Cited by 82Cosmology and Gravitation TheoriesSpace Science and Extraterrestrial LifeMultidisciplinary Warburg-centric Studies

Multiverses and physical cosmology

Open access
Ellis, G. F. R., Kirchner, U., Stoeger, W. R.·2004·Monthly Notices of the Royal Astronomical Society

Abstract

The idea of a multiverse — an ensemble of universes — has received increasing attention in cosmology, both as the outcome of the originating process that generated our own Universe, and as an explanation for why our Universe appears to be fine-tuned for life and consciousness. Here we carefully consider how multiverses should be defined, stressing the distinction between the collection of all possible universes, and ensembles of really existing universes that are essential for an anthropic argument. We show that such realized multiverses are by no means unique. A proper measure on the space of all really existing universes or universe domains is needed, so that probabilities can be calculated, and major problems arise in terms of realized infinities. As an illustration we examine these issues in the case of the set of Friedmann–Lemaître–Robertson–Walker universes. Then we briefly summarize scenarios such as chaotic inflation, which suggest how ensembles of universe domains may be generated, and we point out that the regularities which must underlie any systematic description of truly disjoint multiverses must imply some kind of common generating mechanism. Finally, we discuss the issue of testability, which underlies the question of whether multiverse proposals are really scientific propositions.

AI snapshot

Written from the paper’s full text.

TL;DR

The paper argues that multiverse proposals must distinguish merely possible universes from actually realized ensembles, and that realized ensembles require both a distribution function and a measure over the space of possibilities. It concludes that such ensembles are not unique, face severe infinity and testability problems, and that any regularities across disconnected universes imply a common generating mechanism.

Key findings

  • A realized ensemble is represented by a possibility space \(M\), a measure \(\pi\), and a distribution function \(f(m)\); many different distribution functions can realize all possibilities, so the claim that every possibility is realized does not single out a unique multiverse.
  • In the FLRW illustration, different parameterizations yield different minimum-information measures, such as a constants-of-motion measure proportional to \(d\Lambda\,d\chi/\sqrt{\chi}\) versus an observational measure proportional to \(d\Omega_{m0}/\sqrt{\Omega_{m0}}\,d\Omega_{\Lambda0}\); these measures are often non-normalizable, so probabilities may be undefined.
  • Realized infinities are treated as deeply problematic: if all possibilities occur, uncountably many FLRW models arise, and even a countable infinity would leave almost all possible models unrealized. The paper cites an anthropic bound on the vacuum energy density of order \(10^{-28}\,\mathrm{g\,cm^{-3}}\) and, for \(\Lambda\) in \(\mathbb{R}^+\cup\{0\}\), an expectation value of \(\frac{1}{3}\rho_{\max}\).
  • Regularities across supposedly disconnected universes imply a common causal or generating mechanism; direct testing is impossible, though some multidomain scenarios can be disproved by observations of a small universe.

Methods

  • Conceptual and formal analysis with no new observational data. The paper defines a space of possible universes \(M\), a state space \(S\), and parameter categories \(p_j(i)\) for physics, cosmology, complexity, and biology, distinguishing class parameters from member parameters.
  • It formalizes a realized ensemble as \(E=\{M,\pi,f(m)\}\) and uses distribution and measure integrals to define numbers, averages, and probabilities; Jaynes’ principle is applied to construct minimum-information measures.
  • It illustrates the framework in the FLRW sector using Friedmann and Raychaudhuri equations, density parameters, constants of motion, and discusses chaotic inflation and cosmological-constant probability distributions.

Limitations

  • Stated: multiverse existence and properties are not directly or indirectly testable; only some multidomain scenarios can be falsified. There is no evidence for the required inflaton potential or underlying physics, and the arguments become philosophical or metaphysical.
  • Stated: one cannot fully specify all possibilities or an independent parameter set; measures are often non-normalizable; realized infinities create unresolved conceptual problems.
  • Evident: the analysis is theoretical and programmatic, with no empirical tests or data, and its conclusions depend on assumptions about measures, parameter spaces, and extrapolated physics.

Model-written summary. Check it against the paper before relying on it.

Integrity signals

Registry

Crossref · 10.1111/j.1365-2966.2004.07261.x

Cites

43 of 43 references verified0 citation errors · 0 not checkable

Statistics

Nothing to recompute.

Claims the paper makes

11 of 41 cited sources checked · 5 supported · 0 flagged · accuracy not yet measured

  • Premisecitation

    Ehlers & Rindler (1989) developed a parametrization in terms of observable density parameters and the Hubble parameter.

    “Ehlers & Rindler (1989) developed a parametrization in terms of the observable density parameters (they also include a radiation component) and the Hubble parameter.”
    Quote in the paperNot a substantial claim1 of 1 sources checked
    • cites Ehlers & Rindler 1989 source

      The Introduction (pp. 2–3) parametrizes expanding states using dust and radiation density parameters and the Hubble parameter. But the authors generally also use λ, representing the cosmological constant, and explicitly say its present value is not observable in principle; the claim therefore overstates the parametrization as being in terms of observable parameters. (LLM, conf=0.86)

      Experimental — accuracy not yet measured
  • Premisecitation

    Anthropic restrictions demand ρ ≲ 10^-28 g cm^-3.

