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Cosmology

For other uses, seeCosmology (disambiguation).Not to be confused withCosmetology.

Cosmology (fromAncient Greekκόσμος (cosmos) 'the universe, the world' andλογία (logia) 'study of') is a branch ofphysics andmetaphysics dealing with thenature of theuniverse, thecosmos. The termcosmology was first used in English in 1656 inThomas Blount'sGlossographia,[2] and in 1731 taken up in Latin byGerman philosopherChristian Wolff inCosmologia Generalis.[3]Religious or mythological cosmology is a body of beliefs based onmythological,religious, andesoteric literature and traditions ofcreation myths andeschatology. In the science ofastronomy, cosmology is concerned with the study of thechronology of the universe.

TheHubble eXtreme Deep Field (XDF) was completed in September 2012 and shows the farthestgalaxies ever photographed at that time. Except for the few stars in the foreground (which are bright and easily recognizable because only they havediffraction spikes), every speck of light in the composite photo is an individual galaxy, some of them as old as 13.2 billion years; the observable universe is estimated to contain more than 2 trillion galaxies.[1]

Physical cosmology is the study of theobservable universe's origin, its large-scale structures and dynamics, and theultimate fate of the universe, including thelaws of science that govern these areas.[4] It is investigated by scientists, includingastronomers andphysicists, as well asphilosophers, such asmetaphysicians,philosophers of physics, andphilosophers of space and time. Because of this shared scope withphilosophy,theories in physical cosmology may include bothscientific and non-scientific propositions and may depend upon assumptions that cannot betested. Physical cosmology is a sub-branch of astronomy that is concerned with the universe as a whole. Modern physical cosmology is dominated by theBig Bang Theory which attempts to bring togetherobservational astronomy andparticle physics;[5][6] more specifically, a standard parameterization of the Big Bang withdark matter anddark energy, known as theLambda-CDM model.

Theoretical astrophysicistDavid N. Spergel has described cosmology as a "historical science" because "when we look out in space, we look back in time" due to the finite nature of thespeed of light.[7]

Disciplines

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Physics andastrophysics have played central roles in shaping our understanding of the universe through scientific observation and experiment.Physical cosmology was shaped through both mathematics and observation in an analysis of the whole universe. The universe is generally understood to have begun with theBig Bang, followed almost instantaneously bycosmic inflation, anexpansion of space from which the universe is thought to have emerged13.799 ± 0.021billion years ago.[8]Cosmogony studies the origin of the universe, andcosmography maps the features of the universe.

InDiderot'sEncyclopédie, cosmology is broken down into uranology (the science of the heavens), aerology (the science of the air), geology (the science of the continents), and hydrology (the science of waters).[9]

Metaphysical cosmology has also been described as the placing of humans in the universe in relationship to all other entities. This is exemplified byMarcus Aurelius's observation that a man's place in that relationship: "He who does not know what the world is does not know where he is, and he who does not know for what purpose the world exists, does not know who he is, nor what the world is."[10]

Discoveries

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Physical cosmology

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Main article:Physical cosmology

Physical cosmology is the branch of physics and astrophysics that deals with the study of the physical origins and evolution of the universe. It also includes the study of the nature of the universe on a large scale. In its earliest form, it was what is now known as "celestial mechanics," the study of theheavens. Greek philosophersAristarchus of Samos,Aristotle, andPtolemy proposed different cosmological theories. ThegeocentricPtolemaic system was the prevailing theory until the 16th century whenNicolaus Copernicus, and subsequentlyJohannes Kepler andGalileo Galilei, proposed aheliocentric system. This is one of the most famous examples ofepistemological rupture in physical cosmology.

Isaac Newton'sPrincipia Mathematica, published in 1687, was the first description of thelaw of universal gravitation. It provided a physical mechanism forKepler's laws and also allowed the anomalies in previous systems, caused by gravitational interaction between the planets, to be resolved. A fundamental difference between Newton's cosmology and those preceding it was theCopernican principle—that the bodies on Earth obey the samephysical laws as all celestial bodies. This was a crucial philosophical advance in physical cosmology.

