Stochastic background from inspiralling double neutron stars
| dc.creator | Regimbau, Tania | |
| dc.date | 2006-12-30 | |
| dc.date.accessioned | 2026-07-07T11:00:35Z | |
| dc.date.available | 2026-07-07T11:00:35Z | |
| dc.description | 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 $ν_o \simeq 2\times 10^{-3}$. | |
| dc.description | accepted for publication in physical review D 8 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701004 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701004 | |
| dc.identifier | Phys.Rev.D75:043002,2007 | |
| dc.identifier | doi:10.1103/PhysRevD.75.043002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/187709 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Stochastic background from inspiralling double neutron stars | |
| dc.type | text |