    “It has been shown that anthropic restrictions demand ρ 10 -28 g cm -3 (Kallosh & Linde 2002;Garriga & Vilenkin 2002).”
    Quote in the paperSubstantial claim2 of 2 sources checked
    • cites Kallosh & Linde 2002 source

      The Introduction (p. 2) discusses anthropic limits on the cosmological constant, including an argument that life of our type is impossible when Λ is much greater than 10^-29 g/cm³. It does not establish a firm upper bound of 10^-28 g/cm³: its galaxy-formation examples give thresholds of about 10^-27 and 10^-25 g/cm³, depending on the regions considered. (LLM, conf=0.86)

      Experimental — accuracy not yet measured
    • cites Garriga & Vilenkin 2002 source

      The discussion of anthropic selection (section ⑴; page unavailable) says that a large positive dark-energy density can prevent galaxies from forming. But the paper does not state a required bound of 10^-28 g cm^-3; its reported constraints on Ω_D depend on assumptions about galaxy mass and the fluctuation spectrum (section ⑵; page unavailable). (LLM, conf=0.82)

      Experimental — accuracy not yet measured
  • Premisecitation

    Weinberg and Garriga & Vilenkin derive a probability distribution for the cosmological constant in an ensemble of regions generated in the same inflationary sequence via a given inflaton potential, where the cosmological constant is the potential energy of a scalar field.

    “Weinberg (2000a,b) and Garriga & Vilenkin (2000) derive a probability distribution for the cosmological constant in the context of an ensemble of regions generated in the same inflationary sequence via the action of a given inflaton potential, where the cosmological constant is given by the potential energy of a scalar field.”
    Quote in the paperNot a substantial claim1 of 2 sources checked
    • cites Weinberg 2000a,b

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

    • cites Garriga & Vilenkin 2000 source
  • Premisecitation

    Usually models in the doomsday argument literature either assume an ensemble exists or deal with potentially existing ensembles rather than actually existing ones.

    “However, usually these models either in effect assume an ensemble exists, or else are content to deal with potentially existing ensembles rather than actually existing ones (see, for example, Olum 2002).”
    Quote in the paperSubstantial claim1 of 1 sources checked
    • cites Olum 2002 source
  • Premisecitation

    For power-law potentials V(φ) = φ^n with n > 1, there is an integrable divergence at ρ = 0.

    “Nevertheless, as has been shown in Garriga & Vilenkin (2002), this is not always the case; in particular, for power-law potentials V(φ) = φ n with n > 1 we find an integrable divergence at ρ = 0.”
    Quote in the paperSubstantial claim1 of 1 sources checked
    • cites Garriga & Vilenkin 2002 source

      Section II, “The Prior Distribution” (Eq. 9; page not available) gives a prior density proportional to 1/|V′|, and the paper states that its singularity where V′=0 is integrable. It does not state the result for all power-law potentials with n>1 or locate the divergence specifically at ρ=0; its quadratic example instead describes an approximately flat prior near zero density. (LLM, conf=0.82)

      Experimental — accuracy not yet measured
  • Classified as probably not a substantial claim. 63
  • May combine two claims. 51
  • Borderline: one of the tests for a substantial claim is unclear. 1
  • Classified as probably not a substantial claim.

    Premisecitation

    The probability distribution for the existence of galaxies as a function of the cosmological constant can be approximated by P_gal = N(ρ)P(ρ), where N(ρ) is the fraction of baryons that form galaxies.

    “It has been suggested (Vilenkin 1995;Weinberg 1997) that the way the probability distribution for the existence of galaxies depends on the cosmological constant can be approximated by P gal = N (ρ )P(ρ ) (24 ) where N(ρ ) is the fraction of baryons that form galaxies.”
    Quote in the paperSubstantial claim1 of 2 sources checked
    • cites Vilenkin 1995 source

      In “Predictions from Quantum Cosmology” (page unavailable), Vilenkin describes a probability distribution weighted by N(α) and discusses how the cosmological constant can affect galaxy formation. But N(α) is defined as the average number of civilizations in a universe, not the fraction of baryons that form galaxies; our copy does not give the claimed P_gal = N(ρ)P(ρ) approximation. (LLM, conf=0.87)

      Experimental — accuracy not yet measured
    • cites Weinberg 1997

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • May combine two claims.

    Premisecitation

    The 'small universe' situation is observationally testable, and the cosmic background radiation power spectrum might already be giving evidence for it because of its lack of power on the largest angular scales.

    “This 'small universe' situation is observationally testable, and indeed it has been suggested that the cosmic background radiation power spectrum might already be giving us evidence that this is indeed so, because of its lack of power on the largest angular scales (Luminet et al. 2003).”
    Quote in the paperNot a substantial claim1 of 1 sources checked
    • cites Luminet et al. 2003 source
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    A proper measure on the space of all really existing universes or universe domains is needed so that probabilities can be calculated.

    “A proper measure on the space of all really existing universes or universe domains is needed, so that probabilities can be calculated”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationnone given

    The astrophysical issues expressed in the product are the easier ones to investigate.

    “The astrophysical issues expressed in the product are the easier ones to investigate.”
    Quote in the paperNot a substantial claim
  • Classified as probably not a substantial claim.

    Interpretationnone given

    It has not been demonstrated that a generic well-defined ensemble will admit life.

    “nor has it been demonstrated that a generic well-defined ensemble will admit life.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    The full space M must be large enough to represent all possibilities, along with many others we cannot even conceive of, but which can nevertheless in principle also be described by such parameters.

