The Stochastic Gravitational Wave Background from Magnetars

Magnetars have already been a potential candidate as gravitational wave sources that could be detected by current and future terrestrial well ground based detectors. In this article, we focus on the emission from distorted rotating neutron stars. The deformation is assumed to symmetric around an axis perpendicular rotation axis. form applied in context of star whose magnetic field has deformed its own. By introducing effects all magnetars Universe, various proposed configurations, such poloidal, toroidal; stochastic background (SGWB) can generated. We choose figure out exactly how observations gravitational-wave should used understand much more about physics correlated with magnetar behaviour, restriction eccentricity magnetar.