The Info List - Cosmology

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(from the Greek κόσμος, kosmos "world" and -λογία, -logia "study of") is the study of the origin, evolution, and eventual fate of the universe. Physical cosmology
Physical cosmology
is the scientific study of the universe's origin, its large-scale structures and dynamics, and its ultimate fate, as well as the scientific laws that govern these areas.[2] The term cosmology was first used in English in 1656 in Thomas Blount's Glossographia,[3] and in 1731 taken up in Latin by German philosopher Christian Wolff, in Cosmologia Generalis.[4] Religious or mythological cosmology is a body of beliefs based on mythological, religious, and esoteric literature and traditions of creation myths and eschatology. Physical cosmology
Physical cosmology
is studied by scientists, such as astronomers and physicists, as well as philosophers, such as metaphysicians, philosophers of physics, and philosophers of space and time. Because of this shared scope with philosophy, theories in physical cosmology may include both scientific and non-scientific propositions, and may depend upon assumptions that cannot be tested. Cosmology
differs from astronomy in that the former is concerned with the Universe
as a whole while the latter deals with individual celestial objects. Modern physical cosmology is dominated by the Big Bang
Big Bang
theory, which attempts to bring together observational astronomy and particle physics;[5] more specifically, a standard parameterization of the Big Bang
Big Bang
with dark matter and dark energy, known as the Lambda-CDM
model. Theoretical astrophysicist David 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 the speed of light.[6]


1 Disciplines

1.1 Physical cosmology 1.2 Religious or mythological cosmology 1.3 Philosophical cosmology

2 Historical cosmologies 3 See also 4 References 5 External links


Nature timeline

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cosmic expansion

Earliest light

cosmic speed-up

Solar System


Single-celled life


Multicellular life

Land life

Earliest gravity

Dark energy

Dark matter

Earliest universe (−13.80)

Earliest stars

Earliest galaxy

Earliest quasar/sbh

Omega Centauri
Omega Centauri

Andromeda Galaxy
Andromeda Galaxy

Milky Way
Milky Way
Galaxy spiral arms form

Alpha Centauri
Alpha Centauri

Earliest Earth (−4.54)

Earliest life

Earliest oxygen

Atmospheric oxygen

Earliest sexual reproduction

Cambrian explosion

Earliest humans

L i f e

P r i m o r d i a l

Axis scale: billion years Also see: Human
timeline and Life timeline

and astrophysics have played a central role in shaping the understanding of the universe through scientific observation and experiment. Physical cosmology
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 the Big Bang, followed almost instantaneously by cosmic inflation; an expansion of space from which the universe is thought to have emerged 13.799 ± 0.021 billion years ago.[7] Cosmogony
studies the origin of the Universe, and cosmography maps the features of the Universe. In Diderot's Encyclopédie, 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).[8] Metaphysical cosmology has also been described as the placing of man in the universe in relationship to all other entities. This is exemplified by Marcus 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."[9] Physical cosmology[edit] Main article: Physical cosmology 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 the heavens. Greek philosophers Aristarchus of Samos, Aristotle, and Ptolemy
proposed different cosmological theories. The geocentric Ptolemaic system
Ptolemaic system
was the prevailing theory until the 16th century when Nicolaus Copernicus, and subsequently Johannes Kepler
Johannes Kepler
and Galileo Galilei, proposed a heliocentric system. This is one of the most famous examples of epistemological rupture in physical cosmology.

Evidence of gravitational waves in the infant universe may have been uncovered by the microscopic examination of the focal plane of the BICEP2
radio telescope.[10][11][12]

When Isaac Newton
Isaac Newton
published the Principia Mathematica in 1687, he finally figured out how the heavens moved. Newton provided a physical mechanism for Kepler's laws
Kepler's laws
and his law of universal gravitation 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 the Copernican principle—that the bodies on earth obey the same physical laws as all the celestial bodies. This was a crucial philosophical advance in physical cosmology. Modern scientific cosmology is usually considered to have begun in 1917 with Albert Einstein's publication of his final modification of general relativity in the paper "Cosmological Considerations of the General Theory
of Relativity" (although this paper was not widely available outside of Germany until the end of World War I). General relativity
General relativity
prompted cosmogonists such as Willem de Sitter, Karl Schwarzschild, and Arthur Eddington
Arthur Eddington
to explore its astronomical ramifications, which enhanced the ability of astronomers 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.

Part of a series on

Physical cosmology

Big Bang · Universe Age of the universe Chronology of the universe

Early universe

Planck epoch Grand unification epoch Quark epoch Hadron epoch Lepton epoch Photon epoch Big Bang
Big Bang
nucleosynthesis Inflation Dark Ages


Cosmic background radiation
Cosmic background radiation
(CBR) Gravitational wave background
Gravitational wave background
(GWB) Cosmic microwave background
Cosmic microwave background
(CMB) · Cosmic neutrino background (CNB) Cosmic infrared background
Cosmic infrared background

Expansion · Future

Hubble's law · Redshift Metric expansion of space FLRW metric · Friedmann equations Inhomogeneous cosmology Future of an expanding universe Ultimate fate of the universe Heat death of the universe Big Rip Big Crunch Big Bounce

Components · Structure


model Baryonic matter Energy Radiation Dark energy

Quintessence Phantom energy

Dark matter

Cold dark matter Warm dark matter Hot dark matter

Dark radiation


Shape of the universe Reionization · Structure formation Galaxy formation Large-scale structure Large quasar group Galaxy filament Supercluster Galaxy cluster Galaxy group Local Group Void


Black Hole Initiative
Black Hole Initiative
(BHI) BOOMERanG Cosmic Background Explorer
Cosmic Background Explorer
(COBE) Illustris project Planck space observatory Sloan Digital Sky Survey
Sloan Digital Sky Survey
(SDSS) 2dF Galaxy Redshift
Survey ("2dF")

Wilkinson Microwave Anisotropy Probe (WMAP)


Aaronson Alfvén Alpher Bharadwaj Copernicus de Sitter Dicke Ehlers Einstein Ellis Friedman Galileo Gamow Guth Hawking Hubble Lemaître Mather Newton Penrose Penzias Rubin Schmidt Smoot Suntzeff Sunyaev Tolman Wilson Zel'dovich

Subject history

Discovery of cosmic microwave background radiation

History of the Big Bang
Big Bang

Religious interpretations of the Big Bang
Big Bang

Timeline of cosmological theories

 Category Cosmology
portal Astronomy

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In parallel to this dynamic approach to cosmology, one long-standing debate about the structure of the cosmos was coming to a climax. Mount Wilson astronomer Harlow Shapley
Harlow Shapley
championed the model of a cosmos made up of the Milky Way
Milky Way
star system only; while Heber D. Curtis
Heber D. Curtis
argued for the idea that spiral nebulae were star systems in their own right as island universes. This difference of ideas came to a climax with the organization of the Great Debate on 26 April 1920 at the meeting of the U.S. National Academy of Sciences
National Academy of Sciences
in Washington, D.C.
Washington, D.C.
The debate was resolved when Edwin Hubble
Edwin Hubble
detected Cepheid Variables
Cepheid Variables
in the Andromeda galaxy
Andromeda galaxy
in 1923 and 1924. Their distance established spiral nebulae well beyond the edge of the Milky Way. Subsequent modelling of the universe explored the possibility that the cosmological constant, introduced by Einstein in his 1917 paper, may result in an expanding universe, depending on its value. Thus the Big Bang model was proposed by the Belgian priest Georges Lemaître
Georges Lemaître
in 1927 which was subsequently corroborated by Edwin Hubble's discovery of the red shift in 1929 and later by the discovery of the cosmic microwave background radiation by Arno Penzias
Arno Penzias
and Robert Woodrow Wilson in 1964. These findings were a first step to rule out some of many alternative cosmologies. Since around 1990, several dramatic advances in observational 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 the COBE, WMAP
and Planck satellites, large new galaxy redshift surveys including 2dfGRS and SDSS, and observations of distant supernovae and gravitational lensing. These observations matched the predictions of the cosmic inflation theory, a modified Big Bang
Big Bang
theory, and the specific version known as the Lambda-CDM
model. This has led many to refer to modern times as the "golden age of cosmology".[13] On 17 March 2014, astronomers at the Harvard-Smithsonian Center for Astrophysics
announced the detection of gravitational waves, providing strong evidence for inflation and the Big Bang.[10][11][12] However, on 19 June 2014, lowered confidence in confirming the cosmic inflation findings was reported.[14][15][16] On 1 December 2014, at the Planck 2014 meeting in Ferrara, Italy, astronomers reported that the universe is 13.8 billion years old and is composed of 4.9% atomic matter, 26.6% dark matter and 68.5% dark energy.[17] Religious or mythological cosmology[edit] See also: Religious cosmology Religious or mythological cosmology is a body of beliefs based on mythological, religious, and esoteric literature and traditions of creation and eschatology. Philosophical cosmology[edit] See also: Cosmology
(philosophy) 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 founded in religion.[citation needed] The ancient Greeks did not draw a distinction between this use and their model for the cosmos.[citation needed] However, in modern use metaphysical cosmology addresses questions about the Universe
which are beyond the scope of science. It is distinguished from religious cosmology in that it approaches these questions using philosophical methods like dialectics. Modern metaphysical cosmology tries to address questions such as:[citation needed]

What is the origin of the Universe? What is its first cause? Is its existence necessary? (see monism, pantheism, emanationism and creationism) What are the ultimate material components of the Universe? (see mechanism, dynamism, hylomorphism, atomism) What is the ultimate reason for the existence of the Universe? Does the cosmos have a purpose? (see teleology) Does the existence of consciousness have a purpose? How do we know what we know about the totality of the cosmos? Does cosmological reasoning reveal metaphysical truths? (see epistemology)

Historical cosmologies[edit] Further information: Timeline of cosmology
Timeline of cosmology
and Nicolaus Copernicus § Copernican system

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Name Author and date Classification Remarks

Hindu cosmology Rigveda
(c. 1700–1100 BC) Cyclical or oscillating, Infinite in time One cycle of existence is around 311 trillion years and the life of one universe around 8 billion years. This Universal cycle is preceded by an infinite number of universes and to be followed by another infinite number of universes. Includes an infinite number of universes at one given time.

Jain cosmology Jain Agamas
Jain Agamas
(written around 500 AD as per the teachings of Mahavira 599–527 BC) Cyclical or oscillating, eternal and finite Jain cosmology
Jain cosmology
considers the loka, 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 to Jainism, is broad at the top, narrow at the middle and once again becomes broad at the bottom.

Babylonian cosmology Babylonian literature (c. 3000 BC) Flat earth floating in infinite "waters of chaos" The Earth and the Heavens 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 cosmology Parmenides
(c. 515 BC) Finite and spherical in extent The 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.

Biblical cosmology Genesis creation narrative Earth floating in infinite "waters of chaos" The Earth and the Heavens form a unit within infinite "waters of chaos"; the "firmament" keeps out the outer "chaos"-ocean.

Atomist universe Anaxagoras
(500–428 BC) & later Epicurus Infinite in extent The 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. Incorporates Leucippus' principle of causality: "nothing happens at random; everything happens out of reason and necessity". The universe was not ruled by gods.[citation needed]

Pythagorean universe Philolaus
(d. 390 BC) 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
and planets 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.[18]

De Mundo Pseudo- Aristotle
(d. 250 BC or between 350 and 200 BC) The Universe
then 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."[19]

Stoic universe Stoics
(300 BC – 200 AD) Island universe The cosmos 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.

Aristotelian universe Aristotle
(384–322 BC) Geocentric, static, steady state, finite extent, infinite time Spherical earth is surrounded by concentric celestial spheres. Universe
exists unchanged throughout eternity. Contains a fifth element, called aether, that was added to the four classical elements.

Aristarchean universe Aristarchus (circa 280 BC) Heliocentric Earth rotates daily on its axis and revolves annually about the sun in a circular orbit. Sphere of fixed stars is centered about the sun.

Ptolemaic model Ptolemy
(2nd century AD) Geocentric
(based on Aristotelian universe) Universe
orbits around a stationary Earth. Planets move in circular epicycles, 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 of equants 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. Almagest
(the Great System).

Aryabhatan model Aryabhata
(499) Geocentric
or Heliocentric The Earth rotates and the planets move in elliptical 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.

