宇宙背景场的粒子物理检验方法
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  • 英文题名:The Test of the Background Field in the Universe with the Particle Physics Method
  • 作者:戎树军
  • 论文级别:硕士
  • 学科专业名称:理论物理
  • 学位年度:2009
  • 导师:任继荣
  • 学科代码:070201
  • 学位授予单位:兰州大学
  • 论文提交日期:2009-04-01
摘要
本文研究了检验宇宙背景场的粒子物理方法,通过背景标量场与量子规范场的耦合,分析了宇宙背景场对粒子静质量的影响,得出了粒子静质量随背景场涨落的附加质量公式,并给出了初步的实验检验建议.
     首先,本文介绍了宇宙学的基本背景知识,暗能量问题的研究状况以及各种暗能量模型,提出了检验宇宙背景场的粒子物理方法.
     其次,本文介绍了希格斯机制,包括费米子的左手和右手表示,规范群的选择,希格斯场与规范场的耦合,希格斯场与轻子场以及夸克场的耦合,希格斯粒子的质量范围,以及实验检验状况.讨论了经典宇宙背景场满足的约束条件,即能量动量守恒、电荷守恒、无额外歌德斯通粒子。通过类比标准模型中的希格斯机制,以标量场为例,引入了背景标量场与量子规范场的耦合,得出了宇宙背景场涨落对粒子质量的修正公式.
     最后,本文给出了粒子质量修正公式初步的实验检验建议,并对可能的实验结果作了讨论.
In this dissertation,we have made the reseach on the test of the background field in the universe with the particle physics method.By the coupling betwwen the background scalar field and the quantized gauge field,we obtained the modified formula of the particle's static mass with the fluctuation of the background field.We also gave a primary advice on the experimental test of our method.
     Firstly,we introduced background knowlede of the cosmology and the situation of the dark energy resaech and various dark energy model.We proposed a particle physics method to test the backgroud scalar field in the universe.
     Secondly,we introduced the Higss mechanism,including the representation of the left hand and right hand fermion,option of gauge group,the coupling of Higss field and gauge field,the coupling of Higgs field and lepton field and quark field,the extent of Higgs particle's mass and the experimental test of the Higgs mechanism.We discussed the constraint on the classical backgroud field,including the conservation of energy momentum and charge,non Goldstone boson.By the analogy to the Higss mechanism in the standard model,we introduced the coupling between the bachground scalar field in the universe and quantized gauge field.We obtained the modified formula of particle's static mass with the fluctuation of the background fied.
     Finally,we gave a primary advice on the experimental test on the modified formula of particle's static mass.We also discussed possible experimental consequences.
引文
[1]Wei Hao and Cai Rong-gen.A Brief Overview of Recent Theoretical Study on Dark Energy,Science and Technology Review,23,12(2005).
    [2]Riess A.G.and etal.Type Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope:Evidence for Past Deceleration and Constraints on Dark Energy Evolution,Astrophys.J[J],607,665(2004).
    [3]Knop R.A.and etal.Dark Energy and the Accelerating Universe,Astrophys.J[J],598,102(2003).
    [4]Riess A.G.and etal.Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,Astron.J[J],116,109(1998).
    [5]Perlmutter S.and etal.Measurements of Ω and A from 42 High-Redshift Supernovae,Astrophys.J[J],517,565(1999).
    [6]Bennett C.L.and etal.First year Wilkinson Microwave Anisotropy Probe(WMAP) observations:Preliminary maps and basic results,Astrophys.J.Suppl.[J],148,1(2003).
    [7]Spergel D.N.and etal.Astrophys.J.Suppl.[J],148,175(2003).
    [8]Tegmark M.and etal.Cosmological parameters from SDSS and WMAP,Phys.Rev.D,69,103501(2004).
    [9]Tegmark M.and etal.The Three-Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey,Astrophys.J[J],606,702(2004).
    [10]Allen S.W and etal.Mon.Not.Roy.Astron.Soc[J]353,457(2004).
    [11]Caldwell R.R and etal.Cosmological Imprint of an Energy Component with General Equation of State,Phys.Rev.Lett,80,1582(1998).
    [12]Wetterich C.and etal.Cosmology and the fate of dilatation symmetry,Nucl.Phys.B,302,668(1988).
    [13]Peeples P.JE.and etal.Astrophys.J[J],325,L17(1988).
    [14]Boyle L.A.and etal.Spintessence! New models for dark matter and dark energy,Phys.Lett.B,545,17(2002).
    [15]Gu J.A.and Hwang W.Y.Can the quintessence be a complex scalar field,Phys.Lett.B,517,1(2001).
    [16]Kasuya S.Difficulty of a spinning complex scalar field to be dark energy,Phys.Lett.B,515,121(2001).
    [17]Sean M.Carroll,Lecture Notes on general relativity,gr-qc/9712019(1997).
    [18]Caldwell R.R.A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state,Phys.Lett.B,545,23(2002).
    [19]Caldwell R.R and etal.Phantom Energy:Dark Energy with w < -1 Causes a Cosmic Doomsday,Phys.Rev.Lett,91,071301(2003).
    [20]Carroll S.M.and etal.Can the dark energy equation-of-state parameter w be less than -1,Phys.Rev.D,68,023509(2003).