Modern scientific cosmology is widely considered to have begun in 1917 withAlbert Einstein's publication of his final modification ofgeneral relativity in the paper "Cosmological Considerations of the General Theory of Relativity"[11] (although this paper was not widely available outside of Germany until the end ofWorld War I). General relativity promptedcosmogonists such asWillem de Sitter,Karl Schwarzschild, andArthur Eddington to explore its astronomical ramifications, which enhanced the ability ofastronomers to study very distant objects. Physicists began changing the assumption that the universe was static and unchanging. In 1922,Alexander Friedmann introduced the idea of an expanding universe that contained moving matter.

In parallel to this dynamic approach to cosmology, one long-standing debate about the structure of the cosmos was coming to a climax – theGreat Debate (1917 to 1922) – with early cosmologists such asHeber Curtis andErnst Öpik determining that somenebulae seen in telescopes were separate galaxies far distant from our own.[12] While Heber Curtis argued for the idea that spiral nebulae were star systems in their own right as island universes, Mount Wilson astronomerHarlow Shapley championed the model of a cosmos made up of theMilky Waystar system only. This difference of ideas came to a climax with the organization of theGreat Debate on 26 April 1920 at the meeting of the U.S.National Academy of Sciences inWashington, D.C. The debate was resolved whenEdwin Hubble detectedCepheid Variables in theAndromeda Galaxy in 1923 and 1924.[13][14] Their distance established spiral nebulae well beyond the edge of the Milky Way.

Subsequent modelling of the universe explored the possibility that thecosmological constant, introduced by Einstein in his 1917 paper, may result in anexpanding universe, depending on its value. Thus theBig Bang model was proposed by theBelgian priestGeorges Lemaître in 1927[15] which was subsequently corroborated byEdwin Hubble's discovery of theredshift in 1929[16] and later by the discovery of thecosmic microwave background radiation byArno Penzias andRobert Woodrow Wilson in 1964.[17] These findings were a first step to rule out some of manyalternative cosmologies.

Since around 1990, several dramatic advances inobservational cosmology have transformed cosmology from a largely speculative science into a predictive science with precise agreement between theory and observation. These advances include observations of the microwave background from theCOBE,[18]WMAP[19] andPlanck satellites,[20] large new galaxyredshift surveys including2dfGRS[21] andSDSS,[22] and observations of distantsupernovae andgravitational lensing. These observations matched the predictions of thecosmic inflation theory, a modifiedBig Bang theory, and the specific version known as theLambda-CDM model. This has led many to refer to modern times as the "golden age of cosmology".[23]

In 2014, the BICEP2 collaboration claimed that they had detected the imprint ofgravitational waves in thecosmic microwave background. However, this result was later found to be spurious: the supposed evidence of gravitational waves was in fact due to interstellar dust.[24][25]

On 1 December 2014, at thePlanck 2014 meeting inFerrara,Italy, astronomers reported that theuniverse is13.8 billion years old and composed of 4.9%atomic matter, 26.6%dark matter and 68.5%dark energy.[26]

Religious or mythological cosmology

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Religious or mythological cosmology is a body of beliefs based onmythological,religious, andesoteric literature and traditions ofcreation andeschatology. Creation myths are found in most religions, and are typically split into five different classifications, based on a system created byMircea Eliade and his colleague Charles Long.

  • Types of Creation Myths based on similar motifs:
    • Creationex nihilo in which the creation is through the thought, word, dream or bodily secretions of a divine being.
    • Earth diver creation in which a diver, usually a bird or amphibian sent by a creator, plunges to the seabed through aprimordial ocean to bring up sand or mud which develops into a terrestrial world.
    • Emergence myths in which progenitors pass through a series of worlds and metamorphoses until reaching the present world.
    • Creation by the dismemberment of a primordial being.
    • Creation by the splitting or ordering of a primordial unity such as the cracking of acosmic egg or a bringing order fromchaos.[27]

Philosophy

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Representation of theobservable universe on alogarithmic scale. Distance from the Sun increases from center to edge. Planets and other celestial bodies were enlarged to appreciate their shapes.

