Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes

The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the th...
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Autor*in:	Andrew Thomas West [verfasserIn] Henric Krawczynski [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 957(2023), 1, p 9
Übergeordnetes Werk:	volume:957 ; year:2023 ; number:1, p 9

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/acf612

Katalog-ID:	DOAJ101341512

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520			\|a The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements.
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allfields	10.3847/1538-4357/acf612 doi (DE-627)DOAJ101341512 (DE-599)DOAJ6f2e45a57ec243a7b6509d7294219968 DE-627 ger DE-627 rakwb eng QB460-466 Andrew Thomas West verfasserin aut Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements. Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics Henric Krawczynski verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 957(2023), 1, p 9 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:957 year:2023 number:1, p 9 https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/article/6f2e45a57ec243a7b6509d7294219968 kostenfrei https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 957 2023 1, p 9
spelling	10.3847/1538-4357/acf612 doi (DE-627)DOAJ101341512 (DE-599)DOAJ6f2e45a57ec243a7b6509d7294219968 DE-627 ger DE-627 rakwb eng QB460-466 Andrew Thomas West verfasserin aut Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements. Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics Henric Krawczynski verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 957(2023), 1, p 9 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:957 year:2023 number:1, p 9 https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/article/6f2e45a57ec243a7b6509d7294219968 kostenfrei https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 957 2023 1, p 9
allfields_unstemmed	10.3847/1538-4357/acf612 doi (DE-627)DOAJ101341512 (DE-599)DOAJ6f2e45a57ec243a7b6509d7294219968 DE-627 ger DE-627 rakwb eng QB460-466 Andrew Thomas West verfasserin aut Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements. Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics Henric Krawczynski verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 957(2023), 1, p 9 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:957 year:2023 number:1, p 9 https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/article/6f2e45a57ec243a7b6509d7294219968 kostenfrei https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 957 2023 1, p 9
allfieldsGer	10.3847/1538-4357/acf612 doi (DE-627)DOAJ101341512 (DE-599)DOAJ6f2e45a57ec243a7b6509d7294219968 DE-627 ger DE-627 rakwb eng QB460-466 Andrew Thomas West verfasserin aut Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements. Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics Henric Krawczynski verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 957(2023), 1, p 9 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:957 year:2023 number:1, p 9 https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/article/6f2e45a57ec243a7b6509d7294219968 kostenfrei https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 957 2023 1, p 9
allfieldsSound	10.3847/1538-4357/acf612 doi (DE-627)DOAJ101341512 (DE-599)DOAJ6f2e45a57ec243a7b6509d7294219968 DE-627 ger DE-627 rakwb eng QB460-466 Andrew Thomas West verfasserin aut Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements. Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics Henric Krawczynski verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 957(2023), 1, p 9 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:957 year:2023 number:1, p 9 https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/article/6f2e45a57ec243a7b6509d7294219968 kostenfrei https://doi.org/10.3847/1538-4357/acf612 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 957 2023 1, p 9
language	English
source	In The Astrophysical Journal 957(2023), 1, p 9 volume:957 year:2023 number:1, p 9
sourceStr	In The Astrophysical Journal 957(2023), 1, p 9 volume:957 year:2023 number:1, p 9
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topic_facet	Black hole physics Astrophysical black holes Rotating black holes Stellar mass black holes Astrophysics
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authorswithroles_txt_mv	Andrew Thomas West @@aut@@ Henric Krawczynski @@aut@@
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spellingShingle	Andrew Thomas West misc QB460-466 misc Black hole physics misc Astrophysical black holes misc Rotating black holes misc Stellar mass black holes misc Astrophysics Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes
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topic	misc QB460-466 misc Black hole physics misc Astrophysical black holes misc Rotating black holes misc Stellar mass black holes misc Astrophysics
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title	Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes
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title_auth	Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes
abstract	The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements.
abstractGer	The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements.
abstract_unstemmed	The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes. In this paper, we study the impact of the accretion disk geometry on the polarization of the thermal emission of mass-accreting stellar-mass black holes. We present a ray-tracing code that allows us to predict how the X-ray polarization energy spectra change as we dial up the thickness of the accretion disk from a geometrically thin accretion disk to a torus-shaped geometrically thick accretion disk. The results show that thicker disks can produce higher polarization degrees as the thick disk geometries lead to a larger fraction of X-rays reflecting off portions of the disk. We study the observational degeneracies between the disk shape on the one hand and the black hole spin and disk inclination on the other hand. We conclude with a discussion of the implications of our studies for black hole spin measurements.
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title_short	Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes
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Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes

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