    [21]Cdine J.M.R.R and etal.The phantom menaced:Constraints on low-energy effective ghosts,Phys.Rev.D,70,043543(2004).
    [22]Yi-Shi Duan and etal.Cosmic Strings and Quintessence,Chin.Phys.Lett.20,2133(2003).
    [23]Kamenshchik A.Y.and etal.An alternative to quintessence,Phys.Lett.B,511,265(2001).
    [24]Bilic N.and etal.Unification of dark matter and dark energy:the inhomogeneous Chaplygin gas,Phys.Lett.B,535,17(2002)
    [25]Bento M.C.and etal.Generalized Chaplygin gas,accelerated expansion,and dark-energy-matter unification,Phys.Rev.D,66,043507(2002)
    [26]Bertolami O.Challenges to the Generalized Chaplygin Gas Cosmology,astro-ph/0403310,17(2004)
    [27]J.Schwinger,On Gauge Invariance and Vacuum Polarization,Phys.Rev.82,664(1951).
    [28]Novaes S.F.Introduction to standard Model,hep-ph/0001283,043543(2004).
    [29]Fermi,Z.Phys 82,161(1934).
    [30]G.Gamow and E.Teller,Selection Rules for the β-Disintegration,Phys.Rev.49,895(1937).
    [31]Yang C.N and Mills R.L,Conservation of Isotopic Spin and Isotopic Gauge Invariance,Phys.Rev.96,191(1954)..
    [32]Goldstone.J,Nuovo Cim.19,154(1961).
    [33]Cabibbo.N,Unitary Symmetry and Leptonic Decays,Phys.Rev.Lett 10,531(1963).
    [34]Higgs P.W.Broken symmetries,massless particlees and gauge fields,Phys.Lett.12,132(1964).
    [35]Englert F.and Brout R.Broken Symmetry and the Mass of Gauge Vector Mesons,Phys.Rev.Lett 13,321(1964).
    [36]Guralnik G.S.,Hagen C.R.and Kibble T.W.B.Global Conservation Laws and Massless Particles,Phys.Rev.Lett 13,585(1964).
    [37]Christenson J.H.,Cronin J.W.,Fitch V.L and Turlay,.Evidence for the 2π Decay of the K2_0 Meson R.Phys.Rev.Lett 13,138(1964).
    [38]Salam A.and Ward J.C.Electromagnetic and weak interactions,Phys.Lett.13,168(1964).
    [39]Weinberg S.A Model of Leptons,Phys.Rev.Lett 19,1264(1967).
    [40]Faddeev L.D.and Popv V.N.Feynman diagrams for the Yang-Mills field,Phys.Lett.B 25,29(1967).
    [41]Glashow S.L.and etal.Weak Interactions with Lepton-Hadron Symmetry,Phys.Rev.D 2,1285(1970).
    [42]G.'t Hooft,Renormalization of massless Yang-Mills fields,Nucl.Phys.B 33,173(1971).
    [43]Kobayashi M.and Maskawa M.Prog.Theor.Phys.49,652(1973).
    [44]Machacek M.E.and etal.Higgs Bosons from Two-Gluon Annihilation in Proton-Proton Collisions,Phys.Rev.Lett 40,692(1978).
    [45]Hasert F.J.and etal.Search for elastic muon-neutrino electron scattering,Phys.Lett.B 46,121(1973).
    [46]Perl M.L.and etal.Evidence for Anomalous Lepton Production in e + e~+ Annihilation,Phys.Rev.Lett 35,1489(1975).
    [47]Amison G.and etal.Experimental observation of isolated large transverse energy electrons with associated missing energy at s~(1/2)=540GeV,Phys.Lett.B 122,103(1983),Phys.Lett.B 122,398(1983),
    [48]Bagnaia P.and etal.Evidence for Z~0→e+e~+ at the CERN p collider,Phys.Lett.B 129,130(1983).
    [49]Caso and etal.The European Physician Journal,1,(1998).
    [50]Suzuki Y.and etal.talk given at the ⅩⅨ International Symposium on Lepton and Photon Interactions at High energies Stanford University(1999)
    [51]ALEPH,DELPHI,L3,OPAL,and the LEP Working Group for Higgs Bosun Seaches,Technical Report No.ALEPH 99-081 CONF 99-052
    [52]Sher M.Electroweak Higgs potential and vacuum stability,Phys.Rep 179,273(1989).
    [53]Quiros M.etal.Improved Higgs mass stability bound in the standard model and implications for supersymmetry,Phys.Lett.B 342,171(1995).
    [54]Thacker H.B and etal.Weak interactions at very high energies:The role of the Higgs-boson mass,Phys.Rev.D 16,1519(1977).
    [55]Ross G.G.Grand Unified Theory,(Addision-Wesley Pub.CO.,Menlo Park)(1985).
    [56]Chanowitz M.and Gaillard M.K.The TeV physics of strongly interacting W's and Z's,Nucl.Phys.B 261,379(1985).
    [57]Bjorken J.D.,Proccedings of the Summer Institute on Particle Physics,technical Report No.LLAC-198
    [58]Cahn R.and Dawson S.Production of very massive Higgs bosons,Phys.Lett.B 136,196(1984).
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