Mimetic Einstein-Cartan-Sciama-Kibble (ECSK) gravity

被引:11
|
作者
Izaurieta, Fernando [1 ]
Medina, Perla [1 ,2 ,3 ]
Merino, Nelson [4 ]
Salgado, Patricio [4 ]
Valdivia, Omar [4 ,5 ]
机构
[1] Univ Concepcion, Dept Fis, Casilla 160-C, Concepcion, Chile
[2] Univ Austral Chile UACh, Campus Isla Teja,Ed Emilio Pugin, Valdivia, Chile
[3] Ctr Estudios Cient, Ave Arturo Prat 514, Valdivia, Chile
[4] Univ Arturo Prat, Inst Ciencias Exactas & Nat ICEN, Fac Ciencias, Iquique, Chile
[5] Inst Space Sci IEEC CSIC, C Can Magrans S-N, Cerdanyola Del Valles 08193, Barcelona, Chile
关键词
Classical Theories of Gravity; Cosmology of Theories beyond the SM; GENERAL-RELATIVITY; GAUGE-THEORY; DARK-MATTER; TORSION; SPIN; CONNECTION; INFLATION; EQUATIONS; UNIVERSE;
D O I
10.1007/JHEP10(2020)150
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
In this paper, we formulate the Mimetic theory of gravity in first-order formalism for differential forms, i.e., the mimetic version of Einstein-Cartan-Sciama-Kibble (ECSK) gravity. We consider different possibilities on how torsion is affected by Weyl transformations and discuss how this translates into the interpolation between two different Weyl transformations of the spin connection, parameterized with a zero-form parameter lambda. We prove that regardless of the type of transformation one chooses, in this setting torsion remains as a non-propagating field. We also discuss the conservation of the mimetic stress-energy tensor and show that the trace of the total stress-energy tensor is not null but depends on both, the value of lambda and spacetime torsion.
引用
收藏
页数:25
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