Tier I · A Mind behind nature
The universe had a beginning
For most of recorded history the leading philosophies held that the world had always existed. The Bible said it began. What does modern cosmology actually show, and how much is that worth as evidence for God?
The short version
- Our universe was hot and dense about 13.8 billion years ago.
Three independent lines show it: the expansion, the microwave background, and the amounts of helium and deuterium, which match a prediction whose one free number is set by a different measurement.
The evidence ↓ - A theorem says expansion cannot run back forever.
A history that keeps expanding on average cannot be extended forever into the past. That our own history therefore has a first state is a strong but unproven inference, with named exceptions; no model that avoids it has support.
The evidence ↓ - Physics does not yet reach the first moment.
The theorems are classical, and quantum gravity is unknown. Two authors of the same theorem disagree: one says the universe "probably did" begin; the other, as a colleague reports his view, that it is "very likely eternal".
The evidence ↓ - A first state needs an explanation that is not an earlier state.
Given a principle of sufficient reason, which physics cannot supply, it is necessary or explained by a law of the initial state, a necessary fact, or something beyond physics. That narrows naturalism's options; it does not refute it.
The evidence ↓ - So it counts, but modestly.
A beginning fits a Creator better than it fits naturalism, by a likelihood ratio of about 1.3. That ratio can never exceed the physics' own support for a beginning, so this line cannot be a proof.
The evidence ↓
The question
Does physical reality, all of it, including anything that came "before" the hot Big Bang, have a finite past? And if it does, how much does that fact tell us about whether there is a Creator?
Three different claims hide under "the universe had a beginning". Most popular arguments, on both sides, slide between them. We keep them apart, and the whole page hangs on this ladder.
| Rung | Claim | Status | Who disputes it |
|---|---|---|---|
| L1 Our cosmic history | Our observable universe evolved from a hot, dense state a finite time ago (the hot Big Bang model). | Established | Almost no working cosmologist. |
| L2 Past-incompleteness | A model of spacetime that keeps expanding on average cannot be continued indefinitely into the past (the singularity theorems; the BGV theorem, amended in 2024). | Theorem about models | Nobody disputes the mathematics. Whether our own past is such a model is a separate question (L2b). |
| L2b A first state | Our history has a state that no earlier state explains: no endless chain of earlier states behind it. | Strong inference, unproven | Named exceptions: "seed" universes, a direction of time not set by entropy, a past ending in a singularity, and quantum gravity, which is unknown. |
| L3 Absolute beginning | Physical reality as a whole began to exist, with no physical "before": time itself began. | Not established | Guth, Carroll, Aguirre, Steinhardt, Penrose and others. |
Only L3 is scored as evidence. L1 is as secure as anything in cosmology, but it does not discriminate: nearly every naturalistic cosmology also puts a hot Big Bang in our past, as a local event inside something larger or older. L2b is not L3. Some models that are eternal in time still have a first state in the order of explanation (a moment of lowest entropy from which time's arrow runs both ways), and a past that ends at a singularity is finite in time but has no first state.
The hypotheses.
- H, biblical theism. A transcendent God created "the heavens and the earth" (Genesis 1:1), and "all things were made through him" (John 1:3). H strongly expects an absolute beginning. One caveat from inside the tradition: Thomas Aquinas held that a beginning is known by faith, not by demonstration, because God could have created an eternal world.1 So generic theism expects a beginning less strongly than the Bible does.
- N1, naturalism with an eternal past. A steady state, eternal inflation, a cyclic or bouncing cosmos, an eternal static seed, or a timeless quantum state that evolves forever.
- N2, naturalism with an uncaused beginning. Reality has a first state or a boundary of time, and nothing caused it: Vilenkin's tunnelling "from nothing", the Hartle–Hawking no-boundary state, or the view that "the universe simply is".
What each hypothesis predictstable · 6 rows
| Observation | H (theism) | N1 (eternal) | N2 (uncaused start) |
|---|---|---|---|
| L1: a hot Big Bang in our past | Compatible, not specifically predicted | Compatible, if the Big Bang is a local event | Compatible |
| L2: classical past-incompleteness | Expected | Must be evaded (no net expansion, or a quantum era) | Expected |
| L2b: a first state | Expected | Denied (needs one of the named exceptions) | Expected; fixed by a law of the initial state, or simply brute |
| L3: an absolute beginning | Strongly expected | False by definition | True, but uncaused |
| Low entropy in the past | Compatible (see fine-tuning) | A problem for simple eternal models; needs designs where entropy can grow without limit | Must be posited as a starting condition |
| No viable past-eternal model | Expected | An embarrassment, not a refutation | Neutral |
Rules of evidence
We fixed these before scoring anything.
- Only an absolute beginning (L3) counts. The hot Big Bang (L1) is not scored by itself. The theorems (L2) count only through what they say about L3.
- Calibrate on working cosmologists, from both sides. How far the data push toward L3 is judged against what the theorem's own authors conclude (Vilenkin and Guth disagree), not against apologetics summaries.
- Theorems are scored by their assumptions. A theorem about classical spacetime cannot settle the quantum era. A theorem about models is not a fact about our universe: the step from one to the other is graded separately, with its exceptions. We report the authors' reading and their published critics.
- Quotations only from sources we opened. Widely circulated quotes we could not trace are listed under What we don't claim, not used.
- The whole null space is on the table. Every serious past-eternal and "from nothing" proposal is listed with its status, including the live ones. So are the facts that cut against the argument: the lithium problem, the classical scope of the theorem, the split among its authors, and the Kalam's need for a premise physics cannot supply.
- No double counting. The extraordinarily low entropy of the early universe is a fine-tuning fact and is discussed on the fine-tuning page, where it is deliberately left out of the ratio. Whether Genesis "predicted" a beginning is scored on the Genesis 1 page; here it appears only as history. The philosophical argument that an actual infinite is impossible is stated but given no weight, because it would double-count the causal intuition already inside the model.
- Two stages. The model separates how strongly the data favour an absolute beginning from how strongly each hypothesis predicts one. This stops the certainty of L1 from standing in for the uncertainty of L3.
The evidence
1. The hot Big Bang (L1): established
Galaxies recede faster the farther away they are, as Lemaître and Hubble found in 1927 and 1929.2 The Planck satellite puts today's expansion rate at 67.4 ± 0.5 km/s per megaparsec; nearby distance-ladder measurements give a higher value, the unresolved "Hubble tension". That is a dispute about the rate, not about the expansion.3
The sky glows with microwaves at 2.72548 ± 0.00057 K, with the spectrum of a near-perfect blackbody: the cooled light of a time when the universe was hot and opaque.4,5 The pattern of ripples in that light fits, in Planck's words, "the standard spatially-flat 6-parameter ΛCDM cosmology", and gives an age of about 13.8 billion years.3
The strongest single test is the light elements. A hot Big Bang cooks hydrogen into helium and deuterium in its first minutes, and the amounts depend on one number, the density of ordinary matter. The microwave background fixes that number independently. With nothing left to adjust, the predictions land within half a standard deviation of what is observed.6,7
Helium and deuterium land on the prediction; lithium misses
Gap between observed and predicted primordial abundance, in standard deviations (observed is lower in all three). Fields et al. 2020; Cooke et al. 2018.
Show the data
| Element | Gap (σ) | Note |
|---|---|---|
| Helium-4 | 0.5σ | predicted 0.24691 ± 0.00018; observed 0.2449 ± 0.0040 |
| Deuterium | 0.3σ | predicted (2.57 ± 0.13)×10⁻⁵; observed (2.527 ± 0.030)×10⁻⁵ |
| Lithium-7 | 4.0σ | predicted (4.72 ± 0.72)×10⁻¹⁰; observed (1.6 ± 0.3)×10⁻¹⁰, about 3 times low |
Lithium is the honest exception. Observed lithium-7 is about three times lower than predicted, a gap of about 4 standard deviations. The authors of the standard analysis say plainly that "the lithium problem remains".6 Whether the cause is in the stars that were measured, in nuclear physics or in new physics is open. It does not threaten L1, but a fair page has to show it.
