Oscillator strengths for electric dipole transitions in spectrum series of neutral helium