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Black hole demographics from TDE modeling

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dc.contributor.author Mageshwaran, T
dc.contributor.author Mangalam, A
dc.date.accessioned 2020-11-27T12:53:13Z
dc.date.available 2020-11-27T12:53:13Z
dc.date.issued 2018-05
dc.identifier.citation Proceedings of the International Astronomical Union, Vol. 342, pp. 260-262 en_US
dc.identifier.issn 1743-9213
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7499
dc.description Restricted Access © International Astronomical Union https://doi.org/10.1017/S1743921318007305 en_US
dc.description.abstract The occurence rate of tidal disruption events (TDEs) by survey missions depend on the black hole mass function of the galaxies, properties of the stellar cusp and mass of the central black hole. Using a power law density profile with Kroupa mass function, we solve the steady state Fokker-Planck to calculate the theoretical capture rate of stars by the black hole. Using a steady accretion model, the Schechter black hole mass function (BHMF) and the cosmological parameters, we calculate the detection rate of TDEs for various surveys which is then fit with the observed TDE rates to extract the Schechter parameters. The rate tension between observation (∼10−5yr−1) and theory (∼10−4yr−1 for individual galaxies is explained by the statistical average over the BHMF. en_US
dc.language.iso en en_US
dc.publisher Cambridge University Press en_US
dc.relation.ispartofseries IAU Symposium No. 342;
dc.subject galaxies: nuclei en_US
dc.subject galaxies: luminosity function en_US
dc.subject mass function en_US
dc.subject Galaxy: kinematics and dynamics en_US
dc.subject galaxies: statistics en_US
dc.title Black hole demographics from TDE modeling en_US
dc.type Article en_US


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