Results 171 to 180 of about 910,791 (369)
Black Hole-Neutron Star Mergers: Disk Mass Predictions
Determining the final result of black hole-neutron star mergers, and in particular the amount of matter remaining outside the black hole at late times and its properties, has been one of the main motivations behind the numerical simulation of these ...
Francois Foucart+3 more
core +1 more source
10 Years Development of Potassium‐Ion Batteries
Significant progress is made in PIBs over the past decade, but the improvements based on half‐cell testing, low mass loading, and low energy density are insufficient for practical applications. This review summarizes the challenges and strategies for PIBs, highlights the importance of further research focusing on full cells, and provides an analysis of
Mingnan Li+7 more
wiley +1 more source
Detecting the Hadron-Quark Phase Transition with Gravitational Waves
The long-awaited detection of a gravitational wave from the merger of a binary neutron star in August 2017 (GW170817) marks the beginning of the new field of multi-messenger gravitational wave astronomy.
Matthias Hanauske+9 more
doaj +1 more source
An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]
Pang PTH+20 more
europepmc +1 more source
We use a post-Newtonian diagnostic tool to examine numerically generated quasiequilibrium initial data sets for non-spinning double neutron star and neutron star-black hole binary systems.
Clifford M. Will+6 more
core +1 more source
A strangely light neutron star within a supernova remnant
Victor Doroshenko+3 more
semanticscholar +1 more source
The crust of neutron stars [PDF]
The structure of the crust of a neutron star is completely determined by the experimentally measured nuclear masses up to a density of the order of 10^11 g.cm^{-3}. At higher densities, the composition of the crust still remains uncertain, mainly due to the presence of ``free'' superfluid neutrons which affect the properties of the nuclear ``clusters''.
openaire +3 more sources
By targeting nominally non‐stoichiometric LiNi1–xTi3x/4O2 compositions, a multi‐domain nanocomposite rock salt positive electrode material with exceptional cycling stability and excellent rate performance is obtained. This enhanced performance particularly under high oxidative potential protocols and cell electrode mass loadings applicable to ...
Jungwoo Lim+13 more
wiley +1 more source
Black Hole-Neutron Star Binaries in General Relativity: Quasiequilibrium Formulation
We present a new numerical method for the construction of quasiequilibrium models of black hole-neutron star binaries. We solve the constraint equations of general relativity, decomposed in the conformal thin-sandwich formalism, together with the Euler ...
G. B. Cook+10 more
core +1 more source
In this contribution I briefly review the dynamics of strange mesons and baryons with dense nuclear matter, paying a special attention to their pres ence in the inner core of neutron stars and the consequences for the structure of these compact stars.
openaire +4 more sources