Cosmology deals with the world as the totality of space, time and all phenomena. Historically, it has had quite a broad scope, and in many cases was found in religion.[28] Some questions about the Universe are beyond the scope of scientific inquiry but may still be interrogated through appeals to other philosophical approaches likedialectics. Some questions that are included in extra-scientific endeavors may include:[29][30]

  • What is the origin of the universe? What is its first cause (if any)? Is its existence necessary? (seemonism,pantheism,emanationism andcreationism)
  • What are the ultimate material components of the universe? (seemechanism,dynamism,hylomorphism,atomism)
  • What is the ultimate reason (if any) for the existence of the universe? Does the cosmos have a purpose? (seeteleology)
  • Does the existence of consciousness have a role in the existence of reality? How do we know what we know about the totality of the cosmos? Does cosmological reasoning reveal metaphysical truths? (seeepistemology)

Charles Kahn, a historian of philosophy, attributed the origins of ancient Greek cosmology toAnaximander.[31]

Historical cosmologies

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NameAuthor and dateClassificationRemarks
Hindu cosmologyRigveda (c. 1700–1100BCE)Cyclical or oscillating, Infinite in timePrimal matter remains manifest for 311.04 trillion years andunmanifest for an equal length of time. The universe remains manifest for4.32 billion years andunmanifest for an equal length of time. Innumerable universes exist simultaneously. These cycles have and will last forever, driven by desires.
Zoroastrian CosmologyAvesta (c. 1500–600 BCE)Dualistic CosmologyAccording to Zoroastrian Cosmology, the universe is the manifestation of perpetual conflict between Existence and non-existence, Good and evil and light and darkness. the universe will remain in this state for 12000 years; at the time of resurrection, the two elements will be separated again.
Jain cosmologyJain Agamas (written around 500CE as per the teachings ofMahavira 599–527 BCE)Cyclical or oscillating, eternal and finiteJain cosmology considers theloka, or universe, as an uncreated entity, existing since infinity, the shape of the universe as similar to a man standing with legs apart and arm resting on his waist. This Universe, according toJainism, is broad at the top, narrow at the middle and once again becomes broad at the bottom.
Babylonian cosmologyBabylonian literature (c. 2300–500 BCE)Flat Earth floating in infinite "waters of chaos"The Earth and theHeavens form a unit within infinite "waters of chaos"; the Earth is flat and circular, and a solid dome (the "firmament") keeps out the outer "chaos"-ocean.
Eleatic cosmologyParmenides (c. 515 BCE)Finite and spherical in extentThe Universe is unchanging, uniform, perfect, necessary, timeless, and neither generated nor perishable. Void is impossible. Plurality and change are products of epistemic ignorance derived from sense experience. Temporal and spatial limits are arbitrary and relative to the Parmenidean whole.
Samkhya Cosmic EvolutionKapila (6th century BCE), pupilAsuriPrakriti (Matter) and Purusha (Consiouness) RelationPrakriti (Matter) is the source of the world of becoming. It is pure potentiality that evolves itself successively into twenty four tattvas or principles. The evolution itself is possible becausePrakriti is always in a state of tension among its constituent strands known asgunas (Sattva (lightness or purity),Rajas (passion or activity), andTamas (inertia or heaviness)). The cause and effect theory of Sankhya is calledSatkaarya-vaada (theory of existent causes), and holds thatnothing can really be created from or destroyed into nothingness—all evolution is simply the transformation of primal Nature from one form to another.[citation needed]
Biblical cosmologyGenesis creation narrativeEarth floating in infinite "waters of chaos"The Earth and theHeavens form a unit within infinite "waters of chaos"; the "firmament" keeps out the outer "chaos"-ocean.
Anaximander's modelAnaximander (c. 560 BCE)Geocentric, cylindrical Earth, infinite in extent, finite time; first purely mechanical modelThe Earth floats very still in the centre of the infinite, not supported by anything.[32] At the origin, after the separation of hot and cold, a ball of flame appeared that surrounded Earth like bark on a tree. This ball broke apart to form the rest of the Universe. It resembled a system of hollow concentric wheels, filled with fire, with the rims pierced by holes like those of a flute; no heavenly bodies as such, only light through the holes. Three wheels, in order outwards from Earth: stars (includingplanets), Moon and a large Sun.[33]
