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A&A 447, 785-796 (2006)
DOI: 10.1051/0004-6361:20052843
Astrophysical unipolar inductors powered by GW emission
S. Dall'Osso, G. L. Israel and L. StellaINAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio Catone (Roma), Italy
e-mail: [dallosso;gianluca;stella]@mporzio.astro.it
(Received 8 February 2005 / Accepted 8 July 2005 )
Abstract
We consider the Unipolar Inductor Model (Goldreich & Lynden-Bell
1969, ApJ, 156, 59) applied to Double Degenerate Binaries (DDBs) with ultrashort periods
(Wu et al. 2002, MNRAS, 331, 221).
In this model a magnetized primary white dwarf has a slight asynchronism
between its spin and orbital motion, so that the (non-magnetic) secondary
experiences a motional electric field when moving through the primary field
lines. This induces a current flow between the two stars and provides
an electric spin-orbit coupling mechanism for the primary.
We study the combined effect of Gravitational Wave emission and
electric spin-orbit coupling on the evolution of the primary degree of
asynchronism and the associated rate of electric current dissipation in such systems, assuming that the primary's spin is not affected
by other mechanisms such as tidal interactions with the companion. In
particular, we show that in ultrashort period binaries the emission of GW pumps
energy in the electric circuit as to keep it steadily active.
This happens despite the fact that spin-orbit coupling can rapidly synchronize
the primary, because GW represent a slow desynchronizing mechanism that
steadily substracts orbital angular momentum to the system. A slightly
asynchronous steady-state is thus achieved, determined by the balance between
these two competing effects. This can be shown to correspond to a condition
where the total available electric energy is conserved, because of GW emission,
while dissipation, synchronization and orbital shrinking continue.
Key words: gravitational waves -- magnetic fields -- stars: binaries: close -- stars: dwarfs novae -- X-rays: individuals: RX J0806.3+1527 -- X-rays: individuals: RX J1914.4+2456
SIMBAD Objects
© ESO 2006
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