The nine observations, with numbers and statustable · 9 rows
| Claim | Data | Status |
|---|---|---|
| The universe is expanding | Redshift grows with distance (Lemaître 1927, Hubble 1929).2 H0 = 67.4 ± 0.5 km/s/Mpc (Planck, model-inferred); local measurements give about 73.3 | Established expansion; Contested exact rate |
| The universe was once hot and opaque | Microwave background: a blackbody at 2.72548 ± 0.00057 K (discovered 1965; COBE/FIRAS spectrum 1994).4,5 | Established |
| The background's ripples fit the six-parameter model | Acoustic scale measured to 0.03%; baryon density Ωbh² = 0.0224 ± 0.0001.3 | Established |
| Light elements were made in the first minutes | Helium-4: predicted 0.24691 ± 0.00018, observed 0.2449 ± 0.0040 (−0.5σ). Deuterium: predicted (2.57 ± 0.13)×10−5, observed (2.527 ± 0.030)×10−5 (−0.3σ).6,7 | Established |
| A known anomaly: lithium-7 | Predicted (4.72 ± 0.72)×10−10, observed (1.6 ± 0.3)×10−10, about 3 times low (−4.0σ).6 | Established anomaly; cause open |
| Ages agree | Model age about 13.8 billion years; no star reliably older.3 | Established |
| JWST's "too early" massive galaxies | Candidate galaxies of 1010–1011 solar masses about 600 million years after the Big Bang;8 at the edge of what the standard model allows;9 after removing contamination by active nuclei, the excess "can be explained by modest changes to star formation physics" and is "not in tension with modern cosmology".10 | Contested for galaxy formation; no bearing on L1 |
| The universe is far from equilibrium | Entropy today about 3.1×10104 k; maximum (event horizon) about 2.6×10122 k. See below.11 | Established (order of magnitude) |
| Is dark energy a constant? | DESI's second data release (DR2, analysed in 2026), with the microwave background, prefer a dark energy that changes over time "at 2.7σ", and "at 3.2σ when also including supernovae".12 Below the 5σ physicists require, and sensitive to the statistical choices made. | Contested; no bearing on whether the universe began |
The second law: an old argument, rightly limited
Entropy (roughly, disorder) rises over time. So the past had less of it. A simple closed universe that had existed forever should long ago have run down to equilibrium. Vilenkin uses this against the old cyclic models: "If the universe had already completed an infinite number of cycles, it would have reached a state of thermal equilibrium".13 Ours has not: its entropy today, about 3.1×10104 in natural units, is far below the 2.6×10122 its horizon could hold.11
But the argument has a limit. It defeats the naive eternal universe, not every eternal one. Carroll and Chen propose a model in which "inflation can increase the total entropy of the universe without bound", so there is no maximum to run down to.14 That model is speculative, but it shows the second law alone does not force a beginning.
The entropy numbers, and why they belong to fine-tuningcalculation · context only
Entropies of the observable universe (Egan & Lineweaver 2010), in units of Boltzmann's constant:11
microwave-background photons 2.0 x 10^89 everything today (mostly black holes) 3.1 x 10^104 cosmic event horizon (the maximum) 2.6 x 10^122 How rare is a state like the early one, compared with the maximum? exp(S_early - S_max) ~ 10^(-1.1 x 10^122) i.e. about 1 in 10^(10^122)
With a cosmological constant (our universe), the most one horizon patch can hold is the de Sitter horizon entropy, about 3.3 x 10^122. On a measure that counts every state of the patch equally: a state like the early one ~ 10^(-1.44 x 10^122) today's matter-only state ~ 10^(-1.44 x 10^122) (the same) Penrose's black hole of all the matter in the observable universe: 1.5 times wider than the horizon, so it does not fit.
Two corrections to the usual telling. First, Penrose's famous "1 in 1010123"15 is, in Goldstein's summary, an estimate of the phase space "for a closed universe".16 In a universe with a cosmological constant the comparable figure is about 1 in 1010122. Second, the same exponent comes out for today's state of matter, so the number says that our patch of the universe is far from its own equilibrium; it does not single out the beginning as special. Whether it is a meaningful probability for the initial state at all is contested.17 For these reasons the low-entropy start belongs to the fine-tuning page, which discusses it but adds it to no ratio. It is not scored here either.
2. The theorems (L2): what they prove and what they don't
In 1965–70 Penrose and Hawking proved that, under general relativity and an energy condition (roughly, that gravity always attracts), spacetime cannot be extended indefinitely into the past.18 Hawking himself later argued that quantum effects remove the singularity.19
In 2003 Borde, Guth and Vilenkin (BGV) proved something with far fewer assumptions: "a simple kinematical argument, requiring no energy condition, that a cosmological model which is inflating – or just expanding sufficiently fast – must be incomplete in null and timelike past directions".20 In Vilenkin's words, "It makes no assumptions about gravity or matter."13 "Incomplete" means that the paths of light and of observers, traced back, run out after a finite time.
In 2024 Garcia-Saenz, Hua and Zhao closed a loophole critics had found and proved a companion result: for uniform universes, "geodesic completeness implies (i) the existence of a bounce, loitering phase or an emergent cosmology". Their results "are purely kinematic and do not assume general relativity or energy conditions".21 Later work extends the theorem to Penrose's cyclic cosmology and to the 2019 cyclic model, both of which come out incomplete.22,23
A history whose average expansion rate stays above some positive bound, over every stretch of its past that ends at a given point, cannot be extended forever into the past. Something else (a boundary, a quantum era, or a phase that was not expanding) must be there. It is a theorem about models.
That is weaker than "time began". It says where a description of that kind must fail. It does not say what lies there, and it does not by itself say that our universe is such a history: "it has expanded on average over its whole past" is a property of a model of the whole past, not something a telescope sees. (De Sitter space, the simplest inflating universe, is incomplete in one standard set of coordinates and complete in another.) Carroll's objection is exact: "the BGV theorem assumes a classical spacetime, so it says nothing definitive about what actually happens in the universe".24
Each theorem: what it assumes, proves and does not provetable · 8 rows
| Theorem | Assumes | Proves | Does not prove |
|---|---|---|---|
| Penrose 1965; Hawking 1967; Hawking–Penrose 197018 | General relativity; an energy condition (gravity attracts); causality conditions; a trapped surface or similar | Spacetime is geodesically incomplete: past worldlines end after a finite time | That time began; that there is an infinite-density event; anything about the quantum regime |
| Borde–Guth–Vilenkin 200320 | Only that the expansion rate, averaged along a past path, is positive. No energy condition, no particular theory of gravity13 | Such a spacetime is past-incomplete; "inflationary models require physics other than inflation to describe the past boundary of the inflating region" | What lies at the boundary; that time began; anything about spacetimes whose average expansion is zero or negative; quantum gravity24 |
| Amended BGV (Garcia-Saenz, Hua & Zhao 2024)21 | Average expansion above a positive bound over every stretch of the past ending at a given point; no general relativity, no energy condition | Past-incompleteness, with the earlier loophole closed; a complete uniform history must bounce, loiter or be emergent | That our past meets the hypothesis; what lies at the boundary; that time began |
| Extensions (Kinney and colleagues, 2024, 2026)22,23 | As BGV, applied to cyclic and uneven models | "the Conformal Cyclic extension of an asymptotically de Sitter universe is geodesically incomplete"; "the cyclic model proposed by Ijjas and Steinhardt is geodesically incomplete" | Anything about models with no net expansion |
| Wall 2013, from the generalized second law25 | The generalized second law (entropy, horizons included, never falls); semiclassical gravity where curvature is low | Incompleteness "to the past of spatially infinite" expanding universes; if space is finite, only a finite amount of entropy production in the past, "unless there is a reversal of the arrow of time" | Anything about models whose arrow of time reverses; anything without the generalized second law |
| BGV applied to cyclic and emergent models (Mithani & Vilenkin)26,27 | BGV plus a quantum-tunnelling analysis | Eternal inflation and cyclic models with net growth are past-incomplete; the emergent static seed "can collapse quantum mechanically, and therefore cannot have an eternal past" | That every quantum-gravity model must begin; the instability argument depends on the model |
| Critics of BGV's scope28,29 | Different definitions of average expansion; extensions of spacetime | Lesnefsky, Easson and Davies call the standard claim "an open issue" and construct "an uncountably infinite cohort of cosmological solutions which are geodesically complete despite having Havg>0". Geshnizjani, Ling and Quintin conclude that "past-eternal inflationary scenarios are most likely physically singular, except in situations with very special initial conditions" | Neither shows that our universe is past-eternal |
| Carroll's "quantum eternity theorem"24 | Ordinary quantum mechanics, non-zero energy, unchanging laws of evolution | Such a universe lasts forever toward past and future | That those assumptions hold for quantum gravity (a closed universe may have zero total energy, and then there is no external time) |
BGV in one line of algebraderivation · simplest case
Take the simplest case: a flat, uniform universe with scale factor a(t) and expansion rate H = ạ/a. Follow a light ray backward. With its affine parameter λ normalized so that dλ = (a/anow) dt,
integral of H d(lambda) = integral of (a-dot / a_now) dt
= (a_now - a_then) / a_now
= 1 - a_then / a_now < 1So the expansion accumulated along the ray, traced back as far as you like, can never exceed 1. If the average expansion rate along the ray is some positive number Hav, the ray's whole past length is at most 1/Hav: finite. BGV's achievement was to prove a bound of this kind for any spacetime, uniform or not, without using Einstein's equations at all.20,13 The proof says nothing about what the ray meets at the end.
