Bulk viscosity and r-modes of neutron stars
Abstract
The bulk viscosity due to the non-leptonic process involving hyperons in K- condensed matter is discussed here. We find that the bulk viscosity is modified in a superconducting phase. Further, we demonstrate how the exotic bulk viscosity coefficient influences r-modes of neutron stars which might be sources of detectable gravitational waves.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.