27 research outputs found
Reaction rates and transport in neutron stars
Full text linkUnderstanding signals from neutron stars requires knowledge about the
transport inside the star. We review the transport properties and the
underlying reaction rates of dense hadronic and quark matter in the crust and
the core of neutron stars and point out open problems and future directions.Comment: 74 pages; commissioned for the book "Physics and Astrophysics of
Neutron Stars", NewCompStar COST Action MP1304; version 3: minor changes,
references updated, overview graphic added in the introduction, improvements
in Sec IV.A.
Phase-Separation Phenomena during Thermal Aging of Multicomponent Thermometer Glasses and their Influence on Physical Properties
No full textEffect of Degree of Oxidation and Element Form in Vanadium Slag on Its Treatment Production Capacity
No full textThe quantitative relationship between metal radii, cationic radii and electronic configurations of elements
No full textParameter consistency and quadratically constrained errors-in-variables least-squares identification
No full textThe Structure and EPR Behavior of Nitroxide Biradical Containing Phosphorus Atom in the Bridge
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Updating QR factorization procedure for solution of linear least squares problem with equality constraints
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Cosmology with the Laser Interferometer Space Antenna
Get PDFThe Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational wave observations by LISA to probe the universe
