Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · ·...
Transcript of Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · ·...
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Theories of the Initial State
Chris Smeenk
University of Western Ontario
Department of Philosophy
Rotman Institute
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Initial State Ination Eternal Ination Boltzmann Brains
Aims for Cosmological Theories
Indierence / Independence
- Dynamics sucient to produce order out of chaos- Equilibrium explanation
Specic Initial State
- Theoretical principles, special postulate, or brute fact
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Initial State Ination Eternal Ination Boltzmann Brains
Aims for Cosmological Theories
Indierence / Independence
- Dynamics sucient to produce order out of chaos- Equilibrium explanation
Specic Initial State
- Theoretical principles, special postulate, or brute fact
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Eliminating Initial Conditions
[We must] nd some way ofeliminating the need for an initialcondition to be specied. Onlythen will the universe be subjectto the rule of theory. ... Thisprovides us with a criterion socompelling that the theory of theuniverse which best conforms usto it is almost certain to be right.(Sciama 1959)
Defending steady state theory...replace with steady state eternalination?
Dennis Sciama
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Eliminating Initial Conditions
[We must] nd some way ofeliminating the need for an initialcondition to be specied. Onlythen will the universe be subjectto the rule of theory. ... Thisprovides us with a criterion socompelling that the theory of theuniverse which best conforms usto it is almost certain to be right.(Sciama 1959)
Defending steady state theory...replace with steady state eternalination?
Dennis Sciama
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Initial State Ination Eternal Ination Boltzmann Brains
Outline
An Initial State?
Theories of the Initial State
Inationary Dialectic
Eternal Ination
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Does the universe have an initial state?... or, better: Is the universe nite to the past?
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Initial State Ination Eternal Ination Boltzmann Brains
Singularities
FLRW Models
Image Credit: John Norton
Einstein's eld equationsreduce to two equationsfor R(t)
Extrapolating backwards:R(t) → 0 and ρ(t) →∞within nite time T
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Initial State Ination Eternal Ination Boltzmann Brains
Singularities
FLRW Models
Image Credit: John Norton
Generalizing:
Gravity is attractive →positive energy densityleads to geodesicconvergence, conjugatepoints
Maximal curves: geodesicswith no conjugate points
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Given a spacetime with the following properties (Wald, Thm 9.5.4):
1 Curvature: (a) Rabξaξb ≥ 0 for all timelike or null ξa. (Follows
from Einstein's eld eqns. and strong energy condition.)(b) Timelike and null generic conditions hold.
2 Causal Structure: There are no closed timelike curves.
3 Cosmology: There is a point such that the expansion of acongruence of past- (future-) directed null geodesics isnegative.
Conclusion
The spacetime has at least one incomplete geodesic (singularspacetime).
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Initial State Ination Eternal Ination Boltzmann Brains
Status of the Theorems?
To what extent do the assumptions depend on classical GR?
1 Curvature: Weak dependence on EFE... but energy conditions fail! (e.g., strong energy conditionviolated by ination and dark energy)
2 Causal Structure: Constraints on spacetime geometry, moregeneral than EFE.
3 Cosmology: Modest: expansion of null geodesics from presenttime becomes negative more recently than decoupling.
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Initial State Ination Eternal Ination Boltzmann Brains
Extending Singularity Theorems?
Singularity theorems for Ination
- Borde, Guth, Vilenkin (2003): consider local expansion rate H
for a congruence of geodesics. If average expansionH ≥ Hlb > 0 → upper bound on the integral of the expansionrate, past incomplete curve. No energy conditions assumed.
- But doesn't imply curvature singularity. Better: boundarytheorem. (Cf. Aguirre 0712.0571; Vilenkin 2013)
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Initial State Ination Eternal Ination Boltzmann Brains
Extending Singularity Theorems?
Quantum Gravity Eects
- Loop Quantum Cosmology (Bojowald, Ashtekar et al.):curvature bounded above, dynamical evolution extendsthrough (classical) singularity
- String theory: some singularities may be resolved by extradegrees of freedom
- Cyclic cosmologies: argue for continuation through singularityin higher dimensional spaces
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Does the universe have an initial state / is it nite to the past?
