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The Physics of Magnetars and Their Astrophysical Significance

彭秋和 教授,南京大学天文与空间科学学院
Mon, 2014-06-23 14:30 - 16:30
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We find that the electron Fermi energy,  , increases with the magnetic field strength and it is proportional to  . We note that this result is exactly the opposite of the popular idea that the electron Fermi energy decreases with the magnetic field. The key reason for the dilemma is that an incorrect formulae of the microscopic number of states for the electrons in intense magnetic field from some internationally well known popular textbooks on statistical physics has been repeatedly quoted by many authors.
3. We propose a new mechanism for the production of the high soft X-ray luminosities of magnetars. In particular, the Fermi energy of the electrons is higher than 60MeV in ultra-strong magnetic fields, B>> Bcr (=4.4141013 gauss), which is much higher than the Fermi energy of the neutrons.

彭秋和,南京大学天文系教授, 博士生导师。彭秋和教授是我国著名的核天体物理学家,主要致力于核天体物理学(包括高能天体物理)和星系天文学的研究, 是我国核天体物理学的主要学术带头人。

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