研究生: |
羅令崴 Luo, Ling-Wei |
---|---|
論文名稱: |
替代的引力理論與其宇宙學中的應用 Alternative Gravitational Theories and Their Cosmological Applications |
指導教授: |
耿朝強
Geng, Chao-Qiang |
口試委員: |
張維甫
Chang, We-Fu 何小剛 He, Xiao-Gang 倪維斗 Ni, Wei-Tou 高文芳 Kao, Win-Fun |
學位類別: |
博士 Doctor |
系所名稱: |
理學院 - 物理學系 Department of Physics |
論文出版年: | 2014 |
畢業學年度: | 102 |
語文別: | 英文 |
論文頁數: | 68 |
中文關鍵詞: | 引力理論 、規範理論 、宇宙學 、替代引力理論 、暗能量 、撓率 、絕對平行引力 、f(T) 理論 、大尺度磁場 、額外空間 、膜理論 、Kaluza-Klein 理論 |
外文關鍵詞: | gravitational theory, gauge theory, cosmology, alternative gravitational theories, dark energy, torsion, teleparallel gravity, f(T) theories, large-scale magnetic fields, extra dimension, braneworld theory, Kaluza-Klein theory |
相關次數: | 點閱:2 下載:0 |
分享至: |
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We study the cosmological evolutions of the equation of state for dark energy $w_{\mathrm{DE}}$ in the exponential and logarithmic as well as their combination $f(T)$ theories. We show that the crossing of the phantom divide line of $w_{\mathrm{DE}} = -1$ can be realized in the combined $f(T)$ theory even though it cannot be in the pure exponential or logarithmic $f(T)$ theory. In particular, the crossing is from $w_{\mathrm{DE}} > -1$ to $w_{\mathrm{DE}} < -1$, in the opposite manner from $f(R)$ gravity models. We also demonstrate that this feature is favored by the recent observational data.
We explore the generation of large-scale magnetic fields from inflation in teleparallelism, in which the gravitational theory is described by the torsion scalar instead of the scalar curvature in general relativity. In particular, we examine the case that the conformal invariance of the electromagnetic field during inflation is broken by a non-minimal gravitational coupling between the torsion scalar and the electromagnetic field. It is shown that for a power-law type coupling, the magnetic field on 1~Mpc scale with its strength of $\sim 10^{-9}$~G at the present time can be generated.
We study teleparallel gravity in five-dimensional spacetime with particular discussions on Kaluza-Klein (KK) and braneworld theories. We directly perform the dimensional reduction by differential forms. In the braneworld theory, the teleparallel gravity formalism in the Friedmann-Lema\^{i}tre-Robertson-Walker cosmology is equivalent to GR due to the same Friedmann equation, whereas in the KK case the reduction of our formulation does not recover the effect as GR of 4-dimensional spacetime due to an additional coupling between the derivative of scalar field and torsion, which results in some different behavior from general relativity.
We study the cosmological evolutions of the equation of state for dark energy $w_{\mathrm{DE}}$ in the exponential and logarithmic as well as their combination $f(T)$ theories. We show that the crossing of the phantom divide line of $w_{\mathrm{DE}} = -1$ can be realized in the combined $f(T)$ theory even though it cannot be in the pure exponential or logarithmic $f(T)$ theory. In particular, the crossing is from $w_{\mathrm{DE}} > -1$ to $w_{\mathrm{DE}} < -1$, in the opposite manner from $f(R)$ gravity models. We also demonstrate that this feature is favored by the recent observational data.
We explore the generation of large-scale magnetic fields from inflation in teleparallelism, in which the gravitational theory is described by the torsion scalar instead of the scalar curvature in general relativity. In particular, we examine the case that the conformal invariance of the electromagnetic field during inflation is broken by a non-minimal gravitational coupling between the torsion scalar and the electromagnetic field. It is shown that for a power-law type coupling, the magnetic field on 1~Mpc scale with its strength of $\sim 10^{-9}$~G at the present time can be generated.
We study teleparallel gravity in five-dimensional spacetime with particular discussions on Kaluza-Klein (KK) and braneworld theories. We directly perform the dimensional reduction by differential forms. In the braneworld theory, the teleparallel gravity formalism in the Friedmann-Lema\^{i}tre-Robertson-Walker cosmology is equivalent to GR due to the same Friedmann equation, whereas in the KK case the reduction of our formulation does not recover the effect as GR of 4-dimensional spacetime due to an additional coupling between the derivative of scalar field and torsion, which results in some different behavior from general relativity.
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