Bulk viscosity and r-modes of neutron stars

Details Bulk viscosity and r-modes of neutron stars Bulk viscosity and r-modes of neutron stars

2008-08-08

arxiv.org/abs/0808.1145v1

Astronomy and Astrophysics

Astrophysics

4 page, 2 figures; presented in the Quark Matter 2008 held in Jaipur, India from 4-10 February, 2008; to be published in J. Ph

Scientific paper

10.1088/0954-3899/35/10/104078

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.

Affiliated with

Also associated with

No associations

Rating

Bulk viscosity and r-modes of neutron stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Bulk viscosity and r-modes of neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bulk viscosity and r-modes of neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-29228