    “The full space M must be large enough to represent all of these possibilities, along with many others we cannot even conceive of, but which can nevertheless in principle also be described by such parameters.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationreasoning

    Infinity cannot be arrived at or realized.

    “However, if that is the case, then 'infinity' cannot be arrived at, or realized.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    For providing an explanation of existence, simply having a conceptually possible ensemble is not adequate; a link to objects or things that actually exist, or to mechanisms that make them exist, is needed.

    “For the purposes of providing an explanation of existence, simply having a conceptually possible ensemble is not adequate -we need a link to objects or things that actually exist, or to mechanisms that make them exist.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S4 (based).

    Interpretationnone given

    Universes in a multiverse should be able to differ in at least some properties from each other.

    “It is clear that universes in a multiverse should be able to differ in at least some properties from each other.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationnone given

    It is not at all clear that we shall ever be able to accurately delineate the class of all possible universes.

    “Furthermore, it is not at all clear that we shall ever be able to accurately delineate the class of all possible universes.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationreasoning

    We can, in principle, make a cut between those consistent with the eventual emergence of life and those incompatible with it.

    “We can, in principle, make a cut between those consistent with the eventual emergence of life and those incompatible with it”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationcitation

    The relevant integrals may diverge, making assignment of mean values or averages for physical quantities in an ensemble problematic.

    “Finally, the relevant integrals may diverge.In that case, assigning mean values or averages for physical quantities in an ensemble of universes is problematic”
    Quote in the paperNot a substantial claim0 of 1 sources checked
    • cites Kirchner & Ellis 2003 source
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).

    Interpretationreasoning

    In an ensemble in which all that is possible happens, all parameters will be member parameters.

    “In an ensemble in which all that is possible happens, all parameters will be member parameters”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisecitation

    The existence of the actually infinite inevitably leads to unresolvable contradictions in set theory and in definitions and deductive foundations of mathematics.

    “As he points out, following many others, the existence of the actually infinite inevitably leads to well-recognized unresolvable contradictions in set theory, and thus in definitions and deductive foundations of mathematics itself”
    Quote in the paperNot a substantial claim0 of 1 sources checked
    • cites Hilbert 1964

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisenone given

    No proof has been given that the physics that maximizes black hole production also favours life.

    “no proof has been given of the last step, that the physics that maximizes black hole production also favours life.”
    Quote in the paperNot a substantial claim0 of 1 sources checked
    • cites Smolin's (1999)

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • May combine two claims.

    Interpretationnone given

    If the set of realized models is finite or countably infinite, then almost all possible models are not realized and the ensemble represents a set of measure zero in the set of possible universes.

    “However, on the other hand, if the set of realized models is either finite or countably infinite, then almost all possible models are not realized -the ensemble represents a set of measure zero in the set of possible universes.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    There are infinitely many distribution functions that realize all possible universes, so a really existing 'ensemble of all possible universes' is not unique.

    “However, there are an infinite number of distribution functions which would fulfil this condition, and so a really existing 'ensemble of all possible universes' is not unique.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationnone given

    There is still considerable uncertainty as to the nature of an ensemble even within the restricted FLRW context.

    “There is still considerable uncertainty as to the nature of an ensemble even within this restricted context.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    Problems arise when it is claimed that there is an actually existing ensemble containing an infinite number of universes or of expanding universe regimes.

    “the problems arising when it is claimed that there is an actually existing ensemble containing an infinite number of universes or of expanding universe regimes.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationnone given

    The structures defined so far are uniform across the class of models in the possibility space, characterized by laws of physics and a restricted class of geometries.

    “The structures defined so far are the uniform structures across the class of models in this possibility space, characterized both by laws of physics (in particular, general relativity) and by a restricted class of geometries.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The assumption that the product N_S * f_S * f_p * n_e * f_l * f_i > 0 might be acceptable in our physically realized Universe but there is no reason to believe it holds generally in an ensemble.

    “This assumption might be acceptable in our physically realized Universe, but there is no reason to believe it would hold generally in an ensemble because these parameters will depend on other ensemble parameters, which will vary.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationreasoning

    Because the parameters P determine the dynamics, the set of paths in S characterizing individual universes m are determined by this prescription.

    “Because the parameters P determine the dynamics, the set of paths in S characterizing individual universes m are determined by this prescription.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationcitation

    The existence of multiverses or ensembles is in principle untestable by any direct observations, and the same applies to any hypothesized properties we may suppose for them.

    “the existence of multiverses or ensembles is in principle untestable by any direct observations, and the same applies to any hypothesized properties we may suppose for them.”
    Quote in the paperNot a substantial claim0 of 2 sources checked
    • cites Leslie 1996

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

    • cites Gardner 2003

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationnone given

    There is no conceptual problem with an infinite set of possible or conceivable universes.

    “There is no conceptual problem with an infinite set -countable or uncountable -of possible or conceivable universes.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing). May combine two claims.

    Interpretationreasoning

    The arguments against an infinite past time are strong; it is not constructible in terms of events or instants of time.

    “The arguments against an infinite past time are strong -it is simply not constructible in terms of events or instants of time, besides being conceptually indefinite.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based). May combine two claims.

    Interpretationreasoning

    Realizing probabilities for points of M implies a causal mechanism relating created members of the multiverse; otherwise there is no reason any probability law should be obeyed.

    “Realizing such probabilities seems to imply a causal mechanism relating the created members of the multiverse to one another so they are not, in fact, causally disjoint.Otherwise, there is no reason why any probability law (Gaussian normal, for example) should be obeyed.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    The regularities which must underlie any systematic description of truly disjoint multiverses must imply some kind of common generating mechanism.

