What specific observational signature in the Cosmic Microwave Background (CMB) is crucial for distinguishing between the inflationary model and the gravitational wave alternative?

Answer

B-mode polarization patterns.

The key difference in predictions between the models often boils down to the specific spectrum and intensity of gravitational wave signatures imprinted on the CMB, specifically detected via B-mode polarization.

What specific observational signature in the Cosmic Microwave Background (CMB) is crucial for distinguishing between the inflationary model and the gravitational wave alternative?

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