Results 191 to 200 of about 910,791 (369)
The Astrophysical JournalWe report simultaneous detection of twin kHz and ∼40 Hz quasiperiodic oscillations (QPOs) in the time-resolved analysis of the AstroSat/LAXPC observation of the neutron star low-mass X-ray binary, 4U 1728-34.
Kewal Anand +5 more
doaj +1 more source
Disordered Rocksalts as High‐Energy and Earth‐Abundant Li‐Ion Cathodes
Advanced Materials, EarlyView.Disordered rocksalts with lithium excess (DRX) offer a new direction in Li‐ion cathode design beyond conventional Ni‐ and Co‐based materials. This review highlights the design principles, synthesis strategies, and performance optimization of DRX oxides and oxyfluorides for energy‐dense, sustainable batteries using Earth‐abundant transition metals and ...
Han‐Ming Hau +10 more
wiley +1 more source
Electrobaryonic axion: hair of neutron stars
Journal of High Energy PhysicsAxion-like particles are predicted in many physics scenarios beyond the Standard Model (SM). Their interactions with SM particles may arise from the triangle anomaly of the associated global symmetry, along with other SM global and gauge symmetries ...
Yang Bai, Carlos Henrique de Lima
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Neutron Star Structure from Pulsar Observations [PDF]
, 1974 David Pines, J. Shaham, M. Ruderman
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Stiffening Liquid Crystal Elastomers with Liquid Crystal Inclusions
Advanced Materials, EarlyView.Incorporation of low molecular weight liquid crystals (LC) into liquid crystal elastomers (LCE) leads to a significant increase in their stiffness and output work density. Such remarkable stiffening is attributed to nanoscale phase‐separation and the formation of induced‐smectic domains in polydomain and monodomain LC‐LCEs, respectively.
Sahad Vasanji +7 more
wiley +1 more source
On the Dynamical Evolution of the Asteroid Belt in a Massive Star–Neutron Star Binary
The Astrophysical JournalSome fast radio bursts (FRBs) exhibit repetitive behaviors, and their origins remain enigmatic. It has been argued that repeating FRBs could be produced by the interaction between a neutron star and an asteroid belt.
Chen Deng +4 more
doaj +1 more source
Accretion onto a small black hole at the center of a neutron star. [PDF]
Phys Rev D, 2021 Richards CB, Baumgarte TW, Shapiro SL.
europepmc +1 more source
Instability of Neutron Star Matter for Pion Condensation [PDF]
, 1975 Akira Suzuki, Y. Futami, Y. Takahashi
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AI‐Driven Defect Engineering for Advanced Thermoelectric Materials
Advanced Materials, EarlyView.This review presents how AI accelerates the design of defect‐tuned thermoelectric materials. By integrating machine learning with high‐throughput data and physics‐informed representations, it enables efficient prediction of thermoelectric performance from complex defect landscapes.
Chu‐Liang Fu +9 more
wiley +1 more source
Accretion in supergiant High Mass X-ray Binaries
EPJ Web of Conferences, 2014 Supergiant High Mass X-ray Binary systems (sgHMXBs) consist of a massive, late type, star and a neutron star. The massive stars exhibits strong, radiatively driven, stellar winds.
Manousakis Antonios +2 more
doaj +1 more source