EXOTIC NUCLEAR ROD FORMATION INDUCED BY SUPERFLUID VORTICES IN NEUTRON-STAR CRUSTS

Citation
Ys. Mochizuki et al., EXOTIC NUCLEAR ROD FORMATION INDUCED BY SUPERFLUID VORTICES IN NEUTRON-STAR CRUSTS, The Astrophysical journal, 489(2), 1997, pp. 848-864
Citations number
27
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
489
Issue
2
Year of publication
1997
Part
1
Pages
848 - 864
Database
ISI
SICI code
0004-637X(1997)489:2<848:ENRFIB>2.0.ZU;2-U
Abstract
The inner crust of a neutron star consists of a lattice of nuclei, rel ativistic degenerate electrons, and a neutron superfluid. Since the st ar is rotating, there are a number of quantized vortices in the superf luid. Mochizuki & Izuyama pointed out that such vortex lines may induc e nuclear matter rods along the vortex cores. The exotic nuclear struc ture is possible in a very limited region of the inner crust. However, the short nuclear rod can completely pin the vortex line and can be a n origin of vortex accumulation. The accumulation goes on until the lo cal Magnus force among the accumulated vortices reaches a critical mag nitude for unpinning of the trapped vortices. The unpinning at this st age, which must be collective, leads to pulsar glitches. In this paper , we first reconsider the energetics of this vortex-induced nuclear ma tter rod given by Mochizuki & Izuyama. We present a picture in which t he nuclear rod is constructed by successive captures of certain neighb oring nuclei into the vortex core, and subsequent fusion reactions of the captured nuclei with those inside the vortex core. We found that t he marginal region, where the induced nuclear rods are stable, is not trivial. As the next step, the possibility of nuclear rod formation sh ould be warranted by dynamical analysis. The crucial part of the dynam ics is the Coulomb potential barrier, which seems at first sight to pr ohibit fusion if one neglects the screening due to electrons. Then we also report our theoretical estimate of this Coulomb barrier, i.e., th e energy increase when a nucleus deviates form its equilibrium site to the onset position of nuclear fusion. The screening of nuclear charge by the background electrons is accurately taken into consideration. W e found that the Coulomb barrier against the rod formation is of the o rder of 1 MeV throughout the marginal region. The obtained barrier is only several times as large as the zero-point energy of the nuclei-for ming crystalline lattice. This result suggests that pycnonuclear react ions for the rod formation are feasible.