Invariant solutions and Noether symmetries in hybrid gravity

被引:33
|
作者
Borowiec, Andrzej [1 ]
Capozziello, Salvatore [2 ,3 ,4 ]
De laurentis, Mariafelicia [2 ,3 ,5 ,6 ]
Lobo, Francisco S. N. [7 ]
Paliathanasis, Andronikos [2 ,3 ]
Paolella, Mariacristina [2 ,3 ]
Wojnar, Aneta [1 ]
机构
[1] Inst Theoret Phys, PL-50204 Wroclaw, Poland
[2] Univ Naples Federico II, Dipartimento Fis, I-80126 Naples, Italy
[3] Compl Univ Monte S Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[4] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy
[5] Tomsk State Pedag Univ, Tomsk 634061, Russia
[6] Natl Res Tomsk State Univ, Tomsk 634050, Russia
[7] Univ Lisbon, Ctr Astron & Astrofis, P-1749016 Lisbon, Portugal
来源
PHYSICAL REVIEW D | 2015年 / 91卷 / 02期
关键词
NOTHERS SYMMETRIES; COSMOLOGY;
D O I
10.1103/PhysRevD.91.023517
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Symmetries play a crucial role in physics and, in particular, the Noether symmetries are a useful tool both to select models motivated at a fundamental level, and to find exact solutions for specific Lagrangians. In this work, we apply Noether point symmetries to metric-Palatini hybrid gravity in order to select the f(R) functional form and to find analytical solutions for the field equations and for the related Wheeler-DeWitt (WDW) equation. It is important to stress that hybrid gravity implies two definitions of curvature scalar: R for standard metric gravity and R for further degrees of freedom related to the Palatini formalism. We use conformal transformations in order to find out integrable f(R) models. In this context, we explore two conformal transformations of the forms d tau = N(a)dt and dt = N(phi)dt. For the former, we found two cases of f(R) functions where the field equations admit Noether symmetries. In the second case, the Lagrangian reduces to a Brans-Dicke-like theory with a general coupling function. For each case, it is possible to transform the field equations by using normal coordinates to simplify the dynamical system and to obtain exact solutions. Furthermore, we perform quantization and derive the WDW equation for the minisuperspace model. The Lie point symmetries for the WDW equation are determined and used to find invariant solutions. In particular, hybrid gravity introduces a further term in cosmic dynamics whose interpretation is related to the signature of an auxiliary scalar field. Solutions are compared with ACDM.
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页数:14
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