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/

Zendy Plus

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

Zendy Tools

Zendy Open

Recent works have included the effect of rotation on simulations of blackhole events at the LHC, showing that the angular momentum of the black holecannot be ignored and it makes a non-trivial contribution for most of thelifetime of the black hole. A key consequence of the rotation of the black holeis that the Hawking radiation is no longer isotropic, making it more difficultto infer space-time parameters from measurements of the emitted particles. Inthis letter we study the angular distribution of the Hawking emission ofnon-zero spin particles with specific helicity on the brane. We argue that theshape of the distribution could be used as a measure of the angular momentum ofthe black hole.

Angular profile of emission of non-zero spin fields from a higher-dimensional black hole