Results 91 to 100 of about 23,681 (306)
Wiederherstellung chiraler Symmetrie und des Deconfinements in Neutronensternen
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
Multiferroic order parameters – polarization, magnetization, and ferroelastic strain – are positioned as dynamic design variables for batteries. Their mechanistic roles, practical tuning through fabrication and external fields, and ferroic‐resolved characterization routes are unified into a closed‐loop framework, revealing how coupled ferroic responses
Jiaqi Su +13 more
wiley +1 more source
Solidification of neutron matter
A t-matrix calculation of the ground-state energy of cold neutron matter has been performed and it is shown that neutron matter solidifies at a density of the order of 1.6 × 1015 g/cm3, thus implying the existence of a solid core inside heavy neutron ...
Chitre, S. M., Canuto, V.
core +1 more source
Constraint on Dark Matter Using Neutron Stars [PDF]
In this study, the nature and properties of dark matter are explored with the help of neutron stars. Dark matter is assumed to have a particle nature, and different dark matter candidates are considered and tested using neutron stars.
Husain, Wasif
core
A universal metal pre‐fixation (MPF) strategy directs the precise crystallization of diverse metal‐organic frameworks (Co‐MOF, ZIF‐8, Fe‐MOF, UIO‐66) on covalent organic framework (PY‐COF) scaffolds. The resulting hierarchical hybrids exhibit tunable porosity, structural defective and dimensional, as well as enhanced performance in CH4/C2H6/C3H8 ...
Ying Zhao +5 more
wiley +1 more source
Neutron Star Matter as a Dilute Solution of Protons in Neutrons
Neutron stars contain neutron-rich matter with around 5% protons at nuclear saturation density. In this Letter, we consider equilibrium between bulk phases of matter based on asymmetric nuclear matter calculations using chiral effective field theory interactions rather than, as has been done in the past, by interpolation between the properties of ...
Keller, J. +3 more
openaire +6 more sources
ABSTRACT Glioblastoma multiforme (GBM) remains largely incurable due to the blood‐brain barrier (BBB) and immunosuppressive microenvironment. While boron neutron capture therapy (BNCT) selectively eradicates tumor cells via 10B(n, α)‐7Li reactions, its clinical potential in GBM is unrealized because of the suboptimal pharmacokinetics of conventional ...
Jiawen Chen +22 more
wiley +1 more source
Cooling curves for neutron stars with hadronic matter and quark matter [PDF]
The thermal evolution of isothermal neutron stars is studied with matter both in the hadronic phase as well as in the mixed phase of hadronic matter and strange quark matter.
Diederix, J.M. +5 more
core
Conjugated poly(imide dioxime)‐based microspheres establish a radiometal coordination‐driven conformational interlocked network with ultra‐high radiostability. This platform enables low‐temperature, multi‐radionuclide labeling for SPECT/PET/MRI imaging and radionuclide therapy. Mechanistic insights from EXAFS and DFT reveal enhanced stability, while in
Xiao Xu +10 more
wiley +1 more source
Strongly interacting dark matter admixed neutron stars
Dark matter may accumulate in neutron stars given its gravitational interaction and abundance. We investigate the influence of strongly-interacting dark matter, described by a QCD-like one-flavor $G_2$ gauge theory, on neutron stars.
Yannick Dengler, Suchita Kulkarni, Axel Maas, Kevin Radl
doaj +1 more source

