Steady state theory - wikipedia Steady state theory This article is about the cosmological theory. For other uses, see Steady state ( disambiguation ). Part of a series on Physical cosmology Big Bang Universe Age of the universe Chronology of the universe Early universe Inflation Nucleosynthesis Backgrounds Gravitational wave ( GWB ) Microwave ( CMB ) Neutrino ( CNB ) 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 Components Structure Components Lambda - CDM model Dark energy Dark fluid Dark matter Structure Shape of the universe Galaxy filament Galaxy formation Large quasar group Large - scale structure Reionization Structure formation Experiments BOOMERanG Cosmic Background Explorer ( COBE ) Illustris project Planck space observatory Sloan Digital Sky Survey ( SDSS ) 2dF Galaxy Redshift Survey ( `` 2dF '' ) Wilkinson Microwave Anisotropy Probe ( WMAP ) Scientists 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 List of cosmologists Subject history Discovery of cosmic microwave background radiation History of the Big Bang theory Religious interpretations of the Big Bang theory Timeline of cosmological theories Cosmology portal Astronomy portal In cosmology, the Steady State theory is an alternative to the Big Bang model of the evolution of the universe. In the steady - state theory, the density of matter in the expanding universe remains unchanged due to a continuous creation of matter, thus adhering to the perfect cosmological principle, a principle that asserts that the observable universe is basically the same at any time as well as at any place. While the steady state model enjoyed some popularity in the mid-20th century, it is now rejected by the vast majority of cosmologists, astrophysicists and astronomers, as the observational evidence points to a hot Big Bang cosmology with a finite age of the universe, which the Steady State model does not predict. Contents 1 History 2 Observational tests 2.1 Counts of radio sources 2.2 Cosmic microwave background 3 Quasi-steady state 4 Notes and citations 5 Further reading 6 External links History Cosmological expansion was originally discovered through observations by Edwin Hubble. Theoretical calculations also showed that the static universe as modeled by Einstein ( 1917 ) was unstable and contradicted general relativity. The modern Big Bang theory is one in which the universe has a finite age and has evolved over time through cooling, expansion, and the formation of structures through gravitational collapse. The steady state theory asserts that although the universe is expanding, it nevertheless does not change its appearance over time ( the perfect cosmological principle ) ; the universe has no beginning and no end. This requires that matter be continually created in order to keep the universe 's density from decreasing. Influential papers on steady state cosmologies were published by Hermann Bondi, Thomas Gold, and Fred Hoyle in 1948. It is now known that Albert Einstein considered a steady - state model of the expanding universe, as indicated in a 1931 manuscript, many years before Hoyle, Bondi and Gold. However, he quickly abandoned the idea. Observational tests Counts of radio sources Problems with the steady - state theory began to emerge in the 1950s and 60s, when observations began to support the idea that the universe was in fact changing : bright radio sources ( quasars and radio galaxies ) were found only at large distances ( therefore could have existed only in the distant past ), not in closer galaxies. Whereas the Big Bang theory predicted as much, the Steady State theory predicted that such objects would be found throughout the universe, including close to our own galaxy. By 1961, statistical tests based on radio - source surveys had ruled out the steady state model in the minds of most cosmologists, although some proponents of the steady state insisted that the radio data were suspect. Cosmic microwave background For most cosmologists, the definitive refutation of the steady - state theory came with the discovery of the cosmic microwave background radiation in 1964, which was predicted by the Big Bang theory. Stephen Hawking described this discovery as `` the final nail in the coffin of the steady - state theory. '' The steady - state theory explained microwave background radiation as the result of light from ancient stars that has been scattered by galactic dust. However, the cosmic microwave background level is very even in all directions, making it difficult to explain how it could be generated by numerous point sources and the microwave background radiation shows no evidence of characteristics such as polarization that are normally associated with scattering. Furthermore, its spectrum is so close to that of an ideal black body that it could hardly be formed by the superposition of contributions from a multitude of dust clumps at different temperatures as well as at different redshifts. Steven Weinberg wrote in 1972, The steady state model does not appear to agree with the observed d versus z relation or with source counts... In a sense, this disagreement is a credit to the model ; alone among all cosmologies, the steady - state model makes such definite predictions that it can be disproved even with the limited observational evidence at our disposal. The steady - state model is so attractive that many of its adherents still retain hope that the evidence against it will eventually disappear as observations improve. However, if the cosmic microwave radiation... is really black - body radiation, it will be difficult to doubt that the universe has evolved from a hotter denser early stage. Since this discovery, the Big Bang theory has been considered to provide the best explanation of the origin of the universe. In most astrophysical publications, the Big Bang