Results 71 to 80 of about 547,290 (394)
Influence of the symmetry energy on nuclear pasta in neutron star crusts [PDF]
We investigate the effects of the symmetry energy on nuclear pasta phases and the crust-core transition in neutron stars. We employ the relativistic mean-field approach and the coexisting phases method to study the properties of pasta phases presented in the inner crust of neutron stars.
arxiv +1 more source
Silicic magma reservoirs in the Earth’s crust
Magma reservoirs play a key role in controlling numerous processes in planetary evolution, including igneous differentiation and degassing, crustal construction, and volcanism.
O. Bachmann, C. Huber
semanticscholar +1 more source
Earthquake-induced transformation of the lower crust
The structural and metamorphic evolution of the lower crust has direct effects on the lithospheric response to plate tectonic processes involved in orogeny, including subsidence of sedimentary basins, stability of deep mountain roots and extension of ...
B. Jamtveit+3 more
semanticscholar +1 more source
Challenges and Opportunities for Rechargeable Aqueous Sn Metal Batteries
Rechargeable aqueous batteries with metal anodes promise enhanced energy density, combining higher output voltage and capacity with high safety. This perspective highlights the emerging potential of the Sn metal anode, emphasizing its resistance to hydrogen evolution, high reversibility, and sustainability.
Haozhe Zhang+3 more
wiley +1 more source
Superfluidity in Disordered Neutron Stars Crusts [PDF]
Nonequilibrium conditions imposed by neutrino cooling through the liquid-solid transition lead to disorder in the solid crust of neutron stars. Disorder reduces the superfluid fraction, $\rho_s/\rho$, at densities above that of neutron drip, $\rho_d \approx 4\times 10^{11}\,g/cm^3$.
arxiv
Nuclear heating and melted layers in the inner crust of an accreting neutron star [PDF]
A neutron star in a long-lived, low-mass binary can easily accrete enough matter to replace its entire crust. Previous authors noted that an accreted crust, being formed from the burning of accreted hydrogen and helium, allows a series of non-equilibrium reactions, at densities >6e11 g/cc, which release a substantial amount of heat (1 MeV per accreted ...
arxiv +1 more source
Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission [PDF]
Motivated by the narrow range of spin frequencies of nearly 20 accreting neutron stars, Bildsten (1998) conjectured that their spin-up had been halted by the emission of gravitational waves. He also pointed out that small nonaxisymmetric temperature variations in the accreted crust will lead to "wavy" electron capture layers, whose horizontal density ...
arxiv +1 more source
A cross-sectional analysis of mental toughness in a professional football academy [PDF]
This study investigated mental toughness in an English Premier League football academy. 112 football players aged between 12 and 18 years of age completed the Mental Toughness Questionnaire 18 (Clough, Earle, & Sewell, 2002) as a measure of mental ...
Crust, Lee+2 more
core
Persistent crust-core spin lag in neutron stars [PDF]
It is commonly believed that the magnetic field threading a neutron star provides the ultimate mechanism (on top of fluid viscosity) for enforcing long-term corotation between the slowly spun down solid crust and the liquid core.
Glampedakis, Kostas, Lasky, Paul
core +2 more sources
This study investigates the antifungal efficacy of ultrashort pulsed laser‐induced periodic surface structures (USP‐DLIP) on copper, brass, and steel surfaces. Using Aspergillus niger as a model, the research highlights a 99% reduction in spore viability on 9 µm structured copper surfaces due to enhanced copper ion release. Scanning electron microscopy
Stella Marie Timofeev+10 more
wiley +1 more source