Results 111 to 120 of about 107,571 (269)
Generative Models for Crystalline Materials
Generative machine learning models are increasingly used in crystalline materials design. This review outlines major generative approaches and assesses their strengths and limitations. It also examines how generative models can be adapted to practical applications, discusses key experimental considerations for evaluating generated structures, and ...
Houssam Metni +15 more
wiley +1 more source
How neutron stars constrain the nuclear equation of state
Recent neutron star observations set new constraints for the equation of state of baryonic matter. A chiral effective field theory approach is used for the description of neutron-dominated nuclear matter present in the outer core of neutron stars ...
Hell Thomas +2 more
doaj +1 more source
The d⁎(2380) in Neutron Stars — A New Degree of Freedom?
Elucidating the appropriate microscopic degrees of freedom within neutron stars remains an open question which impacts nuclear physics, particle physics and astrophysics.
I. Vidaña +3 more
doaj +1 more source
Statistical theory of thermal evolution of neutron stars - II. Limitations on direct Urca threshold
We apply our recently suggested statistical approach to thermal evolution of isolated neutron stars and accreting quasistationary neutron stars in X-ray transients for constraining the position and relative broadening alpha of the direct Urca threshold ...
Beznogov, M. V., Yakovlev, D. G.
core +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E +6 more
europepmc +1 more source
Using femtosecond ablation, we show that an ordered, stoichiometric crystalline PdSe2 target can be controllably converted into a stable, disordered, non‐stoichiometric, and highly functional amorphous nanomaterial, PdSe2−x${\rm PdSe}_{2-x}$. The obtained nanoparticles offer significant advantages over conventional planar plasmon‐free substrates due to
Andrei Ushkov +18 more
wiley +1 more source
Narrow Atomic Features from Rapidly Spinning Neutron Stars
Neutron stars spinning at moderate rates (~300-600Hz) become oblate in shape and acquire a nonzero quadrupole moment. In this paper, we calculate profiles of atomic features from such neutron stars using a ray-tracing algorithm in the Hartle-Thorne ...
Bauböck +15 more
core +1 more source
Neutron stars harboring a primordial black hole: Maximum survival time. [PDF]
Baumgarte TW, Shapiro SL.
europepmc +1 more source
Optical Manipulation of Multiferroic Phases in BiFeO3 Thin Films
At the strain‐driven morphotropic phase boundary, optical control over the multiferroic rhombohedral and tetragonal phase mixture is demonstrated using above‐bandgap light illumination. The photoinduced charge carriers modify the electrostatic environment and induce the conversion into a single tetragonal phase.
Bixin Yan +7 more
wiley +1 more source
Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers. [PDF]
Bandyopadhyay D.
europepmc +1 more source