3. The attempts to avoid a beginning
If the universe is eternal after all, there should be a model that shows how. Many have been proposed. Here is the fair state of play.
- Refuted or abandoned: Einstein's static universe (unstable, then contradicted by expansion), the Hoyle–Bondi–Gold steady state (refuted by radio-source counts, the microwave background and helium), the old oscillating universe (entropy grows each cycle).30,31,13
- Unconfirmed: Penrose's conformal cyclic cosmology. Its claimed signals in the microwave sky were not reproduced: one reanalysis found the data "fully consistent with the LCDM model", another found its "Hawking points" at "only an 87% confidence level".32,33,34
- Beginning after all: eternal inflation is eternal toward the future but, as Guth writes, "not eternal into the past".35 The 2019 cyclic model grows by "an exponential factor from one cycle to the next", so BGV applies to it.36,13
- Alive but speculative: Aguirre and Gratton's steady-state eternal inflation, Carroll and Chen's spontaneous inflation, eternal "seed" universes, quantum bounces, the quantum-eternity line, and a 2024 model of inflation that is "geodesically complete for all time, including into the past" at the price of locally violating an energy condition.37,14,38,39,24,40 They are coherent. None has observational support, and several need special conditions at a boundary where the arrow of time starts: the place where explanation by earlier states stops.
The "from nothing" models (Vilenkin's tunnelling, Hartle and Hawking's no-boundary state) do have a beginning. But by their authors' own account they presuppose the laws of quantum mechanics. Vilenkin: "The theory of quantum creation is no more than a speculative hypothesis", and the laws "have some independent existence. What exactly this means, we don't know."13
So the honest summary is not "science has proven the universe began". It is: every attempt to avoid a beginning has so far failed or remains speculative, and our best classical theorem says expansion cannot be past-eternal. And the experts split. Vilenkin: "The answer to the question, 'Did the universe have a beginning?' is, 'It probably did.'"13 Carroll reports that Guth, his co-author, holds "that the universe probably didn't have a beginning, and is very likely eternal".24
All 16 proposals, with status and sourcestable · 16 rows
| Proposal | Claim | Status |
|---|---|---|
| Einstein static universe (1917) | Eternal, static, closed; a cosmological constant added to hold it still | Refuted Unstable; contradicted by expansion; Einstein abandoned it30 |
| Einstein's unpublished steady state (1931) | Constant density kept by "continuous formation of matter from empty space" | Abandoned The manuscript "contains a fundamental flaw"41 |
| Hoyle–Bondi–Gold steady state (1948) | Infinite age; matter continuously created | Refuted By radio-source counts, the microwave background (1965) and helium42,31 |
| Old oscillating universe (Tolman, 1930s) | Endless cycles | Refuted Entropy grows each cycle, so it cannot be past-eternal13 |
| Eternal inflation (Linde, Vilenkin, Guth) | Endless production of pocket universes | Begins Eternal to the future, "not eternal into the past"35 |
| Aguirre–Gratton steady-state inflation (2002–03) | Geodesically complete eternal inflation; the arrow of time reverses across a boundary | Speculative Consistent at the semiclassical level; critics read it as two universes with opposite arrows sharing a boundary37 |
| Carroll–Chen spontaneous inflation (2004) | Inflation from a de Sitter vacuum, time-symmetric on the largest scales | Speculative Relies on contested probability reasoning; untested14 |
| Cyclic and ekpyrotic (Steinhardt–Turok 2001; Ijjas–Steinhardt 2019) | Endless bangs and crunches | Begins The 2019 version grows each cycle, so BGV applies; "a cyclic universe cannot be past-eternal" (Vilenkin); shown "geodesically incomplete" in 202643,36,13,23 |
| Conformal cyclic cosmology (Penrose, 2010) | An endless sequence of "aeons" | Unconfirmed Claimed circles and "Hawking points" not reproduced;32,33,34 and the cyclic extension is argued to be past-incomplete22 |
| Emergent universe (Ellis–Maartens 2004; Graham et al. 2011) | An eternal static or oscillating seed, which then inflates | Doubtful Classically stable, but can tunnel to collapse, so "cannot have an eternal past";38,44,27,26 for a quantum-gravity seed, "All solutions are unstable with respect to collapse by quantum tunneling to zero size", though the collapsed state may tunnel back;45 the long tuning it needs "is unstable quantum mechanically".46 Its defenders reply that the collapse rate may depend on unknown high-energy physics. Even a stable classical seed does not remove the starting condition: it moves it to the infinite past. The cleanest escape left; needs positive curvature |
| Vilenkin, tunnelling "from nothing" (1982) | A closed universe nucleates from no space and no time | Speculative Has a beginning; presupposes quantum laws47,13 |
| Hartle–Hawking no-boundary (1983) | Time becomes space-like near the origin; no boundary. Hartle later presented such a state as a law in its own right, since prediction "requires both a Hamiltonian and a state"48 | Disputed Feldbrugge, Lehners and Turok report "a fundamental obstruction" to it and to the tunnelling proposal; replies continue49,50 |
| Krauss, A Universe from Nothing (2012) | Physics explains how a universe arises from "nothing" | Not nothing The "nothing" is a quantum vacuum with laws; Albert's review is the standard rebuttal51,52 |
| Loop quantum cosmology bounce (Ashtekar, Bojowald) | The Big Bang replaced by a bounce from a prior contracting phase | Speculative Can have zero average expansion, which evades BGV; the prior phase needs its own low-entropy explanation.39 If time's arrow runs the same way through the bounce, Wall's theorem applies;25 if it reverses, the bounce is where explanation by earlier states stops |
| Easson–Lesnefsky inflation (2024) | Inflation "smooth, nonsingular, and geodesically complete for all time, including into the past" | Speculative Needs a confined, controlled violation of the null energy condition; untested40 |
| A past that ends at a singularity | Spacetime simply stops at a singularity that is not part of it, so there is no first moment | Weak Logically clean, but it trusts classical general relativity to infinite curvature, which the theorem's own authors decline20,53 |
Carroll's "brute fact" view, that "the universe simply is, without ultimate cause or explanation", is a philosophical position, not a model.54
Does our history have a first state? Class by classtable · 6 rows · graded
"A first state" means a state of the world that no earlier state explains. This is what the explanatory argument below needs, and it is not the same as "time began". The grades are from a separate adversarial review of these models, with an advocate, a skeptic and an arbiter.
