  Over the past couple of decades, researchers have predicted more than a dozen
super-Chandrasekhar white dwarfs from the detections of over-luminous type Ia
supernovae. It turns out that magnetic fields and rotation can explain such
massive white dwarfs. If these rotating magnetized white dwarfs follow specific
conditions, they can efficiently emit continuous gravitational waves and
various futuristic detectors, viz. LISA, BBO, DECIGO, and ALIA can detect such
gravitational waves with a significant signal-to-noise ratio. Moreover, we
discuss various timescales over which these white dwarfs can emit dipole and
quadrupole radiations and show that in the future, the gravitational wave
detectors can directly detect the super-Chandrasekhar white dwarfs depending on
the magnetic field geometry and its strength.
