BIG-BANG COSMOLOGY

发布时间：2018-05-14 08:33

  本文选题：inevitable + isotropic　； 参考：《Chinese Physics C》2014年09期

【摘要】：正Revised September 2013 by K.A.Olive(University of Minnesota)and J.A.Peacock(University of Edinburgh).22.1.Introduction to Standard Big-Bang Model The observed expansion of the Universe[1-3]is a natural(almost inevitable)result of any homogeneous and isotropic cosmological model based on general relativity.However,by itself,the Hubble expansion does not provide sufficient evidence for what we generally refer to as the Big-Bang model of cosmology.While general relativity is in principle capable of describing the cosmology of any given distribution of matter,it is extremely fortunate that our Universe appears to be homogeneous and isotropic on large scales.Together,homogeneity and isotropy allow us to extend the Copernican Principle to the Cosmological Principle,stating that all spatial positions in the
[Abstract]:Revised September 2013 by K.A.Olive(University of Edinburgh).22.1.Introduction to Standard Big-Bang Model The observed expansion of the Universe [1-3] is a natural(almost inevitable)result of any homogeneous and isotropic cosmological model based on general relativity.Howeverby self Hubble expansion does not provide sufficient evidence for what we generally refer to as the Big-Bang model of cosmology.While general relativity is in principle capable of describing the cosmology of any given distribution of Matter,it is extremely fortunate that our Universe appears to be homogeneous and isotropic on large scales.Together,homogeneity and isotropy allow us to extend the Copernican Principle to the Cosmological Principle,stating that all spatial positions in the
【作者单位】： University
【分类号】：P159.3

【共引文献】

相关期刊论文 前4条

1 李淼;李霄栋;王爽;王一;;Dark Energy[J];Communications in Theoretical Physics;2011年09期

2 K.A.Olive;K.Agashe;C.Amsler;M.Antonelli;J.-F.Arguin;D.M.Asner;H.Baer;H.R.Band;R.M.Barnett;T.Basaglia;C.W.Bauer;J.J.Beatty;V.I.Belousov;J.Beringer;G.Bernardi;S.Bethke;H.Bichsel;O.Biebe;E.Blucher;S.Blusk;G.Brooijmans;O.Buchmueller;V.Burkert;M.A.Bychkov;R.N.Cahn;M.Carena;A.Ceccucci;A.Cerr;D.Chakraborty;M.-C.Chen;R.S.Chivukula;K.Copic;G.Cowan;O.Dahl;G.D'Ambrosio;T.Damour;D.de Florian;A.de Gouvea;T.DeGrand;P.de Jong;G.Dissertor;B.A.Dobrescu;M.Doser;M.Drees;H.K.Dreiner;D.A.Edwards;S.Eidelman;J.Erler;V.V.Ezhela;W.Fetscher;B.D.Fields;B.Foster;A.Freitas;T.K.Gaisser;H.Gallagher;L.Garren;H.-J.Gerber;G.Gerbier;T.Gershon;T.Gherghetta;S.Golwala;M.Goodman;C.Grab;A.V.Gritsan;C.Grojean;D.E.Groom;M.Gr，

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