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Building post-Newtonian neutron stars

Building post-Newtonian neutron stars
Building post-Newtonian neutron stars

Owed to their compactness, neutron stars involve strong gravity and extreme density physics. Nevertheless, at present, there are a variety of problems where progress (at least conceptually) can be made in the context of weak gravity. Motivated by this we examine how accurately one can model neutron stars using the post-Newtonian (pN) approximation to general relativity. In general, we find there is a significant degree of freedom in how the pN equations of stellar structure can be formulated. We discuss this flexibility in the formulation and provide examples to demonstrate the impact on stellar models. We also consider the (closely related) problem of building neutron stars using isotropic coordinates. In this context, we provide a new strategy for solving the equations (based on a scaling argument) which significantly simplifies the problem.

neutron stars, post-Newtonian theory, stellar structure
0264-9381
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Gittins, Fabian
657ec875-fac3-4606-9dcd-591ef22fc9f6
Yin, Shanshan
1a1d6d2f-3b19-4ac9-9151-e496b32be131
Panosso Macedo, Rodrigo
8f176eb4-ca20-492b-a41e-e78d47d6fefe
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Gittins, Fabian
657ec875-fac3-4606-9dcd-591ef22fc9f6
Yin, Shanshan
1a1d6d2f-3b19-4ac9-9151-e496b32be131
Panosso Macedo, Rodrigo
8f176eb4-ca20-492b-a41e-e78d47d6fefe

Andersson, Nils, Gittins, Fabian, Yin, Shanshan and Panosso Macedo, Rodrigo (2023) Building post-Newtonian neutron stars. Classical and Quantum Gravity, 40 (2), [025016]. (doi:10.1088/1361-6382/acace5).

Record type: Article

Abstract

Owed to their compactness, neutron stars involve strong gravity and extreme density physics. Nevertheless, at present, there are a variety of problems where progress (at least conceptually) can be made in the context of weak gravity. Motivated by this we examine how accurately one can model neutron stars using the post-Newtonian (pN) approximation to general relativity. In general, we find there is a significant degree of freedom in how the pN equations of stellar structure can be formulated. We discuss this flexibility in the formulation and provide examples to demonstrate the impact on stellar models. We also consider the (closely related) problem of building neutron stars using isotropic coordinates. In this context, we provide a new strategy for solving the equations (based on a scaling argument) which significantly simplifies the problem.

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Accepted/In Press date: 19 December 2022
e-pub ahead of print date: 3 January 2023
Published date: 19 January 2023
Additional Information: Funding Information: N A and F G are grateful for support from STFC via Grant Numbers ST/R00045X/1 and ST/V000551/1. Parts of NA’s contribution to this work were carried out at the Aspen Center for Physics, which is supported by National Science Foundation Grant PHY-1607611. He also thanks the Simons Foundation for generous travel support. Publisher Copyright: © 2023 The Author(s). Published by IOP Publishing Ltd.
Keywords: neutron stars, post-Newtonian theory, stellar structure

Identifiers

Local EPrints ID: 474276
URI: http://eprints.soton.ac.uk/id/eprint/474276
ISSN: 0264-9381
PURE UUID: 11cc63f9-0cea-4a8f-afbb-f8eef2fe088d
ORCID for Nils Andersson: ORCID iD orcid.org/0000-0001-8550-3843
ORCID for Fabian Gittins: ORCID iD orcid.org/0000-0002-9439-7701
ORCID for Rodrigo Panosso Macedo: ORCID iD orcid.org/0000-0003-2942-5080

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Date deposited: 17 Feb 2023 17:30
Last modified: 17 Mar 2024 04:09

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Contributors

Author: Nils Andersson ORCID iD
Author: Fabian Gittins ORCID iD
Author: Shanshan Yin

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