Answer depends on:(1) status of energy conditions,(2) implications of more general singularity theorems,(3) quantum gravity eects at Planck scale
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Initial State Ination Eternal Ination Boltzmann Brains
Responses to Singularities
Nature abhors a singularity? (cf. Earman 1995)
- Failure of determinism ... not in FLRW models → cosmiccensorship
- Break-down of GR ... singularities not localized regions, noregion within classical spacetime where GR fails
Boundary of domain of applicability
Quantum eects important in strong curvature regime
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Initial State Ination Eternal Ination Boltzmann Brains
Responses to Singularities
Nature abhors a singularity? (cf. Earman 1995)
- Failure of determinism ... not in FLRW models → cosmiccensorship
- Break-down of GR ... singularities not localized regions, noregion within classical spacetime where GR fails
Boundary of domain of applicability
Quantum eects important in strong curvature regime
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Initial State Ination Eternal Ination Boltzmann Brains
Responses to Singularities
Nature abhors a singularity? (cf. Earman 1995)
- Failure of determinism ... not in FLRW models → cosmiccensorship
- Break-down of GR ... singularities not localized regions, noregion within classical spacetime where GR fails
Boundary of domain of applicability
Quantum eects important in strong curvature regime
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Initial State Ination Eternal Ination Boltzmann Brains
Handling the Initial State
Dynamical Approaches
- V 1.0: wash away dependence on ICs (old rhetoric)- V 2.0: multiverse leads to equilibrium state, predictionsindependent of ICs (new rhetoric)
Postulate / Constraint on Initial State
- Past Hypothesis- Quantum Cosmology
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Initial State Ination Eternal Ination Boltzmann Brains
Handling the Initial State
Dynamical Approaches
- V 1.0: wash away dependence on ICs (old rhetoric)- V 2.0: multiverse leads to equilibrium state, predictionsindependent of ICs (new rhetoric)
Postulate / Constraint on Initial State
- Past Hypothesis- Quantum Cosmology
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Old Rhetoric: Ination and Initial Conditions
Due to causal structure (horizon) and dynamics (atness), standardcosmological model apparently requires pre-established harmonyand nely-tuned initial value of Ω ...
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Horizon / Smoothness Problem
Flatness Problem
Density parameter Ω = ρcρ evolves away from 1 (at model) with
expansion (R(t) =: scale factor):
|Ω− 1|Ω
∝ R2(t) (1)
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Horizon / Smoothness Problem
Flatness Problem
Density parameter Ω = ρcρ evolves away from 1 (at model) with
expansion (R(t) =: scale factor):
|Ω− 1|Ω
∝ R2(t) (1)
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... Solved by Ination?
- Horizon distance stretched by a factor of eN for N e-foldings,during ination dynamics drives Ω → 1
- Uniform, at patch as the generic post-inationary state, forsuciently large N
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Penrose Objection
Assume that measure is invariant under dynamics duringinationary stage (e.g., µGHS).
Then pre-inationary state must be less probable than thepost-inationary state. Replace original ne-tuning withne-tuning of initial state of inaton eld.
(See Penrose 2004 for recent formulation.)
Question
Is the dynamics during ination measure-preserving? (Unitary?)(Cf. Kofman et al. 2002, Hollands and Wald 2002)
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Penrose Objection
Assume that measure is invariant under dynamics duringinationary stage (e.g., µGHS).
Then pre-inationary state must be less probable than thepost-inationary state. Replace original ne-tuning withne-tuning of initial state of inaton eld.
(See Penrose 2004 for recent formulation.)
Question
Is the dynamics during ination measure-preserving? (Unitary?)(Cf. Kofman et al. 2002, Hollands and Wald 2002)
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Retrodicting Ination?
- Given present state, retrodict generic (according to µGHS)trajectories → nothing like observed history. Growinginhomogeneities, no inationary phase, etc.
- Past Hypothesis: constraint on initial conditions of inatoneld. (Conict between use of PH and old rhetoric.)
- Dissatisfaction: ICs for ination still unnatural, smallmeasure (... hence improbable?)
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Retrodicting Ination?
- Given present state, retrodict generic (according to µGHS)trajectories → nothing like observed history. Growinginhomogeneities, no inationary phase, etc.
- Past Hypothesis: constraint on initial conditions of inatoneld. (Conict between use of PH and old rhetoric.)
- Dissatisfaction: ICs for ination still unnatural, smallmeasure (... hence improbable?)
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Aside: Ination ... as a theory of structure formation
...[T]hese problems [related to initial conditions] can no longer beregarded as the strongest motivation for inationary cosmologybecause it is not at all clear that they could ever be used to falsifyination. [...] By contrast to ination as a theory of initialconditions, the model of ination as a possible origin of structure inthe Universe is a powerfully predictive one. Dierent inationmodels typically lead to dierent predictions for observedstructures, and observations can discriminate strongly betweenthem. ... Ination as the origin of structure is therefore very mucha proper science of prediction and observation. (Liddle and Lyth2000, p. 5; my emphasis)
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Aside: Ination ... as a theory of structure formation
- Law-like connections between properties of inaton and densityperturbations, etc.
- Challenges: (1) independent measurements of properties of theinaton eld; (2) degree of overdetermination of details ofination
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Initial State Ination Eternal Ination Boltzmann Brains
Status of the Past Hypothesis
What is the status of the PH compared to other basic principles orassumptions in physical theories?