Atomist universeAnaxagoras (500–428 BCE) and laterEpicurusInfinite in extentThe universe contains only two things: an infinite number of tiny seeds (atoms) and the void of infinite extent. All atoms are made of the same substance, but differ in size and shape. Objects are formed from atom aggregations and decay back into atoms. IncorporatesLeucippus' principle ofcausality: "nothing happens at random; everything happens out of reason and necessity". The universe was not ruled bygods.[citation needed]
Pythagorean universePhilolaus (d. 390 BCE)Existence of a "Central Fire" at the center of the Universe.At the center of the Universe is a central fire, around which the Earth, Sun, Moon andplanets revolve uniformly. The Sun revolves around the central fire once a year, the stars are immobile. The Earth in its motion maintains the same hidden face towards the central fire, hence it is never seen. First known non-geocentric model of the Universe.[34]
De MundoPseudo-Aristotle (d. 250 BCE or between 350 and 200 BCE)The Universe is a system made up of heaven and Earth and the elements which are contained in them.There are "five elements, situated in spheres in five regions, the less being in each case surrounded by the greater – namely, earth surrounded by water, water by air, air by fire, and fire by ether – make up the whole Universe."[35]
Stoic universeStoics (300 BCE – 200 CE)Island universeThecosmos is finite and surrounded by an infinite void. It is in a state of flux, and pulsates in size and undergoes periodic upheavals and conflagrations.
Platonic universePlato (c. 360 BCE)Geocentric, complexcosmogony, finite extent, implied finite time, cyclicalStatic Earth at center, surrounded by heavenly bodies which move in perfectcircles, arranged by the will of theDemiurge[36] in order: Moon, Sun, planets andfixed stars.[37][38] Complex motions repeat every'perfect' year.[39]
Eudoxus' modelEudoxus of Cnidus (c. 340 BCE) and laterCallippusGeocentric, first geometric-mathematical modelThe heavenly bodies move as if attached to a number of Earth-centeredconcentrical, invisible spheres, each of them rotating around its own and different axis and at different paces.[40] There are twenty-seven homocentric spheres with each sphere explaining a type of observable motion for each celestial object. Eudoxus emphasised that this is a purely mathematical construct of the model in the sense that the spheres of each celestial body do not exist, it just shows the possible positions of the bodies.[41]
Aristotelian universeAristotle (384–322 BCE)Geocentric (based on Eudoxus' model), static, steady state, finite extent, infinite timeStatic and spherical Earth is surrounded by 43 to 55concentriccelestial spheres, which are material and crystalline.[42] Universe exists unchanged throughout eternity. Contains a fifth element, calledaether, that was added to the fourclassical elements.[43]
Aristarchean universeAristarchus (c. 280 BCE)HeliocentricEarth rotates daily on its axis and revolves annually about the Sun in a circular orbit. Sphere of fixed stars is centered about the Sun.[44]
Ptolemaic modelPtolemy (2nd century CE)Geocentric (based on Aristotelian universe)Universe orbits around a stationary Earth. Planets move in circularepicycles, each having a center that moved in a larger circular orbit (called an eccentric or a deferent) around a center-point near Earth. The use ofequants added another level of complexity and allowed astronomers to predict the positions of the planets. The most successful universe model of all time, using the criterion of longevity. TheAlmagest (the Great System).
Capella's modelMartianus Capella (c. 420)Geocentric and HeliocentricThe Earth is at rest in the center of the universe and circled by the Moon, the Sun, three planets and the stars, whileMercury andVenus circle the Sun.[45]
Aryabhatan modelAryabhata (499)Geocentric or HeliocentricTheEarth rotates and the planets move inelliptical orbits around either the Earth or Sun; uncertain whether the model is geocentric or heliocentric due to planetary orbits given with respect to both the Earth and Sun.
