Super-eddington accreting massive black holes as long-lived cosmological standards

Jian Min Wang, Pu Du, David Valls-Gabaud, Chen Hu, Hagai Netzer

Research output: Contribution to journalArticlepeer-review

Abstract

Super-Eddington accreting massive black holes (SEAMBHs) reach saturated luminosities above a certain accretion rate due to photon trapping and advection in slim accretion disks. We show that these SEAMBHs could provide a new tool for estimating cosmological distances if they are properly identified by hard x-ray observations, in particular by the slope of their 2-10 keV continuum. To verify this idea we obtained black hole mass estimates and x-ray data for a sample of 60 narrow line Seyfert 1 galaxies that we consider to be the most promising SEAMBH candidates. We demonstrate that the distances derived by the new method for the objects in the sample get closer to the standard luminosity distances as the hard x-ray continuum gets steeper. The results allow us to analyze the requirements for using the method in future samples of active black holes and to demonstrate that the expected uncertainty, given large enough samples, can make them into a useful, new cosmological ruler.

Original languageEnglish
Article number081301
JournalPhysical Review Letters
Volume110
Issue number8
DOIs
StatePublished - 19 Feb 2013

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