On scalar and vector fields coupled to the energy-momentum tensor

被引:7
|
作者
Beltran Jimenez, Jose [1 ,2 ]
Cembranos, Jose A. R. [3 ,4 ]
Sanchez Velazquez, Jose M. [3 ,4 ]
机构
[1] Univ Autonoma Madrid, Inst Fis Teor, CSIC, E-28049 Madrid, Spain
[2] Univ Salamanca, Dept Fis Fundamental, E-37008 Salamanca, Spain
[3] Univ Complutense Madrid, Dept Fis Teor, E-28040 Madrid, Spain
[4] Univ Complutense Madrid, UPARCOS, E-28040 Madrid, Spain
来源
关键词
Classical Theories of Gravity; Effective Field Theories; ANGULAR-MOMENTUM; BRANE; GRAVITATION; DIMENSIONS; COSMOLOGY; DYNAMICS; SEARCH; TRACE;
D O I
10.1007/JHEP05(2018)100
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We consider theories for scalar and vector fields coupled to the energy momentum tensor. Since these fields also carry a non-trivial energy-momentum tensor, the coupling prescription generates self-interactions. In analogy with gravity theories, we build the action by means of an iterative process that leads to an infinite series, which can be resumed as the solution of a set of differential equations. We show that, in some particular cases, the equations become algebraic and that is also possible to find solutions in the form of polynomials. We briefly review the case of the scalar field that has already been studied in the literature and extend the analysis to the case of derivative (disformal) couplings. We then explore theories with vector fields, distinguishing between gauge and non-gauge-invariant couplings. Interactions with matter are also considered, taking a scalar field as a proxy for the matter sector. We also discuss the ambiguity introduced by superpotential (boundary) terms in the definition of the energy-momentum tensor and use them to show that it is also possible to generate Galileon-like interactions with this procedure. We finally use collider and astrophysical observations to set constraints on the dimensionful coupling which characterises the phenomenology of these models.
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页数:45
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