Results 131 to 140 of about 115,270 (322)
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E +6 more
europepmc +1 more source
15 pages, 8 figure, to be published in Frontiers of ...
openaire +3 more sources
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
Adsorption and Separation by Flexible MOFs
Flexible metal–organic frameworks (MOFs) present significant potential for gas storage and separation due to their structural dynamic. This review explores the rationale behind the flexible MOFs' enhanced working capacity and separation factors. It also addresses key challenges, including phase transition kinetics, crystal robustness, cycling, shaping,
Irena Senkovska +4 more
wiley +1 more source
Delta isobars in neutron stars
The appearance of delta isobars in beta-stable matter is regulated by the behavior of the symmetry energy at densities larger than saturation density. We show that by taking into account recent constraints on the density derivative of the symmetry energy
Pagliara Giuseppe +3 more
doaj +2 more sources
Neutron stars harboring a primordial black hole: Maximum survival time. [PDF]
Baumgarte TW, Shapiro SL.
europepmc +1 more source
The internal composition of proto-neutron stars under strong magnetic fields
In this work, we study the effects of magnetic fields and rotation on the structure and composition of proto-neutron stars (PNS's). A hadronic chiral SU(3) model is applied to cold neutron stars (NS) and proto-neutron stars with trapped neutrinos and at ...
Dexheimer, V., Franzon, B., Schramm, S.
core +1 more source
This review explores how in situ and operando spectroscopic techniques reveal the real‐time behavior of reticular materials, including MOFs and COFs. These methods track material formation and functionalization, structural changes, defect formation, dynamic responses to external triggers, and catalytic processes.
Bettina Baumgartner +4 more
wiley +1 more source
The observed chemical diversity of Milky Way stars places important constraints on Galactic chemical evolution and the mixing processes that operate within the interstellar medium. Recent works have found that the chemical diversity of disk stars is low.
Catherine Manea +5 more
doaj +1 more source
Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers. [PDF]
Bandyopadhyay D.
europepmc +1 more source

