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BIG-BANG NUCLEOSYNTHESIS

發(fā)布時間:2018-03-11 19:31

  本文選題:primordial 切入點(diǎn):impressive 出處:《Chinese Physics C》2014年09期  論文類型:期刊論文


【摘要】:正Revised October 2013 by B.D.Fields.(Univ.of Illinois)P.Molaro(Trieste Observatory)and S.Sarkar(Univ.of OxfordNiels Bohr Institute.Copenhagen).Big-Bang nucleosynthesis(BBN)offers the deepest reliable probe of the early Universe,being based on well-understood Standard Model physics[1].Predictions of the abundances of the light elements.D.~3He,~4He,and~7Li,synthesized at the end of the'first three minutes'.are in good overall agreement with the primordial abundances inferred from observational data,thus validating the standard hot Big-Bang cosmology(see[2-4]for reviews).This is particularly impressive given that these abundances span nine orders of magnitude-from~4He/H~0.08 down to~7Li/H~10~(-10)(ratios by number).Thus BBN provides powerful constraints on possible deviations from the standard cosmology,and on new physics beyond the Standard Model[5-8].
[Abstract]:Revised October 2013 by based on well-understood Standard physics [1] .Predictions of the abundances of the abundances of the light Elements.3Heand7Lially synthesized at end of the'first three minutes'.are in good overall agreement with the with Observatory)and Observatory)and with Observatory)and Observatory)and with with Observatory)and Observatory)and with Observatory)and Observatory)and with. Of magnitude-from~4He/H~0.08 down to~7Li/H~10~(-10)(ratios by number).Thus BBN provides powerful constraints on possible deviations from the standard cosmologyand on new physics beyond the Standard Model [5-8].
【作者單位】: University
【分類號】:P159.3

【共引文獻(xiàn)】

相關(guān)期刊論文 前2條

1 李淼;李霄棟;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,

本文編號:1599590


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