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Pre-inflation from the multiverse: can it solve the quadrupole problem in the cosmic microwave background?
João Morais1, Mariam Bouhmadi-López1,2, Manuel Krämer3
11Department of Theoretical Physics, University of the Basque Country UPV/EHU, P.O. Box 644, 48080 Bilbao, Spain.
This study explores a multiverse model using quantum cosmology. It finds that while the pre-inflationary phase doesn't resolve the cosmic microwave background quadrupole issue, it suggests potential alternative explanations.
Area of Science:
- Cosmology
- Quantum Gravity
- Theoretical Physics
Background:
- Eternal inflation proposes continuous universe creation.
- The Wheeler-DeWitt equation is a key tool in quantum cosmology.
- The cosmic microwave background (CMB) exhibits anomalies on large scales, like the quadrupole issue.
Purpose of the Study:
- To analyze a quantized toy model of eternal inflation.
- To investigate the pre-inflationary phase of sub-universes within a multiverse.
- To determine if this pre-inflationary phase can explain CMB anomalies, specifically the quadrupole issue.
Main Methods:
- Utilizing a quantum-field-theoretical formulation of the Wheeler-DeWitt equation.
- Applying the 'third quantization' method to model universe creation.
- Calculating the influence of the pre-inflationary phase on the CMB power spectrum.
Main Results:
- The eternally inflating universe is modeled as a multiverse with distinct sub-universe phases.
- The pre-inflationary phase of a sub-universe was analyzed from its perspective.
- The specific model analyzed did not resolve the CMB quadrupole issue.
Conclusions:
- The analyzed pre-inflationary phase does not explain the CMB quadrupole anomaly.
- The study suggests potential avenues for resolving the CMB quadrupole issue.
- The third quantization method provides a framework for multiverse cosmology.
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