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Asymptotically FRW black holes

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Abstract

Special solutions of the LTB family representing collapsing over-dense regions corresponding to asymptotically closed, open, or flat FRW models are found. These solutions may be considered as representing dynamical mass condensations leading to black holes immersed in a FRW universe. We study the dynamics of the collapsing region, and its density profile. The question of the strength of the central singularity and its nakedness, as well as the existence of an apparent horizon and an event horizon is dealt with in detail, shedding light to the notion of cosmological black holes. Differences to the Schwarzschild black hole are addressed.

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Authors and Affiliations

  1. Department of Physics, Sharif University of Technology, Tehran, Iran

    J. T. Firouzjaee & Reza Mansouri

  2. School of Astronomy, Institute for Research in Fundamental Sciences (IPM), Tehran, Iran

    Reza Mansouri

Authors
  1. J. T. Firouzjaee
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  2. Reza Mansouri
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Correspondence to J. T. Firouzjaee.

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Firouzjaee, J.T., Mansouri, R. Asymptotically FRW black holes. Gen Relativ Gravit 42, 2431–2452 (2010). https://doi.org/10.1007/s10714-010-0991-7

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