| Автор | Edwin E Salpeter |
| Дата выпуска | 1998-12-14 |
| dc.description | In magnetic fields of very much more than G, polyatomic hydrogen molecules, in the form of long chains, are stable. In neutron star surfaces, fields of G are commonplace and G has been reported. Liquid hydrogen can form at the higher field with a zero-pressure density of about . At these densities, hydrogen can burn to helium by pycnonuclear reactions even at low temperatures - the `real cold fusion'. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Hydrogen in strong magnetic fields in neutron star surfaces |
| Тип | paper |
| DOI | 10.1088/0953-8984/10/49/017 |
| Electronic ISSN | 1361-648X |
| Print ISSN | 0953-8984 |
| Журнал | Journal of Physics: Condensed Matter |
| Том | 10 |
| Первая страница | 11285 |
| Последняя страница | 11288 |
| Аффилиация | Edwin E Salpeter; Space Sciences Building, Cornell University, Ithaca, NY 14853, USA |
| Выпуск | 49 |
