Abstract AM Canum Venaticorum (AM CVn) systems are ultracompact binaries where a
white dwarf accretes from a helium-rich degenerate or semidegenerate donor. Some AM …

We extend a magnetic braking (MB) model, which has been used earlier to address the
evolution of cataclysmic variables, to address the spin period P spin evolution of fully …

We model cataclysmic variables (CVs) with solar metallicity donors (X= 0.7 and Z= 0.02) that
evolve to form AM CVn stars through the evolved CV formation channel using various …

Context. AM CVn binaries are potential progenitors of thermonuclear supernovae and strong
sources of persistent gravitational wave radiation. For a long time, it has been believed that …

We extend our model of magnetic braking (MB), driven by an α–Ω dynamo mechanism, from
fully convective M-dwarfs (FCMDs) to explain the surface and internal spin evolution of partly …

Abstract Gravitational Waves (GWs) provide a unique way to explore our Universe. The
ongoing ground-based detectors, eg, LIGO, Virgo, and KAGRA, and the upcoming next …

We present the results of the study of cataclysmic variables (CVs) and AM Canum
Venaticorum (AM CVn) stars with our double dynamo (DD) formalism of angular momentum …

AM CVn systems are ultra-compact binaries where a white dwarf accretes from a helium-rich
degenerate or semi-degenerate donor. Some AM CVn systems will be among the loudest …