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Laws vs. Initial Conditions?
Mill-Ramsey-Lewis Approach
Capture some body of physical knowledge in a deductive system.
Laws = axioms in the best such systemization, one thatmaximizes strength (large number of derived consequences) andsimplicity (small number of basic principles).
Consequence
PH (plausibly) comes out as a law given this denition. Evidencefor PH based on systematic role.
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Laws vs. Initial Conditions?
Mill-Ramsey-Lewis Approach
Capture some body of physical knowledge in a deductive system.
Laws = axioms in the best such systemization, one thatmaximizes strength (large number of derived consequences) andsimplicity (small number of basic principles).
Consequence
PH (plausibly) comes out as a law given this denition. Evidencefor PH based on systematic role.
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Initial State Ination Eternal Ination Boltzmann Brains
New Approach: Eternal Ination
Argument that ination is generically eternal, leads to multiversefrom initial uctuation.Replace question regarding unnaturalness of ICs for ination with:What does a typical observer in the multiverse see?
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Initial State Ination Eternal Ination Boltzmann Brains
Eternal Ination
Probability for inaton eld to uctuate up from de Sitter vacuumto appropriate initial state for eternal ination (Carroll and Chen2004):
P ≈ 10−1010
56
Footnote: We suspect that this may be smallest positivenumber in the history of physics... [... only has to benon-zero]
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Initial State Ination Eternal Ination Boltzmann Brains
Rening the Question?
From unnaturalness of ICs for ination → predictions in EI:
- Shift in understanding equilibrium state for quantum gravity?
- Bubble nucleation / account of spontaneous uctuation?
- Status of the PH and time's arrow in EI? Does granting PHundermine this further step?
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Initial State Ination Eternal Ination Boltzmann Brains
Rening the Question?
From unnaturalness of ICs for ination → predictions in EI:
- Shift in understanding equilibrium state for quantum gravity?
- Bubble nucleation / account of spontaneous uctuation?
- Status of the PH and time's arrow in EI? Does granting PHundermine this further step?
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Initial State Ination Eternal Ination Boltzmann Brains
Predictions in EI
In an eternally inating universe, anything that canhappen will happen; in fact, it will happen an innitenumber of times. Thus, the question of what is possiblebecomes trivial anything is possible, unless it violatessome absolute conservation law. To extract predictionsfrom the theory, we must therefore learn to distinguishthe probable from the improbable. (Guth 2007)
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Initial State Ination Eternal Ination Boltzmann Brains
Obstacles
Measure Problem
... even granting that a measure is found:
- justication of principle of mediocrity / typicality?- anthropic reasoning?
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Initial State Ination Eternal Ination Boltzmann Brains
Obstacles
Measure Problem
... even granting that a measure is found:
- justication of principle of mediocrity / typicality?- anthropic reasoning?
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Initial State Ination Eternal Ination Boltzmann Brains
Doomsday Argument (Gott 1994)
Evaluate prediction of the total number of humans N based onour birth rank r
Assume that we have typical r , motivating Pr(r |N) = 1/N.Further assume, for a constant k , the vague priors:
Pr(N) = k/N,Pr(r) = k/r
Application of Bayes's theorem leads to posterior:
Pr(N|r) = r/N2
Favors small N: probability that N > 20r is < 5 %
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Initial State Ination Eternal Ination Boltzmann Brains
Doomsday Argument (Gott 1994)
Evaluate prediction of the total number of humans N based onour birth rank r
Assume that we have typical r , motivating Pr(r |N) = 1/N.Further assume, for a constant k , the vague priors:
Pr(N) = k/N,Pr(r) = k/r
Application of Bayes's theorem leads to posterior:
Pr(N|r) = r/N2
Favors small N: probability that N > 20r is < 5 %
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Initial State Ination Eternal Ination Boltzmann Brains
Doomsday Argument (Gott 1994)
Evaluate prediction of the total number of humans N based onour birth rank r
Assume that we have typical r , motivating Pr(r |N) = 1/N.Further assume, for a constant k , the vague priors:
Pr(N) = k/N,Pr(r) = k/r
Application of Bayes's theorem leads to posterior:
Pr(N|r) = r/N2
Favors small N: probability that N > 20r is < 5 %
![Page 43: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/43.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
Problems with Typicality
Doomsday Argument: Learn too much!
How to describe real ignorance?
- Norton (2010): uniform probability distribution does notrepresent ignorance or neutral evidence, advocatesalternative inductive logic
- Imprecise probabilities in Bayesian approach (Joyce 2010,Benétreau-Dupin 2013)Both approaches block conclusion of doomsday argument
![Page 44: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/44.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
Problems with Typicality
Doomsday Argument: Learn too much!
