Cosmology in the Lorentz gauge theory

被引:4
|
作者
Koivisto, Tomi [1 ,2 ]
机构
[1] Univ Tartu, Inst Phys, Lab Theoret Phys, W Ostwaldi 1, EE-50411 Tartu, Estonia
[2] NICPB, Ravala Pst 10, EE-10143 Tallinn, Estonia
关键词
Foundations of cosmology; the problem of time; gauge theory of spacetime and gravity; dark energy and dark matter; cosmological inflation; pregeometric theory of physics; GRAVITY; VARIABLES; GEOMETRY;
D O I
10.1142/S0219887824500403
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This proceeding is an introduction to cosmological applications of the Lorentz gauge theory. It provides the ingredients for a unique, though yet tentative Lambda CDM theory of cosmology. Emergence of spacetime is described by the spontaneous symmetry breaking called here the khronogenesis. Space is then associated with the field strength of the antiself-dual gauge potential, and gravity is associated with the self-dual field strength. In the cosmological setting, khronogenesis seems to predict inflation. It is shown that the Lorentz gauge theory allows the consistent description of spin currents which could have important roles in cosmological phenomenology.
引用
收藏
页数:24
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