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Towards the Super-Massive Black Hole Seeds

  • Eduardo S. Pereira
  • Pedro A. Santos
  • Haroldo F. de Campos VelhoEmail author
Chapter

Abstract

Massive and super-massive black-holes (BH) can be found in the center of all galaxies, according to the opinion from the scientific community. However, an open question is to know the origin of such BHs. One explanation is to consider such objects coming from the stars with large redshifts—very old stars collapsed during the ancient eras (population-III stars: the first-born stars created in the universe). A framework to investigate this scenario is to derive a mathematical model describing the evolution of the black hole distribution. From nowadays, observations show super-massive black holes with mass about 109M are ubiquitous in galaxy centers. The regularized inverse solution can be computed using an optimizer to identify the best solution for the functional to be minimized. Preliminary results are shown using synthetic observational data.

Notes

Acknowledgements

The authors would like to thank the FAPESP and CNPq, Brazilian agencies for research support.

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Copyright information

© Springer Nature Switzerland AG 2019

Authors and Affiliations

  • Eduardo S. Pereira
    • 1
  • Pedro A. Santos
    • 1
  • Haroldo F. de Campos Velho
    • 1
    Email author
  1. 1.Instituto Nacional de Pesquisas Espaciais (INPE)São José dos CamposBrazil

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