How to describe real ignorance?
- Norton (2010): uniform probability distribution does notrepresent ignorance or neutral evidence, advocatesalternative inductive logic
- Imprecise probabilities in Bayesian approach (Joyce 2010,Benétreau-Dupin 2013)Both approaches block conclusion of doomsday argument
![Page 45: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/45.jpg)
Anthropic Reasoning
- Consider observational bounds on a parameter: α ∈ ∆, call Sthe region satisfying this constraint. Given regularized measureµ∗.
- Further ingredient: anthropic subset A, parameter valuesα ∈ ∆′ compatible with life
Pr(S) =µ∗(S)
µ∗(A)
- Evaluate a theory based only on anthropic subset, notdisconrmed by observer-less pocket universes with α 6∈ ∆
- Problems: What is the extent of the anthropic subset A, e.g.in regions of parameter space far from observed values?Reference class dependence? ...
![Page 46: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/46.jpg)
Anthropic Reasoning
- Consider observational bounds on a parameter: α ∈ ∆, call Sthe region satisfying this constraint. Given regularized measureµ∗.
- Further ingredient: anthropic subset A, parameter valuesα ∈ ∆′ compatible with life
Pr(S) =µ∗(S)
µ∗(A)
- Evaluate a theory based only on anthropic subset, notdisconrmed by observer-less pocket universes with α 6∈ ∆
- Problems: What is the extent of the anthropic subset A, e.g.in regions of parameter space far from observed values?Reference class dependence? ...
![Page 47: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/47.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
Boltzmann Brains
Theory with nite maximum entropy, Smax .
Consider collection of physical states = current brain state ofsome observer.
Typical member of this collection will be a Boltzmann brain,given relative probabilities of small vs. large uctuations awayfrom Smax .
Conclusion: This theory is falsied!
... but this fails to take BB seriously (cf. Winsberg 2012).
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Initial State Ination Eternal Ination Boltzmann Brains
Boltzmann Brains
Theory with nite maximum entropy, Smax .
Consider collection of physical states = current brain state ofsome observer.
Typical member of this collection will be a Boltzmann brain,given relative probabilities of small vs. large uctuations awayfrom Smax .
Conclusion: This theory is falsied!
... but this fails to take BB seriously (cf. Winsberg 2012).
![Page 49: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/49.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
Boltzmann Brains
Theory with nite maximum entropy, Smax .
Consider collection of physical states = current brain state ofsome observer.
Typical member of this collection will be a Boltzmann brain,given relative probabilities of small vs. large uctuations awayfrom Smax .
Conclusion: This theory is falsied!
... but this fails to take BB seriously (cf. Winsberg 2012).
![Page 50: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/50.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
Empirically Self-Undermining (Barrett 1999)
A theory is ESU if accepting the theory undermines the veryevidence used to support the theory.
Boltzmann Brains
- Skeptical scenario: Any given brain state could be chosen,including one of an observer obsessively checking thehypothesis. Not falsiable.
- ESU: Beliefs systematically misleading, including all theevidence that supported theory leading to BB.
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Initial State Ination Eternal Ination Boltzmann Brains
Empirically Self-Undermining (Barrett 1999)
A theory is ESU if accepting the theory undermines the veryevidence used to support the theory.
Boltzmann Brains
- Skeptical scenario: Any given brain state could be chosen,including one of an observer obsessively checking thehypothesis. Not falsiable.
- ESU: Beliefs systematically misleading, including all theevidence that supported theory leading to BB.
![Page 52: Theories of the Initial Statehipacc.ucsc.edu/IPC2013/slides/130709_ChrisSmeenk... · · 2015-10-06Theories of the Initial State Chris Smeenk ... cosmological model apparently requires](https://reader031.fdocuments.us/reader031/viewer/2022030508/5ab73f4d7f8b9ad5338b53c6/html5/thumbnails/52.jpg)
Initial State Ination Eternal Ination Boltzmann Brains
1 Boltzmann Brains as Empirical Check
- Reject theory with nite Smax , or constraint on rate of bubblenucleation relative to BB uctuations.
2 Boltzmann Brains as Skeptical Scenario
- Immune to empirical refutation, but empiricallyself-undermining.
- Require posit that earlier states were lower entropy in order forour evidence to be veridical.
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Initial State Ination Eternal Ination Boltzmann Brains
1 Boltzmann Brains as Empirical Check
- Reject theory with nite Smax , or constraint on rate of bubblenucleation relative to BB uctuations.
2 Boltzmann Brains as Skeptical Scenario
- Immune to empirical refutation, but empiricallyself-undermining.
- Require posit that earlier states were lower entropy in order forour evidence to be veridical.