Results 181 to 190 of about 280,623 (343)
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M+21 more
europepmc +1 more source
Electrobaryonic axion: hair of neutron stars
Axion-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
doaj +1 more source
Decoupling Degradation at the Electrode Interfaces in Prussian White Full Cells
Prussian White (PW) as a sodium‐ion battery (SIB) cathode material is advancing, having already been commercialized. Yet, capacity fade and cyanide‐related safety risks persist. By integrating Mössbauer‐ and online electrochemical mass spectrometry, this study analyzes degradation in PW cells, observing hydrogen and cyanide evolution.
Casimir Misiewicz+4 more
wiley +1 more source
We 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
X-Rays Radiation of a Neutron Star as a Result of Gas Accretion [PDF]
Ja. B. Zel’dovič
openalex +1 more source
A novel and efficient method is explored to synthesize 1D single‐crystal sub‐stoichiometric WnO3n‐2 (n = 25) nanowire bundles. The approach utilizes selective low‐energy He+ ion irradiation (27 eV) on Mo‐Ni doped WOx surface, achieving efficient catalyst‐free self‐organized growth of high aspect ratio nanowires at the temperature of 700 °C.
Maryna Bilokur+3 more
wiley +1 more source
Room Temperature Dy Spin‐Flop Switching in Strained DyFeO3 Thin Films
The two‐spin system DyFeO3, a canted bulk antiferromagnet with a spin reorientation between 40 and 50 K is epitaxially grown as thin film with compressive in‐plane strain. As a result, the spin reorientation increased by more than 20 K and a sign‐dependent linear M(T) dependence between 100 and 400 K is measured due to an induced alignment of Dy spins.
Banani Biswas+5 more
wiley +1 more source
Accretion onto a small black hole at the center of a neutron star. [PDF]
Richards CB, Baumgarte TW, Shapiro SL.
europepmc +1 more source
On the Dynamical Evolution of the Asteroid Belt in a Massive Star–Neutron Star Binary
Some 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 in supergiant High Mass X-ray Binaries
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