    “the regularities which must underlie any systematic description of truly disjoint multiverses must imply some kind of common generating mechanism.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    Specifying the set of possible parameters determines a uniform high-level structure that is obeyed by all universes in M.

    “specifying the set of possible parameters determines a uniform high-level structure that is obeyed by all universes in M.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    Some such structuring is necessary if we are to be able to describe a multiverse with specified properties; a coherent description is only possible through the existence of such regularities.

    “Some such structuring is necessary if we are to be able to describe a multiverse with specified properties -a coherent description is only possible through the existence of such regularities.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    M anthropic does not intersect M FLRW, because realistic models of a life-bearing universe like ours cannot be exactly FLRW, for then there is no structure.

    “but does not intersect M FLRW (realistic models of a life-bearing universe like ours cannot be exactly FLRW, for then there is no structure).”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).

    Interpretationreasoning

    It is often convenient to use a set of parameters which are comoving in state space, i.e. constants of motion.

    “For these reasons it is often convenient to use a set of parameters which are comoving in the state space, i.e. parameters which are constants of motion.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationnone given

    There is vagueness about the proposed nature of multiverses.

    “There is, however, a vagueness about the proposed nature of multiverses.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    The same universe may occur several times over in the space of possible universes; the equivalence problem determines when such multiple representations occur.

    “Note that the same universe may occur several times over in this space; the equivalence problem determines when such multiple representations occur.”
    Quote in the paperSubstantial claim
  • Classified as probably not a substantial claim.

    Interpretationnone given

    For a complete probabilistic description of an ensemble we need both a distribution function P and a measure π.

    “For a complete probabilistic description of an ensemble we need not only a distribution function P, but also a measure π = µ(x) dx for each parameter space with parameter x”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S4 (based).

    Interpretationnone given

    In order to define a FLRW ensemble, we need a set of independent parameters which uniquely identify all possible FLRW models.

    “In order to define a FLRW ensemble, we need a set of independent parameters which uniquely identify all possible FLRW models.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S4 (based). May combine two claims.

    Premisenone given

    In any given ensemble, not all possible universes may be realized, and some may be realized many times.

    “However, in any given ensemble, they may not all be realized, and some may be realized many times.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationreasoning

    It will be impossible at any stage to characterize that set of the multiverse in which all the conditions necessary for the emergence of self-conscious life and its maintenance have been met, because we do not know what those conditions are.

    “It will be impossible at any stage to characterize that set of the multiverse in which all the conditions necessary for the emergence of self-conscious life and its maintenance have been met, for we do not know what those conditions are”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.

    Premisecitation

    Realized infinite sets are not constructible; there is no procedure to complete such a set.

    “Others (see Spitzer 2000;Stoeger 2003, and references therein) have further pointed out that realized infinite sets are not constructible -there is no procedure we can in principle implement to complete such a set -they are simply incompletable.”
    Quote in the paperNot a substantial claim0 of 2 sources checked
    • cites Spitzer 2000 source
    • cites Stoeger 2003

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationreasoning

    M Observational is a subset of M anthropic because we need observers to make observations.

    “Precisely because we need observers to make observations, this is a subset of M anthropic .”
    Quote in the paperNot a substantial claim
  • Classified as probably not a substantial claim.

    Interpretationcitation

    Life demands unique combinations of many different parameter values that must be realized simultaneously.

    “life demands unique combinations of many different parameter values that must be realized simultaneously.”
    Quote in the paperSubstantial claim0 of 2 sources checked
    • cites Davies 2003

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

    • cites Tegmark 2003 source
  • May combine two claims.

    Interpretationreasoning

    We can provide necessary sets of parameter values but cannot guarantee completeness or independence.

    “This means we can provide necessary sets of parameter values but cannot guarantee completeness or independence.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationreasoning

    The detailed characterization of the space M and its relationship to S depends on the matter description used and its behaviour.

    “The detailed characterization of this space, and its relationship to S, will depend on the matter description used and its behaviour.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    Future infinite time is never realized; whatever time we reach, there is always more time available.

    “Future infinite time also is never realized; rather, the situation is that whatever time we reach, there is always more time available.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    Genuine existence of an uncountable infinitude of models is highly problematic.

    “Because of the real number continuum, this is an uncountably infinite set of models -and genuine existence of such an uncountable infinitude is highly problematic.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisecitation

    A really existing infinite set is not possible.

    “However, as stressed by Hilbert (1964), it can be argued that a really existing infinite set is not possible.”
    Quote in the paperNot a substantial claim0 of 1 sources checked
    • cites Hilbert 1964

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based). May combine two claims.

    Interpretationnone given

    Many inflaton potentials may yield ensembles uninteresting for life, but some will be bio-friendly.

    “Many of these potentials may yield ensembles which are uninteresting as far as the emergence of life is concerned, but some will be bio-friendly.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    Chaotic inflation proposals are not directly observationally testable, and there is no astronomical evidence that the supposed other FLRW-like regions exist.

    “Also, these proposals are not directly observationally testable -we have no astronomical evidence the supposed other FLRW-like regions exist.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    Overarching physics, or a 'law of laws' represented by the inflaton field and its potential, can lead to a really existing ensemble of many very different FLRW-like regions of a larger universe.

