Magnetic topology in coupled binaries, spin-orbital resonances, and flares

Abstract

We consider topological configurations of the magnetically coupled spinning stellar binaries (e.g., merging neutron stars or interacting star-planet systems). We discuss conditions when the stellar spins and the orbital motion nearly `compensate' each other, leading to very {\it slow} overall winding of the coupled magnetic fields; slowly winding configurations allow gradual accumulation of magnetic energy, that is eventually released in a flare when the instability threshold is reached. We find that this slow winding can be global and/or local. We describe the topology of the relevant space $\mathbb{F}=T^1{S}^2$ as the unit tangent bundle of the two-sphere and find conditions for slowly winding configurations in terms of magnetic moments, spins and orbital momentum. These conditions become ambiguous near the topological bifurcation points; in certain cases they also depend on the relative phases of the spin and orbital motions. In the case of merging magnetized neutron stars, if one of the stars is a millisecond pulsar, spinning at $\sim$ 10 msec, the global resonance ${\omega }_1+{\omega }_2=2\Omega$ (spin-plus beat is two times the orbital period) occurs approximately a second before the merger; the total energy of the flare can be as large as $10\%$ of the total magnetic energy, producing bursts of luminosity $\sim 10^{44}$ erg s${}^{-1}$. Higher order local resonances may have similar powers, since the amount of involved magnetic flux tubes may be comparable to the total connected flux.

References in corpus (7)

• Magnetic field strengths of hot Jupiters from signals of star-planet interactions
• The search for radio emission from the exoplanetary systems 55 Cancri, $\upsilon$ Andromedae, and $\tau$ Boötis using LOFAR beam-formed observations
• Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
• Electromagnetic power of merging and collapsing compact objects
• A First Search for Prompt Radio Emission from a Gravitational-Wave Event
• Physics of star-planet magnetic interactions
• Further Evidence for Tidal Spin-Up of Hot Jupiter Host Stars

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• Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system $\epsilon$ Lupi
• Electromagnetic draping of merging neutron stars
• Event Rate of Fast Radio Burst from Binary Neutron-star Mergers
• Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring