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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Warm Dark Matter (WDM) research is progressing fast, the subject is new andWDM essentially works, naturally reproducing the astronomical observations overall scales: small (galactic) and large (cosmological) scales (LambdaWDM).Evidence that Cold Dark Matter (LambdaCDM) and its proposed tailored cures donot work at small scales is staggering. Fedor Bezrukov, Pier-StefanoCorasaniti, Hector J. de Vega, Stefano Ettori, Frederic Hessmann, Ayuki Kamada,Marco Lombardi, Alexander Merle, Christian Moni Bidin, Angelo Nucciotti onbehalf of the MARE collaboration, Sinziana Paduroiu, Henri Plana, NormaSanchez, Patrick Valageas, Shun Zhou present here their highlights of theWorkshop. LambdaWDM simulations with keV particles remarkably reproduce theobservations, small and large structures and velocity functions. Cored DM halosand WDM are clearly determined from theory and astronomical observations, theynaturally produce the observed structures at all scales. keV sterile neutrinosare the leading candidates, they naturally appear extensions of the standardmodel of particle physics. Astrophysical constraints including Lyman alphabounds put its mass in the range 1< m <13 keV. Predictions for EUCLID andPLANCK have been presented. MARE and an adapted KATRIN experiment could detecta keV sterile neutrino. It will be a fantastic discovery to detect dark matterin a beta decay. A formidable WDM work to perform is ahead of us, thesehighlights point out some relevant research directions to put the effort.Photos of the Workshop are included (Abridged).

Warm dark matter in the galaxies:theoretical and observational progresses. Highlights and conclusions of the chalonge meudon workshop 2011