Medieval universe Medieval philosophers (500–1200) Finite in time A universe that is finite in time and has a beginning is proposed by the Christian philosopher John Philoponus, who argues against the ancient Greek notion of an infinite past. Logical arguments supporting a finite universe are developed by the early Muslim philosopher Alkindus, the Jewish philosopher Saadia Gaon, and the Muslim theologian Algazel.

Multiversal cosmology Fakhr al-Din al-Razi (1149–1209) Multiverse, multiple worlds and universes There 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 models Maragha school (1259–1528) Geocentric Various modifications to Ptolemaic model and Aristotelian universe, including rejection of equant and eccentrics at Maragheh observatory, and introduction of Tusi-couple
by Al-Tusi. Alternative models later proposed, including the first accurate lunar model by Ibn al-Shatir, a model rejecting stationary Earth in favour of Earth's rotation
Earth's rotation
by Ali Kuşçu, and planetary model incorporating "circular inertia" by Al-Birjandi.

Nilakanthan model Nilakantha Somayaji (1444–1544) Geocentric
and heliocentric A universe in which the planets orbit the Sun, which orbits the Earth; similar to the later Tychonic system

Copernican universe Nicolaus Copernicus
Nicolaus Copernicus
(1473–1543) Heliocentric
with circular planetary orbits First described in De revolutionibus orbium coelestium.

Tychonic system Tycho Brahe
Tycho Brahe
(1546–1601) Geocentric
and Heliocentric A universe in which the planets orbit the Sun
and the Sun
orbits the Earth, similar to the earlier Nilakanthan model.

Bruno's cosmology Giordano Bruno
Giordano Bruno
(1548–1600) Infinite extent, infinite time, homogeneous, isotropic, non-hierarchical Rejects 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 with aether, and matter is composed of the same four elements (water, earth, fire, and air), and is atomistic, animistic and intelligent.

Keplerian Johannes Kepler
Johannes Kepler
(1571–1630) Heliocentric
with elliptical planetary orbits Kepler's discoveries, marrying mathematics and physics, provided the foundation for our present conception of the Solar system, but distant stars were still seen as objects in a thin, fixed celestial sphere.

Static Newtonian Isaac Newton
Isaac Newton
(1642–1727) Static (evolving), steady state, infinite Every particle in the universe attracts every other particle. Matter on the large scale is uniformly distributed. Gravitationally balanced but unstable.

Cartesian Vortex universe René Descartes, 17th century Static (evolving), steady state, infinite System of huge swirling whirlpools of aethereal or fine matter produces what we would call gravitational effects. But his vacuum was not empty; all space was filled with matter.

Hierarchical universe Immanuel Kant, Johann Lambert, 18th century Static (evolving), steady state, infinite Matter
is clustered on ever larger scales of hierarchy. Matter
is endlessly recycled.

Einstein Universe
with a cosmological constant Albert Einstein, 1917 Static (nominally). Bounded (finite) " Matter
without motion". Contains uniformly distributed matter. Uniformly curved spherical space; based on Riemann's hypersphere. Curvature is set equal to Λ. In effect Λ is equivalent to a repulsive force which counteracts gravity. Unstable.

De Sitter universe Willem de Sitter, 1917 Expanding flat space. Steady state. Λ > 0

"Motion without matter." Only apparently static. Based on Einstein's general relativity. Space expands with constant acceleration. Scale factor increases exponentially (constant inflation).

MacMillan universe William Duncan MacMillan 1920s Static and steady state New matter is created from radiation; starlight perpetually recycled into new matter particles.

Friedmann universe, spherical space Alexander Friedmann
Alexander Friedmann
1922 Spherical expanding space. k= +1 ; no Λ

Positive curvature. Curvature constant k = +1 Expands then recollapses. Spatially closed (finite).

Friedmann universe, hyperbolic space Alexander Friedmann, 1924 Hyperbolic expanding space. k= -1 ; no Λ

Negative curvature. Said to be infinite (but ambiguous). Unbounded. Expands forever.

Dirac large numbers hypothesis Paul Dirac
Paul Dirac
1930s Expanding Demands a large variation in G, which decreases with time. Gravity weakens as universe evolves.