Quranic cosmologyQuran (610–632 CE)Flat-earthThe universe consists of stacked flat layers, including seven levels of heaven and in some interpretations seven levels of earth (including hell)
Medieval universeMedieval philosophers (500–1200)Finite in timeA universe that is finite in time and has a beginning is proposed by theChristian philosopherJohn Philoponus, who argues against the ancient Greek notion of an infinite past. Logical arguments supporting a finite universe are developed by theearly Muslim philosopherAl-Kindi, theJewish philosopherSaadia Gaon, and theMuslim theologianAl-Ghazali.
Non-Parallel MultiverseBhagvata Puran (800–1000)Multiverse, Non ParallelInnumerable universes is comparable to themultiverse theory, except nonparallel where each universe is different and individualjiva-atmas (embodied souls) exist in exactly one universe at a time. All universes manifest from the same matter, and so they all follow parallel time cycles, manifesting and unmanifesting at the same time.[46]
Multiversal cosmologyFakhr al-Din al-Razi (1149–1209)Multiverse, multiple worlds and universesThere exists an infinite outer space beyond the known world, and God has the power to fill the vacuum with an infinite number of universes.
Maragha modelsMaragha school (1259–1528)GeocentricVarious modifications to Ptolemaic model and Aristotelian universe, including rejection ofequant andeccentrics atMaragheh observatory, and introduction ofTusi-couple byAl-Tusi. Alternative models later proposed, including the first accuratelunar model byIbn al-Shatir, a model rejecting stationary Earth in favour ofEarth's rotation byAli Kuşçu, and planetary model incorporating "circularinertia" byAl-Birjandi.
Nilakanthan modelNilakantha Somayaji (1444–1544)Geocentric and heliocentricA universe in which the planets orbit the Sun, which orbits the Earth; similar to the laterTychonic system.
Copernican universeNicolaus Copernicus (1473–1543)Heliocentric with circular planetary orbits, finite extentFirst described inDe revolutionibus orbium coelestium. The Sun is in the center of the universe, planets including Earth orbit the Sun, but the Moon orbits the Earth. The universe is limited by the sphere of thefixed stars.
Tychonic systemTycho Brahe (1546–1601)Geocentric and HeliocentricA universe in which the planets orbit the Sun and the Sun orbits the Earth, similar to the earlierNilakanthan model.
Bruno's cosmologyGiordano Bruno (1548–1600)Infinite extent, infinite time, homogeneous, isotropic, non-hierarchicalRejects the idea of a hierarchical universe. Earth and Sun have no special properties in comparison with the other heavenly bodies. The void between the stars is filled withaether, and matter is composed of the samefour elements (water, earth, fire, and air), and is atomistic, animistic and intelligent.
De MagneteWilliam Gilbert (1544–1603)Heliocentric, indefinitely extendedCopernican heliocentrism, but he rejects the idea of a limitingsphere of the fixed stars for which no proof has been offered.[47]
KeplerianJohannes Kepler (1571–1630)Heliocentric with elliptical planetary orbitsKepler's discoveries, marrying mathematics and physics, provided the foundation for the present conception of theSolar System, but distant stars were still seen as objects in a thin, fixed celestial sphere.
Static NewtonianIsaac Newton (1642–1727)Static (evolving), steady state, infiniteEvery particle in the universe attracts every other particle. Matter on the large scale is uniformly distributed. Gravitationally balanced but unstable.
Cartesian Vortex universeRené Descartes 17th centuryStatic (evolving), steady state,infiniteSystem of huge swirling whirlpools of aethereal or fine matter produces gravitational effects. But his vacuum was not empty; all space was filled with matter.
Hierarchical universeImmanuel Kant,Johann Lambert 18th centuryStatic (evolving), steady state, infiniteMatter is clustered on ever larger scales of hierarchy. Matter is endlessly recycled.
Einstein Universe with a cosmological constantAlbert Einstein 1917Static (nominally). Bounded (finite)"Matter without motion". Contains uniformly distributed matter. Uniformly curved spherical space; based onRiemann's hypersphere. Curvature is set equal to Λ. In effect Λ is equivalent to a repulsive force which counteracts gravity. Unstable.
De Sitter universeWillem de Sitter 1917Expandingflat space.