| Kind of history | First state? | The way out, and its price |
|---|---|---|
| Expanding on average (eternal inflation, growing cycles, Penrose's cycles) | Strong inference, if quantum gravity replaces the singularity with a state | A past that ends at a singularity (Weak) |
| A contracting past with one arrow of time | Strong, given the generalized second law25 | A phantom-energy "turnaround" cycle (Weak; a sketch by its authors' account) |
| A bounce where time's arrow reverses (Aguirre–Gratton) | Strong: the moment of lowest entropy is where explanation by earlier states stops | A direction of time not set by entropy (Weak to Contested) |
| An eternal "seed" (static or oscillating) | Weak to Contested escape | The cleanest physical escape; a classical seed only moves the starting condition to the infinite past |
| Carroll–Chen spontaneous inflation | Contested escape | Also needs a direction of time not set by entropy |
| The quantum-gravity era | Open | Unknown; it counts neither way, and every expanding history meets it at its edge |
Overall: a strong inference, not established. In the exceptions the argument is not refuted; it is silent. And a reversed-arrow history has a first state in this sense while being eternal in time, which is why "a first state" must never be quoted as "time began".
4. Who expected what
Most of the ancient world expected no beginning. Aristotle: "there never was a time when there was not motion, and never will be a time when there will not be motion".55 The Buddha, in the Pali canon: "Mendicants, this transmigration has no known beginning. No first point is found".56 Indian traditions more broadly taught cycles without a first cycle.
Twentieth-century science started there too. Einstein added a constant to his equations to keep the universe static and eternal; in 1929 he still held that "the [space-time] continuum is infinite in its timelike extent".31,30 Eddington, in 1928: "As a scientist I simply do not believe that the Universe began with a bang".31 Nernst: "To deny the infinite duration of time would be to betray the very foundations of science."13 Hoyle named the rival theory in a 1949 broadcast, "the hypothesis that all the matter of the universe was created in one big bang at a particular time in the remote past", and rejected it.31
The beginning won because of data (the microwave background, helium, radio counts), not preference. Two cautions keep this honest. Some theists never thought a beginning necessary: Aquinas held it "by faith alone".1 And the leading modern defender of a beginning draws no theological conclusion. Vilenkin: "my own view is that the theorem does not tell us anything about the existence of God."13
A timeline of resistance and replytable · 11 rows
| Who | When | What |
|---|---|---|
| Aristotle | 4th c. BC | Motion has no beginning and no end (Physics VIII.1)55 |
| The Buddha (Pali canon) | c. 5th–3rd c. BC | "this transmigration has no known beginning" (SN 15.1)56 |
| Thomas Aquinas | 1270s | "By faith alone do we hold, and by no demonstration can it be proved, that the world did not always exist"1 |
| Einstein | 1917, 1929 | Adds a cosmological constant for a static, eternal universe; in 1929 the continuum is still "infinite in its timelike extent". The later "biggest blunder" remark is reported second-hand; historians find the remark "highly compatible" with his cosmology of the time31,30 |
| Eddington | 1928, 1931 | "As a scientist I simply do not believe that the Universe began with a bang" (1928).31 In 1931, as Lemaître reports it, "the notion of a beginning of the present order of Nature is repugnant to him"57 |
| Lemaître, a Catholic priest | 1931 | "the beginning of the world happened a little before the beginning of space and time"57 |
| Walther Nernst | early 20th c. | A finite past would "betray the very foundations of science" (as quoted by Vilenkin)13 |
| Fred Hoyle | 1949 | Coins "big bang" for the rival theory and rejects it. Kragh argues the name was not meant as a sneer31 |
| Edward Milne | 1952 | "As to the first cause of the universe ... this is left for the reader to insert, but our picture is incomplete without Him." (as quoted by Vilenkin)13 |
| Penzias and Wilson | 1965 | Discover the microwave background; the steady state loses its footing5 |
| Borde, Guth, Vilenkin; Vilenkin | 2003; 2015 | The BGV theorem; Vilenkin: the theorem "does not tell us anything about the existence of God"20,13 |
5. What the Bible claims
In the beginning, God created the heavens and the earth.Genesis 1:1, WEB58
All things were made through him. Without him, nothing was made that has been made.John 1:3, WEB
By faith we understand that the universe has been framed by the word of God, so that what is seen has not been made out of things which are visible.Hebrews 11:3, WEB
The Hebrew Bible says God made everything and was there before it: "Before the mountains were born, before you had formed the earth and the world, even from everlasting to everlasting, you are God" (Psalm 90:2, WEB). "I am Yahweh, who makes all things" (Isaiah 44:24, WEB).
One honest complication. Genesis 1:1 has a grammatical rival. The Jewish Publication Society translates it "When God began to create heaven and earth— the earth being unformed and void", with the footnote "Others 'In the beginning God created.'"59 On that reading, the verse does not by itself assert an absolute beginning. Most translations, and the oldest Greek one, take the traditional reading. We treat the verse as contested and do not rest anything on it alone. Whether the Bible's picture matches cosmology is scored on the Genesis 1 page; here the point is narrower: the biblical tradition took the side of a made world while its great rivals took the side of an eternal one.
"In the beginning" or "When God began to create"?translation debate
The Hebrew word reshit ("beginning") almost everywhere else stands in a construct form, "the beginning of ...". Rashi, in the 11th century, used this to read the verse as "At the beginning of God's creating ...".60 The 1985 and 2006 JPS translations follow that line.59 Everett Fox notes that the phrase "has long been the focus of debate among grammarians", and that "heavens and earth" is "Probably a merism—an inclusive idiom meaning 'everything'".61
On the dependent reading, the formless earth and the deep of verse 2 could already be there when God begins. On the traditional reading (the Septuagint, the Masoretic accents and most older translations), verse 1 is a headline statement of absolute creation.62 Respectable scholars hold each view. The case for a biblical beginning does not depend on this verse: John 1:3, Hebrews 11:3 and Psalm 90:2 carry it whichever way Genesis 1:1 is read.
Where "creation from nothing" comes fromtexts · 2nd c. BC to 2nd c. AD
| Text | What it says (WEB) | Note |
|---|---|---|
| 2 Maccabees 7:28 (c. 2nd–1st c. BC) | "recognize that God made them not of things that were" | Often called the first explicit statement. Whether "not from existing things" means absolute nothing is disputed (May says not yet; Copan disagrees)63,64 |
| Wisdom 11:17 (same period) | "your all-powerful hand that created the world out of formless matter" | A counter-text: a Jewish work of the same era describes creation from formless matter |
| Romans 4:17 | God "calls the things that are not, as though they were" | Close to the language of creation from nothing |
| Hebrews 11:3 | "what is seen has not been made out of things which are visible" | Not quite "from nothing", but it excludes pre-existing visible matter |
| Tatian, Theophilus of Antioch, Irenaeus (c. 170–190) | (early Christian writers, not Scripture) | State creation from nothing explicitly, against the Platonic idea of eternal matter63 |
So, carefully: explicit, worked-out creation from nothing is clear by the late 2nd century AD and has roots in 2 Maccabees, Romans and Hebrews. It is not uniquely biblical (Zoroastrianism has a created world and a linear history, and Islam teaches creation), but it stood against the dominant Greek and Indian views.
The analysis
The Kalam argument, stated carefully
The best-known form, from William Lane Craig, as the Stanford Encyclopedia of Philosophy sets it out:65,66
- Everything that begins to exist has a cause of its existence.
- The universe began to exist.
- Therefore the universe has a cause of its existence.
- (A further argument.) Such a cause must be beyond space and time, enormously powerful and, Craig argues, personal.
