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Samanta, G.C., Mishra, B.. (1394). Anisotropic Cosmological Model in presence of holographic dark energy and quintessence. , (), -. doi: 10.22099/ijsts.2015.3226
G.C. Samanta; B. Mishra. "Anisotropic Cosmological Model in presence of holographic dark energy and quintessence". , , , 1394, -. doi: 10.22099/ijsts.2015.3226
Samanta, G.C., Mishra, B.. (1394). 'Anisotropic Cosmological Model in presence of holographic dark energy and quintessence', , (), pp. -. doi: 10.22099/ijsts.2015.3226
Samanta, G.C., Mishra, B.. Anisotropic Cosmological Model in presence of holographic dark energy and quintessence. , 1394; (): -. doi: 10.22099/ijsts.2015.3226

Anisotropic Cosmological Model in presence of holographic dark energy and quintessence

Iranian Journal of Science
مقالات آماده انتشار، پذیرفته شده، انتشار آنلاین از تاریخ 26 مهر 1394
نوع مقاله: Regular Paper
شناسه دیجیتال (DOI): 10.22099/ijsts.2015.3226
نویسندگان
G.C. Samanta1؛ B. Mishra* 2
1Birla Institute of Technology and Science-Pilani, KK Birla Goa Campus
2Birla Institute of Technology and Science-Pilani, Hyderabad Campus
چکیده
The problem of Bianchi type III universe filled with matter and holographic dark energy (DE) components is investigated. In order to obtain a determinant solution, special law of variation for Hubble's parameter proposed by Berman (1983) has been considered. The relationship between holographic dark energy model with the quintessence dark energy has been established. Quintessence potential and dynamics of the quintessence scalar field are reconstructed, which describes the accelerated phase of the
expanding universe.
کلیدواژه‌ها
Holographic dark energy؛ quintessence؛ Equation of state؛ Bianchi type-III space time؛ General relativity
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تعداد مشاهده مقاله: 7,414


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