Spin Evolution of Neutron Stars-Reference-Cited by-同舟云学术

Spin Evolution of Neutron Stars

Published:2024-02-10 Issue:1 Volume:12 Page:7
ISSN:2075-4434
Container-title:Galaxies
language:en
Short-container-title:Galaxies

Author:

Abolmasov Pavel¹,Biryukov Anton²³^ORCID,Popov Sergei B.²⁴^ORCID

Affiliation:

1. The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel

2. Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Pr. 13, 119234 Moscow, Russia

3. Faculty of Physics, HSE University, 21/4 Staraya Basmannaya Str., 105066 Moscow, Russia

4. ICTP, Strada Costiera 11, 34151 Trieste, Italy

Abstract

In this paper we review the basics of magneto-rotational properties of neutron stars focusing on spin-up/spin-down behavior at different evolutionary stages. The main goal is to provide equations for the spin frequency changes in various regimes (radio pulsar, propeller, accretor, etc.). Since presently the spin behavior of neutron stars at all stages remains a subject of many uncertainties, we review different suggestions made over the years in the literature.

Funder

Simons Foundation

Publisher

MDPI AG

Link

https://www.mdpi.com/2075-4434/12/1/7/pdf

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