Stochastic background from inspiralling double neutron stars

Details Stochastic background from inspiralling double neutron stars Stochastic background from inspiralling double neutron stars

2006-12-30

arxiv.org/abs/astro-ph/0701004v1

Phys.Rev.D75:043002,2007

Astronomy and Astrophysics

Astrophysics

accepted for publication in physical review D 8 pages, 3 figures

Scientific paper

10.1103/PhysRevD.75.043002

We review the contribution of extra galactic inspiralling double neutron stars, to the LISA astrophysical gravitational wave foreground. Using recent fits of the star formation rate, we show that sources beyond $z_*=0.005$ contribute to a truly continuous background, which may dominate the LISA instrumental noise in the range $3 \simeq 10^{-4}$ - $1 \times 10^{-2}$ Hz and overwhelm the galactic WD-WD confusion noise at frequencies larger than $\nu_o \simeq 2\times 10^{-3}$.

Affiliated with

Also associated with

No associations

Rating

Stochastic background from inspiralling double 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 Stochastic background from inspiralling double neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stochastic background from inspiralling double neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-485564