Results 131 to 140 of about 125,236 (339)
Relativistic mean-field theories for neutron-star physics based on chiral effective field theory
, 2022 Mark Alford +3 more
openalex +2 more sources
Advanced Healthcare Materials, EarlyView.Next‐Generation Psoriasis Therapy – With advanced dendrimer‐based formulations, this study paves the way for highly effective, skin‐permeable treatments. Encapsulated in fluid catanionic vesicles, IMD‐006 and its analogues show promising anti‐psoriatic effects offering a targeted, non‐invasive approach to managing chronic skin inflammation.
Ranime Jebbawi +10 more
wiley +1 more source
NEUTRON RICH NUCLEI AND NEUTRON STARS [PDF]
Fission and Properties of Neutron-Rich Nuclei, 2013 The PREX experiment at Jefferson Laboratory measures the neutron radius of 208Pb with parity violating electron scattering in a way that is free from most strong interaction uncertainties. The 208Pb radius has important implications for neutron rich matter and the structure of neutron stars.
openaire +2 more sources
Superfluidity of $\Lambda$ hyperons in neutron stars
, 2010 We study the $^1S_0$ superfluidity of $\Lambda$ hyperons in neutron star matter and neutron stars. We use the relativistic mean field (RMF) theory to calculate the properties of neutron star matter.
B. D. Serot, H. Shen, Y. N. Wang
core +1 more source
Synthetic Aspects and Characterization Needs in MOF Chemistry – from Discovery to Applications
Advanced Materials, EarlyView.Overcoming the challenges of phase discovery, synthesis optimization and scale‐up, characterization, and computational studies is essential to accelerate the large‐scale application of MOFs. Life‐cycle analyses and techno‐economic analyses need to be performed to realistically assess their potential for industrial relevance.
Bastian Achenbach +4 more
wiley +1 more source
Frontiers of Physics, 2013 15 pages, 8 figure, to be published in Frontiers of ...
openaire +2 more sources
Too massive neutron stars: The role of dark matter?
, 2012 The maximum mass of a neutron star is generally determined by the equation of state of the star material. In this study, we take into account dark matter particles, assumed to behave like fermions with a free parameter to account for the interaction ...
Huang, Feng +3 more
core +1 more source
Computational Modeling of Reticular Materials: The Past, the Present, and the Future
Advanced Materials, EarlyView.Reticular materials are advanced materials with applications in emerging technologies. A thorough understanding of material properties at operating conditions is critical to accelerate the deployment at an industrial scale. Herein, the status of computational modeling of reticular materials is reviewed, supplemented with topical examples highlighting ...
Wim Temmerman +3 more
wiley +1 more source
Detecting the Hadron-Quark Phase Transition with Gravitational Waves
Universe, 2019 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
Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
, 2014 The nuclear symmetry energy is intimately connected with nuclear astrophysics. This contribution focuses on the estimation of the symmetry energy from experiment and how it is related to the structure of neutron stars.
Lattimer, James M., Steiner, Andrew W.
core +1 more source