English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Distortions of Cosmic Microwave Background (CMB) temperature and polarizationmaps caused by gravitational lensing, observable with high angular resolutionand high sensitivity, can be used to measure the neutrino mass. Assuming twomassless species and one with mass m_nu we forecast sigma(m_nu) = 0.15 eV fromthe Planck satellite and sigma(m_nu)=0.04 eV from observations with twice theangular resolution and about 20 times the sensitivity. A detection is likely atthis higher sensitivity since the observation of atmospheric neutrinooscillations require mass-squared differences greater than about (0.04 eV)^2.Comment: 4 pages, 1 figure; Version accepted for publication in PR

Determining Neutrino Mass from the Cosmic Microwave Background Alone