is implicitly accepted and is used as the basis of more complete theories. Quasi-steady state Quasi-steady state cosmology ( QSS ) was proposed in 1993 by Fred Hoyle, Geoffrey Burbidge, and Jayant V. Narlikar as a new incarnation of the steady state ideas meant to explain additional features unaccounted for in the initial proposal. The theory suggests pockets of creation occurring over time within the universe, sometimes referred to as minibangs, mini-creation events, or little bangs. After the observation of an accelerating universe, further modifications of the model were made. Astrophysicist and cosmologist Ned Wright has pointed out flaws in the theory. These first comments were soon rebutted by the proponents. Wright and other mainstream cosmologists reviewing QSS have pointed out new flaws and discrepancies with observations left unexplained by proponents. Notes and citations Jump up ^ `` Steady State theory ''. BBC. Retrieved January 11, 2015. ( T ) he Steady State theorists ' ideas are largely discredited today... Jump up ^ Kragh, Helge ( 1999 ). Cosmology and Controversy : The Historical Development of Two Theories of the Universe. Princeton University Press. ISBN 0 - 691 - 02623 - 8. Jump up ^ Bondi and Gold, `` The Steady - State Theory of the Expanding Universe, '' MNRAS 108 ( 1948 ) 252. Bibcode : 1948MNRAS. 108... 252B Jump up ^ Hoyle, `` A New Model for the Expanding Universe, '' MNRAS 108 ( 1948 ) 372. Bibcode : 1948MNRAS. 108... 372H Jump up ^ `` Einstein 's lost theory uncovered ''. Nature News & Comment. Jump up ^ Ryle and Clarke, `` An examination of the steady - state model in the light of some recent observations of radio sources, '' MNRAW 122 ( 1961 ) 349 Jump up ^ Weinberg, S. ( 1972 ). Gravitation and Cosmology. John Whitney & Sons. pp. 495 -- 464. ISBN 978 - 0 - 471 - 92567 - 5. Jump up ^ Narlikar, J.V. ; Vishwakarma, R.G. ; Burbidge, G. ( 2002 ). `` Interpretations of the Accelerating Universe ''. Publications of the Astronomical Society of the Pacific. 114 : 1092 -- 1096. Bibcode : 2002PASP... 114.1092 N. arXiv : astro - ph / 0205064 ( astro - ph ). doi : 10.1086 / 342374. Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1993 ). `` A quasi-steady state cosmological model with creation of matter ''. The Astrophysical Journal. 410 : 437 -- 457. Bibcode : 1993ApJ... 410... 437H. doi : 10.1086 / 172761. Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1994 ). `` Astrophysical deductions from the quasi-steady state cosmology ''. Monthly Notices of the Royal Astronomical Society. 267 : 1007 -- 1019. Bibcode : 1994MNRAS. 267.1007 H. doi : 10.1093 / mnras / 267.4. 1007. Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1994 ). `` Astrophysical deductions from the quasi-steady state : Erratum ''. Monthly Notices of the Royal Astronomical Society. 269 : 1152. Bibcode : 1994MNRAS. 269.1152 H. doi : 10.1093 / mnras / 269.4. 1152. Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1994 ). `` Further astrophysical quantities expected in a quasi-steady state Universe ''. Astronomy and Astrophysics. 289 ( 3 ) : 729 -- 739. Bibcode : 1994A&A... 289... 729H. Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1995 ). `` The basic theory underlying the quasi-steady state cosmological model ''. Proceedings of the Royal Society A. 448 : 191. Bibcode : 1995RSPSA. 448... 191H. doi : 10.1098 / rspa. 1995.0012. Jump up ^ Wright, E.L. ( 1994 ). `` Comments on the Quasi-Steady - State Cosmology ''. Monthly Notices of the Royal Astronomical Society. Bibcode : 1995MNRAS. 276.1421 W. arXiv : astro - ph / 9410070 ( astro - ph ). doi : 10.1093 / mnras / 276.4. 1421. Jump up ^ Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 1994 ). `` Note on a Comment by Edward L. Wright ''. arXiv : astro - ph / 9412045 ( astro - ph ). Jump up ^ Wright, E.L. ( 20 December 2010 ). `` Errors in the Steady State and Quasi-SS Models ''. UCLA, Physics & Astronomy Department. Further reading Burbidge, G., Hoyle, F., The Origin of Helium and the Other Light Elements, The Astrophysical Journal, 509 : L1 -- L3, 10 December 1998 Hoyle, F. ; Burbidge, G. ; Narlikar, J.V. ( 2000 ). A Different Approach to Cosmology. Cambridge University Press. ISBN 0 - 521 - 66223 - 0. Mitton, S. ( 2005 ). Conflict in the Cosmos : Fred Hoyle 's Life in Science. Joseph Henry Press. ISBN 0 - 309 - 09313 - 9. Mitton, S. ( 2005 ). Fred Hoyle : A Life in Science. Aurum Press. ISBN 1 - 85410 - 961 - 8. Narlikar, Jayant ; Burbidge, Geoffrey ( 2008 ). Facts and Speculations in Cosmology. Cambridge University Press. ISBN 978 - 0521865043. External links Cosmology portal Historical note : the steady - state model -- a brief presentation of the mathematical content of the Hoyle theory Retrieved from `` https://en.wikipedia.org/w/index.php?title=Steady_State_theory&oldid=802180496 '' Categories : Physical cosmology Obsolete scientific theories Cosmogony 1948 in science Talk Contents About Wikipedia Azərbaycanca বাংলা Català Čeština Dansk Deutsch Ελληνικά Español Euskara فارسی Français 한국어 हिन्दी Hrvatski Bahasa Indonesia Italiano עברית Қазақша Kreyòl ayisyen മലയാളം मराठी Nederlands 日本 語 Norsk nynorsk Polski Português Русский Simple English Slovenčina Slovenščina Suomi Svenska Татарча / tatarça Українська 中文 Edit links This page was last edited on 24 September 2017, at 14 : 10. Text is available under the Creative Commons Attribution - ShareAlike License ; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. 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Question: what is the meaning of steady state theory
Answer: the density of matter in the expanding universe remains unchanged due to a continuous creation of matter, thus adhering to the perfect cosmological principle, a principle that asserts that the observable universe is basically the same at any time as well as at any place