Results 81 to 90 of about 20,312 (304)
Hyperonic Interactions in Neutron Stars [PDF]
The matter of neutron stars is characterised by the density of the order of typical nuclear densities; hence, it can be described with methods of nuclear physics.
Artur Nasakin +3 more
core +1 more source
Hybrid Stars that Masquerade as Neutron Stars [PDF]
22 pages, LaTeX.
Alford, Mark +3 more
openaire +2 more sources
Generating Unconventional Spin‐Orbit Torques With Patterned Phase Gradients in Tungsten Thin Films
ABSTRACT A key aim in spintronics is to achieve current‐induced magnetization switching via spin‐orbit torques without external magnetic fields. For this, the focus of recent work has been on introducing controlled lateral gradients across ferromagnet/heavy‐metal devices, giving variations in thickness, composition, or interface quality.
Lauren J. Riddiford +9 more
wiley +1 more source
Anomalous hydrodynamics kicks neutron stars [PDF]
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. [PDF]
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
QCD in Neutron Stars and Strange Stars [PDF]
This paper provides an overview of the possible role of Quantum Chromo Dynamics (QDC) for neutron stars and strange stars. The fundamental degrees of freedom of QCD are quarks, which may exist as unconfined (color superconducting) particles in the cores of neutron stars. There is also the theoretical possibility that a significantly large number of up,
Weber, F., Negreiros, R.
openaire +2 more sources
Emergent Spin Supersolids in Frustrated Quantum Materials
This review highlights developments in the study of spin super‐solids in frustrated quantum materials. Advanced experimental characterizations and computational studies enable a comprehensive understanding of the driving mechanisms of spin super‐solidity in various layered transition‐metal compounds, bridging materials, experiments, and theory aspects.
Yixuan Huang +2 more
wiley +1 more source
Wiederherstellung chiraler Symmetrie und des Deconfinements in Neutronensternen [PDF]
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
core
Evolution of proto-neutron stars with hadron-quark phase transition [PDF]
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
Axisymmetric cooling of neutron stars with strong magnetic fields
Context. Strong magnetic fields can affect both the structure and particle composition of neutron stars. Aims. We seek to understand the thermal evolution of strongly magnetized neutron stars, particularly investigating how strong magnetic fields and ...
Negreiros R., Peterson J., Dexheimer V.
doaj +1 more source

