Results 101 to 110 of about 729,877 (305)

Generating Unconventional Spin‐Orbit Torques With Patterned Phase Gradients in Tungsten Thin Films

open access: yesAdvanced Materials, EarlyView.
ABSTRACT A key aim in spintronics is to achieve current‐induced magnetization switching via spin‐orbit torques without external magnetic fields. For this, the focus of recent work has been on introducing controlled lateral gradients across ferromagnet/heavy‐metal devices, giving variations in thickness, composition, or interface quality.
Lauren J. Riddiford   +9 more
wiley   +1 more source

Cyclotron lines in highly magnetized neutron stars [PDF]

open access: yesAstronomy & Astrophysics, 2018
Cyclotron lines, also called cyclotron resonant scattering features are spectral features, generally appearing in absorption, in the X-ray spectra of objects containing highly magnetized neutron stars, allowing the direct measurement of the magnetic ...
R. Staubert   +12 more
semanticscholar   +1 more source

Neutrostriction in Neutron Stars [PDF]

open access: yesOld and New Concepts of Physics, 2007
It is demonstrated that not only gravity, but also neutrostriction forces due to optical potential created by coherent elastic neutron-neutron scattering can hold a neutron star together. The latter forces can be stronger than gravitational ones. The effect of these forces on mass, radius and structure of the neutron star is estimated.
openaire   +2 more sources

Hybrid Stars that Masquerade as Neutron Stars [PDF]

open access: yesThe Astrophysical Journal, 2005
22 pages, LaTeX.
Alford, Mark   +3 more
openaire   +2 more sources

Emergent Spin Supersolids in Frustrated Quantum Materials

open access: yesAdvanced Materials, EarlyView.
This review highlights developments in the study of spin super‐solids in frustrated quantum materials. Advanced experimental characterizations and computational studies enable a comprehensive understanding of the driving mechanisms of spin super‐solidity in various layered transition‐metal compounds, bridging materials, experiments, and theory aspects.
Yixuan Huang   +2 more
wiley   +1 more source

Axisymmetric cooling of neutron stars with strong magnetic fields

open access: yesAstronomy & Astrophysics
Context. Strong magnetic fields can affect both the structure and particle composition of neutron stars. Aims. We seek to understand the thermal evolution of strongly magnetized neutron stars, particularly investigating how strong magnetic fields and ...
Negreiros R., Peterson J., Dexheimer V.
doaj   +1 more source

Studying strong phase transitions in neutron stars with gravitational waves [PDF]

open access: yesPhysical Review D, 2019
The composition of neutron stars at the extreme densities reached in their cores is currently unknown. Besides nuclear matter of normal neutrons and protons, the cores of neutron stars might harbor exotic matter such as deconfined quarks.
K. Chatziioannou, Sophia Han
semanticscholar   +1 more source

The physics of neutron stars [PDF]

open access: yesPhysics-Uspekhi, 2010
28 pages, 8 figures (in v2 and v3, several typos have been fixed). Invited topical review for the special issue of Uspekhi Fiz. Nauk (Physics - Uspekhi) in memory of V. L. Ginzburg (translated from Russian by Yu. V. Morozov, edited by A. M. Semikhatov and by the author)
openaire   +2 more sources

Review of Inorganic Separator Engineering for Next‐Generation Lithium–Sulfur Batteries: Compromise or Cornerstone?

open access: yesAdvanced Materials, EarlyView.
Inorganic compound‐modified separators transform lithium–sulfur batteries from passive polysulfide confinement to active reaction‐pathway regulation. A Practical Relevance Index (PRI)‐guided framework bridges interfacial chemistry of inorganic separators with practical constraints, establishing unified design principles for scalable, high‐energy ...
Yuting Qin   +7 more
wiley   +1 more source

Contraction of cold neutron star due to in the presence a quark core

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
Motivated by importance of the existence of quark matter on structure of neutron star. For this purpose, we use a suitable equation of state (EoS) which include three different parts: (i) a layer of hadronic matter, (ii) a mixed phase of quarks and ...
B. Eslam Panah   +2 more
doaj   +1 more source

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