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Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
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Setting Limits on Supersymmetry Using Simplified Models
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Primordial Black Holes with QCD Color Charge.

Elba Alonso-Monsalve1, David I Kaiser1

  • 1Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.

Physical Review Letters
|June 21, 2024
PubMed
Summary

Primordial black holes (PBHs) may have formed in the early Universe with a net color charge by absorbing quarks and gluons. This mechanism could explain their contribution to dark matter if they formed before the QCD confinement transition.

Area of Science:

  • Cosmology
  • Particle Physics
  • Astrophysics

Background:

  • Primordial black holes (PBHs) are hypothetical black holes formed in the early universe.
  • PBHs are a potential candidate for dark matter.
  • The Quantum Chromodynamics (QCD) confinement transition is a key event in the early universe.

Purpose of the Study:

  • To propose a realistic mechanism for the formation of PBHs with significant QCD color charge.
  • To investigate the implications of such colored PBHs for dark matter.
  • To estimate the abundance of near-extremal colored PBHs.

Main Methods:

  • Modeling PBH formation via absorption of unconfined quarks and gluons before QCD confinement.
  • Estimating the number density of colored PBHs per Hubble volume under various scenarios.

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  • Discussing potential phenomenological consequences of colored PBHs.
  • Main Results:

    • A mechanism is described for PBHs to acquire a net color charge by absorbing pre-confinement quarks and gluons.
    • The formation of colored PBHs is linked to the early universe and the QCD transition.
    • Estimates for the abundance of near-extremal colored PBHs are provided for different cosmological scenarios.

    Conclusions:

    • Colored PBHs represent a plausible formation channel in the early universe.
    • These PBHs could constitute a significant fraction of dark matter.
    • Further investigation into the phenomenological implications of colored PBHs is warranted.