Dec 13 – 18, 2015
International Conference Centre Geneva
Europe/Zurich timezone

Cosmological constraints on the neutron lifetime

Dec 14, 2015, 5:15 PM
Level 0, Room 4 (International Conference Centre Geneva)

Level 0, Room 4

International Conference Centre Geneva

17 Rue de Varembé, 1211 Geneva


Laura Salvati (University of Rome, Sapienza)


We show how to derive new constraints on the neutron lifetime based on cosmological observations. Under the assumption of standard Big Bang Nucleosynthesis, the abundance of light elements, in particular Helium, is strongly dependent on the neutron lifetime. From CMB anisotropies it is possible to constrain primordial abundances of light elements, inferring the value of the neutron lifetime. We start considering recent Planck 2015 results of temperature and polarization anisotropies of the CMB. We show how including direct astrophysical measurements of primordial Helium abundance it is possible to obtain stringent constraints on the neutron lifetime. Furthermore, we compute the neutron lifetime theoretical expectation and we compare this value with our results, with the value quoted by the Particle Data Group and with the ones obtained in ``bottle method" and ``beam method" experiments. Finally, we perform forecasts on different future CMB experiments. We highlight the high precision that can be reach from these experiments, such as CMB surveys as COrE+, in combination with a weak lensing survey as EUCLID, that could constrain the neutron lifetime up to a $\sim 6$ s precision.

Primary author

Laura Salvati (University of Rome, Sapienza)


Alessandro Melchiorri (University of Rome, Sapienza) Luca Pagano (University of Rome, Sapienza) Rossella Consiglio (University of Naples, Federico II)

Presentation materials