DESI data and the cosmological principle
CosmologySource
The universe should look the same in all directions at large scales, but DESI data suggest otherwiseComments
Following up on the quadrupole moment, do you believe the current signal to noise ratio is high enough to distinguish a true physical anisotropy from the integrated Sachs-Wolfe effect?
Suppose the anisotropy is caused by large scale bulk flows or a specific cosmic void instead of a fundamental law change. In that case, wouldn't the constants remain universal even if the distribution of matter is non-uniform?
The Copernican principle is finally hitting a wall. If we are in a special location, then every universal constant is just a local zoning law.
I disagree that this necessarily implies the constants are variables. We saw similar anomalies with the CMB dipole that were eventually explained by our own peculiar velocity rather than a shift in the underlying physics.
We should remember that 'preliminary' in these massive surveys often means the systematic error bars are still being tightened. If this is actually just a calibration drift across different sky patches, the shaking of the model is really just a data cleaning issue.
check the quadrupole moment.
The precision of the DESI instrument gives us a real chance to move past the Lambda CDM stalemate. If this anisotropy is real, it provides a specific target for researchers studying primordial magnetic fields.