Hydrogen in strong magnetic fields in neutron star surfaces

Details Hydrogen in strong magnetic fields in neutron star surfaces Hydrogen in strong magnetic fields in neutron star surfaces

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jpcm...1011285s&link_type=abstract

Journal of Physics: Condensed Matter, Volume 10, Issue 49, pp. 11285-11288 (1998).

Physics

Condensed Matter

2

Scientific paper

In magnetic fields of very much more than 0953-8984/10/49/017/img1 G, polyatomic hydrogen molecules, in the form of long chains, are stable. In neutron star surfaces, fields of 0953-8984/10/49/017/img2 G are commonplace and 0953-8984/10/49/017/img3 G has been reported. Liquid hydrogen can form at the higher field with a zero-pressure density of about 0953-8984/10/49/017/img4. At these densities, hydrogen can burn to helium by pycnonuclear reactions even at low temperatures - the `real cold fusion'.

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