We present constraints on the tensor-to-scalar ratio r using a combination of BICEP/Keck 2018 (BK18) and Planck PR4 data allowing us to fit for r consistently with the six parameters of the ΛCDM model. We discuss the sensitivity of constraints on r to uncertainties in the ΛCDM parameters as defined by the Planck data. In particular, we are able to derive a constraint on the reionization optical depth τ and thus propagate its uncertainty into the posterior distribution for r. While Planck sensitivity to r is slightly lower than the current ground-based measurements, the combination of Planck with BK18 and baryon-acoustic-oscillation data yields results consistent with r=0 and tightens the constraint to r<0.032 at 95% confidence.

Improved limits on the tensor-to-scalar ratio using BICEP and Planck / M. Tristram, A.J. Banday, K.M. G('o)rski, R. Keskitalo, C.R. Lawrence, K.J. Andersen, R.B. Barreiro, J. Borrill, L.P.L. Colombo, H.K. Eriksen, R. Fernandez-Cobos, T.S. Kisner, E. Mart('i)nez-Gonz('a)lez, B. Partridge, D. Scott, T.L. Svalheim, I.K. Wehus. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 105:8(2022), pp. 083524.083524-1-083524.083524-7. [10.1103/PhysRevD.105.083524]

Improved limits on the tensor-to-scalar ratio using BICEP and Planck

L.P.L. Colombo;
2022

Abstract

We present constraints on the tensor-to-scalar ratio r using a combination of BICEP/Keck 2018 (BK18) and Planck PR4 data allowing us to fit for r consistently with the six parameters of the ΛCDM model. We discuss the sensitivity of constraints on r to uncertainties in the ΛCDM parameters as defined by the Planck data. In particular, we are able to derive a constraint on the reionization optical depth τ and thus propagate its uncertainty into the posterior distribution for r. While Planck sensitivity to r is slightly lower than the current ground-based measurements, the combination of Planck with BK18 and baryon-acoustic-oscillation data yields results consistent with r=0 and tightens the constraint to r<0.032 at 95% confidence.
Settore FIS/05 - Astronomia e Astrofisica
Settore PHYS-05/A - Astrofisica, cosmologia e scienza dello spazio
2022
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1135255
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