Steady state. Λ > 0

"Motion without matter." Only apparently static. Based on Einstein'sgeneral relativity. Space expands with constantacceleration.Scale factor increases exponentially (constantinflation).
MacMillan universeWilliam Duncan MacMillan 1920sStatic and steady stateNew matter is created fromradiation; starlight perpetually recycled into new matter particles.
Friedmann universe, spherical spaceAlexander Friedmann 1922Spherical expanding space.k = +1 ; no ΛPositive curvature. Curvature constantk = +1

Expands thenrecollapses.Spatially closed (finite).

Friedmann universe, hyperbolic spaceAlexander Friedmann 1924Hyperbolic expanding space.k = −1 ; no ΛNegative curvature. Said to be infinite (but ambiguous). Unbounded. Expands forever.
Dirac large numbers hypothesisPaul Dirac 1930sExpandingDemands a large variation inG, which decreases with time. Gravity weakens as universe evolves.
Friedmann zero-curvatureEinstein and De Sitter 1932Expanding flat space

k = 0 ; Λ = 0 Critical density

Curvature constantk = 0. Said to be infinite (but ambiguous). "Unbounded cosmos of limited extent". Expands forever. "Simplest" of all known universes. Named after but not considered by Friedmann. Has adeceleration termq = 1/2, which means that its expansion rate slows down.
The originalBig Bang (Friedmann-Lemaître)Georges Lemaître 1927–1929Expansion

Λ > 0 ; Λ > |Gravity|

Λ is positive and has a magnitude greater than gravity. Universe has initial high-density state ("primeval atom"). Followed by a two-stage expansion. Λ is used to destabilize the universe. (Lemaître is considered the father of the Big Bang model.)
Oscillating universe (Friedmann-Einstein)Favored byFriedmann 1920sExpanding and contracting in cyclesTime is endless and beginningless; thus avoids the beginning-of-time paradox. Perpetual cycles of Big Bang followed by Big Crunch. (Einstein's first choice after he rejected his 1917 model.)
Eddington universeArthur Eddington 1930First static then expandsStatic Einstein 1917 universe with its instability disturbed into expansion mode; with relentless matter dilution becomes a De Sitter universe. Λ dominates gravity.
Milne universe of kinematic relativityEdward Milne 1933, 1935;

William H. McCrea 1930s

Kinematic expansion without space expansionRejects general relativity and the expanding space paradigm. Gravity not included as initial assumption. Obeys cosmological principle andspecial relativity; consists of a finite spherical cloud of particles (or galaxies) that expands within an infinite and otherwise empty flat space. It has a center and a cosmic edge (surface of the particle cloud) that expands at light speed. Explanation of gravity was elaborate and unconvincing.
Friedmann–Lemaître–Robertson–Walker class of modelsHoward Robertson,Arthur Walker 1935Uniformly expandingClass of universes that are homogeneous and isotropic. Spacetime separates into uniformly curved space and cosmic time common to all co-moving observers. The formulation system is now known as the FLRW or Robertson–Walker metrics of cosmic time and curved space.
Steady-stateHermann Bondi,Thomas Gold 1948Expanding, steady state, infiniteMatter creation rate maintains constant density. Continuous creation out of nothing from nowhere. Exponential expansion. Deceleration termq = −1.
Steady-stateFred Hoyle 1948Expanding, steady state; but unstableMatter creation rate maintains constant density. But since matter creation rate must be exactly balanced with the space expansion rate the system is unstable.
AmbiplasmaHannes Alfvén 1965Oskar KleinCellular universe, expanding by means of matter–antimatter annihilationBased on the concept ofplasma cosmology. The universe is viewed as "meta-galaxies" divided bydouble layers and thus a bubble-like nature. Other universes are formed from other bubbles. Ongoing cosmic matter-antimatterannihilations keep the bubbles separated and moving apart preventing them from interacting.
Brans–Dicke theoryCarl H. Brans,Robert H. DickeExpandingBased onMach's principle.G varies with time as universe expands. "But nobody is quite sure what Mach's principle actually means."[citation needed]
Cosmic inflationAlan Guth 1980Big Bang modified to solvehorizon andflatness problemsBased on the concept of hot inflation. The universe is viewed as a multiple quantum flux – hence its bubble-like nature. Other universes are formed from other bubbles. Ongoing cosmic expansion kept the bubbles separated and moving apart.
Eternal inflation (a multiple universe model)Andreï Linde 1983Big Bang withcosmic inflationMultiverse based on the concept of cold inflation, in which inflationary events occur at random each with independent initial conditions; some expand into bubble universes supposedly like the entire cosmos. Bubbles nucleate in aspacetime foam.
Cyclic modelPaul Steinhardt;Neil Turok 2002Expanding and contracting in cycles;M-theoryTwo parallelorbifold planes orM-branes collide periodically in a higher-dimensional space. Withquintessence ordark energy.
Cyclic modelLauris Baum;Paul Frampton 2007Solution ofTolman's entropy problemPhantom dark energy fragments universe into large number of disconnected patches. The observable patch contracts containing only dark energy with zeroentropy.

Table notes: the term "static" simply means not expanding and not contracting. SymbolG represents Newton'sgravitational constant; Λ (Lambda) is thecosmological constant.

