Autor: |
PADMANABHAN, HAMSA, PADMANABHAN, T. |
Předmět: |
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Zdroj: |
International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology; Oct2013, Vol. 22 Issue 12, p-1, 7p, 2 Graphs |
Abstrakt: |
The current acceleration of the universe can be modeled in terms of a cosmological constant Λ. We show that the extremely small value of , the holy grail of theoretical physics, can be understood in terms of a new, dimensionless, conserved number Cosmic Mode Index (CosMIn), which counts the number of modes crossing the Hubble radius during the three phases of evolution of the universe. Theoretical considerations suggest that N ≈ 4π. This single postulate leads us to the correct, observed numerical value of the cosmological constant! This approach also provides a unified picture of cosmic evolution relating the early inflationary phase to the late accelerating phase. [ABSTRACT FROM AUTHOR] |
Databáze: |
Complementary Index |
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