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Polarization of emission from black hole accretion disks: including returning radiation

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00567704" target="_blank" >RIV/67985815:_____/22:00567704 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1142/9789811258251_0021" target="_blank" >http://dx.doi.org/10.1142/9789811258251_0021</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1142/9789811258251_0021" target="_blank" >10.1142/9789811258251_0021</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Polarization of emission from black hole accretion disks: including returning radiation

  • Original language description

    Accretion disks around stellar-mass black holes (BHs) are observed to emit radiation peaking in the soft X-rays (at about 1 keV) when the source is in the thermal state. This emission is expected to be polarized, because of electron scattering in the disk. However, photons will experience a rotation of the polarization plane due to General Relativity effects. X-ray polarization measurements can then be crucial in assessing strong gravity effects around accreting stellar-mass BHs, providing independent constraints on their spin. In this work, we present the simulated polarization spectra (obtained according to the model by Dovčiak et al.) for the X-ray, thermal radiation emitted by the accretion disk, as expected to be measured by IXPE, an X-ray polarimeter which will be launched in 2021. We also illustrate the code, currently under development, incorporate the contribution of returning radiation and account for absorption effects by the disk material.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    The Fifteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories

  • ISBN

    978-981-125-825-1

  • ISSN

  • e-ISSN

  • Number of pages

    8

  • Pages from-to

    250-257

  • Publisher name

    World Scientific

  • Place of publication

    Singapore

  • Event location

    Rome

  • Event date

    Jul 1, 2018

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article