See also

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References

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  1. ^Hille, Karl, ed. (13 October 2016)."Hubble Reveals Observable Universe Contains 10 Times More Galaxies Than Previously Thought".NASA. Retrieved17 October 2016.
  2. ^Hetherington, Norriss S. (2014).Encyclopedia of Cosmology (Routledge Revivals): Historical, Philosophical, and Scientific Foundations of Modern Cosmology. Routledge. p. 116.ISBN 978-1-317-67766-6.
  3. ^Luminet, Jean-Pierre (2008).The Wraparound Universe. CRC Press. p. 170.ISBN 978-1-4398-6496-8.Extract of page 170.
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  20. ^"Computer Graphics Achievement Award".ACM SIGGRAPH 2018 Awards. SIGGRAPH '18. Vancouver, British Columbia, Canada: Association for Computing Machinery. 12 August 2018. p. 1.doi:10.1145/3225151.3232529.ISBN 978-1-4503-5830-9.S2CID 51979217.
  21. ^Science, American Association for the Advancement of (15 June 2007)."NETWATCH: Botany's Wayback Machine".Science.316 (5831): 1547.doi:10.1126/science.316.5831.1547d.ISSN 0036-8075.S2CID 220096361.
  22. ^Paraficz, D.; Hjorth, J.; Elíasdóttir, Á (1 May 2009)."Results of optical monitoring of 5 SDSS double QSOs with the Nordic Optical Telescope".Astronomy & Astrophysics.499 (2):395–408.arXiv:0903.1027.Bibcode:2009A&A...499..395P.doi:10.1051/0004-6361/200811387.ISSN 0004-6361.
  23. ^Alan Guth is reported to have made this very claim in anEdge Foundation interview.EDGE,Archived 11 April 2016 at theWayback Machine.
  24. ^Sample, Ian (4 June 2014)."Gravitational waves turn to dust after claims of flawed analysis".the Guardian.
  25. ^Cowen, Ron (30 January 2015). "Gravitational waves discovery now officially dead".Nature.doi:10.1038/nature.2015.16830.S2CID 124938210.
  26. ^Dennis Overbye (1 December 2014)."New Images Refine View of Infant Universe".The New York Times. Retrieved2 December 2014.
  27. ^Leonard & McClure 2004, pp. 32–33.
  28. ^Crouch, C. L. (8 February 2010)."Genesis 1:26-7 As a statement of humanity's divine parentage".The Journal of Theological Studies.61 (1):1–15.doi:10.1093/jts/flp185.
  29. ^"BICEP2 2014 Results Release".National Science Foundation. 17 March 2014. Retrieved18 March 2014.
  30. ^"Publications – Cosmos".www.cosmos.esa.int. Retrieved19 August 2018.
  31. ^Charles Kahn. 1994.Anaximander and the Origins of Greek Cosmology. Indianapolis: Hackett.
  32. ^Aristotle,On the Heavens, ii, 13.
  33. ^Most of Anaximander's model of the Universe comes from pseudo-Plutarch (II, 20–28):
    "[The Sun] is a circle twenty-eight times as big as the Earth, with the outline similar to that of a fire-filled chariot wheel, on which appears a mouth in certain places and through which it exposes its fire, as through the hole on a flute. [...] the Sun is equal to the Earth, but the circle on which it breathes and on which it's borne is twenty-seven times as big as the whole earth. [...] [The eclipse] is when the mouth from which comes the fire heat is closed. [...] [The Moon] is a circle nineteen times as big as the whole earth, all filled with fire, like that of the Sun".
  34. ^Carl Benjamin Boyer (1968),A History of Mathematics. Wiley.ISBN 0471543977. p. 54.
  35. ^Aristotle (1914). Forster, E. S.; Dobson, J. F. (eds.).De Mundo. Oxford University Press. 393a.
  36. ^"The components from which he made the soul and the way in which he made it were as follows: In between theBeing that is indivisible and always changeless, and the one that is divisible and comes to be in the corporeal realm, he mixed a third, intermediate form of being, derived from the other two. Similarly, he made a mixture of theSame, and then one of theDifferent, in between their indivisible and their corporeal, divisible counterparts. And he took the three mixtures and mixed them together to make a uniform mixture, forcing the Different, which was hard to mix, into conformity with the Same. Now when he had mixed these two with Being, and from the three had made a single mixture, he redivided the whole mixture into as many parts as his task required, each part remaining a mixture of the Same, the Different and Being." (Timaeus 35a–b), translation Donald J. Zeyl.
  37. ^Plato, Timaeus, 36c.
  38. ^Plato, Timaeus, 36d.
  39. ^Plato, Timaeus, 39d.
  40. ^Yavetz, Ido (February 1998). "On the Homocentric Spheres of Eudoxus".Archive for History of Exact Sciences.52 (3):222–225.Bibcode:1998AHES...52..222Y.doi:10.1007/s004070050017.JSTOR 41134047.S2CID 121186044.
  41. ^Crowe, Michael (2001).Theories of the World from Antiquity to the Copernican Revolution. Mineola, New York: Dover. p. 23.ISBN 0-486-41444-2.
  42. ^Easterling, H. (1961). "Homocentric Spheres in De Caelo".Phronesis.6 (2):138–141.doi:10.1163/156852861x00161.JSTOR 4181694.
  43. ^Lloyd, G. E. R. (1968).The critic of Plato. Aristotle: The Growth and Structure of His Thought. Cambridge University Press.ISBN 978-0-521-09456-6.
  44. ^Hirshfeld, Alan W. (2004)."The Triangles of Aristarchus".The Mathematics Teacher.97 (4):228–231.doi:10.5951/MT.97.4.0228.ISSN 0025-5769.JSTOR 20871578.
  45. ^Bruce S. Eastwood,Ordering the Heavens: Roman Astronomy and Cosmology in the Carolingian Renaissance (Leiden: Brill, 2007), pp. 238–239.
  46. ^Mirabello, Mark (15 September 2016).A Traveler's Guide to the Afterlife: Traditions and Beliefs on Death, Dying, and What Lies Beyond. Simon and Schuster. p. 23.ISBN 978-1-62055-598-9.
  47. ^Gilbert, William (1893). "Book 6, Chapter III".De Magnete. Translated by Mottelay, P. Fleury. (Facsimile). New York: Dover Publications.ISBN 0-486-26761-X.

