Accelerating Universe and the Scalar-Tensor Theory

被引:2
|
作者
Fujii, Yasunori [1 ]
机构
[1] Waseda Univ, Adv Res Inst Sci & Engn, Tokyo 1698555, Japan
关键词
accelerating universe; scalar-tensor theory; Nambu-Goldstone boson; spontaneous breaking; dilaton; conformal transformation; mini-inflation; dark energy; DELTA-ALPHA/ALPHA; CONSTANT; GRAVITY; DILATON; ENERGY;
D O I
10.3390/e14101997
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
To understand the accelerating universe discovered observationally in 1998, we develop the scalar-tensor theory of gravitation originally due to Jordan, extended only minimally. The unique role of the conformal transformation and frames is discussed particularly from a physical point of view. We show the theory to provide us with a simple and natural way of understanding the core of the measurements, Lambda(obs) similar to t(0)(-2) for the observed values of the cosmological constant and today's age of the universe both expressed in the Planckian units. According to this scenario of a decaying cosmological constant, Lambda(obs) is this small only because we are old, not because we fine-tune the parameters. It also follows that the scalar field is simply the pseudo Nambu-Goldstone boson of broken global scale invariance, based on the way astronomers and astrophysicists measure the expansion of the universe in reference to the microscopic length units. A rather phenomenological trapping mechanism is assumed for the scalar field around the epoch of mini-inflation as observed, still maintaining the unmistakable behavior of the scenario stated above. Experimental searches for the scalar field, as light as similar to 10(-9) eV, as part of the dark energy, are also discussed.
引用
收藏
页码:1997 / 2035
页数:39
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