Cosmological reconstruction and Om diagnostic analysis of Einstein-Aether theory

被引:12
作者
Pasqua, Antonio [1 ]
Chattopadhyay, Surajit [2 ]
Momeni, Davood [3 ,4 ]
Raza, Muhammad [5 ,6 ]
Myrzakulov, Ratbay [3 ,4 ]
Faizal, Mir [7 ,8 ]
机构
[1] Univ Trieste, Dept Phys, Via Valerio 2, I-34127 Trieste, Italy
[2] Pailan Coll Management & Technol, Bengal Pailan Pk, Kolkata 700104, India
[3] Eurasian Natl Univ, Eurasian Int Ctr Theoret Phys, Astana 010008, Kazakhstan
[4] Eurasian Natl Univ, Dept Gen & Theoret Phys, Astana 010008, Kazakhstan
[5] COMSATS Inst Informat Technol, Dept Math, Sahiwal 57000, Pakistan
[6] Zhejiang Univ, Dept Opt Engn, State Key Lab Modern Opt Instrumentat, Ctr Opt & Electromagnet Res, Hangzhou 310058, Zhejiang, Peoples R China
[7] Univ British Columbia Okanagan, Irving K Barber Sch Arts & Sci, Kelowna, BC V1V 1V7, Canada
[8] Univ Lethbridge, Dept Phys & Astron, Lethbridge, AB T1K 3M4, Canada
关键词
modified gravity; quantum gravity phenomenology; supernova type Ia - standard candles; PROBE WMAP OBSERVATIONS; EMERGENT UNIVERSE; INFRARED CUTOFF; ACCELERATION; STATEFINDER; GRAVITY; MODELS; CONSTRAINTS; SYMMETRY; SPECTRUM;
D O I
10.1088/1475-7516/2017/04/015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we analyze the cosmological models in Einstein-Aether gravity, which is a modified theory of gravity in which a time-like vector field breaks the Lorentz symmetry. We use this formalism to analyse different cosmological models with different behavior of the scale factor. In this analysis, we use a certain functional dependence of the Dark Energy (DE) on the Hubble parameter H. It will be demonstrated that the Aether vector field has a non-trivial effect on these cosmological models. We also perform the Om diagnostic in Einstein-Aether gravity and we fit the parameters of the cosmological models using recent observational data.
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页数:27
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