Friedmann zero-curvature Einstein and De Sitter, 1932 Expanding flat space k= 0 ; Λ = 0 Critical density

Curvature constant k = 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 a deceleration term q =½, which means that its expansion rate slows down.

The original Big Bang
Big Bang
(Friedmann-Lemaître) Georges Lemaître
Georges Lemaître
1927–29 Expansion 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
Oscillating universe
(Friedmann-Einstein) Favored by Friedmann, 1920s Expanding and contracting in cycles Time 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 universe Arthur Eddington
Arthur Eddington
1930 First static then expands Static Einstein 1917 universe with its instability disturbed into expansion mode; with relentless matter dilution becomes a De Sitter universe. Λ dominates gravity.

Milne universe
Milne universe
of kinematic relativity Edward Milne, 1933, 1935; William H. McCrea, 1930s

Kinematic expansion without space expansion Rejects general relativity and the expanding space paradigm. Gravity not included as initial assumption. Obeys cosmological principle and special 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.

class of models Howard Robertson, Arthur Walker, 1935 Uniformly expanding Class 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-state expanding Hermann Bondi, Thomas Gold, 1948 Expanding, steady state, infinite Matter
creation rate maintains constant density. Continuous creation out of nothing from nowhere. Exponential expansion. Deceleration term q = -1.

Steady-state expanding Fred Hoyle
Fred Hoyle
1948 Expanding, steady state; but unstable Matter
creation rate maintains constant density. But since matter creation rate must be exactly balanced with the space expansion rate the system is unstable.

Ambiplasma Hannes Alfvén
Hannes Alfvén
1965 Oskar Klein Cellular universe, expanding by means of matter–antimatter annihilation Based on the concept of plasma cosmology. The universe is viewed as "meta-galaxies" divided by double layers and thus a bubble-like nature. Other universes are formed from other bubbles. Ongoing cosmic matter-antimatter annihilations keep the bubbles separated and moving apart preventing them from interacting.

Brans–Dicke theory Carl H. Brans, Robert H. Dicke Expanding Based on Mach's principle. G varies with time as universe expands. "But nobody is quite sure what Mach's principle
Mach's principle
actually means."[citation needed]

Cosmic inflation Alan Guth
Alan Guth
1980 Big Bang
Big Bang
modified to solve horizon and flatness problems Based 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, 1983 Big Bang
Big Bang
with cosmic inflation Multiverse
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 our entire cosmos. Bubbles nucleate in a spacetime foam.

Cyclic model Paul Steinhardt; Neil Turok
Neil Turok
2002 Expanding and contracting in cycles; M-theory. Two parallel orbifold planes or M-branes collide periodically in a higher-dimensional space. With quintessence or dark energy.

Cyclic model Lauris Baum; Paul Frampton 2007 Solution of Tolman's entropy problem Phantom dark energy fragments universe into large number of disconnected patches. Our patch contracts containing only dark energy with zero entropy.

Table notes: the term "static" simply means not expanding and not contracting. Symbol G represents Newton's gravitational constant; Λ (Lambda) is the cosmological constant. See also[edit]

Earth science Lambda-CDM
model Absolute time and space Galaxy formation and evolution Illustris project List of astrophysicists Big History Non-standard cosmology Jainism
and non-creationism Taiji (philosophy) Universal rotation curve Warm inflation