Premise 2 has a philosophical defence (an actual infinite cannot exist or be built up step by step) and a scientific one (the Big Bang, the theorems, the second law). This page weighs only the scientific one. Premise 1 is metaphysics. Physics cannot establish it, and physicists such as Carroll and Vilenkin reject it for the universe as a whole (see Objections). So rather than treat premise 1 as certain or as false, the model below lets you set how likely a brute, uncaused beginning is.
What follows from a first state, and what doesn't
Stated with care, the step from a first state goes like this. Suppose our history has a state that no earlier state explains, and that it could have been otherwise. Grant a principle of sufficient reason for particular facts: such a state has some explanation other than itself. A later state cannot explain it, since explanation does not run backward in time. So it is either necessary, or explained by something that is not one of the world's states: a law that fixes the initial state, a necessary fact, or something beyond physics.
That is a valid argument from a principle, and its principle is contested: a naturalist can say the first state is simply a brute fact, at the price of being unable to say why our present states are not "first" too. It is also modest. Naturalists who hold that a law fixes the universe's initial state (the no-boundary proposal, Vilenkin's tunnelling law) already accept its conclusion. So it narrows naturalism's options; it does not refute naturalism, and it says nothing yet about a mind. Two stronger claims do not follow from it: that the cause is "timeless and spaceless", and that the beginning refutes the idea that physical effects have physical causes (it refutes only the extreme version in which even the first event must have an earlier physical cause, a thesis no naturalist needs).
The bigger argument, that the whole history and its laws are explained by something outside the physical order, is the argument from contingency. It does not need a beginning at all, it is graded contested, and it is not scored on this page.
A Bayesian version that needs no certain premise
A likelihood ratio (LR) asks: how much more expected is this evidence if hypothesis A is true than if B is true? An LR of 1 means the evidence does not discriminate; 2 means it is twice as expected under A. Following Miller's Bayesian formulation of the Kalam,67 we split the question in two.
D = the cosmological data (sections 1-3 above) B = an absolute beginning (L3) x = P(D | B) / P(D | no B) how strongly the data favour a beginning pT = P(B | theism) how strongly theism expects a beginning pN = P(B | naturalism) how strongly naturalism expects one LR = P(D | theism) / P(D | naturalism) = [ x*pT + (1 - pT) ] / [ x*pN + (1 - pN) ]
This assumes the data bear on theism and naturalism only through whether there was a beginning.
The top and bottom of that fraction are each a weighted average of x and 1. So whatever pT and pN are, the LR lies between 1/x and x. The beginning of the universe can never be stronger evidence for God than the physics is evidence for a beginning. Claims of "proof" are ruled out by the structure of the evidence, not just by caution.
The inputs, with reasons
- x, the data's support for a beginning: range 0.7–5, central 2. BGV and the failure so far of every past-eternal model push it above 1. The classical scope and live loopholes keep it modest. The theorem's own authors split ("probably did" vs "very likely eternal"), which is what an x of about 1–4 looks like. The low end, 0.7, allows Carroll's view that quantum eternity mildly favours no beginning.
- pT, how strongly theism expects a beginning: range 0.70–0.95, central 0.85. High for biblical theism (John 1:3, Hebrews 11:3, the creation-from-nothing tradition). Lowered by the Genesis 1:1 translation debate and by Aquinas's point that God could have made an eternal world.
- pN, how strongly naturalism expects a beginning: range 0.20–0.60, central 0.40. Naturalism has no law fixing the answer, so 0.5 is a neutral start. Pushed down because an uncaused first state strikes most people's causal intuitions as improbable, and because naturalists historically expected eternity. Pushed up because leading naturalistic cosmologies (tunnelling, no-boundary) predict a boundary of time. An eternal past has its own costs (the second law, BGV), so it is not near zero. The causal intuition pushes down only against a brute beginning: a naturalist with a law of the initial state is untouched by it (see above), which is why a very low pN is a high-end scenario, not the central one.
The result
Mainstream inputs give about 1.3; even Kalam-friendly ones stay in single digits
Likelihood ratio, theism over naturalism, on a log scale. Dots are single scenarios; bars are ranges.
Show the data
| Line of evidence | Low | Central | High |
|---|---|---|---|
| Roll-up (low, central, high) | 0.85 | 1.3 | 3.5 |
| Monte Carlo, 90% band | 0.9 | 1.23 | 1.88 |
| Carroll-leaning (x 0.7) | 0.85 | 0.85 | 0.85 |
| Agnostic physics (x 1) | 1 | 1 | 1 |
| Central (x 2) | 1.32 | 1.32 | 1.32 |
| Vilenkin-leaning (x 4) | 1.95 | 1.95 | 1.95 |
| Kalam-friendly (x 4, pN 0.05) | 3.35 | 3.35 | 3.35 |
| Maximal (x 10, pN 0.05) | 6.59 | 6.59 | 6.59 |
| No-boundary naturalism (pN 0.8) | 1.03 | 1.03 | 1.03 |
| 'First state' read as a beginning (x 3) | 1.5 | 1.5 | 1.5 |
| Law-of-the-state naturalism (x 3, pN 0.7) | 1.13 | 1.13 | 1.13 |
The beginning of the universe favours theism over naturalism by a likelihood ratio of about 1.2–1.3. Drawing the three inputs at random across their ranges 200,000 times gives a median of 1.23 and a 90% band of 0.90–1.88; 18% of draws fall below 1, meaning they slightly favour naturalism. The ratio reaches 3–7 only if you grant both that the physics strongly favours a beginning (x of 4 or more) and the Kalam's causal principle (pN near 0.05).
What moves it.
- Most of all, x, the physics. A result that settled the quantum era (a proof that a bounce is unavoidable, or a no-go theorem for past-eternal quantum cosmologies) would move the ratio more than any philosophical argument.
- Next, pN, the metaphysics of uncaused beginnings. This is where defenders and critics of the Kalam actually disagree, so we let you set it below.
- Least, pT. Any theism that expects a beginning more than naturalism does gives an LR above 1 whenever x is above 1.
All nine scenarios and the Monte Carlo outputtable · calculation
| Scenario | x | pT | pN | LR |
|---|---|---|---|---|
| Carroll-leaning (data mildly favour eternity) | 0.7 | 0.85 | 0.40 | 0.85 |
| Agnostic physics, neutral naturalism | 1.0 | 0.85 | 0.40 | 1.00 |
| Central | 2.0 | 0.85 | 0.40 | 1.32 |
| Vilenkin-leaning | 4.0 | 0.90 | 0.30 | 1.95 |
| Kalam-friendly (brute beginnings improbable under naturalism) | 4.0 | 0.95 | 0.05 | 3.35 |
| Maximal: strong data plus the causal principle | 10.0 | 0.95 | 0.05 | 6.59 |
| No-boundary naturalism (naturalism predicts a boundary too) | 2.0 | 0.85 | 0.80 | 1.03 |
| Sensitivity: the strong inference to a first state read as if it were about a beginning of time | 3.0 | 0.85 | 0.40 | 1.50 |
| Sensitivity: naturalism with a law of the initial state | 3.0 | 0.85 | 0.70 | 1.13 |
The two sensitivity rows were added when we re-checked this page against the newer physics (the amended theorem and the first-state grades). Both stay inside the roll-up range, so the inputs are unchanged.
x log-uniform 0.7-5; pT uniform 0.70-0.95; pN uniform 0.20-0.60; n = 200,000 5th percentile 0.90 median 1.23 95th percentile 1.88 maximum 2.60 fraction with LR < 1: 0.182
The roll-up range (0.85, 1.3, 3.5) is wider than this band on purpose: its high end is the Kalam-friendly scenario, which lies outside the Monte Carlo's pN range.
Try your own numbers
The data favour theism over naturalism by a factor of 1.32. It can never exceed 2.00, the physics' own support for a beginning.
Bars are on a log scale from 1/20 to 20; the middle is 1, no evidence either way. The full cumulative model, where this line combines with the others, is on the verdict page.
