Cosmological neutrino mass detection in the next five years

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• Rupert Allison (Oxford)
• Wednesday 09 December 2015, 13:45-14:15
• Sackler Lecture Theatre, IoA.

If you have a question about this talk, please contact Andrew Shannon.

Future cosmological measurements should enable the sum of neutrino masses to be determined indirectly through their effects on the expansion rate of the Universe and the clustering of matter. I will discuss the cosmological effects of neutrinos and how they appear in CMB and large-scale structure observables. I will outline how the mass measurement may be reached, step-wise, using data collected during the coming decade. Finally, I will explore the dependence of the mass constraint on experimental details and examine degeneracies with other cosmological parameters.

This talk is part of the Institute of Astronomy Seminars series.

This talk is included in these lists:

• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Seminars
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA

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