Email this article On the Pressure of a Neutron Gas Interacting with the Non-Uniform Magnetic Field of a Neutron Star
- Authors: Skobelev V.V.1
-
Affiliations:
- Moscow Polytechnic University
- Issue: Vol 60, No 12 (2018)
- Pages: 2073-2076
- Section: Article
- URL: https://bakhtiniada.ru/1064-8887/article/view/239810
- DOI: https://doi.org/10.1007/s11182-018-1328-3
- ID: 239810
Cite item
Open Access
Access granted
Subscription Access
Abstract
On the basis of simple arguments, practically not going beyond the scope of an undergraduate course in general physics, we estimate the additional pressure (at zero temperature) of degenerate neutron matter due to its interaction with the non-uniform magnetic field of a neutron star. This work has methodological and possibly scientific value as an intuitive application of the content of such a course to a solution of topical problems of astrophysics.
About the authors
V. V. Skobelev
Moscow Polytechnic University
Author for correspondence.
Email: v.skobelev@inbox.ru
Russian Federation, Moscow
Supplementary files
