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
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
19 January 2023
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).
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.
Text
Andersson_2023_Class._Quantum_Grav._40_025016
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More information
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
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Date deposited: 17 Feb 2023 17:30
Last modified: 17 Mar 2024 04:09
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Author:
Fabian Gittins
Author:
Shanshan Yin
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