Affine connections in quantum gravity and new scalar fields

被引:2
作者
Ghosh, Kaushik [1 ]
机构
[1] Univ Calcutta, Vivekananda Coll, 269 Diamond Harbour Rd, Kolkata 700063, India
来源
PHYSICS OF THE DARK UNIVERSE | 2019年 / 26卷
关键词
Affine connections; Quantum cosmology; Scalar fields; Dark energy; Inflation; PROBE WMAP OBSERVATIONS; GENERAL-RELATIVITY; TORSION; RENORMALIZATION; CONSTANT; EINSTEIN;
D O I
10.1016/j.dark.2019.100403
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this manuscript, we will discuss the construction of covariant derivative operator in quantum gravity. We will find it is more perceptive alternative to use affine connections more general than metric compatible connections in quantum gravity. We will demonstrate this using the canonical quantization procedure. This is valid irrespective of the presence and nature of sources. The conventional Palatini and metric-affine formalisms, where the actions are linear in the scalar curvature with metric and affine connections being the independent variables, are not much suitable to construct a source-free theory of gravity with general affine connections. This is also valid for many minimally coupled interacting theories where sources only couple with metric by using the Levi-Civita connections exclusively. We will discuss potential formalism of affine connections to introduce affine connections more general than metric compatible connections in gravity. We will also discuss possible extensions of the actions for this purpose. General affine connections introduce new fields in gravity besides metric. In this article, we will consider a simple potential formalism with symmetric affine connections and symmetric Ricci tensor. Corresponding affine connections introduce only two massless scalar fields. One of these fields contributes a stress-tensor with opposite sign to the sources of Einstein's equation when we state the equation using the Levi-Civita connections. This means we have a massless scalar field with negative stress-tensor in Einstein's equation. These scalar fields can be useful to explain dark energy and inflation. These fields bring us beyond strict local Minkowski geometries. (c) 2019 Elsevier B.V. All rights reserved.
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页数:11
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