| Issue |
EPJ Web Conf.
Volume 173, 2018
Mathematical Modeling and Computational Physics 2017 (MMCP 2017)
|
|
|---|---|---|
| Article Number | 02015 | |
| Number of page(s) | 4 | |
| Section | Mathematical Modeling and Methods | |
| DOI | https://doi.org/10.1051/epjconf/201817302015 | |
| Published online | 14 February 2018 | |
https://doi.org/10.1051/epjconf/201817302015
Minimum Period of Rotation of Millisecond Pulsars and Pulsar Matter Equations of State
Tver State University
* e-mail: Mikheev.SA@tversu.ru
** e-mail: Tsvetkov.VP@tversu.ru
Published online: 14 February 2018
Based on the findings of our previous studies of fast-rotating Newtonian polytropes, we found the relation between the minimum pulsar rotation period, the value of pulsar central density, and the polytropic index. From this relation we come to the conclusion that the value of minimum central density of a pulsar with a peak period is 2.5088 • 1014 g/cm3.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
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