Abstract
Calculations of thermal and electric conductivity, and of shear and bulk viscosity of degenerate strange matter are reviewed and their results compared with those for normal neutron star matter. Neutrino opacities and emissivities of hot strange matter under various astrophysical conditions are discussed, and compared with corresponding quantities for hot neutron star matter.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
