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电磁场作用的Q球解及其能量稳定性质 被引量:1

Q-ball Solutions with Electromagnetic Field Coupling and Their Energy Stability
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摘要 暗物质的理论与实验研究是天体粒子物理学的重要研究课题,暗物质是宇宙中物质的主要组成部分,并对星系的结构和形成产生重要影响.暗物质可能是由最轻的超对称粒子构成,这些标量粒子在宇宙中以非拓扑孤子—Q球的形式存在.通过求解具有耦合势能形式的Klein-Gordon方程,获得了均匀及非均匀标量场模型中带电Q球的精确解,分别用解析和数值分析的方法计算了2种Q球的总能量,结果表明带电Q球模型中也存在能量稳定性.为进一步研究暗物质实验和观测提供研究方法和理论基础. Research of dark-matter theory and experiment study are important topics of astroparticle physics, because dark-matter is the main part of all the matter in the universe, and it has a great influence on the structure and formation of galaxies. Dark matter may be composed of the lightest supersymmetry particles, and these scalar particles exist in the universe in the form of non-topological solitons:Q-ball. In this paper, by solving Klein-Gordon equations with coupling potentials, exact solutions of charged Q-balls in uniform and variational sealer field models are obtained, and the total energy of the two kinds of Q-balls is calculated by using analytic and numerical methods respectively. The results show that energy stability can also exist in the charged Q-ball model, which can supply the research method and theory foundation for the further experiment and observation of dark matter.
出处 《四川师范大学学报(自然科学版)》 CAS CSCD 北大核心 2013年第1期81-86,共6页 Journal of Sichuan Normal University(Natural Science)
基金 四川省教育厅自然科学重点基金(11ZA100)资助项目
关键词 电磁场 复标量场模型 Q球解 能量稳定性 electromagnetic field complex scalar field model Q-ball solutions energy stability
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参考文献42

  • 1Coleman S. Q-balls[J]. Nuel Phys,1985,B262(2) :263 -283.
  • 2Madsen J. Detecting supersymmetric Q -balls with neutron stars[ J]. Phys Lett, 1998,13435 (1/2) :125 - 130.
  • 3Axenides M, Floratos E, Kehagias A. Non-Abelian Q-balls in supersymmetric theories[J]. Plays Lett,1998,B444(1/2):190- 195.
  • 4Kusenko A, Kuzmin V, Shaposhnikov M, et al. Experimental signatures of supersymmetric dark matter Q -balls[ J]. Phys Rev Lett,1998,80(15) :3185 -3188.
  • 5Kusenko A, Shaposhnikov M. Supersymmetric Q - balls as dark matter [ J ]. Phys Lett, 1998, B418 (1/2) :46 - 54.
  • 6Enqvist K, McDonald J. Q -Balls and baryogenesis in the MSSM[J]. Phys Lett,1998,B425(3/4) :309 -321.
  • 7Takenaga Y, Abe K, Hayato Y, et al. Search for neutral Q - halls in super - Kamiokande[J]. Phys Lett ,2007 ,B647 ( 1 ) : 18 - 22.
  • 8Campanelli L, Ruggieri M. Supersymmetric Q- balls:A numerical study[ J]. Phys Rev,2008,1377 (4):043504.
  • 9Shoemaker ! M, Kusenko A. The ground states of baryoleptonic Q - balls in supersymmetric models [ J 1. Phys Rev, 2008, D78 (7) :075014.
  • 10Shoemaker I M. Astrophage of neutron stars from supersymmetric dark matter Q - balls [ J ]. Phys Rev,2009, DS0 (3) :031702.

二级参考文献21

  • 1Coleman S. Q-balls[J]. Nucl Phys,1985,B262(2) :263 -283.
  • 2Arodz H, Karkowski J, Swierczynski Z. Spinning Q - balls in the complex signum - Gorclon model[ J]. Phy Rev,2009, D80(6):067702-1 -4.
  • 3MacKenzie R B . From Q - walls to Q -balls[ J]. J High Energy Physics,2001,0108 :003 -010.
  • 4Kusenko A, Shoemarker Ian M. Neutrinos from the terrestrial passage of supersymmetric dark matter Q ~ balls[ J]. Phys Rev,2009,D80(2) :027701 -1 -4.
  • 5Deshaies - Jacques M,Mackenzie R. Q - balls in Maxwell - Chem - Simons theory[j]. Hiys Rev,2006,D74(2) ;Q25006 -1 一 6.
  • 6Sanchez 一Guillen J, Adam C, Wereszczynski A. Hopf solitons and hopf Q - balls on 53[ J]. Eur Phys J,2006,47:513 — 524.
  • 7Kleihaus B,Kunz J,List M,et al. Rotating boson stars and Q - balls II : Negative parity and ergoregions [ J ]. Phys Rev ,2008,D77(6) :064025 -l -16.
  • 8Kleihaus B, Kunz J, List M. Rotating boson stars and Q - balls[ J]. Phys Rev,2005,D72(6) :064002 - 1 - 17.
  • 9Postam M. Solitosynthesis of Q - balls[ J]. Phys Rev,2002,D65(8) :085035 - 1 -9.
  • 10Palti E, Saffin P M, Copeland E J. Dynamics of Q - balls in an expanding universe[J]. Phys Rev,20(M-,D70(8) ;083520-1 -6.

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同被引文献35

  • 1Hoekstra H,Yee H K C,Gladders M D. Current status of weak gravitational lensing[J].{H}New Astronomy Reviews,2002,(12):767-781.
  • 2Clowe D,Brada(c) M,Gonzalez A H. A direct empirical proof of the existence of dark matter[J].{H}Astrophysics Journal,2006,(2):L109-L113.
  • 3Komatsu E,Dunkley J,Nolta M R. Five-year wilkinson microwave anisotropy probe (WMAP) observations:cosmological interpretation[J].{H}Astrophys J Suppl,2009,(2):330-376.
  • 4Olive K A,Steigman G,Walker T P. Primordial nucleosynthesis:theory and observations[J].{H}PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS,2000,(4/6):389-407.
  • 5Ilyin A S,Zybin K P,Gurevich A V. Dark matter in galaxies and growth of giant black holes[J].J Exp Theory Phys,2004,(1):1-13.
  • 6Filippi S,Ponce W A,Sanchez L A. Dark matter from the scalar sector of 3-3-1 models without exotic electric charges[J].{H}EUROPHYSICS LETTERS,2006,(1):142-148.
  • 7Frenk C S,White S D M,Efstathiou G. Cold dark matter,the structure of galactic haloes and the origin of the Hubble sequence[J].{H}NATURE,1985,(1):595-597.
  • 8Efstathiou G,Sutherland W J,Maddox S J. The cosmological constant and cold dark matter[J].{H}NATURE,1990,(1):705-707.
  • 9Rubin V. The rotation of spiral galaxies[J].{H}SCIENCE,1983,(4604):1339-1344.
  • 10Borriello A,Salucci P. The dark matter distribution in disk galaxies[J].{H}Monthly Notices of the Royal Astronomical Society,2001,(2):285-292.

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