    “This type of scenario suggests how overarching physics, or a 'law of laws' (represented by the inflaton field and its potential), can lead to a really existing ensemble of many very different FLRW-like regions of a larger universe.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationnone given

    If a multiverse contains a finite or infinite countable number of universes, the distribution function contains Dirac δ-functions.

    “A multiverse might contain a finite or infinite countable number of universes.In these cases, the distribution function contains Dirac δ-functions”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    There is no evidence that the postulated physics is true in this universe, much less in some pre-existing metaspace that might generate a multiverse.

    “There is no evidence that the postulated physics is true in this universe, much less in some pre-existing metaspace that might generate a multiverse.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    We seem to face an infinite regress when following the logic of explaining meta-laws, and it is not clear how to end it except by arbitrarily calling a stop.

    “We seem to face an infinite regress as we follow this logic to its conclusion, and it is not clear how to end it except by arbitrarily calling a stop to this process.”
    Quote in the paperNot a substantial claim
    • The authors state this as an assumption: Some relevant meta-laws pre-exist.
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing). May combine two claims.

    Interpretationreasoning

    If a multiverse is 'tested' by its prediction that our universe is a likely member, then an ensemble with many copies should be the most satisfying one, but one copy (just our universe) might be just as well.

    “If a multiverse is 'tested' by its prediction that our universe is a likely member, then such an ensemble should be the most satisfying one -but then we might just as well be happy with one copy, i.e. just our universe.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationreasoning

    Different distribution functions are needed for different possibility spaces.

    “While distribution functions can be parametrized by any set of coordinates over the possibility space, we need different distribution functions for different possibility spaces.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Premisecitation

    If we live in a 'small universe' where we have already seen right round the universe, then the universe closes up on itself in a single FLRW-like domain and no further causally connected such domains can exist.

    “These are when we live in a 'small universe' where we have already seen right round the universe (Ellis & Schrieber 1986;Lachieze-Rey & Luminet 1995) for then the universe closes up on itself in a single FLRW-like domain and so no further such domains that are causally connected to us in a single connected space-time can exist.”
    Quote in the paperSubstantial claim0 of 2 sources checked
    • cites Ellis & Schrieber 1986 source
    • cites Lachieze-Rey & Luminet 1995 source
  • May combine two claims.

    Interpretationreasoning

    These transformations are not unique, and hence it is possible to find many different measures.

    “These transformations are not unique, and hence it is possible to find many different measures.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    Philosophical argumentation is unavoidable if one is to seriously argue the claim for existence of a multiverse.

    “Thus, philosophical argumentation is unavoidable if one is to seriously argue the claim for existence of a multiverse.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    The measure is in general non-normalizable and hence there is no normalizable maximum-entropy distribution; without additional information we cannot calculate definite probabilities.

    “Secondly, the measure is in general non-normalizable and hence there is no normalizable maximum-entropy distribution.Without additional information we are not able to calculate definite probabilities.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based).

    Interpretationnone given

    A particular distribution function can be expressed in any set of coordinates.

    “It is clear that a particular distribution function can be expressed in any set of coordinates.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationnone given

    In order to establish distributions in a non-arbitrary way, we need a theory of how this particular ensemble is selected for from all other possible ones.

    “However, in order to establish these in a non-arbitrary way, we need a theory of how this particular ensemble is selected for from all the other possible ones.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationnone given

    There is a vast set of possible distribution functions.

    “Obviously there is a vast set of possible distribution functions.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The individual universes making up an ensemble with regularities are not actually independent of each other; they are products of a single process.

    “This in turn means that the individual universes making up the ensemble are not actually independent of each other.They are, instead, products of a single process, as in the case of chaotic inflation.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    For the 1/ρ distribution, the divergence is inside the anthropically allowed region and is non-integrable.

    “In this case the divergence is located inside the anthropically allowed region and is non-integrable.”
    Quote in the paperSubstantial claim
  • Borderline on S4 (based): unclear from the text.

    Interpretationnone given

    Ensembles resulting from a single causal process and ensembles consisting of discrete entities are ultimately not distinguishable from each other.

    “We discuss these two cases in turn, and then show that they are ultimately not distinguishable from each other.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    If space-time is quantized at the Planck level, then all physical quantities are quantized and uncountable infinities become finite numbers in any finite interval.

    “The problem would be allayed if space-time is quantized at the Planck level, as suggested for example by loop quantum gravity.In that case we can argue that all physical quantities also are quantized, and the uncountable infinities of the real line become transmuted into finite numbers in any finite interval”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    The proposed underlying physics for chaotic inflation has not been tested and may be untestable.

    “However, the problem is that the proposed underlying physics has not been tested, and indeed may be untestable.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    For the 1/ρ distribution, the expectation value of the cosmological constant vanishes, so we fail to explain the observed non-zero value.

    “For this case, the expectation value vanishes, i.e. ρ = ρ max 0 ρ (1/ρ ) dρ ρ max 0 (1/ρ ) dρ = 0 and we fail to explain the observed non-zero value of the cosmological constant.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    Observational probabilities are never conclusive.

    “In any case, in the end those papers all deal just with observational probabilities, which are never conclusive.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Premisecitation

    In scalar-field models P(ρ) is directly related to the a priori distribution of scalar-field fluctuations, and for a wide class of potentials the variations of P(ρ) over the anthropically allowed range should be negligible.

