Review on Dark Energy Models
- Авторы: Tawfik A.N.1,2,3, El Dahab E.A.3,4
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Учреждения:
- Nile University
- Frankfurt Institute for Advanced Studies
- World Laboratory for Cosmology And Particle Physics (WLCAPP)
- Faculty of Computers and Information
- Выпуск: Том 25, № 2 (2019)
- Страницы: 103-115
- Раздел: Article
- URL: https://ogarev-online.ru/0202-2893/article/view/176293
- DOI: https://doi.org/10.1134/S0202289319020154
- ID: 176293
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Аннотация
Based on quantum mechanics and general relativity, Karolyhazy proposed a generalization to the well-known Heisenberg uncertainty relation in which the energy density of quantum fluctuations of space-time plays a crucial role. Later on, various holographic DE models were suggested, in which the Hubble scale (size) and the age of the universe were assumed as measures for the largest infrared cutoff satisfying the holographic principle and energy bounds assuring applicability of quantum field theory. We review various models based on the holographic principle and the Karolyhazy relation and compare these to the space-time foam and superconducting DE models. We analyze their (in)stability against cosmological perturbation.
Об авторах
Abdel Tawfik
Nile University; Frankfurt Institute for Advanced Studies; World Laboratory for Cosmology And Particle Physics (WLCAPP)
Автор, ответственный за переписку.
Email: atawfik@nu.edu.eg
Египет, Juhayna Square of 26th-July-Corridor, Giza, 12588; Frankfurt, 60438; Cairo, 11571
Eiman El Dahab
World Laboratory for Cosmology And Particle Physics (WLCAPP); Faculty of Computers and Information
Email: atawfik@nu.edu.eg
Египет, Cairo, 11571; Cairo, 11671
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