English

A note of clarification: BICEP2 and Planck are not in tension

Cosmology and Nongalactic Astrophysics 2014-05-07 v1

Abstract

The apparent discrepancy between the value of the tensor-to-scalar ratio reported by the BICEP2 collaboration, r=0.200.05+0.07r = 0.20^{+0.07}_{-0.05} at 68% CL, and the Planck upper limit, r<0.11r < 0.11 at 95% CL, has attracted a great deal of attention. In this short note, we show that this discrepancy is mainly due to an `apples to oranges' comparison. The result reported by BICEP2 was measured at a pivot scale k=0.05k_* = 0.05 Mpc1^{-1}, assuming nt=0n_t = 0, whereas the Planck limit was provided at k=0.002k_* = 0.002 Mpc1^{-1}, assuming the slow-roll consistency relation nt=r/8n_t = -r/8. One should obviously compare the BICEP2 and Planck results under the same circumstances. By imposing nt=0n_t = 0, the Planck constraint at k=0.05k_* = 0.05 Mpc1^{-1} becomes r<0.135r < 0.135 at 9595% CL, which can be compared directly with the BICEP2 result. Once a plausible dust contribution to the BICEP2 signal is taken into account (DDM2 model), rr is reduced to r=0.160.05+0.06r = 0.16^{+0.06}_{-0.05} and the discrepancy becomes of order 1.3σ1.3\sigma only.

Keywords

Cite

@article{arxiv.1405.1390,
  title  = {A note of clarification: BICEP2 and Planck are not in tension},
  author = {Benjamin Audren and Daniel G. Figueroa and Thomas Tram},
  journal= {arXiv preprint arXiv:1405.1390},
  year   = {2014}
}

Comments

Brief note (2 pages, 2 figures), just to clarify certain aspects about the comparison between the BICEP2 and Planck results