Journal
PHYSICAL REVIEW D
Volume 89, Issue 10, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.89.107302
Keywords
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Funding
- NSF [0244990]
- John Templeton Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [0244990] Funding Source: National Science Foundation
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The recent indications for a tensor-to-scalar ratio r similar or equal to 0.2 from BICEP2 measurements of the cosmic microwave background (CMB) B-mode polarization present some tension with upper limits r less than or similar to 0.1 from measurements of CMB temperature fluctuations. Here we point out that tensor perturbations can induce B modes in the CMB polarization without inducing any temperature fluctuations nor E-mode polarization whatsoever, but only at the expense of violating the Copernican principle. We present this mathematical possibility as a new ingredient for the model-builder's toolkit in case the tension between B modes and temperature fluctuations cannot be resolved with more conventional ideas.
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