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MAGNETIC FIELD EVOLUTION OF NEUTRON STARS: LINKING MAGNETARS AND ANTI-MAGNETARSстатья
- Авторы: Popov Sergei B., Kaurov Alexander A., Kaminker Alexander D.
- Сборник: Particle Physics at the Year of Light: Proceedings of the Seventeenth Lomonosov Conference on Elementary Particle Physics
- Год издания: 2017
- Место издания: World Scientific
- Первая страница: 345
- Последняя страница: 349
- DOI: 10.1142/9789813224568_0055
- Аннотация: We propose that observations of ``hidden'' magnetars in central compact objects can be used to probe crustal activity of neutron stars with large internal magnetic fields. Our calculations suggest that central compact objects, which are proposed to be ``hidden'' magnetars, must demonstrate flux variations on the time scale of months-years. We consider the source 1E161348-5055 in RCW103 as a ``hidden'' magnetar candidate. Employing a simple 2D-modeling we argue that properties of the source can be explained by the crustal activity of the magnetar type. Thus, this object may be supplemented for the known candidates for the ``hidden'' magnetars among central compact objects discussed in literature.
- Добавил в систему: Попов Сергей Борисович