Objections
"BGV is classical; it says nothing about quantum gravity." (Carroll; Guth as Carroll reports him)24
Correct, and we say so. Two partial replies. The theorem needs no energy condition and no particular theory of gravity, only average expansion, so any quantum era must either not be expanding on average or not be a classical spacetime at all.20,13 And Vilenkin argues that the main quantum escape route, an eternal static seed, is unstable to quantum collapse.26
"Past-incomplete is not a beginning. Spacetime may continue through the boundary into an earlier phase." (Aguirre and Gratton; Lesnefsky, Easson and Davies; Geshnizjani, Ling and Quintin)37,28,29
Then the earlier phase must be contracting, static or non-classical, and each option has its own problem: entropy, instability, or a reversed arrow of time meeting ours at a boundary. Geshnizjani and colleagues themselves conclude that past-eternal inflation is "most likely physically singular, except in situations with very special initial conditions".29
"The first premise is false, or meaningless, at the level of fundamental physics." Carroll: "the notion of a 'cause' isn't part of an appropriate vocabulary to use for discussing fundamental physics".24 Vilenkin: "No cause is needed for the quantum creation of the universe."13
Causation is not a term in the equations, but scientists infer causes every day. The quantum events offered as uncaused, such as radioactive decay and tunnelling, happen inside a framework that already exists: a field, a law, a space of states. Vilenkin himself says the laws "have some independent existence".13 So "uncaused" there means "not deterministically caused", not "arising from no conditions at all".
"Causes come before their effects. With no time before the Big Bang, nothing could cause it." (Grünbaum, via the SEP: the singularity is "technically a non-event")53,65
Craig replies with simultaneous or timeless causation, and with a definition: something has a beginning if the time during which it has existed is finite.65,66
"A quantum vacuum is nothing, and universes come from it." (Krauss)51
A quantum vacuum is a state of quantum fields governed by laws. Vilenkin's "nothing" is narrower (no space, no time) but still presupposes quantum laws.13 Every quantum model of the origin (a vacuum transition, tunnelling, the no-boundary state) starts from a law, a space of possible states and a rule that fixes the state, and produces none of them; no dynamical law, the Wheeler–DeWitt equation of quantum gravity included, fixes the state by itself.48 The model-builders say so themselves. Gott and Li: "But quantum fluctuation of what? You have to have laws of physics and a potential etc."70 Philosophers widely accept this reply; Albert's review of Krauss is the standard statement.52
"If the past ends at a singularity, there is no first moment, so there is nothing to explain." (Grünbaum)53
Logically, yes. The theorem rules out an infinitely long past, not infinitely many moments: a past that runs back toward a singularity without reaching it has no first moment. But the escape trusts classical general relativity all the way to infinite density, which the theorem's own authors decline; they say "physics other than inflation" is needed at the boundary.20 So it is a weak escape. For the Kalam's own definition (a finite past) it still counts as a beginning.
"A law of nature could fix the starting state. Then nothing outside physics is needed." (Hartle; the no-boundary and tunnelling proposals)48
Granted, and we build it into the argument: a law of the initial state is one of the ways a first state can be explained (see what follows from a first state). That is exactly why this page does not claim the beginning points beyond physics. What the beginning does is narrow the options: a first state must be necessary, fixed by such a law, or explained from beyond physics. Whether the law itself needs explaining is the argument from contingency, which is contested and not scored here.
"The low-entropy start is just a law of initial conditions. It doesn't need a designer." (Albert and Loewer's "Past Hypothesis"; Penrose's Weyl curvature hypothesis)
Agreed, as far as the entropy data go. The argument that our universe is not a chance fluctuation out of an eternal equilibrium is sound and standard: in such a world, observers with memories like ours would almost always be fleeting fluctuations with false records. But that leaves three options: a law or boundary condition, a dynamics in which entropy has no maximum (a research programme), or a choice. The entropy data cannot tell a law from a Creator who aims at an ordered cosmos, because both predict it. The low-entropy start belongs to fine-tuning and adds nothing to this ratio.
"If the real argument is that the universe is contingent, why does the beginning matter at all?"
Fair. The question "why these laws and this history?" arises at every moment of a history, with or without a first moment, so the argument from contingency does not need a beginning. What a beginning adds is narrow: it removes one classic reply, that an endless chain of earlier states explains each state and so the whole.
"Things in the universe have causes; it does not follow that the universe has one." (Russell, in his 1948 debate with Copleston; the fallacy of composition)
The Kalam does not argue "the parts have causes, so the whole does". It argues "whatever begins has a cause, and the universe began": a general principle applied to one case.
Indeterminate events still have necessary conditions. On most interpretations what they lack is a sufficient cause, not any cause at all.
"Even granting a cause, nothing shows it is God, let alone the God of the Bible."
Fully granted. This page at most points to a cause that is not a physical event inside our spacetime. The step to a personal cause is a separate and weaker argument. The step to the God of the Bible belongs to Tier II and Tier III.
"Theists would have claimed confirmation either way."
Partly true: Aquinas said an eternal world was compatible with creation.1 But the Bible's own language (a beginning, all things made through the Word, God before the mountains) commits it more than generic theism does, and the historical record shows it was naturalist-leaning scientists who resisted a beginning on philosophical grounds. Hence pT is above pN, though not by an extreme margin.
What this shows, and what it doesn't
- Our observable universe has a finite past as a hot, dense, expanding system, about 13.8 billion years long. That is established by three independent lines.
- A history that keeps expanding on average over its past cannot be extended forever into the past (a theorem about models, amended in 2024).
- That our history has a first state, one no earlier state explains, is a strong inference, with named exceptions and the quantum era open.
- No past-eternal model has observational support; the older ones are refuted and the live ones are speculative.
- The Bible's side of the ancient question (a made world, not an eternal one) is the side the evidence has moved toward, against the stated preferences of many 20th-century scientists.
- As evidence for theism over naturalism, a beginning counts modestly: a likelihood ratio of about 1.3 (range 0.85–3.5), and never more than the physics' own support.
- That time itself, or all of physical reality, began. That is not established.
- That the beginning had a cause. That needs a philosophical premise physics cannot supply, and even then a law of the initial state would satisfy it.
- Who or what the cause is, or that it is personal, or that it is the God of the Bible.
- Creation from absolute nothing. No physics can reach that.
- That naturalism is refuted. It can hold an eternal past (and fight the theorems) or accept an uncaused start.
What we don't claim
- "The BGV theorem proves the universe, or time, began." It proves that classical spacetimes expanding on average are past-incomplete. Its own authors disagree about whether the universe began.
- "BGV assumes general relativity." It assumes no energy condition and no particular theory of gravity, only average expansion.
- "Hawking–Penrose and BGV are the same result." They rest on different assumptions: energy conditions and general relativity versus average expansion alone.
- "The microwave background, or general relativity, proves a beginning of time." They establish our hot, dense past (L1). The singularity theorems assume classical general relativity and energy conditions.
- "The second law proves the universe had a beginning." It undercuts naive eternal models only. Models in which entropy can grow without limit escape it.
- "Science has proven creation from nothing." No physics reaches absolute nothing; every "from nothing" model presupposes laws.
- "Physics shows the universe came from nothing, so no God is needed." For the same reason: a quantum vacuum is not nothing.
- "Every cosmologist now accepts that the universe began." Guth, Carroll, Aguirre, Steinhardt and Penrose do not, at least not in the absolute sense.
- "JWST has refuted the Big Bang", or "JWST confirmed it". Its early-galaxy puzzles concern how galaxies form; after contamination is handled they are "not in tension with modern cosmology". Neither headline is warranted.
- "Penrose calculated the odds as 1 in 10120." That number belongs to the cosmological-constant problem. Penrose's figure is 1 in 1010123, about entropy, for a closed universe, and it belongs to fine-tuning.
- "The odds of our starting state were 1 in 1010123." With a cosmological constant the comparable figure is about 1 in 1010122; today's state gives the same number, so it measures how far our patch is from equilibrium, not how special the start was; and whether it is a probability of the start at all is contested.
