Inference on neutron star parameters and the nuclear equation of state with RIFT, using prior EOS information

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Vilkha, Askold, Yelikar, Anjali, O'Shaughnessy, Richard, Read, Jocelyn
Format: Preprint
Published: 2024
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866913440399884288
author Vilkha, Askold
Yelikar, Anjali
O'Shaughnessy, Richard
Read, Jocelyn
author_facet Vilkha, Askold
Yelikar, Anjali
O'Shaughnessy, Richard
Read, Jocelyn
contents In this paper, we present an inference method for determining neutron star parameters and constraining the nuclear equation of state (EOS) using the RIFT parameter inference engine. We incorporate externally-produced prior information about the EOS to improve the accuracy and efficiency of the inference process. We apply this method to the GW170817 event and assess its performance. Our results demonstrate the effectiveness of incorporating prior EOS information in the inference process, leading to sharper conclusions and more rapid inference on new detections. This approach has the potential to enhance our understanding of neutron stars and the nuclear EOS in future gravitational wave observations.
format Preprint
id arxiv_https___arxiv_org_abs_2407_15753
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Inference on neutron star parameters and the nuclear equation of state with RIFT, using prior EOS information
Vilkha, Askold
Yelikar, Anjali
O'Shaughnessy, Richard
Read, Jocelyn
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
In this paper, we present an inference method for determining neutron star parameters and constraining the nuclear equation of state (EOS) using the RIFT parameter inference engine. We incorporate externally-produced prior information about the EOS to improve the accuracy and efficiency of the inference process. We apply this method to the GW170817 event and assess its performance. Our results demonstrate the effectiveness of incorporating prior EOS information in the inference process, leading to sharper conclusions and more rapid inference on new detections. This approach has the potential to enhance our understanding of neutron stars and the nuclear EOS in future gravitational wave observations.
title Inference on neutron star parameters and the nuclear equation of state with RIFT, using prior EOS information
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2407.15753