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

We obtain a newly charged BBMB (Bocharova-Bronnikov-Melnikov-Bekenstein)black hole solution from the Einstein-Weyl-Maxwell-conformal (conformallycoupled) scalar theory with a positive Weyl coupling parameter $m^2_2$numerically. This solution has a primary scalar hair, compared to a secondaryscalar hair in the charged BBMB black hole solution. The limiting case of$m_2^2\to\infty$ leads to the series form of the charged BBMB black holesolution. However, for $m^2_2<0$, we could not obtain any asymptotically flatblack hole solution with scalar hair.

Black hole with primary scalar hair in Einstein-Weyl-Maxwell-conformal scalar theory