The impact of compact object deformation on thin accretion disk properties
Abstract We investigate the standard relativistic geometrically thin and optically thick accretion disk in the background of a deformed compact object. The main purpose of this work is to determine whether such a deformed object possesses its own observational fingerprint that can distinguish it fro...
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Format: | Article |
Language: | English |
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SpringerOpen
2025-02-01
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-025-13794-x |
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author | Shokoufe Faraji |
author_facet | Shokoufe Faraji |
author_sort | Shokoufe Faraji |
collection | DOAJ |
description | Abstract We investigate the standard relativistic geometrically thin and optically thick accretion disk in the background of a deformed compact object. The main purpose of this work is to determine whether such a deformed object possesses its own observational fingerprint that can distinguish it from Schwarzschild and Kerr black holes. Our analysis reveals the properties of this relativistic accretion disk model and its dependence on the initial parameters. |
format | Article |
id | doaj-art-96d7ed355da5492d99aa2e29f3abea7f |
institution | Kabale University |
issn | 1434-6052 |
language | English |
publishDate | 2025-02-01 |
publisher | SpringerOpen |
record_format | Article |
series | European Physical Journal C: Particles and Fields |
spelling | doaj-art-96d7ed355da5492d99aa2e29f3abea7f2025-02-09T12:51:41ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-02-0185211010.1140/epjc/s10052-025-13794-xThe impact of compact object deformation on thin accretion disk propertiesShokoufe Faraji0Waterloo Centre for Astrophysics, University of WaterlooAbstract We investigate the standard relativistic geometrically thin and optically thick accretion disk in the background of a deformed compact object. The main purpose of this work is to determine whether such a deformed object possesses its own observational fingerprint that can distinguish it from Schwarzschild and Kerr black holes. Our analysis reveals the properties of this relativistic accretion disk model and its dependence on the initial parameters.https://doi.org/10.1140/epjc/s10052-025-13794-x |
spellingShingle | Shokoufe Faraji The impact of compact object deformation on thin accretion disk properties European Physical Journal C: Particles and Fields |
title | The impact of compact object deformation on thin accretion disk properties |
title_full | The impact of compact object deformation on thin accretion disk properties |
title_fullStr | The impact of compact object deformation on thin accretion disk properties |
title_full_unstemmed | The impact of compact object deformation on thin accretion disk properties |
title_short | The impact of compact object deformation on thin accretion disk properties |
title_sort | impact of compact object deformation on thin accretion disk properties |
url | https://doi.org/10.1140/epjc/s10052-025-13794-x |
work_keys_str_mv | AT shokoufefaraji theimpactofcompactobjectdeformationonthinaccretiondiskproperties AT shokoufefaraji impactofcompactobjectdeformationonthinaccretiondiskproperties |