Connecting the nonsingular origin of the universe, the vacuum structure and the cosmological constant problem

Keyphrases

• Scale Invariance 100%
• Vacuum Structure 100%
• Cosmological Constant Problem 100%
• Origin of the Universe 100%
• Spontaneous Symmetry Breaking 66%
• Vacuum Energy Density 66%
• Dilaton 66%
• Inflationary Phase 66%
• Range of Values 33%
• Scalar Field 33%
• Nonlinearity 33%
• Equations of Motion 33%
• Sqrt 33%
• Accelerating Universe 33%
• Smooth Transition 33%
• Volume Element 33%
• Vacuum Energy 33%
• Flat Region 33%
• Zero-point Fluctuations 33%
• Einstein Frame 33%
• Effective Potential 33%
• Emergent Universe 33%
• Dilaton Field 33%
• Emergent Universe Scenarios 33%
• Einstein Static Universe 33%
• Cosmological Term 33%
• First-order Formalism 33%

Physics

• Flux Density 100%
• Broken Symmetry 100%
• Cosmological Constant 100%
• Origin of the Universe 100%
• Equation of Motion 50%