    “In scalar-field models P(ρ ) is in direct relation to the a priori distribution of the scalar-field fluctuations and it has been argued (Weinberg 2000a,b) that for a wide class of potentials the variations of P(ρ ) over the anthropically allowed range (where N(ρ ) = 0) should be negligible.”
    Quote in the paperSubstantial claim0 of 1 sources checked
    • cites Weinberg 2000a,b

      Couldn’t be matched to a paper in Crossref, so it can’t be checked.

  • May combine two claims.

    Interpretationreasoning

    We cannot link the distribution of the cosmological constant to that of the scalar field in a unique way, and there is a vast choice for possible a priori probability distributions for the cosmological constant.

    “Hence, we cannot link the distribution of the cosmological constant to that of the scalar field in a unique way, and there is a vast choice for possible a priori probability distributions for the cosmological constant.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based). May combine two claims.

    Interpretationnone given

    In the ensemble of all possible universes, all possible inflaton potentials and all solutions to those potentials should exist, including stationary and non-stationary chaotic inflationary models.

    “Finally, from the point of view of the ensemble of all possible universes often invoked in discussions of multiverses, all possible inflaton potentials should be considered, as well as all solutions to all those potentials.They should all exist in such a multiverse, which will include chaotic inflationary models which are stationary as well as those which are non-stationary.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    For the 1/√ρ distribution, there is a divergence in the anthropically allowed region, but it is integrable.

    “Again, there is a divergence in the anthropically allowed region, but this time it is integrable.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationnone given

    There is a philosophical problem surrounding a realized infinite set of any kind.

    “As we have pointed out above, there is a philosophical problem surrounding a realized infinite set of any kind.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The infinities of really existent FLRW-like domains derive from the assumed initial infinite flat or open space sections, and there are problems in assuming such space sections are actually realized.

    “In this case, the infinities of really existent FLRW-like domains derive from the assumed initial infinite flat (or open) space sections -and we have pointed out above the problems in assuming such space sections are actually realized.”
    Quote in the paperSubstantial claim
    • The authors state this as an assumption: The initial space sections are infinite flat or open.
  • Probably not a substantial claim: may not pass S4 (based).

    Premisenone given

    The only known method for constructing such a measure is Jaynes' principle.

    “The only known method for constructing such a measure is Jaynes' principle.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable).

    Interpretationreasoning

    If you cannot show which particular multiverse exists, it is doubtful you have shown any one exists.

    “Indeed, if you cannot show which particular one exists, it is doubtful you have shown any one exists.”
    Quote in the paperNot a substantial claim
  • Classified as probably not a substantial claim.

    Premisereasoning

    Anthropic FLRW universes are those in which the necessary cosmological conditions for life are fulfilled, allowing galaxies, stars and planets if the universe is perturbed, so allowing a non-zero factor N_g * N_S.

    “We can identify those FLRW universes in which the emergence and sustenance of life is possible at a broad levelfoot_8 -the necessary cosmological conditions have been fulfilled allowing the existence of galaxies, stars and planets if the universe is perturbed, so allowing a non-zero factor N g * N S * as discussed above.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationnone given

    In the state of minimum information we do not know the natural parametrization, and different measures correspond to different guesses.

    “Nevertheless, in the state of minimum information we do not know what the natural parametrization is for the possibility space and different measures correspond to different guesses.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing), S4 (based).

    Interpretationnone given

    A similar relation to equation (24) should hold for multiverses in the wider sense.

    “It is clear that a similar relation to equation ( 24) should hold for multiverses in the wider sense.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based).

    Interpretationnone given

    In a true multiverse, there is no possibility of any indirect causal connection of any kind; the universes are completely disjoint.

    “In the case of a true multiverse, there is not even any possibility of any indirect causal connection of any kind -the universes are then completely disjoint and nothing that happens in any one of them is causally linked to what happens in any other one.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    There is no direct evidence of existence of the claimed other universe regions in an ensemble, nor can there be any, because they lie beyond the visual horizon and most beyond the particle horizon.

    “There is no direct evidence of existence of the claimed other universe regions in an ensemble, nor can there be any, for they lie beyond the visual horizon; most will even be beyond the particle horizon, so there is no causal connection with them.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    The one way we might make a reasonable claim for the existence of a multiverse would be if we could show its existence was a more or less inevitable consequence of well-established physical laws and processes.

    “The one way we might make a reasonable claim for the existence of a multiverse would be if we could show its existence was a more or less inevitable consequence of well-established physical laws and processes.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S4 (based).

    Interpretationnone given

    Without knowledge of the creation mechanism, it is impossible to determine the measure with certainty.

    “Without knowledge of the creation mechanism, it is impossible to determine this measure with certainty.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The measure is derived from the chosen set of parameters; generally a different choice of parameters yields a different minimum-information measure, predicting another maximum-entropy distribution function.

    “First, the measure is derived from the chosen set of parameters.Generally a different choice of parameters yields a different minimum-information measure, predicting another maximum-entropy distribution function.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning

    If the existence of a multiverse is a scientific proposition, we need to be able to show which specific multiverse exists, but there is no observational way to do this.

    “The point is that there is not just an issue of showing a multiverse exists -if this is a scientific proposition we need to be able to show which specific multiverse exists; but there is no observational way to do this.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    The requirement of structure formation as a prerequisite for life places strong anthropic constraints on the domains in which observers could exist, and these constraints must be satisfied in the really existing universe.

