CosMIn: THE SOLUTION TO THE COSMOLOGICAL CONSTANT PROBLEM

The current acceleration of the universe can be modeled in terms of a cosmological constant Lambda. We show that the extremely small value of Lambda L-P(2) approximate to 3.4 x 10(-122), 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 approximate to 4 pi. 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.