What is the magnetic field distribution for the equation of state of magnetized neutron stars?

In this Letter, we report a realistic calculation of the magnetic field profile for the equation of state inside strongly magnetized neutron stars. Unlike previous estimates, which are widely used in the literature, we find that magnetic fields increase relatively slowly with increasing baryon chemi...

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Bibliographic Details
Main Authors: V. Dexheimer, B. Franzon, R.O. Gomes, R.L.S. Farias, S.S. Avancini, S. Schramm
Format: Article
Language:English
Published: Elsevier 2017-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269317307062