    “The requirement of structure formation as a prerequisite for life places strong anthropic constraints on the domains in which observers could exist; these constraints must be satisfied in the really existing universe.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    Really existing multiverses that can be defined as candidates for the one to which our Universe belongs are not unique, and neither their properties nor their existence are directly testable.

    “It is, however, abundantly clear that 'really existing multiverses' which can be defined as candidates for the one to which our Universe belongs are not unique, and neither their properties nor their existence are directly testable.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationreasoning

    If all that can exist exists, then there are universe models occupying the biophilic subspace.

    “The issue of fine-tuning is the statement that the biophilic set of universes is a very small subset of the set of possible universes; but if all that can exist exists then there are universe models occupying this biophilic subspace.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    A small universe would disprove the usual chaotic inflationary scenario, but not a true multiverse proposal, for that cannot be shown false by any observation, nor shown true.

    “This would disprove the usual chaotic inflationary scenario, but not a true multiverse proposal, for that cannot be shown to be false by any observation.Neither can it be shown to be true.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationnone given

    Perturbations of exact FLRW models can allow life, but exact FLRW models themselves cannot.

    “More accurately, perturbations of these models can allow life -the exact FLRW models themselves cannot do so.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S1 (asserted), S4 (based).

    Interpretationnone given

    Even if inflation works just once, that is sufficient to give a model close enough to standard FLRW cosmological models to be friendly to life.

    “The counter response is that this does not matter; however small the chances are, if it works just once then that is sufficient to give a model close enough to the standard FLRW cosmological models to be friendly to life.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationreasoning

    The multiverse idea has problems: realized infinities; inability to describe such ensembles because we do not know all possibilities; and it is not testable or provable in the usual scientific sense, remaining a matter of faith rather than proof.

    “However, there are the following problems: (i) the issue of realized infinities discussed above; (ii) the problem of our inability to describe such ensembles because we do not know what all the possibilities are, so our solution is in terms of a category we cannot fully describe; (iii) the multiverse idea is not testable or provable in the usual scientific sense -existence of the hypothesized”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    A really existing ensemble or multiverse is not a priori unique, nor uniquely defined; it must somehow be selected for.

    “Our fundamental starting point is the recognition that there is an important distinction to be made between possible universes and realized universes, and our main conclusion is that a really existing ensemble or multiverse is not a priori unique, nor uniquely defined.It must somehow be selected for.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationnone given

    It is very likely that the simultaneous realization of all the conditions for life will pick out only a very small sector of the parameter space of all possibilities; anthropic universes are fine-tuned.

    “It is very likely that the simultaneous realization of all the conditions for life will pick out only a very small sector of the parameter space of all possibilities; anthropic universes are fine-tuned.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationnone given

    Previous discussions have not made clear what is required in order to define a multiverse, although some specific physical calculations have been given based on restricted low-dimensional multiverses.

    “However, previous discussions have not made clear what is required in order to define a multiverse, although some specific physical calculations have been given based on restricted low-dimensional multiverses.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationreasoning

    The ultimate questions about why this multiverse and its order cannot be answered scientifically because of the lack of any possibility of verification of any proposed underlying theory, and must be argued in philosophical terms.

    “In our view these questions -Issues 1 and 2 discussed in this paper -cannot be answered scientifically because of the lack of any possibility of verification of any proposed underlying theory.They will of necessity have to be argued in philosophical terms.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationreasoning

    The existence of life is quite unlike anything else in the physical world and requires explanation beyond chance.

    “The counter response is that the existence of life is quite unlike anything else in the physical world -its coming into being is not just like choosing one out of numerous essentially identical hands of cards.It is like being transformed into an entirely different higher level game, and so does indeed require explanation.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The claim that inflation explains the current state of the universe is only partially successful, because very anisotropic or inhomogeneous models may never inflate.

    “However, this move is only partially successful, because very anisotropic or inhomogeneous models may never inflate.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    At present, uniqueness eludes us.

    “At present, uniqueness eludes us.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning

    The evolution of life should only be possible in sufficiently flat models, at not too early and not too late times.

    “The evolution of life should only be possible in sufficiently flat models -otherwise the universes either recollapse too early or are too empty -at not too early and not too late times.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationreasoning

    The primordial process or overarching cosmic principle effectively selects a really existing multiverse from the possibilities in M and defines a distribution function over M.

    “These effectively select a really existing multiverse from the possibilities in M, and, as such, effectively define a distribution function over M.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable), S4 (based).

    Interpretationnone given

    The multiverse idea in the end represents a regress of causation.

    “Furthermore, in the end it simply represents a regress of causation.”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S2 (checkable). May combine two claims.

    Interpretationreasoning

    Almost-FLRW universes that are good models of our observable Universe are a small subset of all possible universes, and it is conceivable they are part of a multiverse or ensemble.

    “They are a small subset of all possible universes, and it is conceivable they are part of a multiverse or ensemble of universes.”
    Quote in the paperNot a substantial claim
102 of 102
  • The authors state this as an assumption.

    The description of the space M of possible universes assumes a set of laws of behaviour (laws of physics or meta-laws) that all universes have in common.

    “The very description of this space M of possibilities is based on an assumed set of laws of behaviour, either laws of physics or meta-laws that determine the laws of physics, which all universes m have in common; without this, we have no basis for setting up its description.”
  • The authors state this as an assumption.

    The expected number of planets with intelligent life in a universe is given by an adaptation of the Drake equation.

    “An adaptation of the Drake equation (Bennett et al. 2002) gives for the expected number of planets with intelligent life in any particular universe m in an ensemble”
  • The authors state this as an assumption.

