  A new class of Double Beltrami-Bernoulli equilibria, sustained by electron
degeneracy pressure, are investigated. It is shown that due to electron
degeneracy, a nontrivial Beltrami-Bernoulli equilibrium state is possible even
for a zero temperature plasma. These states are, conceptually, studied to show
the existence of new energy transformation pathways converting, for instance,
the degeneracy energy into fluid kinetic energy. Such states may be of
relevance to compact astrophysical objects like white dwarfs, neutron stars
etc.
