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A test of the Copernican principle
1Department of Physics & Astronomy, 6127 Wilder Lab, Dartmouth College, Hanover, NH 03755, USA.
The cosmic microwave background (CMB) spectrum can test the Copernican principle. Current data excludes large voids mimicking cosmic acceleration, but more sensitive measurements could reveal such structures or confirm our place in the universe.
Area of Science:
- Cosmology
- Astrophysics
- Fundamental Physics
Background:
- The cosmic microwave background (CMB) radiation provides a unique probe of the early universe.
- The Copernican principle posits that Earth does not occupy a privileged position in the universe.
- Deviations from a perfect blackbody spectrum in the CMB could indicate large-scale structures or unusual cosmological conditions.
Purpose of the Study:
- To perform a modern test of the Copernican principle using the CMB spectrum.
- To constrain the possibility of our location within a large cosmic void.
- To investigate whether cosmic acceleration could be mimicked by residing in such a void.
Main Methods:
- Analyzing the blackbody spectrum of the CMB radiation.
- Utilizing the reionized universe as a reflective medium for CMB photons.
- Comparing CMB spectral measurements with theoretical models of large voids.
Main Results:
- Current spectral distortion limits exclude the largest voids that could mimic cosmic acceleration.
- A limit is placed on the possibility of occupying a privileged location at the center of a void.
- The Hubble diagram inferred from a void center might be misinterpreted as cosmic acceleration.
Conclusions:
- The CMB spectrum serves as a powerful tool to test fundamental cosmological principles.
- Sensitive CMB measurements are crucial to either confirm the Copernican principle or detect large-scale voids.
- Misinterpretation of cosmological data, such as cosmic acceleration, is possible without considering peculiar locations.
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