    There is a function on the set of possible universes that describes the probability that life may evolve.

    “we need a function on the set of possible universes that describes the probability that life may evolve.”
  • The authors state this as an assumption.

    The quantities {N_g, N_S, f_S, f_p, n_e, f_l, f_i} are functions of the physical and cosmological parameters.

    “The quantities {N g , N S , f S , f p , n e , f l , f i } are functions of the physical and cosmological parameters characterized above”
  • The authors state this as an assumption.

    The family of FLRW models considered is filled with matter components characterized by a γ-law equation of state.

    “We assume the family considered is filled with matter components characterized by a γ -law equation of state”
  • The authors state this as an assumption.

    Gravity is described by the Einstein field equations.

    “Assuming gravity is described by the Einstein field equations, the evolution of FLRW models is described by the Friedmann equation”
  • The authors state this as an assumption.

    The discussion is restricted to models with only a cosmological constant and one comoving matter component obeying a γ-law equation of state.

    “We restrict our discussion to models with only a cosmological constant and one comoving matter component which obeys a γ -law equation of state”
  • The authors state this as an assumption.

    Only the gravitational constant G and the cosmological constant Λ are variables, with ranges G ∈ [0, ∞) and Λ ∈ (-∞, ∞).

    “For this simplified discussion let us just assume that only the gravitational constant G and the cosmological constant (which also qualifies as a model parameter) are variables, with the rangesfoot_4 G ∈ [0, ∞) and ∈ (-∞, ∞).”
  • The authors state this as an assumption.

    Space-time is quantized at the Planck level (or physical quantities are quantized) to soften the infinity problem.

    “We believe that this is a physically reasonable assumption to make, thus softening a major problem for many ensemble proposals.”
  • The authors state this as an assumption.

    The factor F = f_l * f_i, representing other conditions for life, is non-zero.

    “the above assumes this factor is non-zero.”
  • The authors state this as an assumption.

    The cosmological constant is a remnant of some underlying unknown theory and might be restricted to some domain of values.

    “Let us assume that the cosmological constant is a remnant of some underlying (unknown) theory and as such might be restricted to some domain of values.”
  • The authors state this as an assumption.

    Some relevant meta-laws pre-exist.

    “As emphasized above, we have to assume that some relevant meta-laws pre-exist.”
  • The authors state this as an assumption.

    Quantum field theory remains valid far beyond the domain where it has been tested.

    “It is also that, for example, we are assuming quantum field theory remains valid far beyond the domain where it has been tested, and we have faith in that extreme extrapolation despite all the unsolved problems at the foundation of quantum theory, the divergences of quantum field theory, and the failure of that theory to provide a satisfactory resolution of the cosmological constant problem.”
  • The authors state this as an assumption.

    The initial space sections are infinite flat or open.

    “In this case, the infinities of really existent FLRW-like domains derive from the assumed initial infinite flat (or open) space sections -and we have pointed out above the problems in assuming such space sections are actually realized.”
14 of 14

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • As Ellis et al. (2004) point out, any multiverse proposal will have to deal with the problems of what determines {M; f(m); p}, actualized infinities, non-renormalisability, parameter dependence and non-uniqueness of p, and how one could possibly observationally confirm any of these quantities.

    “As Ellis et al. (2004) point out, any such proposal will have to deal with the problems of what determines {M; f ðmÞ; p}, actualized infinities (in M, f(m) and the spatial extent of universes) and non-renormalisability, the parameter dependence and non-uniqueness of p, and how one could possibly observationally confirm any of these quantities.”

    From The Fine-Tuning of the Universe for Intelligent Life (2012) · cites this paper as Ellis et al. (2004)

    Split into 2 atoms — 1 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.

    Experimental — accuracy not yet measured

Cites

Flagged first, then by citations

Research works printed but not linked: 6

  1. 1991, MEM ITAL ASTRON SOC, 62, 553
  2. 1999, TOWARD A NEW MILLENIUM IN GALAXY MORPHOLOGY, Vol. 269 279, 693
  3. 1979, QJRAS, 20, 37
  4. 1999, THEORETICAL AND OBSERVATIONAL COSMOLOGY, 541, 1
  5. 2002, PHYS REV D, 67, 043503
  6. 2002, PHYS REV D, 67, 023510

Cited by

Sorted by citations

Authors
Ellis, G. F. R., Kirchner, U., & Stoeger, W. R.
Affiliations
University of Cape Town (ZA)
Venue
Monthly Notices of the Royal Astronomical Society
Published
2004-01-21
Volume
347
Issue
3
Pages
921-936
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2124540618
Cited by
82
References
21
Citations by year
2026: 3 · 2025: 5 · 2024: 4 · 2023: 4 · 2022: 4 · 2021: 2 · 2020: 2 · 2019: 21 · 2018: 2 · 2017: 3 · 2016: 1 · 2014: 2 · 2013: 3 · 2012: 4
FWCI
1.82
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
  • Social Sciences › Law › Multidisciplinary Warburg-centric Studies
Keywords
multiverse, anthropic principle, fine-tuning, measure problem, FRW universe, chaotic inflation, testability

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Claims read by deepseek-v4.1-flash under definition version 3 (extract-v3) on 2026-10-11.

Classified by jev-1.13-20260917 (gold-guideline-v0.2) on 2026-10-11.

Cited sources are checked by gpt-6-sol.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

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