Results 81 to 90 of about 18,132 (264)
Mixing‐Driven Defects and Composition Evolution in Multi‐Material Metal Additive Manufacturing
Advanced Science, EarlyView.Operando synchrotron X‐ray imaging coupled with high‐fidelity multiphysics modeling uncovers how inter‐material mixing reshapes keyhole dynamics and drives distinct pore‐formation pathways in multi‐material laser powder bed fusion (LPBF). Composition‐dependent instabilities trigger defects, whereas rescanning suppresses porosity and homogenizes Cu ...
Zhilang Zhang +5 more
wiley +1 more source
, 2012 6 pages, invited review, to appear in the proceedings of the ERPM conference, Zielona Gora, April ...
openaire +3 more sources
Anomalous hydrodynamics kicks neutron stars
, 2016 Observations show that, at the beginning of their existence, neutron stars are accelerated briskly to velocities of up to a thousand kilometers per second.
Uhlemann, Christoph F. +3 more
core
Demography of binary neutron stars: the impact of natal kicks and electron-capture supernovae.
, 2022 This thesis presents a theoretical study on the statistical properties of binary neutron stars, by means of synthetic stellar populations simulated with the SEVN code.
Gaspari, Nicola
core
Outstanding TC Enhancement in 5d–3d Y2NiIrO6 by Compression
Advanced Science, EarlyView.Double perovskite Y2NiIrO6 with half filed 3d eg–5d t2g configuration, exhibits first experimental example of pressure‐enhanced magnetic interaction in iridate and iridate‐related systems. Its Curie temperature increase from 192 to 243 K at 17 GPa. Herein, the orthogonal eg–t2g pathway remains robust even under compression‐induced lattice distortion ...
Zheng Deng +18 more
wiley +1 more source
Wiederherstellung chiraler Symmetrie und des Deconfinements in Neutronensternen
, 2009 Neutron stars are very dense objects. One teaspoon of their material would have a mass of five billion tons. Their gravitational force is so strong that if an object were to fall from just one meter high it would hit the surface of the respective neutron
Dexheimer, Verônica Antocheviz
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Evolution of proto-neutron stars with hadron-quark phase transition
, 2012 We investigate the consequences of the quark deconfinement phase transition on the evolution of proto-neutron stars. Assuming a first order phase transition, we calculate the nucleation time due to thermal and quantum nucleation mechanisms.
BOMBACI, IGNAZIO +3 more
core +1 more source
Wide Temperature Zero Thermal Expansion in Al Matrix Composites with High Thermal Conductivity
Advanced Science, EarlyView.Strain engineering strategy is implemented on the negative thermal expansion (NTE) phase Zn1.6Mg0.4P2O7 within composites, where Al matrix‐induced compressive strain drives uniform polyhedral and unit cell evolution, thereby enabling broad and consistent thermal compensation efficacy and obtaining good thermal performance.
Jinrui Qian +14 more
wiley +1 more source
FRAGMENTATION OF NEUTRON STAR MATTER [PDF]
, 2017 Background: Neutron stars are astronomical systems with nucleons submitted to extreme conditions. Due to the long range coulomb repulsion between protons, the system has structural inhomogeneities. These structural inhomogeneities arise also in expanding systems, where the fragment distribution is highly dependent on the thermodynamic conditions ...
Alcain, Pablo Nicolás +1 more
openaire +3 more sources
High-Frequency QPOs as a Product of Inner Disk Dynamics around Neutron Stars
, 2011 The kHz QPOs observed in a neutron star low mass X-ray binary are likely to be produced in the innermost regions of accretion disk around the neutron star.
Erkut, M. Hakan
core +1 more source