- "Our universe is observed to expand, so the theorem applies to it." The theorem's condition is about the average over a whole past, a property of a model, not an observation.
- "The theorem applies to every bouncing cosmology." Not to one whose earlier phase contracts.
- "The beginning refutes naturalism", or "proves a timeless, spaceless cause". It refutes only the extreme claim that even the first event has an earlier physical cause. "Timeless" and "spaceless" do not follow.
- "Every attempt to avoid a beginning has failed; that is the consensus." Several escapes are live though weak, and the confident verdict is Vilenkin's own, not a consensus.
- "Vilenkin concluded the universe needs a cause." He wrote the opposite: "No cause is needed for the quantum creation of the universe."
- "10122 bits of information appeared from nothing, violating the conservation of information." Conservation of information governs how an existing system evolves, not whether it exists; 10122 bits is the horizon's maximum capacity, not the early universe's content, which was low.
- "The low-entropy start proves an outside ordering principle." A law of initial conditions does the same job, and the entropy data cannot tell the two apart.
- "The theorem rules out every infinite past." It rules out an infinitely long one, not one with infinitely many moments that ends at a singularity.
- "The moment of lowest entropy is the beginning." On the leading accounts it is where explanation by earlier states stops. In some models time runs on beyond it.
- "Dark energy shows the universe will end", or "physics proves time must end". The evidence for changing dark energy is under 5σ and contested, and it says nothing about the beginning.
- "Holography shows our universe is a projection from a higher realm." The holographic principle is real, but it does not show that the universe depends on anything beyond physics.
- "Einstein called the cosmological constant his 'biggest blunder'", as a direct quote. It is reported second-hand, by Gamow and others, and is not in Einstein's writings. Say "reportedly".
- "Hoyle coined 'big bang' to mock the theory." Kragh argues the name was not meant as a sneer, though Hoyle rejected the theory.
- Eddington's "repugnant", without context. It was about "a beginning of the present order of Nature", and we have it only as Lemaître reports it.
- Jastrow's "band of theologians", Penzias's "five books of Moses", and the much-shared Hawking and Smoot quotes. We could not verify them against their original sources, so we do not use them.
- "Genesis 1:1 unambiguously teaches an absolute beginning." The reading "When God began to create" has serious support (Rashi; the JPS translations).
- "The Bible alone among religions teaches a beginning." Zoroastrianism has a created world and a linear history; Islam teaches creation. "Rare in the ancient world, against the dominant Greek and Indian views" is defensible; "unique" is not.
- "2 Maccabees 7:28 proves Jews held creation from absolute nothing." It is the earliest explicit "not from things that were"; what that meant is debated, and Wisdom 11:17 speaks of "formless matter".
Sources
- Thomas Aquinas, Summa Theologiae I, q. 46, a. 2. New Advent. Checked.
- Hubble, E. (1929). "A relation between distance and radial velocity among extra-galactic nebulae." PNAS 15(3): 168-173. Bibliographic.
- Planck Collaboration (2020). "Planck 2018 results. VI. Cosmological parameters." Astronomy & Astrophysics 641: A6. arXiv:1807.06209. Abstract checked; the age (13.8 billion years) is in the body.
- Fixsen, D. J. (2009). "The temperature of the cosmic microwave background." ApJ 707: 916-920. arXiv:0911.1955. Abstract checked.
- Penzias, A. A., Wilson, R. W. (1965). "A measurement of excess antenna temperature at 4080 Mc/s." ApJ 142: 419-421; Mather, J. C. et al. (1994). "Measurement of the cosmic microwave background spectrum by the COBE FIRAS instrument." ApJ 420: 439. Bibliographic.
- Fields, B. D., Olive, K. A., Yeh, T.-H., Young, C. (2020). "Big-Bang Nucleosynthesis after Planck." JCAP 03: 010. arXiv:1912.01132. Full text read for the dossier (eqs. 4, 6, 22-25); abstract checked.
- Cooke, R. J., Pettini, M., Steidel, C. C. (2018). "One percent determination of the primordial deuterium abundance." ApJ 855: 102. arXiv:1710.11129. Abstract checked.
- Labbé, I. et al. (2023). "A population of red candidate massive galaxies ~600 Myr after the Big Bang." Nature 616: 266. arXiv:2207.12446. Abstract checked.
- Boylan-Kolchin, M. (2023). "Stress testing ΛCDM with high-redshift galaxy candidates." Nature Astronomy 7: 731-735. arXiv:2208.01611. Abstract checked.
- Chworowsky, K. et al. (2024). "Evidence for a shallow evolution in the volume densities of massive galaxies at z = 4 to 8 from CEERS." AJ. arXiv:2311.14804. Abstract checked.
- Egan, C. A., Lineweaver, C. H. (2010). "A larger estimate of the entropy of the universe." ApJ 710: 1825-1834. arXiv:0909.3983. Full text read for the dossier (Tables 1-2).
- DESI Collaboration (2026). "DESI DR2 Results IV: Alcock-Paczyński measurements from the Lyman alpha forest and cosmological constraints." arXiv:2607.27410. Abstract checked.
- Vilenkin, A. (2015). "The Beginning of the Universe." Inference: International Review of Science 1(4). inference-review.com. Full text checked.
- Carroll, S. M., Chen, J. (2004). "Spontaneous inflation and the origin of the arrow of time." arXiv:hep-th/0410270. Abstract checked.
- Penrose, R. (2004). The Road to Reality. Jonathan Cape (ch. 27-28); also The Emperor's New Mind (1989). Bibliographic.
- Goldstein, S. (2001). "Boltzmann's approach to statistical mechanics." In J. Bricmont et al. (eds.), Chance in Physics. Springer. arXiv:cond-mat/0105242. Full text checked.
- Carroll, S. M. (2014). "In what sense is the early universe fine-tuned?" arXiv:1406.3057. Abstract checked.
- Hawking, S. W., Penrose, R. (1970). "The singularities of gravitational collapse and cosmology." Proc. R. Soc. A 314: 529-548. ADS. Bibliographic.
- Hawking, S. W. (1988). A Brief History of Time. Bantam. Bibliographic.
- Borde, A., Guth, A. H., Vilenkin, A. (2003). "Inflationary spacetimes are not past-complete." Phys. Rev. Lett. 90: 151301. arXiv:gr-qc/0110012. Abstract checked.
- Garcia-Saenz, S., Hua, J., Zhao, Y. (2024). "Geodesic completeness, cosmological bounces and inflation." Phys. Rev. D 110: L061304. arXiv:2405.04062. Abstract checked.
- Kinney, W. H., Maity, S., Sriramkumar, L. (2024). "The Borde-Guth-Vilenkin theorem in extended de Sitter spaces." Phys. Rev. D 109: 043519. arXiv:2307.10958. Abstract checked.
- Kinney, W. H. (2026). "Geodesic completeness in general cosmological scenarios." Proceedings of the Rencontres de Moriond 2026. arXiv:2604.20809. Abstract checked.
- Carroll, S. M. (2014, February 24). "Post-debate reflections" (on his debate with W. L. Craig). preposterousuniverse.com. Full text checked.
- Wall, A. C. (2013). "The generalized second law implies a quantum singularity theorem." Class. Quantum Grav. 30: 165003. arXiv:1010.5513. Abstract checked.
- Mithani, A., Vilenkin, A. (2012). "Did the universe have a beginning?" arXiv:1204.4658. Abstract checked.
- Mithani, A., Vilenkin, A. (2012). "Collapse of simple harmonic universe." JCAP. arXiv:1110.4096. Abstract checked.
- Lesnefsky, J. E., Easson, D. A., Davies, P. C. W. (2023). "On the past-completeness of inflationary spacetimes." Phys. Rev. D. arXiv:2207.00955. Abstract checked.
- Geshnizjani, G., Ling, E., Quintin, J. (2023). "On the initial singularity and extendibility of flat quasi-de Sitter spacetimes." JHEP 2023: 182. arXiv:2305.01676. Abstract checked.
