CosMIn: The Solution to the Cosmological Constant Problem
arXiv:1302.3226 · doi:10.1142/S0218271813420017
Abstract
The current acceleration of the universe can be modeled in terms of a cosmological constant. We show that the extremely small value of ΛL_P^2 ~ 3.4 x 10^{-122}, the holy grail of theoretical physics, can be understood in terms of a new, dimensionless, conserved number CosMIn (N), 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-time accelerating phase.
ver 2 (6 pages, 2 figures) received Honorable Mention in the Gravity Research Foundation Essay Contest, 2013; to appear in Int.Jour.Mod.Phys. D
References in corpus (5)
Cited by in corpus (39)
- Cosmological constant and vacuum energy: old and new ideas
- Cosmological and Solar System Consequences of f(R,T) Gravity Models
- f(R,T) Cosmological Models in Phase Space
- General Relativity from a Thermodynamic Perspective
- Emergent Gravity Paradigm: Recent Progress
- Lanczos-Lovelock gravity from a thermodynamic perspective
- Grin of the Cheshire cat: Entropy density of spacetime as a relic from quantum gravity
- Consequences of energy conservation violation: Late time solutions of subclass of gravity using dynamical system approach
- Distribution function of the Atoms of Spacetime and the Nature of Gravity
- Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
- Quantum field theory in de Sitter and quasi-de Sitter spacetimes: Revisited
- Cosmic Acceleration From Matter-Curvature Coupling
- Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in gravity
- Cosmic Information, the Cosmological Constant and the Amplitude of primordial perturbations
- Entropy density of spacetime from the zero point length
- Gravity and Quantum Theory: Domains of Conflict and Contact
- Late-time cosmological evolution of a general class of f(R, T) gravity with minimal curvature-matter coupling
- Interpretation of gravity in terms of a conserved effective fluid
- Gravity and/is Thermodynamics
- Chameleon Field Dynamics During Inflation
- Evolution of quantum field, particle content and classicality in the three stage universe
- Emergence of cosmic space and its connection with thermodynamic principles
- Exploring the Nature of Gravity
- Dynamical systems of cosmological models for different possibilities of and
- Gravitational entropy of local cosmic voids
- Massless minimal quantum scalar field with an asymmetric self interaction in de Sitter spacetime
- Non-perturbative analysis for a massless minimal quantum scalar with in the inflationary de Sitter spacetime
- Lagrangian formulation for an extended cosmological equation-of-state
- Emergence of space and expansion of universe
- Cosmological Particle Creation Beyond de Sitter
- Cosmic Acceleration and Geodesic Deviation in Chameleon Scalar Field Model
- Resummation of local and non-local scalar self energies via the Schwinger-Dyson equation in de Sitter spacetime
- Ether and Relativity
- Cosmological Solutions of Chameleon Scalar Field Model
- Chameleon Gravity as an Alternative to Dark Matter
- Phase space analysis of a FRW cosmology in the MaxwellCattaneo approach
- Decaying vacuum and evolution from early inflation to late acceleration
- An interpretive conjecture for physics beyond the standard models: generalized complementarity
- New holographic dark energy and the modified Bekenstein-Hawking entropy