Results 181 to 190 of about 115,270 (322)
Dynamical Stability of Hypermassive Neutron Stars against Quasi-radial Perturbations
The dynamical stability of differentially rotating neutron stars, including hypermassive neutron stars, is of paramount importance in understanding the fate of the postmerger remnant of binary neutron stars mergers and the formation of a black hole ...
Paweł Szewczyk +2 more
doaj +1 more source
Development of High‐Performance Multilayer Monochromators
Detailed insights into the optical and multilayer design of Double Multilayer Monochromators (DMM) are presented and fully characterized, including key optimization strategies and solutions to fabrication challenges. By integrating in‐house Ion Beam Figuring and a high uniformity multilayer coating process, the developed DMMs achieve high reflectivity,
Wadwan Singhapong +11 more
wiley +1 more source
Electron acceleration using multipetawatt femtosecond lasers and subcritical density plasmas achieves a maximum charge of 245 nC, with an injection rate of up to 100 nC per picosecond. The charge variation with plasma density, initially increasing and then decreasing, arises from the competition between the injection of multiple plasma waves and laser ...
Xi‐Chen Hu +9 more
wiley +1 more source
Neutron Stars in Close Binary Systems
J. C. Wheeler, C. F. McKee, M. Lecar
openalex +1 more source
Recent Advances in Ene Reactions with Carbon Enophiles
Recent advances in the classical intra‐ and intermolecular ene nexus with carbon enophiles (alkenes, alkynes, arynes, and allenes) show a considerable increase in structural complexity and an enormous potential for functional applications in polymer science.
Thomas J. J. Müller
wiley +1 more source
The Neutron-Proton Ratio in Stars Exploding from Dense, Hightemperature States
David N. Schramm, Z. Barkat
openalex +1 more source
This study clarifies the critical relationship between operating temperature and two‐phase flow behavior in polymer electrolyte membrane (PEM) electrolyzers by investigating pore‐scale gas bubble transport in the anode porous transport layer. Higher temperatures (80 °C vs 40 °C) result in a lower total bubble volume fraction and smaller bubble ...
Chaeyoung T. Ham +5 more
wiley +1 more source
A Search for Low-mass Neutron Stars in the Third Observing Run of Advanced LIGO and Virgo
Most observed neutron stars have masses around 1.4 M _⊙ , consistent with current formation mechanisms. To date, no subsolar-mass neutron star has been observed.
Keisi Kacanja, Alexander H. Nitz
doaj +1 more source
The Effect of Intrinsic Spin on Neutron Stars in the Einstein-Cartan Theory of Gravity
David G. Kerlick
openalex +2 more sources