- O'Raifeartaigh, C., Mitton, S. (2018). "Interrogating the legend of Einstein's 'biggest blunder'." Physics in Perspective 20: 318-341. arXiv:1804.06768. Abstract checked.
- Kragh, H. (2013). "What's in a name: history and meanings of the term 'Big Bang'." arXiv:1301.0219 (shorter version in Astronomy & Geophysics 54(2): 2.28). Full text checked.
- Gurzadyan, V. G., Penrose, R. (2010). "Concentric circles in WMAP data may provide evidence of violent pre-Big-Bang activity." arXiv:1011.3706. Abstract checked.
- Wehus, I. K., Eriksen, H. K. (2011). "A search for concentric circles in the 7-year WMAP temperature sky maps." ApJ 733: L29. arXiv:1012.1268. Abstract checked.
- Jow, D. L., Scott, D. (2020). "Re-evaluating evidence for Hawking points in the CMB." JCAP 2020(03): 021. arXiv:1909.09672. Abstract checked.
- Guth, A. H. (2007). "Eternal inflation and its implications." J. Phys. A 40: 6811. arXiv:hep-th/0702178. Abstract checked.
- Ijjas, A., Steinhardt, P. J. (2019). "A new kind of cyclic universe." Phys. Lett. B 795: 666-672. arXiv:1904.08022. Abstract checked.
- Aguirre, A., Gratton, S. (2002). "Steady-state eternal inflation." Phys. Rev. D 65: 083507, arXiv:astro-ph/0111191; (2003) "Inflation without a beginning: a null boundary proposal." Phys. Rev. D 67: 083515, arXiv:gr-qc/0301042. Abstracts checked.
- Ellis, G. F. R., Maartens, R. (2004). "The emergent universe: inflationary cosmology with no singularity." Class. Quantum Grav. 21: 223-232. arXiv:gr-qc/0211082. Abstract checked.
- Ashtekar, A., Singh, P. (2011). "Loop quantum cosmology: a status report." Class. Quantum Grav. 28: 213001. arXiv:1108.0893. A general review, cited for the bounce idea only.
- Easson, D. A., Lesnefsky, J. E. (2024). "Inflationary resolution of the initial singularity." arXiv:2402.13031. Abstract checked.
- O'Raifeartaigh, C., McCann, B., Nahm, W., Mitton, S. (2014). "Einstein's steady-state theory: an abandoned model of the cosmos." EPJ H 39: 353-367. arXiv:1402.0132. Abstract checked.
- Hoyle, F. (1948). "A new model for the expanding universe." MNRAS 108: 372. Bibliographic.
- Steinhardt, P. J., Turok, N. (2002). "A cyclic model of the universe." Science 296: 1436. arXiv:hep-th/0111030. Abstract read for the dossier.
- Graham, P. W., Horn, B., Kachru, S., Rajendran, S., Torroba, G. (2011). "A simple harmonic universe." arXiv:1109.0282. Abstract checked.
- Mithani, A., Vilenkin, A. (2014). "Instability of an emergent universe." JCAP 05: 006. arXiv:1403.0818. Abstract checked.
- Aguirre, A., Kehayias, J. (2013). "Quantum instability of the emergent universe." Phys. Rev. D 88: 103504. arXiv:1306.3232. Abstract checked.
- Vilenkin, A. (1982). "Creation of universes from nothing." Phys. Lett. B 117: 25. Bibliographic.
- Hartle, J. B. (2003). "The state of the universe." In G. W. Gibbons, E. P. S. Shellard, S. J. Rankin (eds.), The Future of Theoretical Physics and Cosmology. Cambridge University Press. arXiv:gr-qc/0209046. Abstract checked.
- Hartle, J. B., Hawking, S. W. (1983). "Wave function of the Universe." Phys. Rev. D 28: 2960. Bibliographic.
- Feldbrugge, J., Lehners, J.-L., Turok, N. (2017). "No smooth beginning for spacetime." Phys. Rev. Lett. 119: 171301, arXiv:1705.00192; (2018) "No rescue for the no boundary proposal." Phys. Rev. D 97: 023509, arXiv:1708.05104. Abstracts checked.
- Krauss, L. M. (2012). A Universe from Nothing. Free Press. Bibliographic.
- Albert, D. (2012, March 23). "On the origin of everything" (review of Krauss). New York Times Book Review. Bibliographic; not opened.
- Grünbaum, A. (1991). "Creation as a pseudo-explanation in current physical cosmology." Erkenntnis 35: 233; (1994) "Some comments on William Craig's 'Creation and Big Bang Cosmology'." Philosophia Naturalis 31: 225. Via the SEP entry.
- Carroll, S. M. (2018). "Why is there something, rather than nothing?" arXiv:1802.02231. Abstract checked.
- Aristotle, Physics VIII.1, tr. R. P. Hardie and R. K. Gaye. MIT Internet Classics Archive. Checked.
- Saṃyutta Nikāya 15.1 (Tiṇakaṭṭha Sutta), tr. Bhikkhu Sujato. SuttaCentral. Checked.
- Lemaître, G. (1931). "The beginning of the world from the point of view of quantum theory." Nature 127: 706. PDF. Full text checked.
- World English Bible (public domain), eBible.org. ebible.org/eng-web: Gen 1:1-2; Ps 90:2; Isa 44:24; John 1:3; Rom 4:17; Heb 11:3; 2 Macc 7:28; Wis 11:17. Checked.
- Tanakh (Jewish Publication Society, 1985) and The Contemporary Torah (JPS, 2006), Gen 1:1-2. Sefaria. Checked.
- Rashi on Genesis 1:1, tr. M. Rosenbaum and A. M. Silbermann (1929-34). Sefaria. Read for the dossier.
- Fox, E. (1995). The Five Books of Moses. Schocken. Note on Gen 1:1. Via Sefaria; read for the dossier.
- Wenham, G. J. (1987). Genesis 1-15 (Word Biblical Commentary 1). Word. Bibliographic.
- May, G. (1994). Creatio ex nihilo: The Doctrine of "Creation out of Nothing" in Early Christian Thought, tr. A. S. Worrall. T&T Clark. Bibliographic.
- Copan, P. (1996). "Is creatio ex nihilo a post-biblical invention? An examination of Gerhard May's proposal." Trinity Journal 17: 77-93. PDF. Bibliographic.
- Reichenbach, B. "Cosmological Argument." Stanford Encyclopedia of Philosophy. plato.stanford.edu. Read for the dossier.
- Craig, W. L., Sinclair, J. D. (2009). "The kalam cosmological argument." In W. L. Craig and J. P. Moreland (eds.), The Blackwell Companion to Natural Theology, 101-201. Wiley-Blackwell. Bibliographic.
- Miller, C. (2014). "A Bayesian formulation of the kalam cosmological argument." Religious Studies 50: 521. Abstract read for the dossier.
- Oppy, G. (2006). Arguing about Gods. Cambridge University Press. Bibliographic.
- Morriston, W. (2000). "Must the beginning of the universe have a personal cause?" Faith and Philosophy 17: 149. Bibliographic.
- Gott, J. R., Li, L.-X. (1998). "Can the universe create itself?" Phys. Rev. D 58: 023501. arXiv:astro-ph/9712344. Full text checked.
- Craig, W. L., Smith, Q. (1993). Theism, Atheism, and Big Bang Cosmology. Oxford University Press. Bibliographic.
In the unified argument
This line of evidence supports the hypothesis by a likelihood ratio of about 1.3: a Creator vs naturalism. Only an absolute beginning is scored, not the hot Big Bang itself, and this ratio can never exceed the physics' own support for a beginning. In the model it separates a Mind from naturalism only (deism, Judaism, Islam and Christianity alike; other traditions at half weight), not one faith from another. The low-entropy start is discussed under fine-tuning but added to no ratio, 'Genesis predicted a beginning' is scored under Genesis 1, and the argument from contingency, which does not need a beginning, is not scored here.