New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars

Details New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars

2011-07-20

arxiv.org/abs/1107.4025v1

Physics Letters B 702 (2011) pp. 422-428

Physics

Nuclear Physics

Nuclear Theory

12 pages, 2 figures

Scientific paper

10.1016/j.physletb.2011.07.025

The eigen mode of spin oscillations with $\omega\simeq \sqrt{58/35}\Delta$ is predicted to exist besides already known spin waves with $\omega \simeq\Delta /\sqrt{5}$ in the triplet superfluid neutron condensate in the inner core of neutron stars. The new mode is kinematically able to decay into neutrino pairs through neutral weak currents. The problem is considered in BCS approximation for the case of $^{3}P_{2}-^{3}F_{2}$ pairing with a projection of the total angular momentum $m_{j}=0$ which is conventionally considered as preferable one at supernuclear densities.

Affiliated with

Also associated with

No associations

Rating

New eigen-mode of spin oscillations in the triplet superfluid condensate in 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 New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New eigen-mode of spin oscillations in the triplet superfluid condensate in neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-36009