Please wait a minute...
Chinese Physics, 2007, Vol. 16(12): 3560-3565    DOI: 10.1088/1009-1963/16/12/002
GENERAL Prev   Next  

The double Lagrangian with U(1, J) symmetry and its applications to the cosmology

Wu Ya-Bo(吴亚波), Lü Jian-Bo(吕剑波), He Jing(贺敬), and Fu Ming-Hui(付明慧)
Department of Physics, Liaoning Normal University, Dalian 116029, China
Abstract  By introducing the double complex scalar field, this paper constructs the double Lagrangian with the potential $V({\it\Phi}(J), {\it\Phi}^{*}(J))=V(|{\it\Phi}(J)|)$, which not only can describe the evolution of quintom Universe, but also can naturally give the spintessence and hessence Universe. Furthermore, the $U(1,J)$ symmetry of the double complex Lagrangian is verified, and the total conserved charge within the physical volume is derived by means of the No?ther theorem. Moreover, it can point out that the `imaginary motion' of the angular parameter in Ref.[14], in fact, is only a real phase displacement in our model.
Keywords:  double Lagrangian density      canonical scalar field      dark energy  
Accepted manuscript online: 
PACS:  98.80.Cq (Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))  
  11.10.Ef (Lagrangian and Hamiltonian approach)  
  95.36.+x (Dark energy)  
Fund: Project supported by the National Natural Science Foundation of China (Grant No~10475036) and the Scientific Research Foundation of the Higher Education Institute of Liaoning Province under (Grant No~05L215).

Cite this article: 

Wu Ya-Bo(吴亚波), Lü Jian-Bo(吕剑波), He Jing(贺敬), and Fu Ming-Hui(付明慧) The double Lagrangian with U(1, J) symmetry and its applications to the cosmology 2007 Chinese Physics 16 3560

[1] Quadratic interaction effect on the dark energy density in the universe
Derya G Deveci, Ekrem Aydiner. Chin. Phys. B, 2017, 26(10): 109501.
[2] Mechanical properties of the thermal equilibrium Friedmann-Robertson-Walker universe model
Wei Yi-Huan (魏益焕), Lan Tian-Bao (兰天葆), Zhang Yue-Zhu (张月竹), Fu Yan-Yan (付妍妍). Chin. Phys. B, 2014, 23(5): 050401.
[3] Thermodynamic properties of Reissner–Nordström–de Sitter quintessence black holes
Wei Yi-Huan (魏益焕), Ren Jun (任军). Chin. Phys. B, 2013, 22(3): 030402.
[4] New initial condition of the new agegraphic dark energy model
Li Yun-He (李云鹤), Zhang Jing-Fei (张敬飞), Zhang Xin (张鑫). Chin. Phys. B, 2013, 22(3): 039501.
[5] Constraints on the unified model of dark matter and dark energy
Lü Jian-Bo(吕剑波), Wu Ya-Bo(吴亚波), Xu Li-Xin(徐立昕), and Wang Yu-Ting(王钰婷) . Chin. Phys. B, 2011, 20(7): 079801.
[6] Growth of linear matter perturbations and current observational constraints
Fu Xiang-Yun(付响云), Wu Pu-Xun(吴普训), and Yu Hong-Wei(余洪伟). Chin. Phys. B, 2010, 19(7): 079801.
[7] Exact solution of phantom dark energy model
Wang Wen-Fu(王文福), Shui Zheng-Wei(税正伟), and Tang Bin(唐斌). Chin. Phys. B, 2010, 19(11): 119801.
[8] Effects of dark energy interacting with massive neutrinos and dark matter on universe evolution
Chen Ju-Hua(陈菊华) and Wang Yong-Jiu(王永久). Chin. Phys. B, 2010, 19(1): 010401.
[9] Reconstructing dark energy potentials from parameterized deceleration parameters
Wang Yu-Ting(王钰婷), Xu Li-Xin(徐立昕), Lü Jian-Bo(吕剑波), and Gui Yuan-Xing(桂元星) . Chin. Phys. B, 2010, 19(1): 019801.
[10] New agegraphic dark energy as a rolling tachyon
Cui Jing-Lei(崔晶磊),Zhang Li(张莉), Zhang Jing-Fei(张敬飞), and Zhang Xin(张鑫) . Chin. Phys. B, 2010, 19(1): 019802.
[11] Observational constraints on the accelerating universe in the framework of a 5D bounce cosmological model
Lü Jian-Bo(吕剑波), Xu Li-Xin(徐立昕), Liu Mo-Lin(刘墨林), and Gui Yuan-Xing(桂元星). Chin. Phys. B, 2009, 18(4): 1711-1720.
[12] Influence of dark energy on time-like geodesic motion in Schwarzschild spacetime
Chen Ju-Hua(陈菊华) and Wang Yong-Jiu(王永久). Chin. Phys. B, 2008, 17(4): 1184-1188.
[13] Dynamics of quintessential inflation
Zhai Xiang-Hua(翟向华) and Zhao Yi-Bin(赵一斌). Chin. Phys. B, 2006, 15(10): 2465-2469.
No Suggested Reading articles found!