^ Karl Hille, ed. (13 October 2016). "Hubble Reveals Observable Universe
Contains 10 Times More Galaxies
Than Previously Thought". NASA. Retrieved 17 October 2016.  ^ "Introduction: Cosmology
– space". New Scientist. 4 September 2006 ^ 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.  Extract of page 116 ^ Luminet, Jean-Pierre (2008). The Wraparound Universe. CRC Press. p. 170. ISBN 978-1-4398-6496-8.  Extract of page 170 ^ "Cosmology" Oxford Dictionaries ^ David N. Spergel (Fall 2014). " Cosmology
Today". Daedalus. American Academy of Arts and Sciences. 143 (4): 125–133. doi:10.1162/DAED_a_00312.  ^ Planck Collaboration (2015). "Planck 2015 results. XIII. Cosmological parameters (See Table 4 on page 31 of PDF)". Astronomy & Astrophysics. 594: A13. arXiv:1502.01589 . Bibcode:2016A&A...594A..13P. doi:10.1051/0004-6361/201525830.  ^ "Detailed Explanation of the System of Human
Knowledge". The Encyclopedia of Diderot & d'Alembert Collaborative Translation Project. 1 April 2015. Retrieved 1 April 2015.  ^ The thoughts of Marcus Aurelius
Marcus Aurelius
Antonius viii. 52.  ^ a b " BICEP2
2014 Results Release". National Science
Foundation. 17 March 2014. Retrieved 18 March 2014.  ^ a b Whitney Clavin (17 March 2014). " NASA
Technology Views Birth of the Universe". NASA. Retrieved 17 March 2014.  ^ a b Dennis Overbye (17 March 2014). "Detection of Waves in Space Buttresses Landmark Theory
of Big Bang". New York Times. Retrieved 17 March 2014.  ^ Alan Guth
Alan Guth
is reported to have made this very claim in an Edge Foundation interview EDGE ^ Dennis Overbye (19 June 2014). "Astronomers Hedge on Big Bang Detection Claim". New York Times. Retrieved 20 June 2014.  ^ Amos, Jonathan (19 June 2014). "Cosmic inflation: Confidence lowered for Big Bang
Big Bang
signal". BBC News. Retrieved 20 June 2014.  ^ Ade, P.  A.  R.; Aikin, R.  W.; Barkats, D.; Benton, S.  J.; Bischoff, C.  A.; Bock, J.  J.; Brevik, J.  A.; Buder, I.; Bullock, E.; Dowell, C.  D.; Duband, L.; Filippini, J.  P.; Fliescher, S.; Golwala, S.  R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S.  R.; Hilton, G.  C.; Hristov, V.  V.; Irwin, K.  D.; Karkare, K.  S.; Kaufman, J.  P.; Keating, B.  G.; Kernasovskiy, S.  A.; Kovac, J.  M.; Kuo, C.  L.; Leitch, E.  M.; Lueker, M.; Mason, P.; et al. (2014). "Detection of B-Mode Polarization at Degree Angular Scales by BICEP2". Physical Review Letters. 112 (24): 241101. arXiv:1403.3985 . Bibcode:2014PhRvL.112x1101A. doi:10.1103/PhysRevLett.112.241101. PMID 24996078.  ^ Dennis Overbye (1 December 2014). "New Images Refine View of Infant Universe". New York Times. Retrieved 2 December 2014.  ^ Carl B. Boyer (1968), A History of Mathematics. Wiley. ISBN 0471543977. p. 54. ^ Aristotle
(1914). Forster, E. S.; Dobson, J. F., eds. De Mundo. Oxford University Press. 393a. 

External links[edit]

Look up cosmology in Wiktionary, the free dictionary.

Library resources about Cosmology

Online books Resources in your library Resources in other libraries

NASA/IPAC Extragalactic Database (NED) (NED-Distances) Cosmic Journey: A History of Scientific Cosmology
from the American Institute of Physics Introduction to Cosmology
David Lyth's lectures from the ICTP Summer School in High Energy
and Cosmology The Sophia Centre The Sophia Centre for the Study of Cosmology
in Culture, University of Wales Trinity Saint David Genesis cosmic chemistry module "The Universe's Shape", BBC Radio 4 discussion with Sir Martin Rees, Julian Barbour and Janna Levin (In Our Time, Feb. 7, 2002)

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Age of the universe Big Bang Chronology of the universe Universe

History of cosmological theories

Discovery of cosmic microwave background History of the Big Bang
Big Bang
theory Religious interpretations of the Big Bang Timeline of cosmological theories

Past universe

Cosmic microwave background Gravitational wave background Neutrino background Inflation Nucleosynthesis Habitable epoch

Present universe

FLRW metric Friedmann equations Hubble's law Metric expansion of space Redshift

Future universe

Future of an expanding universe Ultimate fate of the universe


Dark energy Dark fluid Dark matter Lambda-CDM

Structure formation

Galaxy filament Galaxy formation Large quasar group Large-scale structure Reionization Shape of the universe Structure formation


2dF BOOMERanG COBE Illustris project Observational cosmology Planck SDSS WMAP


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portal Cosmology