Cited by 193Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsAdvanced Mathematical Theories and Applications

Did the Universe evolve?

Smolin, L·1992·Classical and Quantum Gravity

Abstract

A new type of explanatory mechanism is proposed to account for the fact that many of the dimensionless numbers which characterize particle physics and cosmology take unnatural values. It is proposed that all final singularities 'bounce' or tunnel to initial singularities of new universes at which point the dimensionless parameters of the standard models of particle physics and cosmology undergo small random changes. This speculative hypothesis, plus the conventional physics of gravitational collapse, together comprise a mechanism for natural selection, in which those choices of parameters that lead to universes that produce the most black holes during their lifetime are selected for. If our Universe is a typical member of the ensemble that results from many generations of such reproducing universes then it follows that the parameters of our present Universe are near a local maximum of the number of black holes produced per universe. Thus, modifications of the parameters of particle physics and cosmology from their present values should tend to decrease the number of black holes in the universe. Three possible examples of this mechanism are described.

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Crossref · 10.1088/0264-9381/9/1/016

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3 of 3 references verified0 citation errors · 0 not checkable

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  • In Einstein-Cartan theory, torsion is determined by the field equations and the resulting torsion tensor is proportional to the spin tensor of fermionic matter.

    “Instead, torsion is determined by the field equations obtained from varying the action with respect to the torsion tensor [6][7][8].The resulting torsion tensor is proportional to the spin tensor of fermionic matter.”
  • Spacetime torsion within Einstein-Cartan theory provides a simple and natural mechanism for preventing gravitational singularities.

    “A simple and natural mechanism for preventing gravitational singularities is provided by spacetime torsion within the Einstein-Cartan (EC) theory of gravity.”
  • Einstein-Cartan theory is equivalent to general relativity with the symmetric Levi-Civita connection, in which the energy-momentum tensor of matter acquires terms quadratic in the spin tensor.

    “Consequently, EC is equivalent to general relativity with the symmetric Levi-Civita connection, in which the energy-momentum tensor of matter acquires terms that are quadratic in the spin tensor.”
  • Such a contraction could correspond to gravitational collapse of matter inside a newly formed black hole existing in another universe.

    “Such a contraction could correspond to gravitational collapse of matter inside a newly formed black hole existing in another universe (Novikov 1966;Pathria 1972;Frolov et al. 1989Frolov et al. , 1990;;Smolin 1992;Stuckey 1994;Easson & Brandenberger 2001;Smoller & Temple 2003;Popławski 2010aPopławski , 2010cPopławski , 2011a)).”

    From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Smolin 1992

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Authors
Smolin, L.
Affiliations
Syracuse University (US)
Corresponding author
Smolin, L
Venue
Classical and Quantum Gravity
Published
1992-01-01
Volume
9
Issue
1
Pages
173-191
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2006208772
Cited by
193
References
3
Citations by year
2026: 6 · 2025: 5 · 2024: 4 · 2023: 4 · 2022: 8 · 2021: 9 · 2020: 14 · 2019: 10 · 2018: 3 · 2017: 5 · 2016: 7 · 2015: 9 · 2014: 11 · 2013: 5 · 2012: 8
FWCI
5.27
Type
journal article
Language
en
Open access
closed
Locations
Classical and Quantum Gravity (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Advanced Mathematical Theories and Applications
Keywords
anthropic principle, fine-tuning, dimensionless constants, multiverse, bounce cosmology, quantum tunneling, initial singularity, black holes, natural selection, gravitational collapse, cosmological constant

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