Sources

edit
  • Bragg, Melvyn (2023)."The Universe's Shape".bbc.co.uk. BBC. Retrieved23 May 2023.Melvyn Bragg discusses shape, size and topology of the universe and examines theories about its expansion. If it is already infinite, how can it be getting any bigger? And is there really only one?
  • "Cosmic Journey: A History of Scientific Cosmology".history.aip.org. American Institute of Physics. 2023. Retrieved23 May 2023.The history of cosmology is a grand story of discovery, from ancient Greek astronomy to -space telescopes.
  • Dodelson, Scott; Schmidt, Fabian (2020).Modern Cosmology 2nd Edition. Academic Press.ISBN 978-0128159484. Download full text:Dodelson, Scott; Schmidt, Fabian (2020)."Scott Dodelson - Fabian Schmidt - Modern Cosmology (2021) PDF"(PDF).scribd.com. Academic Press. Retrieved23 May 2023.
  • Charles Kahn. 1994.Anaximander and the Origins of Greek Cosmology. Indianapolis: Hackett.
  • "Genesis, Search for Origins. End of mission wrap up".genesismission.jpl.nasa.gov. NASA, Jet Propulsion Laboratory, California Institute of Technology. Retrieved23 May 2023.About 4.6 billion years ago, the solar nebula transformed into the present solar system. In order to chemically model the processes which drove that transformation, we would, ideally, like to have a sample of that original nebula to use as a baseline from which we can track changes.
  • Leonard, Scott A; McClure, Michael (2004).Myth and Knowing. McGraw-Hill.ISBN 978-0-7674-1957-4.
  • Lyth, David (12 December 1993). "Introduction to Cosmology".arXiv:astro-ph/9312022.These notes form an introduction to cosmology with special emphasis on large scale structure, the cmb anisotropy and inflation. Lectures given at the Summer School in High Energy Physics and Cosmology, ICTP (Trieste) 1993.) 60 pages, plus 5 Figures.
  • "NASA/IPAC Extragalactic Database (NED)".ned.ipac.caltech.edu. NASA. 2023. Retrieved23 May 2023.April 2023 Release Highlights Database Updates
  • Sophia Centre. The Sophia Centre for the Study of Cosmology in Culture, University of Wales Trinity Saint David.
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